5.1.1Physical Chemistry (Advanced)

Quantum chemistry — particle in a box revisited; H-atom solutions

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1. The master equation

WHY this form? Total energy = kinetic + potential. In QM, momentum becomes the operator p^=i\hat p = -i\hbar\,\nabla, so kinetic energy p22m22m2\frac{p^2}{2m}\to -\frac{\hbar^2}{2m}\nabla^2. Demanding that ψ\psi be the same shape after H^\hat H acts (only rescaled by EE) is what "stationary state" means.


2. Particle in a 1D box — derived from scratch

Setup (WHAT): A particle trapped between x=0x=0 and x=Lx=L with V=0V=0 inside and V=V=\infty outside. Infinite walls ⇒ ψ=0\psi=0 outside, so by continuity ψ(0)=ψ(L)=0\psi(0)=\psi(L)=0 — these are the boundary conditions.

HOW we solve it. Inside the box V=0V=0: 22md2ψdx2=Eψ    d2ψdx2=k2ψ,k2=2mE2-\frac{\hbar^2}{2m}\frac{d^2\psi}{dx^2}=E\psi \;\Rightarrow\; \frac{d^2\psi}{dx^2}=-k^2\psi,\quad k^2=\frac{2mE}{\hbar^2}

Why this step? It's the classic "second derivative = negative constant × itself" ⇒ sine/cosine solutions.

General solution: ψ(x)=Asinkx+Bcoskx\psi(x)=A\sin kx + B\cos kx.

  • Apply ψ(0)=0\psi(0)=0: B=0B=0. (cosine isn't zero at 0, so it must die.)
  • Apply ψ(L)=0\psi(L)=0: AsinkL=0A\sin kL=0. Since A0A\neq0 (else ψ0\psi\equiv0), we need kL=nπkL=n\pi.

k=nπL,n=1,2,3,\boxed{k=\frac{n\pi}{L},\quad n=1,2,3,\dots}

Why quantization appears: the box length must fit a whole number of half-wavelengths. This is the entire reason energy is discrete.

Substitute back k2=2mE/2k^2=2mE/\hbar^2:

Normalization fixes AA. Require 0Lψ2dx=1\int_0^L|\psi|^2dx=1: A20Lsin2 ⁣nπxLdx=A2L2=1A=2LA^2\int_0^L\sin^2\!\frac{n\pi x}{L}dx=A^2\cdot\frac{L}{2}=1\Rightarrow A=\sqrt{\tfrac{2}{L}}

Figure — Quantum chemistry — particle in a box revisited; H-atom solutions

3. From 1D box to the hydrogen atom

WHY the H-atom is harder: it's 3D, and the potential is the central Coulomb attraction V(r)=e24πε0rV(r)=-\frac{e^2}{4\pi\varepsilon_0 r} which depends only on rr. Central potentials let us separate variables in spherical coordinates.

HOW quantum numbers arise (same boundary-condition logic):

Quantum number From which condition Allowed values
nn (principal) radial BC: R0R\to0 as rr\to\infty 1,2,3,1,2,3,\dots
\ell (azimuthal) θ\theta-equation finite at poles 0,1,,n10,1,\dots,n-1
mm_\ell (magnetic) ϕ\phi-equation single-valued: Φ(ϕ)=Φ(ϕ+2π)\Phi(\phi)=\Phi(\phi+2\pi) ,,+-\ell,\dots,+\ell

Why Φ\Phi single-valued ⇒ integer mm: Φ(ϕ)=eimϕ\Phi(\phi)=e^{im\phi} must repeat after 2π2\pieim2π=1e^{im\cdot2\pi}=1mZm\in\mathbb Z. Exactly the same "fit a whole number" idea as the box.


4. Common mistakes (Steel-manned)


5. Active recall

Recall Quick self-test (cover the answers)
  • What boundary conditions quantize the 1D box? → ψ(0)=ψ(L)=0\psi(0)=\psi(L)=0.
  • Why does mm_\ell come out integer? → single-valued ϕ\phi requirement.
  • Number of radial nodes in an orbital? → n1n-\ell-1.
What replaces p2/2mp^2/2m as the kinetic operator in the TISE?
22m2-\dfrac{\hbar^2}{2m}\nabla^2
Why is energy quantized in a box?
Boundary conditions force a whole number of half-wavelengths to fit, giving k=nπ/Lk=n\pi/L.
Energy levels of the 1D box?
En=n2h28mL2E_n=\dfrac{n^2h^2}{8mL^2}, n=1,2,3,n=1,2,3,\dots
Why can't n=0n=0 in the box?
It gives ψ0\psi\equiv0, i.e. no particle — not a valid state.
How many interior nodes does ψn\psi_n have?
n1n-1.
Normalization constant for the 1D box wavefunction?
2/L\sqrt{2/L}.
What does separating variables give for the H-atom wavefunction?
ψ=Rn(r)Ym(θ,ϕ)\psi=R_{n\ell}(r)Y_\ell^m(\theta,\phi).
Allowed values of \ell and mm_\ell?
=0,,n1\ell=0,\dots,n-1; m=,,+m_\ell=-\ell,\dots,+\ell.
Hydrogen energy levels?
En=13.6/n2E_n=-13.6/n^2 eV (depends only on nn).
Why are H-atom energies negative?
The electron is bound; energy lies below the free (rr\to\infty) zero reference.
Radial distribution function for finding the electron?
P(r)=4πr2ψ(r)2P(r)=4\pi r^2|\psi(r)|^2.
Most probable radius of the 1s1s electron?
r=a052.9r=a_0\approx52.9 pm (Bohr radius).
Radial nodes vs angular nodes?
radial =n1=n-\ell-1; angular ==\ell; total =n1=n-1.
Recall Feynman: explain it to a 12-year-old

Imagine a guitar string fixed at both ends. It can only vibrate in special patterns — one bump, two bumps, three bumps — never half a bump, because the ends are pinned. A trapped electron is like that string: only certain "vibration patterns" (energies) are allowed. For the hydrogen atom, the electron is trapped around a positive nucleus instead of between two walls; the rule "the wave must fit perfectly and not blow up far away" again allows only special patterns — and those patterns are the orbitals (1s, 2p, etc.). Same idea, fancier cage.


Connections

  • Schrödinger Equation — the master equation both problems solve.
  • Quantum Numbers — how n,,mn,\ell,m_\ell label H-atom states.
  • Atomic Orbitals and Shapes — spherical harmonics give s, p, d shapes.
  • Zero-point Energy — why the lowest box state isn't E=0E=0.
  • Quantum Dots — PIB applied to nanocrystals.
  • Bohr Model vs Quantum Mechanicsa0a_0 reinterpreted as most probable radius.
  • Operators and Eigenvalues — the math machinery behind H^ψ=Eψ\hat H\psi=E\psi.

Concept Map

kinetic plus potential

apply inside box

V=0 inside, infinite walls

2nd deriv = -k^2 psi

forces B=0 and sin kL = 0

whole number of half-wavelengths

normalization integral = 1

n-1 interior zeros

more curvature

same trick in 3D with Coulomb V

gives

TISE H-psi = E-psi

momentum operator p = -i hbar grad

Particle in a 1D box

Boundary conditions psi 0 = psi L = 0

General solution A sin kx + B cos kx

Quantization k = n pi over L

Energy levels E_n proportional to n^2

Wavefunctions psi_n = sqrt 2 over L sin

Nodes and curvature

Hydrogen atom

Atomic orbitals

Hinglish (regional understanding)

Intuition Hinglish mein samjho

Dekho, quantum chemistry ka pura khel ek hi equation pe tika hai — Schrödinger equation, H^ψ=Eψ\hat H\psi=E\psi. Yeh keh raha hai ki kisi particle ka allowed energy sirf kuch special values pe hoti hai, har value pe nahi. Particle-in-a-box sabse simple example hai: electron ko do deewaron ke beech band kar do. Jaise guitar ki taar dono taraf se bandhi ho aur sirf 1 bump, 2 bump, 3 bump waale pattern bana sakti hai, waise hi electron ki wave ko box me poora fit hona padta hai. Isi "poora fit hona" condition se k=nπ/Lk=n\pi/L aata hai, aur energy quantize ho jaati hai: En=n2h2/8mL2E_n=n^2h^2/8mL^2. Yaad rakho n=0n=0 allowed nahi — uska matlab hoga electron hai hi nahi.

Hydrogen atom bilkul wahi idea hai, bas 3D me aur Coulomb attraction ke saath. Yahan deewar ki jagah nucleus ka attraction electron ko trap karta hai. Spherical coordinates me hum wavefunction ko todte hain: ψ=R(r)Y(θ,ϕ)\psi=R(r)\,Y(\theta,\phi). Har boundary condition se ek quantum number nikalta hai — nn (size/energy), \ell (shape), mm_\ell (orientation). mm_\ell integer isliye aata hai kyunki ϕ\phi pe ghoom ke wapas aane pe wave same honi chahiye — phir wahi "poora fit" logic!

Energy nikalti hai En=13.6/n2E_n=-13.6/n^2 eV. Negative isliye kyunki electron bound hai (free electron ki energy 0 maani jaati hai, bound usse neeche). Ek important trick: "sabse zyada probable radius" wahan nahi hota jahan ψ2|\psi|^2 max hai, balki radial distribution P(r)=4πr2ψ2P(r)=4\pi r^2|\psi|^2 jahan max ho. 1s1s ke liye yeh exactly Bohr radius a052.9a_0\approx52.9 pm pe aata hai. Yeh sab isliye important hai kyunki yahi se saare orbitals (s, p, d) aur periodic table ki samajh banti hai.

Go deeper — visual, from zero

Test yourself — Physical Chemistry (Advanced)

Connections