The Hydrogen Atom, Part 1 of 3: Intro to Quantum Physics
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
🌌 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。
📐 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。
🧲 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。
🔍 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
💡量子力学
💡波函数
💡能量本征态
💡薛定谔方程
💡哈密顿算符
💡动量算符
💡不确定性原理
💡球坐标
💡角动量
💡普朗克常数
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
foreign
look at this beautiful hydrogen atom in
the ground state there's one proton one
electron and the electron is as close as
it can be to the proton until Quantum
fuzziness kicks in and the electrons
kind of in this wave function of
positions and you don't know exactly
where it is but it's something like this
let's shoot a photon at this and see
what happens
look at this it's a two zero zero State
very nice so now the electron is a bit
farther out a bit less bound to the
proton in a higher energy State relative
to the ground state but be careful this
is only metastable it's going to pop
back down soon so any minute now it's
going to pop into the ground state
oh there it goes and look we got our
Photon back did you see that flash of
light
conservation of energy very nice let's
put another Photon into it and see what
happens
hey that's a two one zero State nice you
know that one has some angular momentum
oh there it goes
let's take a moment to meditate on this
situation
[Music]
foreign
[Music]
[Music]
we'll Begin by examining our atom in its
most relaxed form this dazzling little
pattern is one of Nature's most abundant
most ancient motifs
but there's a deep mystery here why is
it that the electron doesn't just fall
into the proton
if you model the electron and the proton
as Point particles and apply Maxwell's
equations you'll find that the electron
will radiate out its energy and will end
up falling into the proton in just a few
nanoseconds
but there's hydrogen out in space that's
like billions of years old so clearly
our math is a little bit off because
hydrogen actually doesn't Decay
instantly so what is it that stops the
collapse
have you ever tried to catch a Quantum
particle
imagine you have one and you've caught
it you're pinching it between your
finger and your thumb and you squeeze it
really tight so you know just exactly
where it is you know it's positioned
with perfect precision
oh well by quantum mechanics now you no
longer know its momentum and so it
escapes
in quantum mechanics you actually can't
perfectly localize a single particle
you can try but it takes a lot of energy
and the tighter you squeeze it the more
you localize it the more energy it takes
if you think about it a proton is
pulling in the electron the electrons
this Quantum particle it wants to
collapse all the way but eventually
there's a point where the quantum
fuzziness makes it so that the
uncertainty and momentum keeps the thing
from falling all the way in
and so you see hydrogen is not just an
atom it's also this portal between the
world of experiment and the very strange
and unusual world of quantum mechanics
that bubbles up into our world wait hold
up so the electron is a Quantum particle
and it's all fuzzy but the proton is
just this point-like thing how does that
make sense
well it's because the proton is about
1836 times as massive as the electron so
just to put this into perspective the
difference in Mass between an electron
and a proton is the difference between
an elephant
and 1836 elephants so the proton is very
very massive because it's so much more
massive it's less fuzzy it is still
fuzzy if you look very closely at it
it's fuzzy but it's much less fuzzy
because there's this inverse
relationship between distance and mass
when it comes to quantum mechanics
because the proton is so much more
massive than the electron we can do all
of our analysis by assuming that the
proton will be at the center of our
coordinate system and that it doesn't
move it just stays put and the electron
does whatever quantum mechanical cloudy
wavy stuff it does okay all right let's
talk about coordinates normally I like
to use Cartesian coordinates X Y and Z
but because of the nature of this
problem it has a spherical Symmetry and
so spherical coordinates fit like a hand
in a glove to this problem so we're
going to use these the coordinates R
Theta and Phi one thing I have to point
out I got to be careful here so normally
I use Theta as the angle around the
longitude like the azimuthal angle and I
used Phi for the elevation angle but for
whatever reason physicists working on
the hydrogen atom always use the other
way of defining Theta and Phi and so I'm
going to go along with that convention
but just be aware this is a little bit
different than the convention that I
normally use so just to be really clear
Theta is actually going to be our
elevation angle so that's going to be
the angle that starts off at zero on the
North Pole and then goes down to Pi or
180 degrees at the South Pole and then
Phi is going to be our azimuthal angle
so that's the angle that's going to go
around the equator zero at the Prime
Meridian and then you know it goes
around a full 360 or full 2 pi
okay so now that we've defined our
coordinate system let's define some of
the most important things in quantum
mechanics the first thing is the wave
function so the wave function is this
complex valued function that's a
function of both space and time so the
wave function is given the symbol PSI
and PSI depends in this case on R Theta
Phi and time
closely related to the wave function is
the probability density that is the
thing that if you integrate over some
volume you get the probability that the
particle is going to be in that volume
the probability density is just the
amplitude squared of the wave function
when you take the amplitude squared of a
complex number you get a real number so
the probability density is a real valued
function and it's also a function of
space and time although as we'll see
when we solve any dragon States it's
just a function of space all right and
finally the reduced Planck's constant
this number h-bar you see this
everywhere in quantum mechanics it's
absolutely ubiquitous it's a measurable
quantity it has about the value of
1.05457 times 10 to the minus 34 Joule
seconds this is a very mysterious number
it is what it is and no one knows why it
is it just is and so you'll see this in
many of our equations today it defines
the relationship between energy and
frequency and momentum and space and all
kinds of stuff sort of the quantum scale
of angular momentum or action and by the
way I should mention you know why they
call it h bar it's actually plan's
constant H divided by 2 pi why but so
often you divide by 2 pi that people got
tired of writing divided by 2 pi so then
they just put a bar on the H now
everyone knows that means divide by 2 pi
so we want to figure out what is our
electron up to what does it do and in
order to do that we need an equation
that lets us relate things like momentum
and space and time
and so what we're going to do is we're
going to use the Schrodinger equation
shown here the Schrodinger equation is
just the idea that if the hamiltonian
operator acts on a wave function that's
the same thing as the energy operator
acting on a wave function now there's a
lot of confusion when people first see
hamiltonian operator they're not sure
what that is because it's just a thing
named after some guy so who knows what
it is well what it is is the energy
written in terms of position and
momentum and we'll see in a moment
exactly how to construct the hamiltonian
for the hydrogen atom
the energy operator is in quantum
mechanics it's defined as I H Bar times
partial PSI partial T so in other words
you take the partial derivative of the
wave function in time then you rotate it
90 degrees in the complex plane by
multiplying by I and then you multiply
it by that Quantum scale parameter h-bar
now if you look at this you might be
wondering why is this the energy
operator where does this come from and
the answer is today we're just going to
take this as one of our principles as
one of our assumptions that we're going
to use to build up this theory if you're
interested more in the nature of the
energy operator I'd recommend the book
quantum mechanics and path integrals by
Feynman and hibs this book constructs
quantum mechanics from a pretty
intuitive starting point well relatively
for quantum mechanics and and then they
show that you can basically derive all
of this Schrodinger wave equations from
path integrals now the problem with path
integrals is they're impossible to work
with but they're very nice to imagine so
if you want to learn more about why the
energy operator is what it is check out
that book but today we're just going to
take the energy operator for granted and
we're going to continue forward now when
we solve the Schrodinger equation we're
not just interested in every possible
wave function as a function of space and
function of time we're actually
particularly interested in these things
called Energy eigenstates they're also
known as stationary States I like to
think of them as resonant mode although
that's maybe kind of an analogy but I
think it's a good one
so an energy eigenstate is a wave
function that doesn't move except it
just rotates in the complex plane
so in other words you can break it up so
the wave function is a function of space
and time
can be thought of as the wave function
as a function of space
times this time parameter which just
swings around in the complex plane and
the frequency of how much it swings
around has to do with the energy of the
wave function
so when we solve for the time
independent Schrodinger equation what
that means is we want to figure out what
are all the patterns what are all the
different wave functions as a function
of space and then what are the
corresponding energy levels by the way
the energy levels are also called Energy
eigenvalues
the deal with all this eigen stuff
anyway well if you've studied linear
algebra then you'll be familiar with
eigenvector and eigenvalue problems
normally you'll have some kind of linear
transformation and then there are
specific vectors that are just uniformly
scaled by that transformation and the
amount to which they're scaled is the
eigenvalue and the vectors themselves
are eigenvectors and eigen I think it
comes from some German word meaning own
or self or like related to the thing
it's confusing terminology admittedly
but let's just apply the energy operator
to an energy eigenstate and see how we
can draw that parallel between
eigenvector eigenvalue problems and this
whole thing about eigenstates if we
apply our energy operator to psi so we
do I H bar partial PSI partial T and we
substitute in our wave function which is
our energy eigenstate where we have a
spatial part and a time part and then
we'd work out the derivatives what we
find is that the energy operator
basically amounts to just scaling the
wave function by a constant everywhere
in space
and so you'll notice that this seemingly
simple looking equation E hat PSI equals
e PSI it's actually pretty profound and
this should look a lot like your classic
you know Matrix times eigenvector equals
eigenvalue times eigenvector equation
from linear algebra by the way that's
not a coincidence if you've studied
structural engineering and you've
calculated resonant modes and
frequencies you'll see there's really a
one-to-one parallel between that
situation and what's going on here today
okay so just to recap the time dependent
Schrodinger equation that is the general
the real for real Schrodinger equation
is the equation that the hamiltonian
operator acting on a wave function is
the same as the energy operator acting
on a wave function and that lets us
relate momentum and space and time and
we can derive the governing equations of
our wave function
if we restrict our attention to solving
for these energy eigenstates which you
can imagine is resonant modes or the
ways in which the equation rings then we
end up with the time independent
Schrodinger equation in which the energy
operator is replaced by a constant that
constant of course depends on the
particular energy eigenstate we're
looking at some of them will have higher
energies some of them will have lower
energies but in any case we can regard
that energy level as an eigenvalue of
the hamiltonian operator acting on our
wave function
let's construct the hamiltonian for the
hydrogen atom to do that we need to add
the electrons kinetic and potential
energy
first let's start with the kinetic
energy
from classical non-relativistic physics
we know that the kinetic energy T is
equal to one-half MV squared where m is
the mass of the particle and V is the
velocity we also know from classical
physics that momentum p is mass times
velocity
therefore if you just rearrange those
equations you can prove to yourself that
the kinetic energy is the momentum
squared divided by twice the mass
and in quantum mechanics we're going to
use that exact same idea except we're
going to make the momentum a Quantum
thing how do we do that well we use the
quantum mechanical momentum operator
so the momentum operator P hat acting on
the wave function PSI is negative i h
Bar times the gradient of PSI
now if we use our formula from classical
physics that the kinetic energy is
momentum squared divided by twice the
mass then we can derive the quantum
mechanical kinetic energy Operator by
applying the momentum operator twice and
dividing by twice the mass
when we do that we find that the kinetic
energy operator t-hat applied to a wave
function PSI gives you negative H bar
squared over 2m times the laplacian of
PSI
and what that means intuitively is that
if you're going to take the kinetic
energy of a wave function you look at
its laplacian the laplacian is basically
the concavity in three dimensions it's
like a second derivative but adding up
along all the different second
derivative and X Plus second derivative
and Y plus second derivative and z and
then you multiply that concavity by H
bar squared over 2m and then you take
the minus sign of that
so you know earlier we were talking
about how it takes energy to localize a
particle the more you squeeze it the
more it sort of pushes back well we can
mathematically encode that in this
equation with the kinetic energy
operator right because you think about
it the more you pinch a particle the
more you're increasing its laplacian you
know the laplacian in a way is sort of
the extent to which the wave function is
pinched right it's the Divergence of the
gradient so the more you pinch it the
more this t-hat term increases
now if we look at the potential energy
from the electron and proton coulomb
potential so in other words just the
regular old static electricity Coulomb's
law we can see that the potential energy
operator V acting on our wave function
PSI is just the Classic minus Elementary
charge squared over 4 pi times the
permittivity of free space times the
radial coordinates all acting on our
wave function PSI
and so what that means is that there's
going to be a potential energy term in
our equation that drops off as 1 over r
but notice there's a minus sign on this
potential energy and so actually a
bigger magnitude means it's more
negative
negative energy in this context just
means that it's less than zero so if the
electron and proton are infinitely far
away let's call that zero then the
coulomb potential is negative because it
represents a kind of energy dead you'd
have to put energy into the hydrogen
atom in order to get the electron out
and so actually this one over R scaling
of the electrostatic potential is going
to tend to pull the electron in to the
proton
and so when we add the kinetic and
potential energy terms together in our
hamiltonian what we're describing when
we do that is that balance of energies
we were talking about earlier between
the electron getting pulled into the
proton but also that quantum mechanical
fuzziness that kinetic energy keeping
the electron from falling all the way in
and so we can finally write our
hamiltonian operator H hat acting on PSI
as negative H bar squared divided by
twice the mass times the laplacian of
our wave function minus the fundamental
charge squared divided by 4 Pi
permittivity of free space r times PSI
okay maybe it looks like a lot if this
is the first time you've seen it but all
that is to say the energy of the
electron has a kinetic term and it has
an electrostatic potential term
now something I should mention here is
that we want to actually use something
called the reduced mass of the electron
so this is basically the same thing as
the electron Mass it's like a little
tiny bit less like a part in a thousand
less kind of thing and what that does is
it lets us account a little bit for the
fact that the proton actually has finite
Mass it's not infinitely massive this
idea comes from orbital mechanics I
believe is where this first comes from
but for our purposes today basically the
main advantage is it lets us replace the
letter M with the letter mu because
we're going to need M later on when we
get to the magnetic quantum number
all right well now that we have our
hamiltonian we can plug it into the time
independent Schrodinger equation that is
H hat PSI equals e PSI where e is the
energy eigenvalue and PSI is an energy
eigenstate
let's massage this equation a little bit
we'll move the E side term on over to
the left side of the equation we'll
cancel out some minus signs and we get
this pretty looking equation that the
laplacian of PSI plus 2 mu over H bar
squared times e squared over 4 Pi
Epsilon not R plus e times PSI equals
zero
so up until this point we've used
physics and this idea of energy
operators and Schrodinger equation and
hamiltonian so we've compiled this
equation but now solving this equation
is an exercise in math
because we can just look at it as a
three-dimensional partial differential
equation and ask what are the functions
PSI that satisfy this equation
So to that end the first thing that we
should do is write out the laplacian in
terms of partial derivatives of PSI with
respect to R Theta and Phi
now here's the thing uh so earlier I
mentioned that using spherical
coordinates was going to help us out
because of the spherical nature of the
problem and that is true spherical
coordinates are very nice trust me we do
want to use them but there's one way in
which they're not so nice and that is
when you write out the laplacian it's
quite an expression anyway I'm not going
to go into the whole derivation of this
now but if you just look up laplacian
written in spherical coordinates you'll
see this expression it's a bit
complicated but it is what it is you
know no matter how fun it is it is what
it is okay now all we have to do is take
our expression for the laplacian and put
it into that equation and what we end up
with is a three-dimensional partial
differential equation for PSI as a
function of the variables R Theta and
Phi
wow look at this thing oh what a mess
but there it is this is a beautiful
equation in a way
so let's solve it let's solve it for PSI
how hard can it be
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