Laser Fundamentals I | MIT Understanding Lasers and Fiberoptics

MIT OpenCourseWare
21 Mar 201258:14

Summary

TLDRThe video script offers an insightful introduction to the course 'Understanding Lasers and Fiber Optics'. It covers the fundamental properties of lasers, such as high monochromaticity and spatial coherence, and their applications in various fields. The instructor promises a simplified approach, focusing on basics over complex details, to make the course accessible to a wider audience. The script also delves into the unique properties of lasers, including their narrow spectral width and high temporal coherence, essential for applications like holography and fiber optic communication.

Takeaways

  • 📚 The script is from a course on 'Understanding Lasers and Fiber Optics', aiming to cover various fundamental aspects of lasers and their applications.
  • 🌟 It emphasizes the unique properties of lasers, such as high monochromaticity, high coherence, and the ability to produce an extremely narrow spectral width, which is vital for numerous applications.
  • 🔍 The course will explore how lasers achieve such properties, starting with the basic principles of oscillators and extending to the concept of an optical oscillator, which is fundamental to laser operation.
  • 🎓 The presentation style is simplified to make the material accessible to people without specialized backgrounds, focusing on fundamentals with minimal mathematical complexity.
  • 🕊️ The script mentions a variety of applications for lasers, including barcode readers, CD players, laser printers, holography, sensors, fiber optic communication, materials processing, non-destructive testing, spectroscopy, military uses, and medical diagnostics.
  • 🔑 The script introduces the concept of a resonator, which is crucial for determining the frequency of the laser and involves two mirrors to create standing waves for different modes.
  • 💡 The importance of a light amplifier within the laser cavity is highlighted as it provides the necessary gain to overcome losses and maintain oscillation.
  • 🔬 The course will delve into the practical aspects of laser operation, including the issues and problems associated with lasers and how they can be mitigated.
  • 🌈 The variety of lasers and their specific characteristics will be discussed, including how different lasers are pumped and operate.
  • 🌐 The basics of fiber optics will also be introduced, setting the stage for understanding the principles and applications of fiber optic communication.
  • 🚀 The script promises to touch on future developments in both lasers and fiber optics, indicating the ongoing innovation and advancement in these fields.

Q & A

  • What is the main topic of the short course presented in the script?

    -The main topic of the short course is 'Understanding Lasers and Fiber Optics', covering various aspects of lasers, their properties, applications, and fiber optics basics.

  • Why are lasers of significant interest today?

    -Lasers are of significant interest due to their unique properties that enable a wide range of applications, from barcode readers and compact disks to medical diagnostics and military systems.

  • What are the key properties of lasers that make various applications possible?

    -The key properties of lasers include high monochromaticity, high coherence, high collimation, high spatial coherence, and the ability to produce high power, tunable wavelengths, and short pulse widths.

  • What is meant by the term 'monochromaticity' in the context of lasers?

    -Monochromaticity refers to the property of lasers emitting light of a single color or having a very narrow spectral width, which is essential for high-resolution applications.

  • How does the script describe the operation of a simple laser?

    -The script describes the operation of a simple laser by discussing the need for a resonator (laser cavity) and a light amplifier to overcome losses and achieve a continuous, coherent light output.

  • What are some of the practical issues and problems associated with lasers?

    -Practical issues with lasers include imperfections in their operation, potential problems if not treated properly, and the need to minimize or eliminate certain issues that can arise from their use.

  • What is the significance of the coherence time in lasers?

    -The coherence time in lasers is significant because it determines the duration over which the phase and amplitude of the laser light can be predicted accurately, which is crucial for applications like holography and interferometry.

  • How do the properties of lasers contribute to fiber optic communication?

    -The properties of lasers, particularly their high monochromaticity and coherence, contribute to fiber optic communication by allowing for the transmission of data over long distances with minimal distortion and high bandwidth.

  • What is the role of the light amplifier in a laser system?

    -The light amplifier in a laser system provides gain to the light oscillating within the laser cavity, overcoming losses and enabling the production of a continuous, coherent light output.

  • How does the script differentiate between continuous wave (CW) lasers and pulsed lasers?

    -The script differentiates between continuous wave (CW) lasers, which produce a constant, uninterrupted beam of light, and pulsed lasers, which emit light in short, discrete pulses of high power.

  • What is the purpose of using demonstrations in the course as mentioned in the script?

    -Demonstrations are used in the course to illustrate fundamental phenomena in lasers and fiber optics, making the concepts more understandable and engaging for people without specialized backgrounds.

  • What is the relationship between the spectral width of a laser and its coherence properties?

    -The spectral width of a laser is directly related to its coherence properties. A laser with a very narrow spectral width exhibits high temporal coherence, meaning it maintains a constant phase relationship over time, which is essential for applications like high-resolution spectroscopy.

  • How do the unique properties of lasers enable various applications such as barcode readers and laser shows?

    -The unique properties of lasers, such as high monochromaticity, coherence, and the ability to focus into a small spot, enable applications like barcode readers by providing precise light for scanning, and laser shows by allowing for the creation of bright, focused beams for visual displays.

Outlines

00:00

📚 Introduction to the Course on Lasers and Fiber Optics

The script introduces a course on 'Understanding Lasers and Fiber Optics' and outlines the topics to be covered. The instructor welcomes the audience and emphasizes the importance of lasers due to their unique properties that enable various applications. The course will delve into the reasons behind the widespread interest in lasers, their key properties, the operation of a simple laser, potential issues, types of lasers, and an introduction to fiber optics. The presentation style will be simplified to cater to a non-specialized audience, focusing on fundamentals with minimal math and plenty of demonstrations.

05:01

🌈 The Unique Properties and Applications of Lasers

This paragraph discusses the unique properties of lasers, such as high monochromaticity, which refers to their single color or narrow spectral width. It also touches on the high temporal coherence of lasers, which is related to the uninterrupted radiation time of atoms. The script provides examples of how these properties contribute to various applications, including barcode readers, compact disks, laser printers, holography, sensors, fiber optic communication, materials processing, non-destructive testing, spectroscopy, military applications, and medical procedures. The wide range of applications is a testament to the versatility and importance of lasers in modern technology.

10:01

🔬 Measuring Spectral Width and Temporal Coherence

The script explains how to measure the spectral width of light sources, such as spectral lamps and lasers, using a spectrometer. It contrasts the broad spectral width of a typical spectral lamp with the extremely narrow spectral width of a laser, which can be in the range of megahertz or even microhertz. The concept of high temporal coherence is introduced, relating it to the uninterrupted radiation time (tau) and its inverse relationship with the spectral line width (delta f). The paragraph also describes how the coherence time is limited to the duration of uninterrupted wavetrains and how this property is crucial for applications like communication, spectroscopy, interferometry, holography, and sensors.

15:01

📡 High Spatial Coherence and Collimation of Lasers

This paragraph delves into the concept of high spatial coherence and collimation in lasers. It explains how the laser beam's high degree of collimation allows for long-distance applications with minimal divergence. The script contrasts this with traditional light sources, which require smaller source sizes or longer focal lengths to achieve similar effects, often at the expense of light intensity. The paragraph also discusses the ability of lasers to produce a very small focus spot due to their diffraction-limited focusing, which is essential for applications like compact discs, laser printers, materials processing, and medical surgery.

20:04

🚀 Applications of Laser Properties in Various Fields

The script highlights the practical applications of laser properties in fields such as alignment, barcode scanning, long-distance communication, and space radar. It also discusses the importance of a laser's small focus spot and high intensity for tasks like cutting, welding, drilling, and medical procedures like retinal surgery. The paragraph emphasizes the advantage of lasers in creating intense, small spots that traditional light sources cannot achieve without losing intensity.

25:07

🔍 Exploring High Spatial Coherence and Its Implications

This paragraph explores the concept of high spatial coherence in lasers, which allows for the prediction of a wave's amplitude and phase at any spatial position at a given time. It contrasts this with traditional light sources that do not exhibit such stable spatial behavior. The script also touches on the ability to create collimated beams and focused spots with high spatial coherence, which is beneficial for applications where precise control of light is required.

30:07

⚡ High Power Capabilities of Lasers and Their Applications

The script discusses the high power capabilities of lasers, both in continuous wave (CW) and pulsed forms. It provides a range of power levels from milliwatts to exowatts, highlighting the versatility of lasers in producing extreme power levels. Applications mentioned include materials processing, fusion research, military uses, and nonlinear optics, which benefit from the high intensity that lasers can generate.

35:10

🌈 Tuning Range and Short Pulse Widths of Lasers

This paragraph covers the wide tuning range of lasers across the electromagnetic spectrum and their ability to produce very short pulse widths. It explains how lasers can be tuned to interact with specific atoms and molecules, study atomic and molecular structures, and be used in medical applications. The script also emphasizes the importance of short pulse widths for studying fast phenomena, high-resolution radar and imaging, and potential applications in optical computing.

40:11

🔧 How Lasers Achieve Their Unique Properties

The script shifts focus to explaining how lasers achieve their unique properties of monochromaticity and high temporal coherence. It introduces the concept of an optical oscillator and compares it with traditional oscillators. The paragraph sets the stage for understanding the workings of a laser by first reviewing the properties of oscillators and how they can be made to produce constant amplitude and narrow spectral width, which are key to the operation of a laser.

45:12

🔄 The Role of Resonators and Amplifiers in Lasers

This paragraph delves into the technical aspects of how lasers function as optical oscillators, highlighting the need for a resonator and an amplifier. It explains the concept of a resonator using two mirrors to create electromagnetic oscillations at specific frequencies. The script also discusses the role of an amplifier in providing gain to overcome losses within the resonator, which is essential for sustaining oscillation and producing the laser's characteristic output.

Mindmap

Keywords

💡Lasers

Lasers are devices that emit light through a process of optical amplification based on the stimulated emission of radiation. In the video, lasers are the central theme, with discussions on their unique properties and applications in various fields such as medicine, communication, and industry.

💡Fiber Optics

Fiber optics refers to the technology of transmitting information as pulses of light through a fiber made of glass or plastic. The script mentions fiber optics as a significant topic, highlighting its basics and issues, as well as its connection to lasers for communication purposes.

💡Monochromaticity

Monochromaticity is the property of having a single color, which in the context of lasers, refers to the high purity of the light's color and its narrow spectral width. The video explains how this property, crucial for applications like holography and spectroscopy, is achieved in lasers.

💡Temporal Coherence

Temporal coherence describes the predictability of a wave's phase over time. The script discusses how lasers have high temporal coherence, meaning the light waves maintain a constant phase relationship, which is vital for applications such as interferometry and holography.

💡Collimation

Collimation refers to the process of making a beam of light parallel. The video script emphasizes that lasers produce highly collimated beams, which is essential for applications requiring precise alignment or long-distance transmission, such as in laser pointers or fiber optic communication.

💡Spectral Width

Spectral width is the range of wavelengths emitted by a light source. The script explains that lasers have an extremely narrow spectral width, which is a key to their monochromaticity and high temporal coherence, and is crucial for high-resolution applications.

💡Demonstrations

Demonstrations in the script refer to the use of visual aids and experiments to illustrate fundamental phenomena in lasers and fiber optics. The instructor intends to use demonstrations to make the complex concepts more understandable and engaging for the audience.

💡Optical Oscillator

An optical oscillator is a system that generates a continuous, coherent beam of light by reflecting it back and forth between two mirrors. The script delves into the concept of an optical oscillator to explain how lasers produce their characteristic narrow spectral width and high coherence.

💡Resonator

A resonator is a part of a laser system that supports the formation of standing waves. The script describes the laser cavity as a type of resonator that defines the laser's frequency and mode, which is essential for achieving the laser's unique properties.

💡Gain

In the context of lasers, gain refers to the amplification of light as it passes through an active medium, overcoming losses in the laser cavity. The script mentions that gain is necessary for the laser action to occur, and it will be discussed in more detail in subsequent sessions.

💡Applications

Applications refer to the various uses of lasers and fiber optics. The script provides numerous examples of applications, such as barcode readers, laser shows, holography, sensors, fiber optic communication, and medical procedures, demonstrating the wide-ranging impact of these technologies.

Highlights

Introduction to the course 'Understanding Lasers and Fiber Optics' and its educational goals.

Explanation of the unique properties of lasers that enable a wide range of applications.

Discussion on how lasers have revolutionized various fields including data storage, printing, and medical procedures.

Overview of the course content, emphasizing the basics of fiber optics and future developments in the field.

Introduction to the concept of monochromaticity and its significance in laser applications.

Illustration of the narrow spectral width of lasers compared to traditional light sources.

Explanation of high temporal coherence and its relation to laser line width.

Demonstration of how to measure the spectral width of lasers using a spectrometer.

Discussion on the applications of high temporal coherence in communication, spectroscopy, and holography.

Introduction to the property of high spatial coherence and its implications for laser beams.

Comparison of laser beams to traditional light sources in terms of collimation and focusability.

Explanation of how laser properties enable precise control in applications like barcode readers and medical surgery.

Overview of the power levels achievable with continuous wave and pulsed lasers.

Discussion on the practical applications of high laser power in materials processing and military uses.

Introduction to the tunability of lasers across the electromagnetic spectrum.

Explanation of how laser tunability is utilized in spectroscopy and medical applications.

Discussion on the ability of lasers to produce extremely short pulse widths and their applications.

Summary of the key properties of lasers and their derivation from the function of an optical oscillator.

Introduction to the concept of an optical oscillator and its role in creating laser properties.

Transcripts

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good morning everyone

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wherever you are

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i'd like to welcome you to this short

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course

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entitled

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understanding lasers

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and fiber optics

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and before i do anything

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i'd like to

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tell you

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what sort of topics i'll be covering

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i will start with

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the many reasons why we're all

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interested in lasers today

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then

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i would like to

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talk about the key properties of lasers

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that make all these applications

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possible

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then once we understand these key

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properties then i would like to discuss

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how these properties

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excuse me come about

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and then

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we'll go describing the operation of a

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simple laser and even show you a

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demonstration how a simple laser works

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what you need to make things happen

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and then we look at variety of

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properties of this

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simple laser

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then

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we go look at

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other issues and problems to do with

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with lasers lasers are not perfect and

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if you don't treat them right you know

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they can give you give you some problems

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and in some cases you can get rid of

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these problems in some cases well you

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try to minimize them

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then i will discuss the the variety of

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lasers and what makes them tick

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because we have all kinds of lasers

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today and it's nice to get a feel for

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the variety of them and how they work

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how they get pumped and so on

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then i'm going to change topics and i

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will

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switch to the basics of fiber optics

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and to to familiarize you with what's

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going on in fiber optics what are the

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issues and but mainly the emphasis on on

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on basics and then finally i'll have a

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few words to say about future

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developments in in lasers and fiber

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optics

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now

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the how will i present uh the material

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well

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i will be using a very simplified

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treatment

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and the reason is so that people without

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specialized background can can follow

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i will emphasize only fundamentals

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and

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not

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not the details so that

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the the understanding can be made

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very easy

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and i will use very little math

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i will certainly not emphasize

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mathematics because i would like to make

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it very understandable and i don't want

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to switch people

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off

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and most important i'll be using lots of

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demonstrations

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to

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to illustrate some of the fundamental

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phenomena in lasers and also in in fiber

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optics

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so now i think we're ready to to start

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the course

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and the uh

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the first topic that i had is why is

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there so much interest in in lasers

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well

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the

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the reason why there's so much interest

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is because

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lasers have these unique properties that

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we're going to discuss

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and it and it's these unique properties

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that make

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all these applications happen

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now these properties have created all

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sorts of new devices

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we'll mention a few of them briefly

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and

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also have improved

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many existing

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devices so the laser

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has been

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very nice

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in in lots of lots of fields just to

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give you some example of of uh just a

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few applications

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well let's just just look at them just

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briefly the barcode readers everybody's

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familiar today with barcode readers now

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lasers certainly make that possible

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and of course the compact disks computer

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printers laser color copiers

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all these depend on on some of these

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properties of lasers that we'll be

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discussing

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then of course you've seen the laser

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shows

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and that certainly uses a specific laser

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property then there is holography

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that's the 3d imaging

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the hologram that you see on

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on credit cards

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that's all due to

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lasers then lasers are also used for

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precise control of position and

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motion

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for example

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sensors

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lasers today can measure all kinds of

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things

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with fiber optics without fiber optics

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or what have you

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the

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the big area

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of today and the future is fiber optic

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communication

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and again it involves not only fiber

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optics but also lasers so we'll see how

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the properties of lasers are used for

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fiber optic communication

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then we have topics like materials

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processing like cutting drilling welding

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and so on in materials

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there is a whole slew of

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uh

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techniques for non-destructive testing

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this is the destruction the testing of

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of systems without without having to

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destroy them and lasers are quite

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sensitive and they can do that without

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the need to damage the the systems

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then we go to spectroscopy and a variety

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of spectroscopic techniques have been

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opened up by by the laser

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chemical process

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then we get to the military application

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military systems and we hear a lot about

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the

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laser

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the use of lasers in in the military

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and finally least

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last but not least we have medical

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procedures medical diagnostics using

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using lasers

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and all these applications come about

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because of very few

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unique properties of lasers and

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certainly in this course we want to make

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sure that that we understand those and

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how they come about in fact the

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we find lasers all over the place today

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we find them in the home in the factory

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in hospitals in laboratory in the the

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military wherever it is in even in space

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in the ocean and even in the in the

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theater so you can see lasers are

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playing a very important role in our

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lives today

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all right so now i would like to go

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and to the next to the next topic and

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that is the the unique properties of uh

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of lasers

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all right so what are these unique

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properties

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well let's start with

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property number one

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now some people refer to it as high

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monochromaticity

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what is monochromaticity well that means

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it's one color

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and we have to see what what people mean

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by that others

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refer to it as as a source of light that

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has very narrow spectral width

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again we want to see what what what it

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means

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and uh and and others may refer to this

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property as high as a as something that

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has a high temporal coherence and we

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want to understand uh what all what the

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meaning of all these things are

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so let's start first with

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with uh

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with the narrow spectral width or the

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single color here what i have and i hope

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you can see it the colors of the

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spectrum

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i did the coloring myself and it's

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pretty close to to the spectrum with

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whatever colors uh i had

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now

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the the visible range as we all know

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extends from about 4 500 angstroms to

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about 6

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500 angstroms in the in the red

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which is about what two thousand

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angstroms or so

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and that's that's the visible

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essentially that's the visible range

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now when we compare

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uh light sources

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to this to this range for example the

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spectral lamp that has a very narrow uh

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line width or spectral width here it is

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here's the typical output of a spectral

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lamp let's say here in the yellow and

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the width

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over which there's this radiation could

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be as low as one-tenth of an angstrom

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okay or 0.1 angstroms or

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in terms of uh frequency it's uh 10 10

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gigahertz

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and then you can get

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some lamps that have smaller line widths

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or you can even get them with broader

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line width depending on on the

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conditions of the discharge and so on

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and when we come to to lasers

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the line width is extremely narrow the

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spectral width is extremely narrow and

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it can be in the megahertz

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but can also be in the micro hertz now

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remember this is 10 to the minus 6 hertz

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or even smaller so the laser

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is an incredible kind of device device

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when it comes to the spectral width

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the line width can be extremely narrow

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now i know in practice that's not what

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one measures but but if you get rid of

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some of the effects we'll talk about

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external effects then you should be able

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to see line widths as narrow as narrow

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as that all right so so the laser then

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is is extremely extremely narrow

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the uh

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let's see how now let's see how you

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might uh

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measure the uh the spectral width so you

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don't have to take my word for it let's

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see how you might measure it well if you

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took a typical spectral lamp here and

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then collect some of the light from it

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and put it into a spectrometer or some

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other device

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device that measures the spectrum then

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what you get you get a plot like this

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intensity versus wavelength and here you

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can either plot wavelength or you can

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plot frequency depending on

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the kind of work you do

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and then you'll see some blob like this

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and it has a certain width over which

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the the the source radiates and we call

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it either delta lambda for the width or

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or delta f

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now

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when we compare it with a

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with a laser again we'll do the same

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thing we'll take the laser and feed it

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into a spectrometer or some other device

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the width here can be very narrow and

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just like i said before can be

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even as narrow as micro hertz

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but these are only under special

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conditions but even if it's uh megahertz

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or tens of megahertz it's way narrower

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than you get from from a from a lamp

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so again if you're not sure then you

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have to do the experiment and check

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indeed that the laser does give you an

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extremely narrow

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narrow line width all right so that's

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basically then the the the line width of

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the of the laser

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now the next thing is what about

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high temporal coherence what has that

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got to do with the line width of the

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laser all right so now we need to

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explain that topic

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now

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let's start first with with a wave with

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a sine wave

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okay now the sine wave let's say starts

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from

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minus infinity in terms of time and goes

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all the way to plus infinity completely

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uninterrupted a pure sine wave now if

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you had a wave like this that has a

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constant frequency and a constant

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amplitude

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then when you look at its spectrum on

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the in the frequency in the frequency

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domain

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what you see you see something that's

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let's say centered at at f zero f sub

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zero with a width delta f here very

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close to to zero all right now this is a

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source

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of radiation it's like a sun wave like

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this that has

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that has what we call perfect temporal

play12:46

coherence or time coherence and that's

play12:49

the best essentially the best that one

play12:52

can have

play12:54

now in in in practice

play12:57

uh light sources

play12:59

uh do not

play13:00

radiate for such a long for a long time

play13:03

without any phase interruption so let's

play13:06

say we have a light source like this

play13:08

that that radiates only for a time town

play13:12

and then shuts off for example

play13:14

now this one because it's it only

play13:17

radiates for a time tau it's going to

play13:20

have a line width in the frequency

play13:21

domain it's going to it's not going to

play13:22

be

play13:23

a delta function like we had before and

play13:25

this width if you do the calculation

play13:27

this width in terms of frequency is

play13:29

proportional to 1 over the the length of

play13:33

this wave train tau

play13:36

again i put approximate so that i don't

play13:38

get into trouble about the exact numbers

play13:40

but it's very close to delta f is one

play13:42

over tau

play13:44

so that if tau is very long if tau is

play13:46

very long then delta f is small as we've

play13:48

shown you before but if tau is short

play13:51

then the

play13:52

line width here will will grow

play13:55

now

play13:56

atoms

play13:58

for example because this is where we get

play14:00

our radiation from from atoms they

play14:03

radiate in bursts

play14:05

bursts like like this

play14:07

now if they radiate in bursts like this

play14:09

then then tau can be sometimes can be

play14:12

quite short which means that the width

play14:14

of the radiation will be will be uh

play14:17

broader so the shorter this is then the

play14:20

broader this this width and here i show

play14:23

bursts from other atoms and when you put

play14:26

them all together essentially that's

play14:27

what you get you get a certain width

play14:30

that's characteristic of the time of the

play14:33

uninterrupted radiation of atom and here

play14:36

we get an interruption therefore the tau

play14:39

then is only when the wave is is

play14:42

uninterrupted now some other atoms

play14:46

will radiate in in decaying

play14:50

sinusoids exponentially decaying sinus

play14:52

so it doesn't matter the calculation is

play14:54

a little bit

play14:56

trickier but again you get a sort of

play14:58

width and for the purpose of this course

play15:01

uh all i'm after is is the uh is the uh

play15:05

is the dominant width and i'm not

play15:07

worried about little side bands down

play15:08

here just just the width and again you

play15:10

can say that the width here is of the

play15:13

order of one over tau whether it's

play15:16

exponentially decaying or it looks like

play15:18

this or what have you

play15:20

all right then then to summarize now

play15:23

high temporal coherence means that the

play15:27

radiation time

play15:29

of the atoms without phase interruption

play15:31

is very long because the line width is

play15:33

one over tau

play15:35

would be very small

play15:37

and when you have

play15:39

something that has a high temporal

play15:40

coherence which means tau very long it

play15:42

means that you can predict

play15:44

the amplitude and the phase of the wave

play15:47

at uh at any time every time because

play15:50

it's a pure wave in fact if i go back to

play15:53

to this uh plot over here so this is

play15:56

where you have

play15:57

infinite uh

play15:59

coherence

play16:01

it means that if i know the amplitude

play16:04

and phase of the wave at this time

play16:06

i can only with using a clock i can

play16:09

predict exactly what the amplitude and

play16:11

phase of the wave would be at some other

play16:13

time later and the separation in the

play16:16

time can be can be very long

play16:18

when when we get to

play16:20

uh

play16:21

when we get into

play16:23

into sources that radiate like this then

play16:26

obviously within

play16:28

this time

play16:30

i can predict uh the the amplitude and

play16:32

phase of the wave but if i stretch the

play16:35

time a little further bigger than this

play16:37

tau then i cannot

play16:39

predict any more the amplitude in the

play16:41

face because this is like another

play16:43

another

play16:44

waveform that is completely uncorrelated

play16:47

with the first one so what we call the

play16:49

coherence time now is going to be

play16:50

limited only to this time during which

play16:54

the the uh the uh

play16:56

the wave is uninterrupted

play16:59

then you might ask well what are typical

play17:01

applications of of of this of this

play17:05

unique property

play17:07

well

play17:08

the uh the fact that it has narrow line

play17:10

with can be used in uh in communication

play17:13

certainly that's a key key property here

play17:15

in spectroscopy especially in high

play17:17

resolution spectroscopy in

play17:20

interferometry

play17:22

uh holography and a variety of sensors

play17:24

so that's a that's a key property for

play17:27

for many many applications

play17:30

now

play17:31

what i'd like to do is discuss the

play17:34

second what i call the second unique

play17:36

property of uh of lasers

play17:39

now here it is

play17:41

the many ways of of describing it one

play17:44

way is

play17:46

that the laser is has a highly

play17:48

collimated beam and we've seen that in

play17:50

laser shows and what have you that the

play17:52

laser has a highly collimated beam

play17:54

other people

play17:56

may use more better scientific language

play17:58

and would call it a diffraction limited

play18:00

collimation and we want to know what

play18:03

that means

play18:05

to sum

play18:07

the fact that the laser has a very small

play18:09

focus spot is a is this meaning of this

play18:13

property

play18:14

and others may call it again in a better

play18:16

scientific language it's a diffraction

play18:18

limited focus

play18:20

all right so whether it's diffraction

play18:22

limited collimation diffraction limited

play18:24

focusing or even

play18:27

as others might call it laser has high

play18:29

spatial coherence they all mean

play18:31

essentially the same thing and let's

play18:33

find out now what uh what we mean by uh

play18:36

by all these

play18:38

uh words

play18:40

all right let's go back and look at a uh

play18:43

a typical uh a typical light source

play18:45

let's say let's spectral lamp we have uh

play18:48

electrodes here plus and minus we have

play18:50

an arc here and then we collect the

play18:51

light from the arc with the lens and

play18:54

that's placed at the at the focus of the

play18:56

lens here this distance here f is the

play18:59

focal length of the lens so now we try

play19:00

to collimate this uh this light source

play19:03

well what sort of collimation do we get

play19:06

you can see here that this point this

play19:08

one end of the of the uh of the uh

play19:12

discharge

play19:13

or uh

play19:15

is you you collect these two arrays from

play19:17

here and you create a collimated beam in

play19:19

this direction

play19:20

uh the other end of this arc for example

play19:24

the other extreme will give you a

play19:25

collimated beam in this direction and

play19:27

when you put them together you have this

play19:30

this widely

play19:31

diverging beam

play19:33

now you can easily estimate the angle of

play19:36

this beam in fact the angle of the

play19:39

divergence of this beam theta is given

play19:41

by h which is half

play19:44

the

play19:44

the size of the source here

play19:48

in this case it's an arc it could be

play19:49

discharge lamp or whatever

play19:51

half the size of the of the source

play19:53

divided by the focal length of the lens

play19:57

and so so the

play19:59

so if if you don't like if this angle is

play20:01

too big then the only thing you can do

play20:04

is either reduce the size of the source

play20:07

or increase

play20:09

the

play20:10

focal length of the lens

play20:13

now if you let's look at the increasing

play20:15

the focal length of the lens if you

play20:17

increase

play20:18

the focal length of the lens means

play20:19

you've got to put it

play20:21

way far from from the source if you do

play20:24

that you're going to lose a lot of light

play20:26

so you may get a better collimation but

play20:28

there's not going to be much light in it

play20:30

the other

play20:31

thing to work on is h the size of

play20:34

of the source and clearly if you make it

play20:36

smaller and smaller then the collimation

play20:38

will be better and better

play20:40

and that's how

play20:42

pre-laser days that's how one got

play20:45

collimated beams with a lot of light in

play20:48

them because you try to generate sources

play20:50

that have their very small socks

play20:53

now let's see what's the best one can do

play20:55

here

play20:57

well the best one can do

play20:58

is called diffraction limited

play21:00

collimation

play21:02

and here if you do the the

play21:04

physics of it

play21:06

uh if you have a beam

play21:08

that's of diameter d

play21:10

then the best you can do this is now a

play21:12

perfect

play21:13

optical beam light beam or what have you

play21:15

beam electromagnetic radiation

play21:18

diameter d i don't care whether it's

play21:19

microwave optical

play21:21

uv or whatever whatever then the best

play21:24

you can do in terms of divergence angle

play21:26

is lambda

play21:28

divided by d lambda being the wavelength

play21:30

of the light dividing by d as simple as

play21:31

that and i make it approximate here

play21:33

because it's just a small factor here

play21:35

which i'm not going to worry about in

play21:36

this in this course the critical thing

play21:39

it depends on the ratio of lambda the

play21:40

wavelength over d the shorter the lambda

play21:43

the better the collimation the larger d

play21:46

the better the collimation or this the

play21:48

smaller is the divergence angle and it

play21:51

doesn't depend on any source size or

play21:53

anything because this is this is due to

play21:55

basic physics of of electromagnetic

play21:59

radiation that's why we call the

play22:01

diffraction

play22:02

limited collimation that's the best you

play22:04

can do so keep that keep that in mind

play22:06

now

play22:07

let's compare

play22:09

the

play22:11

the output of a laser with this uh with

play22:14

this diffraction limited beam here's a

play22:15

laser source

play22:17

and with some optics and what have you i

play22:18

can create a beam that's diameter d and

play22:21

if i go check

play22:22

this its size further down i indeed see

play22:25

that the angle here the angle of

play22:27

divergence is very close to lambda over

play22:30

d

play22:31

just like the the perfect light source

play22:34

that we talked about before

play22:36

so you can say that laser is indeed

play22:38

diffraction limited and and again the

play22:41

divergence is just limited by the

play22:43

wavelength divided by d while in the

play22:45

case of the light source we had to worry

play22:48

about the size of the source

play22:50

and the other important thing here is

play22:52

that all the laser light all the laser

play22:55

light can be put into into that beam so

play22:58

we don't need to lose any any light

play23:00

because we're not collecting enough so

play23:02

it's another fantastic kind of kind of

play23:05

property

play23:06

now the applications of this of this uh

play23:10

property

play23:11

uh

play23:13

let's start with the collimation part

play23:15

the the high degree of collimation can

play23:17

be used of course for alignment you can

play23:19

do go to large distances without the

play23:21

beam

play23:22

expanding too much certainly you see

play23:24

these barcodes with the lights flashing

play23:26

if if there was too much divergence you

play23:28

wouldn't be able to to

play23:31

scan the bars because the spacing is

play23:33

very small between them

play23:35

and certainly if you want to do long

play23:36

distance communication especially in

play23:38

space

play23:40

radar what have you uh high degree of

play23:42

condemnation is

play23:44

is very very important

play23:47

now the uh the next

play23:50

thing here is that i mentioned before is

play23:54

the very small focus spot or the

play23:56

diffraction limited focus

play23:59

now

play24:01

where does that where does that

play24:03

come from and and how does it compare

play24:05

with what we can do without

play24:07

lasers

play24:08

well let's go back to basics back to our

play24:12

arc lamp here

play24:13

and then we collect the light as we did

play24:15

before but now

play24:17

instead of just collimating let's put

play24:18

another lens and focus it down

play24:20

and that's normally how we get intense

play24:23

uh

play24:24

spots

play24:25

high intensity uh focused spots by again

play24:29

taking light from a source and and

play24:31

refocusing

play24:32

now it turns out that because the source

play24:34

has a certain size

play24:36

you're not going to be able to create

play24:38

anything here that's going to be

play24:39

brighter than the source and again if

play24:41

you don't believe me you have to go look

play24:43

up basic physics and and it sort of

play24:46

makes sense that it's very difficult

play24:49

it's impossible to make this brighter

play24:51

than here

play24:52

so you cannot increase the brightness uh

play24:56

as as dictated by uh by the source all

play25:00

right now what about lasers all right

play25:01

before we get to lasers what's the best

play25:04

one can do let's go back to our

play25:06

collimated beam of diameter d

play25:09

that that was our perfect ideal beam now

play25:12

if we take that put a lens here with a

play25:14

focal length f and focus it down it'll

play25:17

focus down to a very small spot

play25:19

now the this is the smallest spot that

play25:21

you can get and the spot size is given

play25:24

by our lambda over d which we remember

play25:26

from before multiplied by f the focal

play25:29

length of the lens

play25:32

now if f is approximately d

play25:35

if you can choose f proximity d then we

play25:37

have a spot size here that's of the

play25:39

order the wavelength of light

play25:42

so again without

play25:43

having to study hard or remember heart

play25:47

then we have two things the collimation

play25:49

is just given the best collimation you

play25:50

can get is lambda over d and the focus

play25:53

spot size is lambda

play25:56

and this is then assumes that it's a

play25:58

perfect a perfect light source

play26:01

all right so that

play26:03

now let's compare with with what the

play26:05

laser with the laser can do all right so

play26:08

now we bring the laser up so here's our

play26:11

laser giving us a beam a collimated beam

play26:14

of diameter d put a lens here focus it

play26:16

down

play26:17

and i go measure the spot size

play26:20

and it turns out that the spot size if

play26:22

i'm careful is very close to the

play26:25

wavelength of the of the light

play26:27

so this means that the the laser beam is

play26:31

as ideal and as close to perfect as one

play26:34

can get both in collimation as well as

play26:37

in focus

play26:38

while with a while with a light source

play26:41

it was difficult to to get something

play26:43

that is that is extremely bright

play26:46

you can make this of course the spot

play26:48

size small here by putting apertures by

play26:50

putting apertures here you can make this

play26:52

spot size small but you cannot have a

play26:55

small spot size with with very high

play26:58

intensity like you can here in this case

play27:00

you can put all that laser light and

play27:03

we'll talk about all kinds of outputs uh

play27:06

very soon and you can put all that into

play27:08

at this tiny spot and that's how you can

play27:11

get these huge

play27:12

intensities

play27:15

well you might say

play27:17

what are the applications of some of

play27:19

these small focus spots with high

play27:21

intensities well there are all kinds of

play27:23

applications there's compact discs

play27:26

for example that rely on a on a tiny uh

play27:28

small spot for the for the resolution

play27:32

certainly for laser printers and again

play27:34

for materials processing as i say for

play27:36

cutting and welding and uh

play27:39

uh

play27:40

drilling and so on and also in medical

play27:42

surgery

play27:43

where the the spot size you know for

play27:45

cutting and what have you has to be has

play27:47

to be pretty small you don't want to

play27:48

make a huge huge cut and also uh because

play27:52

you have to deliver so much intensity

play27:54

you need the uh spot size to be to be

play27:56

small okay especially like for example

play27:59

look at the example of retinal surgery

play28:03

retinal welding where you try to weld

play28:04

the retina the spot size is a key is a

play28:07

key issue

play28:08

because you can almost get any light

play28:10

source to to spot weld the retina the

play28:12

only problem is it's what wells the

play28:14

entire retina but here with a tiny with

play28:17

a tiny beam tiny focused beam you can

play28:20

you can only weld

play28:22

just just small areas of course they're

play28:24

damaged areas and you hopefully you can

play28:26

still see with the rest of the retina so

play28:28

the the small spot size is is a key

play28:31

thing to a lot of these applications

play28:34

now

play28:35

uh i mentioned earlier that uh

play28:38

that some people refer to this property

play28:40

of high collimation or or

play28:43

a small focus spot to high spatial

play28:45

coherence so let's see what uh what is

play28:48

meant by uh by that

play28:52

the uh

play28:54

here is uh

play28:56

high special coherence and and the and

play28:59

the what we mean by that is that the

play29:01

wave is well behaved in space

play29:05

now before

play29:06

we talked about

play29:08

uh

play29:09

waves that are well behaved with respect

play29:10

to time

play29:12

remember we showed that the wave

play29:14

continues uninterrupted for for a long

play29:16

period of time that's very well behaved

play29:18

wave

play29:19

into in time

play29:21

now we're talking about a well-behaved

play29:23

wave

play29:24

in in space which means that we can

play29:27

predict

play29:28

its amplitude and phase at any position

play29:30

at a given time

play29:32

while before it was at the same position

play29:36

at a different time but here at any and

play29:39

any position now any spatial position

play29:42

as a function

play29:43

of time and also of course of space so

play29:45

let's look at it

play29:47

now

play29:48

an ideal point source of radiation is

play29:51

over here

play29:52

and then it puts out you know these

play29:54

spherical waves that we're probably used

play29:56

to seeing if the source is is very small

play29:59

then you have perfect

play30:00

spherical waves

play30:02

if uh i don't like a diverging beam and

play30:05

i put a lens here then i can make this

play30:07

into a collimated beam and this will be

play30:08

perfectly collimated b

play30:11

which means that uh for for what we call

play30:14

high spatial coherence means that if i

play30:16

know the amplitude and phase of the wave

play30:20

here

play30:21

in this position in space i can also

play30:24

predict the amplitude and phase of the

play30:26

wave in another uh position in uh in

play30:30

space

play30:31

and uh

play30:33

and and uh and that's great

play30:35

so whether it says diverging beam or a

play30:37

collimated beam or so on if you tell me

play30:40

what the amplitude and phase of the wave

play30:41

here i can tell it i can tell you what

play30:43

it's going to be over here because the

play30:45

wavelength is is stable and the the

play30:49

spatial

play30:50

behavior is stable

play30:51

well if this doesn't mean much to you

play30:53

let's look at what a what the light

play30:56

source uh puts out and it's back to our

play30:58

spectral lamp here or in our clamp

play31:02

now because we have so many atoms in the

play31:04

source here that they're radiating that

play31:06

we get a mess of a waveform that's uh

play31:09

that's coming out so if even so if i

play31:11

know the amplitude and phase over here

play31:13

it's

play31:15

pretty impossible for me to predict what

play31:17

the amplitude and phase going to be at a

play31:19

different location

play31:20

in space

play31:22

and even as a function of time because i

play31:25

really have no control over uh these

play31:27

light sources over here while in the in

play31:29

the case of the laser i can get uh

play31:32

pretty close to perfect

play31:34

prediction anywhere i want in space but

play31:37

in a in a in a

play31:39

non-laser light source it's very

play31:40

difficult

play31:41

now i can improve things by making the

play31:44

light source very small as we showed you

play31:46

before i take lenses i focus them down

play31:48

put small apertures and can sort of

play31:50

create a tiny focused spot the only

play31:54

problem is

play31:55

there's not much light by the time i do

play31:57

that while the laser you can put all the

play32:00

laser

play32:01

light into let's say collimated beam

play32:03

with diverging beam that has a perfect

play32:06

spatial spatial coherence

play32:09

all right so these are two very key uh

play32:12

properties now what i'd like to do is uh

play32:16

is talk about few more a few more

play32:18

properties

play32:19

all right now here is the next one which

play32:22

is high power

play32:24

the laser as we know lasers have

play32:27

uh incredible power all right so let's

play32:30

let's see where that where that

play32:33

comes from

play32:34

here's again a picture of a laser and

play32:36

putting out a beam of light

play32:38

now there are two kinds of lasers

play32:40

there's what we call cw or continuous

play32:43

wave lasers and there's also pulse so if

play32:45

the output is not continuous and it's

play32:47

possible we call it pulse lasers some of

play32:48

them can be very short and and so on

play32:51

all right now let's see

play32:53

what sort of power levels

play32:55

that we can get from

play32:57

from lasers

play32:59

and these these numbers if you're not

play33:01

familiar with them they're going to

play33:02

really open your eyes out

play33:04

to to what's going on now in terms of

play33:06

continuous lasers

play33:08

well we're all familiar i suppose with

play33:10

the helium neon laser or semiconductor

play33:12

lasers that put out a few milliwatts

play33:15

all right some of us work with bigger

play33:17

lasers that put out sort of watts

play33:20

and uh not that many people uh

play33:24

uh work with kilowatt lasers today these

play33:27

are you can buy these lasers for all

play33:29

kinds of applications and

play33:32

you can also generate even megawatts of

play33:35

of continuous lasers that's 10 to the

play33:37

power 6 watts that's huge

play33:39

huge uh

play33:41

continuous power that comes out from

play33:42

these lasers

play33:44

now in terms of pulse lasers

play33:46

well the numbers get really very big

play33:49

here we're talking about in continuous

play33:50

document tender six watts here we're

play33:52

talking about anywhere from 10 to the

play33:55

nine watts which is a or gigawatt

play33:57

depending on where you come from and

play33:59

then we also have can produce pulse

play34:01

lasers with with

play34:05

peak pulse power of 10 to the 12 watts

play34:07

terawatts

play34:08

and even 10 to the 15 watts and i don't

play34:11

know if you've heard of this word here

play34:12

petawatt and pitawatt means 10 to the 15

play34:15

this case 10 to the 15 watts and also

play34:18

recently we read that some people have

play34:21

produced exowatt uh peak power which is

play34:25

10 to the 10 to the 18 watts and these

play34:28

fantastic fantastic power levels and

play34:30

we'll see how they generate it soon and

play34:33

and what we can use them for but for

play34:35

here i'll just mention just a few

play34:37

applications

play34:38

of these peak powers certainly in

play34:40

materials processing where you want to

play34:42

do welding cutting and what have you

play34:45

uh for

play34:46

fusion today as we know there's a big

play34:48

fusion program

play34:50

for many years now uh that uses that's

play34:53

based on on lasers called laser fusion

play34:56

and the military of course would love to

play34:58

use these high-power lasers where the

play35:01

pulsed or cw and certainly a lot of

play35:04

nonlinear optics application uh are

play35:06

based on the fact that we have a lot of

play35:10

uh a lot of power in these in these

play35:12

lasers because it depends on the on the

play35:14

intensity now the

play35:17

next property that i want to mention is

play35:20

the tuning range of

play35:22

of lasers

play35:24

lasers again are sources of radiation

play35:27

and can have incredible uh tuning range

play35:30

now let's see

play35:31

over the spectrum

play35:33

of electromagnetic radiation where

play35:35

lasers are first of all

play35:37

we have the visible lasers you know the

play35:39

ones we we see are basically basically

play35:42

over here

play35:43

and

play35:44

and you they may have a certain tuning

play35:47

let's say from here to here

play35:49

and

play35:50

and we'll discuss them later i mean here

play35:52

this is just in a pictorial form i want

play35:54

to show you where the lasers are and

play35:56

then maybe as we get into the infrared

play35:57

there may be other lasers like this one

play35:59

here some laser here let's say over here

play36:02

is in the firing of getting close to the

play36:04

final infrared some lasers that have

play36:06

large large tuning range

play36:08

we go from the visible we can go to the

play36:10

ultraviolet or even to the vacuum

play36:12

ultraviolet and today we've gone all the

play36:15

way to to x-rays so lasers are found

play36:18

all over the spectrum all over the

play36:20

electromagnetic spectrum

play36:22

but their tuning range or their widths

play36:25

over with width the spectrum or the

play36:28

spectral width

play36:29

of the lasers or the tuning range of the

play36:31

lasers can be can be quite broad

play36:34

and then we'll discuss them later but

play36:36

today we have lasers all over the

play36:39

electromagnetic spectrum sure we may

play36:41

have some gaps here and there but there

play36:43

are techniques of filling these gaps by

play36:45

by mixing techniques and so on that will

play36:48

fill these gaps and today we really have

play36:49

no excuse to say that i don't have a

play36:51

laser at a specific uh wavelength

play36:54

because all sorts of techniques to uh to

play36:57

create lasers there if there aren't any

play36:59

lasers there already

play37:01

now the applications of

play37:04

of

play37:05

wide tuning range

play37:07

could be in the interaction with

play37:08

specific atoms and molecules where you

play37:10

need to tune the light sources to be

play37:12

able to interact with specific atoms and

play37:14

molecules to reach their resonances and

play37:16

so on

play37:17

in

play37:18

studying structure of atoms molecules

play37:21

solids and so on you need a widely

play37:23

tunable source

play37:25

in the area of spectroscopy and then for

play37:27

propagation uh sometimes uh you know if

play37:30

you want to dodge certain molecules in

play37:32

the atmosphere and the water and so on

play37:34

you need to tune the laser away from

play37:38

the absorption of these

play37:40

molecules or atoms and in

play37:43

in medical applications sometimes you

play37:46

need to

play37:46

uh to tune the laser so that it's at the

play37:49

right wavelength for interacting with

play37:52

tissue or or what have you uh and and

play37:56

it's nice to have lasers that are uh

play37:58

that are tunable now i have one more key

play38:01

property and that's it it's going to be

play38:02

just the fifth one

play38:04

and and here it is that lasers can

play38:07

produce very short

play38:09

pulse width

play38:11

now these these are incredibly short

play38:14

pulse width much shorter than any any

play38:16

electronic circuit can can generate and

play38:20

here we are

play38:22

here's a laser pulse that one can

play38:24

generate and the pulse width

play38:26

can be

play38:28

well this is

play38:29

big 10 to the minus nine seconds which

play38:31

called nanosecond

play38:33

uh certainly we can pre produce these on

play38:36

a routine basis picosecond or 10 to the

play38:38

minus 12 seconds

play38:40

and today we're very close the record is

play38:43

that we're very close to 10 to the minus

play38:45

15 seconds

play38:46

excuse me which is a femtosecond

play38:49

that's incredible

play38:50

because because even 10 to the minus 12

play38:53

seconds very difficult impossible to

play38:54

reach with electronic sources so already

play38:57

from from below 10 to the minus 12 let's

play39:00

say 10 minus 11 or so this is all lasers

play39:03

because you can't do it

play39:04

electronically all right so again

play39:07

this this is fantastic property of uh

play39:10

of lasers and and let's mention at this

play39:13

stage what are some some applications of

play39:15

very short pulses we can certainly use

play39:18

them to study very fast phenomena

play39:22

uh where the let's say the relaxation

play39:24

time is so fast that normal uh

play39:26

techniques don't work that cannot be

play39:28

used to observe them because

play39:31

too long all right so so in order to

play39:32

study fast phenomena you need very short

play39:35

pulsed lasers

play39:37

then of course the exciting thing

play39:39

about optical computers if they will

play39:42

ever come about is to take advantage of

play39:44

these very short pulses so you can have

play39:46

can have faster clocks and

play39:49

and so on

play39:50

and for high resolution radar and

play39:52

imaging these very short pulses can give

play39:55

you again incredible

play39:58

resolution

play39:59

and so so there's lots of applications

play40:01

of these short pulses and we'll have uh

play40:04

something to say about them

play40:05

later

play40:06

now

play40:07

i would like to to switch to to the my

play40:10

my next topic

play40:12

which is how

play40:15

these properties how these properties uh

play40:18

come about

play40:20

and uh and again we'll start with uh

play40:23

with the first with the first property

play40:26

which is this monochromaticity uh

play40:29

narrow spectral width and the high tempo

play40:31

coherence which i hope you still

play40:32

remember from from earlier

play40:34

the question is

play40:36

how does this property where does this

play40:39

property come from

play40:41

okay

play40:42

so the answer is that the laser is an

play40:45

optical oscillator

play40:48

and

play40:49

so some people might say well what's an

play40:51

optical oscillator i know it comes out

play40:53

like a sine wave but what's an optical

play40:54

oscillator

play40:55

well

play40:58

the what's an optical oscillator is

play41:03

the first in order to understand an

play41:04

optical oscillator you have to

play41:05

understand what an oscillator is so now

play41:09

we're ready to talk about uh the

play41:11

properties of an oscillator and we hope

play41:14

then we can extend it to an optical

play41:15

oscillator and then we can appreciate

play41:16

where that first property of lasers

play41:18

comes from so here we are let's review

play41:21

the basic properties of oscillators i

play41:24

know

play41:25

a lot of you know about oscillators but

play41:26

i have to start at some level so i'm

play41:28

going to start right here so if we have

play41:30

here black box that puts out this

play41:33

sinusoidal oscillation this perfect

play41:35

sinusoidal oscillation where the length

play41:38

of this wave train as we've seen before

play41:39

goes all the way from minus infinity

play41:41

plus infinity very long uninterrupted

play41:44

constant amplitude then in in the

play41:46

frequency domain that as we've done

play41:48

before that is that delta function

play41:50

centered at some frequency here that

play41:52

depends on the wavelength of this of

play41:54

this radiation source

play41:55

all right so that's what we generally

play41:57

call an oscillator and especially

play41:59

electrical oscillators we see them on an

play42:02

oscilloscope we see this beautiful sine

play42:04

wave on on on the oscilloscope and uh

play42:08

and the the the the source of the

play42:10

oscillation well we'll have to see how

play42:12

that comes about in the case of lasers

play42:15

and and the spectral width is is

play42:17

extremely narrow and we see that

play42:19

electrical oscillators all the time and

play42:20

we don't even think about it

play42:23

now

play42:24

now i would like to

play42:26

tell you a little bit about how an

play42:28

oscillator is made

play42:29

and once we understand oscillators made

play42:31

then we can extend it to to the optical

play42:33

domain and and then be able to explain

play42:35

how a laser works okay so let's review

play42:38

some background here in in oscillators

play42:44

well there are all kinds of uh

play42:46

oscillators i'm going to start with with

play42:47

a pendulum

play42:48

here's a simple pendulum length length d

play42:51

and i let it i let it swing

play42:55

what does it do when i let it swing well

play42:57

it will go backwards and forwards just

play42:58

like this will

play43:00

generate an oscillation here of the

play43:02

pendulum which will die down

play43:04

and the frequency of this oscillation is

play43:07

given by

play43:08

1 over 2 pi the square root of

play43:10

g the acceleration of gravity divided by

play43:13

d the length of the of the pendulum

play43:16

now

play43:17

the uh so the the

play43:19

longer d is the

play43:22

smaller the the frequency of oscillation

play43:24

but but as we can see this oscillation

play43:27

dies down and the question why does it

play43:29

die down well why does it die down

play43:31

because there are some losses

play43:33

and the losses for example come in this

play43:35

pivot here comes pushing air around and

play43:37

so on but basically it will die down

play43:40

because it's difficult to get rid of

play43:42

all these losses so we don't have that

play43:45

constant oscillation that i showed you

play43:47

before

play43:48

now we go to the frequency domain

play43:50

reminding you what we did before because

play43:52

i have a dying oscillation like this

play43:55

then if the time constant is is tau

play43:57

then the line width is going to be

play43:59

approximately uh delta f which is

play44:01

approximately one over tau

play44:04

and and that is proportional directly

play44:06

proportional to the losses the higher

play44:08

the losses the larger

play44:10

larger is the line width and the shorter

play44:13

is the uh the uh

play44:16

the decay time

play44:18

all right so that

play44:20

if i improve the losses if i reduce the

play44:22

losses then i can get this to narrow

play44:24

down and i can get this to last to last

play44:27

uh longer

play44:29

now the um

play44:32

if i as i just mentioned just now this

play44:34

is in in pictorial form if i reduce the

play44:36

losses if i'm clever in reducing the

play44:38

friction in this pivot and so on i can

play44:41

make the wave last

play44:42

longer and this width gets

play44:44

gets narrower but in order to make it

play44:47

constant amplitude i have to do

play44:49

something else

play44:51

all right this is what i have to do i

play44:52

have to call on this fellow here to to

play44:55

push on this pendulum to push on this

play44:58

pendulum so that

play45:00

it stops it from from

play45:02

dying down in a way what this fellow is

play45:04

doing by doing his pushing at the right

play45:07

time it's really overcoming the losses

play45:09

whether at the the pivot here or pushing

play45:11

air around and and so on so in order

play45:14

instead of having just the dying

play45:16

oscillation like this where i end up

play45:18

with a constant amplitude because of

play45:20

this fellow here is putting energy into

play45:22

this system and compensating for

play45:25

so as the amplitude here becomes becomes

play45:28

constant then the line width here

play45:31

starts the delta f starts to shrink and

play45:34

goes close to zero so in this way i

play45:37

produce a an oscillator and in this case

play45:40

of course it's a it's a pendulum

play45:42

oscillator that's used like a clock and

play45:44

and so on but i do need

play45:46

this energy source this person here to

play45:48

overcome to overcome the losses

play45:51

now this is not the only type of uh of

play45:54

oscillator i have all kinds

play45:56

uh let's say i have a mass spring system

play45:59

i can make that into oscillator let's

play46:00

say here i have a spring and there's a

play46:02

mass connected to it and then if i pull

play46:04

the mass away it's going to wobble

play46:06

backwards and forward it's going to

play46:07

oscillate

play46:08

again it's going to be a dying

play46:09

oscillation like this because of well

play46:12

friction

play46:13

mass friction has a friction between the

play46:15

friction between the mass and and the

play46:17

stable and losses in the spring and so

play46:19

on the frequency here will be determined

play46:22

by the

play46:23

square root of the of the spring

play46:25

constant k and divided by the mass

play46:28

if i change the mass i change the

play46:30

frequency and and so on and so so again

play46:33

just like in the pendulum it's a dying

play46:34

oscillation and has a in the frequency

play46:37

domain has a certain width and the width

play46:40

is proportional to

play46:41

one over

play46:42

one over tau and that's again

play46:44

proportional to losses

play46:46

if i look at a stretch string

play46:48

here straight string if i hit it then it

play46:51

it bobs up and down here in the middle

play46:54

and then the frequency will be

play46:55

determined by the speed of sound in the

play46:57

material divided by by twice the

play47:00

separation between the ends and again it

play47:03

dies down okay this bubbling up and down

play47:05

will die down

play47:07

because again of losses and also we'll

play47:09

have we'll have a width

play47:11

and then finally here if i have an lc

play47:14

circuit

play47:15

inductor in a capacitor again if i if i

play47:18

inject a pulse into it i see that again

play47:21

i get an oscillation if i look let's say

play47:23

the voltage across the capacitor here i

play47:25

have this oscillation that dies down

play47:27

and the frequency is given by in this

play47:30

case by the square root of 1 over lc l

play47:32

being the inductor c is the is the value

play47:35

of the capacitance

play47:36

and the this decay is due to losses now

play47:40

in electrical circuit where the losses

play47:42

come from well they come from ohmic

play47:43

losses essentially dissipation in the in

play47:45

the wires according to uh

play47:48

ohm's law

play47:50

so that

play47:51

uh uh the

play47:53

all these kinds of oscillators whether

play47:55

pendulum or or uh mass spring and

play47:58

vibrating string or electrical

play47:59

oscillator they essentially they all

play48:02

have specific frequencies all right they

play48:04

oscillate at and but they all have

play48:07

losses and to make them into into an

play48:09

oscillator you have to overcome these

play48:11

losses and as we as we saw that in the

play48:15

in the case of the pendulum you need

play48:16

somebody to push here you may also need

play48:18

somebody to push over here you again you

play48:21

you have to uh

play48:23

you have to keep vibrating these things

play48:25

to maintain oscillation and of course in

play48:27

the electrical one we add a an amplifier

play48:30

to overcome

play48:32

to overcome the the losses now to uh to

play48:35

then then summarize then we need to make

play48:37

an oscillator

play48:39

then we need a a resonator

play48:41

that will determine the frequency for us

play48:44

and we need a means of overcoming uh the

play48:48

loss so if we have that then we can

play48:51

then we can

play48:52

get this

play48:53

oscillation this nice oscillation that

play48:56

that comes out from that black box i

play48:58

showed you earlier now what about the

play48:59

laser

play49:00

okay how does the laser work

play49:02

well

play49:04

in in uh

play49:05

in lasers because it lasers is an

play49:08

oscillator we need a a resonator first

play49:11

of all so let's look at how we can

play49:13

create electromagnetic uh resonator

play49:16

well

play49:17

just like this is very similar to the to

play49:19

the stretch string we need uh we need

play49:21

two ends we need two nodes and here we

play49:24

have uh to create this we have two

play49:26

mirrors

play49:28

uh here the two mirrors m and they're

play49:30

spaced a certain distance l apart

play49:33

now the

play49:34

the lowest frequency that can fit

play49:37

between these two modes and oscillate

play49:38

backwards and forwards between these two

play49:40

modes is the one where half the

play49:42

wavelength where l is half half this

play49:46

wavelength because the wave would be

play49:48

would be about the size now such a wave

play49:50

would be able to bounce backwards and

play49:51

forwards between the two mirrors

play49:53

and

play49:55

and will

play49:56

be at that frequency determined by in

play49:58

this case will be determined by

play50:01

uh f equals c over 2l because uh lambda

play50:05

times uh times the frequency equals the

play50:07

velocity of light

play50:10

so either that the the wavelength is 2l

play50:13

all right or its frequency is just c

play50:15

over 2l okay so this is then the the the

play50:18

lowest uh frequency that will be

play50:21

supported in this kind of uh structure

play50:23

with two reflectors or two nodes at the

play50:25

ends just like in the vibrating string

play50:28

now this oscillation will die down if i

play50:31

injected some light in here and i get it

play50:33

to

play50:34

to oscillate like this it will die down

play50:36

because of losses

play50:38

and again in the frequency domain this

play50:40

will have a width

play50:41

question is what uh where are the losses

play50:44

in this case

play50:46

well the losses come from the reflection

play50:49

in the

play50:50

in the mirrors if the

play50:52

reflectivity of the mirror is not

play50:53

perfect

play50:54

then then every time the light bounces

play50:56

from one mirror to the other then the

play50:58

amplitude will go down and very quickly

play51:00

it will die down altogether

play51:03

so in order to to make this then

play51:06

oscillate or essentially lays

play51:08

we need to overcome uh these losses but

play51:11

before i get to this i want to talk

play51:13

about uh other other

play51:16

modes in in this kind of resonator

play51:20

the uh

play51:22

so far i've talked about this one where

play51:24

only half the wavelength fits between

play51:26

the two mirrors but i can also get a

play51:29

condition where a full wavelength foot

play51:31

fits between the two mirrors these are

play51:33

sort of normal modes

play51:35

of

play51:36

of these resonators

play51:38

now where lambda 1 was here was equal to

play51:41

2l and f1 was c over 2l in this case

play51:45

lambda 2

play51:46

is is essentially l or i like to write

play51:49

it as 2 l over 2 but i cancel to do the

play51:51

twos and i get l

play51:53

and the frequency is just 2 c over 2 l

play51:57

so here we had 1 times c over 2 l here

play51:59

is 2 c over 2 l and and so here i'm

play52:02

spacing it along in the frequency uh

play52:05

along the frequency scale here's my f1

play52:08

and here's f2 and the separation is c

play52:10

over 2l and each one has a width because

play52:13

of the

play52:14

of the losses now we can go a little

play52:16

further here

play52:18

and consider a few more of these uh

play52:20

oscillations in this case uh well i have

play52:23

one and a half waves that will fit

play52:25

between the the cavity uh between the

play52:28

two mirrors and or within the cavity and

play52:30

then the wavelength will be 2l over 3

play52:33

instead of 2l over 2

play52:35

and the frequency will be 3 c over 2l

play52:38

instead of 2c over 2l here so now again

play52:41

you can see i'm going to stack them up

play52:42

f1 f2 n3 and the separation is equal

play52:46

between them which is c over 2l

play52:48

and we can uh

play52:51

go to many more and i'm jumping here to

play52:54

to the what we call the qth mode lambda

play52:57

sum q and just because the way i was

play53:00

doing it uh previously you can see that

play53:03

the wavelength will be 2l

play53:05

divided by q this is the the q number

play53:08

just like in here this was three two

play53:10

two one and now in this case will be the

play53:12

key

play53:13

the qth mode

play53:15

and the frequency will be just q c over

play53:17

2 l just like here we have 3 c over 2 l

play53:19

2 c over 2 l and so on so on the on the

play53:22

on the frequency scale then we have all

play53:23

these resonances that come from that i

play53:26

can excite in in one resonator and can

play53:29

we can be

play53:30

as high as uh as you want it and the

play53:32

width each one will have a width because

play53:34

of the losses now not all the widths

play53:37

will be the same because uh because not

play53:40

all the losses will the sun losses will

play53:42

depend on the wavelength or the

play53:44

frequency you're at

play53:45

so

play53:46

since the mirrors can have loss but the

play53:48

loss can depend on the wavelength and so

play53:52

so these widths can

play53:54

can vary

play53:55

so now

play53:57

this explains the the uh the uh

play54:00

resonator and uh and and just the let me

play54:03

summarize the uh

play54:06

the uh information here we have a

play54:09

typical now a laser uh cavity which is

play54:13

again two mirror spaced by l in this

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case i'm going to take l as a hundred

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centimeters one meter if i choose for

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the wavelength to be half a

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micron or five times 10 minus 5

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centimeters then q

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comes out to be this q this integer we

play54:28

talked about comes out to be uh 2l over

play54:30

lambda from from the uh from this

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formula here and it's 200 divided by 5

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times 10 minus 5 which comes out to be

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about 4 times 10 to the 6 which means

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that q has the value of few million all

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right which means there's lots of little

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waves in here in a in a cavity of a 100

play54:48

centimeters

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separation the frequency associated with

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that is against f sub q from here uh is

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uh six times comes out to be six times

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10 to 14 hertz

play54:59

and the width will depend on the losses

play55:01

uh which are uh mainly due to let's say

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mirror losses and and so on which we'll

play55:06

get into into later

play55:08

so

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so the uh so then to make a an optical

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uh oscillator or like a laser we need

play55:15

the resonator that we that we have

play55:18

talked about but it has not just one

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frequency but has many frequencies and

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it has we have to have a a means of

play55:25

overcoming the loss

play55:27

and and that

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uh is

play55:30

is uh

play55:31

that comes about with with a light with

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a light amplifier

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so the the light amplifier is the is the

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key element uh in inlays in a laser

play55:42

because without the amplifier you can

play55:43

have all these cavities empty cavities

play55:46

that do absolutely nothing for you but

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in order to make create lasers out of

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them then you have to put an amplifier

play55:53

okay so here is then

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then uh the laser

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here's the cavity that we talked about

play55:59

and then we have to insert this this

play56:01

amplifier

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and this amplifier which we will talk

play56:04

about uh later in more depth this

play56:07

amplifier then provides

play56:10

gain

play56:12

for the light that goes backwards and

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forwards between these two mirrors to

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overcome the losses wherever the losses

play56:17

come from

play56:18

and the whole idea is to make the losses

play56:20

as small as possible so you don't you

play56:22

need to use a big amplifier because in

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order to generate this gain which we'll

play56:28

talk about later

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uh it costs a lot of effort a lot of

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money and so on so so we want to

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minimize the the uh the gain that's

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needed

play56:38

but we certainly have to have enough

play56:40

gain to overcome uh the losses and uh

play56:43

and here for example i have this this

play56:46

amplifier this this gain of this

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amplifier located at this particular

play56:50

frequency and over here i have all the

play56:53

modes of of the cavity that we talked

play56:55

about before but if there is one of

play56:57

these cavity modes under the bandwidth

play57:00

of this amplifier

play57:02

then if there is enough gain to overcome

play57:05

the loss

play57:06

then i can get this to to oscillate and

play57:09

in fact

play57:10

here it is as we know that this width of

play57:14

the of the cavity comes about because of

play57:16

the losses in the cavity but if i have

play57:18

enough gain to overcome the losses

play57:21

then i collapse this width to this delta

play57:24

function that we had before and and the

play57:27

output that comes out from this mirror

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if i put some transmission in this

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mirror here i leak a little bit of light

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out then that light will will have this

play57:36

spectrum this very narrow spectral width

play57:37

or in terms of the time domain i have a

play57:41

this this lovely

play57:43

oscillation here that has a constant

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frequency determined by this cavity mode

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and a constant amplitude

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so i think

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uh

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the

play57:53

this will be a very fitting time to uh

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to stop for this uh first session

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because uh because i brought you just to

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the stage where i think now you wanna

play58:02

know where this uh where this gain comes

play58:06

from that makes lasers possible so when

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we come back we'll start exactly with

play58:11

that with that topic

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