The Hydrogen Atom, Part 1 of 3: Intro to Quantum Physics

Richard Behiel
2 Jun 202318:34

Summary

TLDR视频脚本通过氢原子模型深入探讨了量子力学的基本原理。首先,介绍了氢原子的基态,其中电子围绕质子运动,但由于量子不确定性,电子的位置是概率性的。接着,通过向氢原子发射光子,展示了电子跃迁到较高能级的过程,并最终返回基态,释放光子,体现了能量守恒。视频还讨论了为何电子不会落入质子,引入了量子力学中的不确定性原理。此外,通过比较电子和质子的质量差异,解释了为何可以假设质子固定不动。最后,使用球坐标系和薛定谔方程,建立了氢原子的哈密顿算符,并推导了时间独立的薛定谔方程,为解决电子的行为提供了数学基础。整个脚本是对量子力学核心概念的精彩阐释,旨在激发观众对这一神秘领域的兴趣。

Takeaways

  • 🚀 氢原子的基态包含一个质子和一个电子,电子尽可能地靠近质子,直到量子不确定性起作用,电子的位置变得模糊。
  • 🔬 当向氢原子发射光子时,电子会被激发到一个更高的能级,但这个状态是亚稳态,电子很快会回落到基态并释放光子,这是能量守恒的体现。
  • 🌌 电子作为量子粒子,其位置和动量不能同时被精确知晓,这种量子不确定性阻止了电子落入质子中,从而解释了氢原子为何不会衰变。
  • 📍 在量子力学中,我们通常使用球坐标系(R, Θ, Φ)来描述具有球对称性的问题,如氢原子。
  • 📈 波函数(Ψ)是一个复数函数,它依赖于空间和时间,概率密度是波函数的模长平方,用于描述粒子出现在某个体积内的概率。
  • 🎓 约化普朗克常数(ℏ)在量子力学中非常重要,它关联了能量、频率、动量和空间等量子尺度的物理量。
  • 🧲 薛定谔方程是量子力学中的基本方程,它关联了哈密顿算符(能量算符)和波函数,用于描述量子系统的时间演化。
  • ⚙️ 哈密顿算符结合了电子的动能和与质子的电势能,动能算符与波函数的二阶导数(拉普拉斯算子)有关,而电势能算符与1/R有关。
  • 🔧 通过求解时间独立的薛定谔方程,我们可以得到氢原子的能量本征态(或称定态),这些状态描述了电子在不同能级上的概率分布。
  • 🧮 球坐标系下的拉普拉斯算子形式较为复杂,但它是求解氢原子波函数的关键数学工具。
  • 🔬 电子和质子之间的相互作用通过库仑定律描述,电子被质子吸引,但由于量子力学的不确定性原理,电子不会完全落入质子中。
  • 📚 解决氢原子的薛定谔方程是一个数学问题,需要找到满足特定偏微分方程的函数,这些函数将给出电子在不同能级上的概率分布。
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Outlines

00:00

🌌 氢原子的量子行为

本段介绍了氢原子的基本结构,包括质子、电子以及电子在量子力学中的波动性。通过发射光子观察电子从基态到激发态的跃迁,并讨论了量子力学中的不确定性原理,即无法同时准确知道粒子的位置和动量。此外,还探讨了为何电子不会落入质子,以及量子力学与经典力学在描述微观世界时的差异。

05:01

📐 量子力学的数学基础

这一段深入讨论了量子力学中的几个关键概念,包括波函数、概率密度、约化普朗克常数以及薛定谔方程。解释了波函数是如何描述粒子在空间和时间中的状态,以及如何通过波函数的幅度平方得到粒子出现在某一体积内的概率。还介绍了哈密顿算符和能量算符,以及它们在量子力学中的重要性。

10:02

🧲 氢原子的哈密顿量构建

本段内容聚焦于构建氢原子的哈密顿量,这是量子力学中描述系统总能量的算符。首先介绍了动能的量子力学表达式,然后讨论了电子和质子之间的库仑势能。通过将动能项和势能项结合起来,得到了氢原子的哈密顿量,这个量描述了电子与质子之间的能量平衡。

15:04

🔍 求解薛定谔方程

最后一段讲述了如何将哈密顿量代入时间独立的薛定谔方程中,并将其转换为一个三维偏微分方程。这个方程用于寻找满足特定条件的波函数,即能量本征态。通过将拉普拉斯算子在球坐标系中表达,并将其代入方程,得到了描述氢原子中电子行为的复杂数学模型。

Mindmap

Keywords

💡氢原子

氢原子是最简单的原子,由一个质子和一个电子组成。在视频中,氢原子被用来展示量子力学的基本原理,如电子不能落入质子中,而是存在于一定的能量状态中。这与经典物理学的预测不符,展示了量子力学与经典物理学的区别。

💡量子力学

量子力学是描述微观粒子行为的物理理论。视频中通过氢原子模型解释了量子力学中的一些基本概念,如波函数、量子不确定性和能量本征态。量子力学揭示了原子和亚原子粒子的奇异行为,与我们日常经验中的物理现象截然不同。

💡波函数

波函数(Ψ)是量子力学中的一个复数函数,它与粒子在空间中的位置和时间有关。视频中提到,波函数的绝对值的平方给出了粒子在某个区域内被发现的概率密度。波函数是理解量子系统状态的基础。

💡能量本征态

能量本征态是量子力学中描述系统可能状态的解,它们对应于特定的能量值。视频中通过氢原子的模型展示了能量本征态的概念,说明了电子在不同能量状态下的行为,以及如何通过吸收和释放光子在不同的能量状态之间跃迁。

💡薛定谔方程

薛定谔方程是量子力学中的基本方程,用于描述量子系统的时间演化。视频中提到了时间依赖和时间独立的薛定谔方程,这些方程帮助我们理解量子系统的行为,尤其是如何通过哈密顿算符来描述系统的能量。

💡哈密顿算符

哈密顿算符是量子力学中用于描述系统能量的算符。它由系统的动能和势能组成。在视频中,哈密顿算符被用来构建氢原子的量子模型,并求解电子的波函数。

💡动量算符

动量算符是量子力学中用来表示粒子动量的算符。它与粒子的波函数相联系,并在薛定谔方程中起到关键作用。视频中通过动量算符解释了量子粒子的动量和位置如何通过不确定性原理相互关联。

💡不确定性原理

不确定性原理是量子力学的一个基本原理,表明不能同时精确知道粒子的位置和动量。视频中通过尝试“捕捉”量子粒子的比喻来解释这一原理,说明了量子系统的固有模糊性。

💡球坐标

球坐标是描述三维空间中点位置的坐标系统,由半径、极角和方位角组成。视频中提到,由于氢原子具有球对称性,使用球坐标可以更方便地解决薛定谔方程。

💡角动量

角动量是描述粒子旋转运动的物理量。在量子力学中,角动量是量子化的,意味着它只能取特定的值。视频中提到了角动量在氢原子的量子态中的作用,以及如何通过不同的角度(如θ和φ)来描述粒子的轨道。

💡普朗克常数

普朗克常数是量子力学中的一个基本常数,它关联了粒子的能量和其频率。视频中提到了约化普朗克常数(ħ),它是普朗克常数除以2π,用于描述量子系统中的能量和动量关系。

Highlights

氢原子的电子在基态时,与质子的距离由量子不确定性决定,电子存在于一种波函数中。

通过向氢原子发射光子,可以观察到电子跃迁到高能级状态,但这种状态是亚稳态,电子会很快跃迁回基态。

氢原子展示了量子力学中电子与质子之间的相互作用,电子不会落入质子中,因为量子不确定性和动量的作用。

量子力学中,无法精确定位一个粒子的位置和动量,这种不确定性随着粒子的局域化程度增加而增加。

质子的质量远大于电子,因此在分析中可以假设质子固定不动,而电子进行量子力学的运动。

使用球坐标系统(R, Θ, Φ)来描述氢原子问题,因为其球对称性。

波函数Ψ是一个复数函数,依赖于空间和时间,是量子力学中描述粒子状态的基本工具。

概率密度是波函数的幅度平方,用于描述粒子出现在某个体积内的概率。

约化普朗克常数ħ是量子力学中的关键常数,关联能量、频率、动量和空间。

薛定谔方程是量子力学中描述粒子状态随时间演化的基本方程。

能量本征态(或称定态)是波函数在空间中不随时间变化,仅在复平面中旋转的状态。

哈密顿算符是能量的量子力学表示,由位置和动量的表达式构成。

氢原子的哈密顿算符由电子的动能项和电子-质子间的库仑势能项组成。

使用约化质量代替电子质量可以更准确地描述氢原子中的电子运动。

通过时间独立的薛定谔方程,可以得到描述电子在不同能量本征值下的空间波函数。

球坐标下的拉普拉斯算符表达式复杂,但在解决氢原子问题时非常有用。

将拉普拉斯算符代入薛定谔方程,得到一个三维偏微分方程,用于求解波函数Ψ。

Transcripts

play00:02

foreign

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look at this beautiful hydrogen atom in

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the ground state there's one proton one

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electron and the electron is as close as

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it can be to the proton until Quantum

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fuzziness kicks in and the electrons

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kind of in this wave function of

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positions and you don't know exactly

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where it is but it's something like this

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let's shoot a photon at this and see

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what happens

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look at this it's a two zero zero State

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very nice so now the electron is a bit

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farther out a bit less bound to the

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proton in a higher energy State relative

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to the ground state but be careful this

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is only metastable it's going to pop

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back down soon so any minute now it's

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going to pop into the ground state

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oh there it goes and look we got our

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Photon back did you see that flash of

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light

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conservation of energy very nice let's

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put another Photon into it and see what

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happens

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hey that's a two one zero State nice you

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know that one has some angular momentum

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oh there it goes

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let's take a moment to meditate on this

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situation

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[Music]

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foreign

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[Music]

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[Music]

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we'll Begin by examining our atom in its

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most relaxed form this dazzling little

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pattern is one of Nature's most abundant

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most ancient motifs

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but there's a deep mystery here why is

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it that the electron doesn't just fall

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into the proton

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if you model the electron and the proton

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as Point particles and apply Maxwell's

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equations you'll find that the electron

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will radiate out its energy and will end

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up falling into the proton in just a few

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nanoseconds

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but there's hydrogen out in space that's

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like billions of years old so clearly

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our math is a little bit off because

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hydrogen actually doesn't Decay

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instantly so what is it that stops the

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collapse

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have you ever tried to catch a Quantum

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particle

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imagine you have one and you've caught

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it you're pinching it between your

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finger and your thumb and you squeeze it

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really tight so you know just exactly

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where it is you know it's positioned

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with perfect precision

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oh well by quantum mechanics now you no

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longer know its momentum and so it

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escapes

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in quantum mechanics you actually can't

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perfectly localize a single particle

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you can try but it takes a lot of energy

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and the tighter you squeeze it the more

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you localize it the more energy it takes

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if you think about it a proton is

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pulling in the electron the electrons

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this Quantum particle it wants to

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collapse all the way but eventually

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there's a point where the quantum

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fuzziness makes it so that the

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uncertainty and momentum keeps the thing

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from falling all the way in

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and so you see hydrogen is not just an

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atom it's also this portal between the

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world of experiment and the very strange

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and unusual world of quantum mechanics

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that bubbles up into our world wait hold

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up so the electron is a Quantum particle

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and it's all fuzzy but the proton is

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just this point-like thing how does that

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make sense

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well it's because the proton is about

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1836 times as massive as the electron so

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just to put this into perspective the

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difference in Mass between an electron

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and a proton is the difference between

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an elephant

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and 1836 elephants so the proton is very

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very massive because it's so much more

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massive it's less fuzzy it is still

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fuzzy if you look very closely at it

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it's fuzzy but it's much less fuzzy

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because there's this inverse

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relationship between distance and mass

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when it comes to quantum mechanics

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because the proton is so much more

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massive than the electron we can do all

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of our analysis by assuming that the

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proton will be at the center of our

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coordinate system and that it doesn't

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move it just stays put and the electron

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does whatever quantum mechanical cloudy

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wavy stuff it does okay all right let's

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talk about coordinates normally I like

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to use Cartesian coordinates X Y and Z

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but because of the nature of this

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problem it has a spherical Symmetry and

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so spherical coordinates fit like a hand

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in a glove to this problem so we're

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going to use these the coordinates R

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Theta and Phi one thing I have to point

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out I got to be careful here so normally

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I use Theta as the angle around the

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longitude like the azimuthal angle and I

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used Phi for the elevation angle but for

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whatever reason physicists working on

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the hydrogen atom always use the other

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way of defining Theta and Phi and so I'm

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going to go along with that convention

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but just be aware this is a little bit

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different than the convention that I

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normally use so just to be really clear

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Theta is actually going to be our

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elevation angle so that's going to be

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the angle that starts off at zero on the

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North Pole and then goes down to Pi or

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180 degrees at the South Pole and then

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Phi is going to be our azimuthal angle

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so that's the angle that's going to go

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around the equator zero at the Prime

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Meridian and then you know it goes

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around a full 360 or full 2 pi

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okay so now that we've defined our

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coordinate system let's define some of

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the most important things in quantum

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mechanics the first thing is the wave

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function so the wave function is this

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complex valued function that's a

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function of both space and time so the

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wave function is given the symbol PSI

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and PSI depends in this case on R Theta

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Phi and time

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closely related to the wave function is

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the probability density that is the

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thing that if you integrate over some

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volume you get the probability that the

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particle is going to be in that volume

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the probability density is just the

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amplitude squared of the wave function

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when you take the amplitude squared of a

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complex number you get a real number so

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the probability density is a real valued

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function and it's also a function of

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space and time although as we'll see

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when we solve any dragon States it's

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just a function of space all right and

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finally the reduced Planck's constant

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this number h-bar you see this

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everywhere in quantum mechanics it's

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absolutely ubiquitous it's a measurable

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quantity it has about the value of

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1.05457 times 10 to the minus 34 Joule

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seconds this is a very mysterious number

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it is what it is and no one knows why it

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is it just is and so you'll see this in

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many of our equations today it defines

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the relationship between energy and

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frequency and momentum and space and all

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kinds of stuff sort of the quantum scale

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of angular momentum or action and by the

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way I should mention you know why they

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call it h bar it's actually plan's

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constant H divided by 2 pi why but so

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often you divide by 2 pi that people got

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tired of writing divided by 2 pi so then

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they just put a bar on the H now

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everyone knows that means divide by 2 pi

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so we want to figure out what is our

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electron up to what does it do and in

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order to do that we need an equation

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that lets us relate things like momentum

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and space and time

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and so what we're going to do is we're

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going to use the Schrodinger equation

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shown here the Schrodinger equation is

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just the idea that if the hamiltonian

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operator acts on a wave function that's

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the same thing as the energy operator

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acting on a wave function now there's a

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lot of confusion when people first see

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hamiltonian operator they're not sure

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what that is because it's just a thing

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named after some guy so who knows what

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it is well what it is is the energy

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written in terms of position and

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momentum and we'll see in a moment

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exactly how to construct the hamiltonian

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for the hydrogen atom

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the energy operator is in quantum

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mechanics it's defined as I H Bar times

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partial PSI partial T so in other words

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you take the partial derivative of the

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wave function in time then you rotate it

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90 degrees in the complex plane by

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multiplying by I and then you multiply

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it by that Quantum scale parameter h-bar

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now if you look at this you might be

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wondering why is this the energy

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operator where does this come from and

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the answer is today we're just going to

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take this as one of our principles as

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one of our assumptions that we're going

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to use to build up this theory if you're

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interested more in the nature of the

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energy operator I'd recommend the book

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quantum mechanics and path integrals by

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Feynman and hibs this book constructs

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quantum mechanics from a pretty

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intuitive starting point well relatively

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for quantum mechanics and and then they

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show that you can basically derive all

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of this Schrodinger wave equations from

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path integrals now the problem with path

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integrals is they're impossible to work

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with but they're very nice to imagine so

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if you want to learn more about why the

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energy operator is what it is check out

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that book but today we're just going to

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take the energy operator for granted and

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we're going to continue forward now when

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we solve the Schrodinger equation we're

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not just interested in every possible

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wave function as a function of space and

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function of time we're actually

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particularly interested in these things

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called Energy eigenstates they're also

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known as stationary States I like to

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think of them as resonant mode although

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that's maybe kind of an analogy but I

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think it's a good one

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so an energy eigenstate is a wave

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function that doesn't move except it

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just rotates in the complex plane

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so in other words you can break it up so

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the wave function is a function of space

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and time

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can be thought of as the wave function

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as a function of space

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times this time parameter which just

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swings around in the complex plane and

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the frequency of how much it swings

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around has to do with the energy of the

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wave function

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so when we solve for the time

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independent Schrodinger equation what

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that means is we want to figure out what

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are all the patterns what are all the

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different wave functions as a function

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of space and then what are the

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corresponding energy levels by the way

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the energy levels are also called Energy

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eigenvalues

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the deal with all this eigen stuff

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anyway well if you've studied linear

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algebra then you'll be familiar with

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eigenvector and eigenvalue problems

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normally you'll have some kind of linear

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transformation and then there are

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specific vectors that are just uniformly

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scaled by that transformation and the

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amount to which they're scaled is the

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eigenvalue and the vectors themselves

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are eigenvectors and eigen I think it

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comes from some German word meaning own

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or self or like related to the thing

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it's confusing terminology admittedly

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but let's just apply the energy operator

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to an energy eigenstate and see how we

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can draw that parallel between

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eigenvector eigenvalue problems and this

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whole thing about eigenstates if we

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apply our energy operator to psi so we

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do I H bar partial PSI partial T and we

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substitute in our wave function which is

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our energy eigenstate where we have a

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spatial part and a time part and then

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we'd work out the derivatives what we

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find is that the energy operator

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basically amounts to just scaling the

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wave function by a constant everywhere

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in space

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and so you'll notice that this seemingly

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simple looking equation E hat PSI equals

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e PSI it's actually pretty profound and

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this should look a lot like your classic

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you know Matrix times eigenvector equals

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eigenvalue times eigenvector equation

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from linear algebra by the way that's

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not a coincidence if you've studied

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structural engineering and you've

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calculated resonant modes and

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frequencies you'll see there's really a

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one-to-one parallel between that

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situation and what's going on here today

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okay so just to recap the time dependent

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Schrodinger equation that is the general

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the real for real Schrodinger equation

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is the equation that the hamiltonian

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operator acting on a wave function is

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the same as the energy operator acting

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on a wave function and that lets us

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relate momentum and space and time and

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we can derive the governing equations of

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our wave function

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if we restrict our attention to solving

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for these energy eigenstates which you

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can imagine is resonant modes or the

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ways in which the equation rings then we

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end up with the time independent

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Schrodinger equation in which the energy

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operator is replaced by a constant that

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constant of course depends on the

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particular energy eigenstate we're

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looking at some of them will have higher

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energies some of them will have lower

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energies but in any case we can regard

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that energy level as an eigenvalue of

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the hamiltonian operator acting on our

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wave function

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let's construct the hamiltonian for the

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hydrogen atom to do that we need to add

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the electrons kinetic and potential

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energy

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first let's start with the kinetic

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energy

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from classical non-relativistic physics

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we know that the kinetic energy T is

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equal to one-half MV squared where m is

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the mass of the particle and V is the

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velocity we also know from classical

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physics that momentum p is mass times

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velocity

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therefore if you just rearrange those

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equations you can prove to yourself that

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the kinetic energy is the momentum

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squared divided by twice the mass

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and in quantum mechanics we're going to

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use that exact same idea except we're

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going to make the momentum a Quantum

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thing how do we do that well we use the

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quantum mechanical momentum operator

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so the momentum operator P hat acting on

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the wave function PSI is negative i h

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Bar times the gradient of PSI

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now if we use our formula from classical

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physics that the kinetic energy is

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momentum squared divided by twice the

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mass then we can derive the quantum

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mechanical kinetic energy Operator by

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applying the momentum operator twice and

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dividing by twice the mass

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when we do that we find that the kinetic

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energy operator t-hat applied to a wave

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function PSI gives you negative H bar

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squared over 2m times the laplacian of

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PSI

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and what that means intuitively is that

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if you're going to take the kinetic

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energy of a wave function you look at

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its laplacian the laplacian is basically

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the concavity in three dimensions it's

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like a second derivative but adding up

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along all the different second

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derivative and X Plus second derivative

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and Y plus second derivative and z and

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then you multiply that concavity by H

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bar squared over 2m and then you take

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the minus sign of that

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so you know earlier we were talking

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about how it takes energy to localize a

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particle the more you squeeze it the

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more it sort of pushes back well we can

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mathematically encode that in this

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equation with the kinetic energy

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operator right because you think about

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it the more you pinch a particle the

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more you're increasing its laplacian you

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know the laplacian in a way is sort of

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the extent to which the wave function is

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pinched right it's the Divergence of the

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gradient so the more you pinch it the

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more this t-hat term increases

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now if we look at the potential energy

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from the electron and proton coulomb

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potential so in other words just the

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regular old static electricity Coulomb's

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law we can see that the potential energy

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operator V acting on our wave function

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PSI is just the Classic minus Elementary

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charge squared over 4 pi times the

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permittivity of free space times the

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radial coordinates all acting on our

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wave function PSI

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and so what that means is that there's

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going to be a potential energy term in

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our equation that drops off as 1 over r

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but notice there's a minus sign on this

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potential energy and so actually a

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bigger magnitude means it's more

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negative

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negative energy in this context just

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means that it's less than zero so if the

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electron and proton are infinitely far

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away let's call that zero then the

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coulomb potential is negative because it

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represents a kind of energy dead you'd

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have to put energy into the hydrogen

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atom in order to get the electron out

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and so actually this one over R scaling

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of the electrostatic potential is going

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to tend to pull the electron in to the

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proton

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and so when we add the kinetic and

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potential energy terms together in our

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hamiltonian what we're describing when

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we do that is that balance of energies

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we were talking about earlier between

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the electron getting pulled into the

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proton but also that quantum mechanical

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fuzziness that kinetic energy keeping

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the electron from falling all the way in

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and so we can finally write our

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hamiltonian operator H hat acting on PSI

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as negative H bar squared divided by

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twice the mass times the laplacian of

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our wave function minus the fundamental

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charge squared divided by 4 Pi

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permittivity of free space r times PSI

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okay maybe it looks like a lot if this

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is the first time you've seen it but all

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that is to say the energy of the

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electron has a kinetic term and it has

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an electrostatic potential term

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now something I should mention here is

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that we want to actually use something

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called the reduced mass of the electron

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so this is basically the same thing as

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the electron Mass it's like a little

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tiny bit less like a part in a thousand

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less kind of thing and what that does is

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it lets us account a little bit for the

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fact that the proton actually has finite

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Mass it's not infinitely massive this

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idea comes from orbital mechanics I

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believe is where this first comes from

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but for our purposes today basically the

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main advantage is it lets us replace the

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letter M with the letter mu because

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we're going to need M later on when we

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get to the magnetic quantum number

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all right well now that we have our

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hamiltonian we can plug it into the time

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independent Schrodinger equation that is

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H hat PSI equals e PSI where e is the

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energy eigenvalue and PSI is an energy

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eigenstate

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let's massage this equation a little bit

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we'll move the E side term on over to

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the left side of the equation we'll

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cancel out some minus signs and we get

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this pretty looking equation that the

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laplacian of PSI plus 2 mu over H bar

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squared times e squared over 4 Pi

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Epsilon not R plus e times PSI equals

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zero

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so up until this point we've used

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physics and this idea of energy

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operators and Schrodinger equation and

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hamiltonian so we've compiled this

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equation but now solving this equation

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is an exercise in math

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because we can just look at it as a

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three-dimensional partial differential

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equation and ask what are the functions

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PSI that satisfy this equation

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So to that end the first thing that we

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should do is write out the laplacian in

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terms of partial derivatives of PSI with

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respect to R Theta and Phi

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now here's the thing uh so earlier I

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mentioned that using spherical

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coordinates was going to help us out

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because of the spherical nature of the

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problem and that is true spherical

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coordinates are very nice trust me we do

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want to use them but there's one way in

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which they're not so nice and that is

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when you write out the laplacian it's

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quite an expression anyway I'm not going

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to go into the whole derivation of this

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now but if you just look up laplacian

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written in spherical coordinates you'll

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see this expression it's a bit

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complicated but it is what it is you

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know no matter how fun it is it is what

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it is okay now all we have to do is take

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our expression for the laplacian and put

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it into that equation and what we end up

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with is a three-dimensional partial

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differential equation for PSI as a

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function of the variables R Theta and

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Phi

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wow look at this thing oh what a mess

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but there it is this is a beautiful

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equation in a way

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so let's solve it let's solve it for PSI

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how hard can it be

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