Abstract quantum wave interference patterns representing quantum mechanics

Hydrogen energy levels and wavefunctions

PHYS 410 · The Hydrogen Atom

Hydrogen's bound-state energies depend primarily on the principal quantum number. This lesson explains the Bohr energy formula, degeneracy, radial probability, and orbital interpretation.

Key equations

E_n=- rac{13.6 eV}{n^2}n=1,2,3,ldotsn oinftyE_n o0l=0,1,ldots,n-1m=-l,ldots,ln^2psi*{nlm}(r, heta,phi)=R*{nl}(r)Y_l^m( heta,phi)dP=|psi*{nlm}|^2d^3rd^3r=r^2sin heta,dr,d heta,dphiP(r)=r^2|R*{nl}(r)|^2a_0= rac{4piepsilon_0hbar^2}{m_ee^2}a_0approx0.529 ext{Å}n=1,quad l=0,quad m=0psi*{100}propto e^{-r/a_0}n-1n-l-1

Learning objectives

  • State the hydrogen energy level formula.
  • Explain degeneracy in the ideal hydrogen atom.
  • Describe the form of hydrogen wavefunctions.
  • Interpret radial probability distributions.
  • Identify nodes and distinguish orbitals from classical orbits.

Hydrogen energy spectrum

Solving the Schrödinger equation for the Coulomb potential gives hydrogen bound-state energies

E_n=- rac{13.6 eV}{n^2}

for

n=1,2,3,ldotsn=1,2,3,ldots

More precisely, the energy includes the reduced mass and fundamental constants, but the simple formula is extremely useful. The negative sign means the electron is bound. As noinftyn oinfty, Eno0E_n o0, corresponding to ionization.

Principal quantum number

In the ideal nonrelativistic hydrogen atom without fine structure, energy depends only on the principal quantum number nn, not on ll or mm. This creates degeneracy: many different states have the same energy.

For a given nn, allowed values are

l=0,1,ldots,n1l=0,1,ldots,n-1

and for each ll,

m=l,ldots,lm=-l,ldots,l

The total number of spatial states for a given nn is

n2n^2

not including spin.

Wavefunction structure

Hydrogen wavefunctions have the separated form

psinlm(r,heta,phi)=Rnl(r)Ylm(heta,phi)psi*{nlm}(r, heta,phi)=R*{nl}(r)Y_l^m( heta,phi)

The radial function controls dependence on distance from the nucleus. The spherical harmonic controls angular shape.

The probability of finding the electron in a volume element is

dP=psinlm2d3rdP=|psi*{nlm}|^2d^3r

with

d3r=r2sinheta,dr,dheta,dphid^3r=r^2sin heta,dr,d heta,dphi

Radial probability distribution

To ask for the probability of finding the electron between rr and r+drr+dr, integrate over angles. The radial probability density is

P(r)=r2Rnl(r)2P(r)=r^2|R*{nl}(r)|^2

up to angular normalization conventions. The factor r2r^2 comes from the volume of spherical shells. Even if R(r)R(r) is largest near the origin, the most probable radius may be away from the origin because larger shells contain more volume.

For the ground state, the most probable radius is the Bohr radius:

a_0= rac{4piepsilon_0hbar^2}{m_ee^2}

approximately

a0approx0.529extA˚a_0approx0.529 ext{Å}

Ground state

The hydrogen ground state has quantum numbers

n=1,quadl=0,quadm=0n=1,quad l=0,quad m=0

It is spherically symmetric. Its wavefunction is proportional to

psi100proptoer/a0psi*{100}propto e^{-r/a_0}

The probability density is highest at the nucleus, but the radial probability distribution peaks at r=a0r=a_0.

Nodes

Hydrogen orbitals have radial and angular nodes. The total number of nodes is

n1n-1

The number of angular nodes is ll, and the number of radial nodes is

nl1n-l-1

Nodes are surfaces or radii where the wavefunction is zero.

Orbitals, not orbits

Hydrogen orbitals are probability distributions, not classical electron paths. The electron is not a tiny planet moving along a definite orbit in the Schrödinger picture. The orbital describes probability amplitudes for position measurements.

The big idea

Hydrogen's quantum states are labeled by nn, ll, and mm. In the simplest model, energies follow En=13.6eV/n2E_n=-13.6 eV/n^2 and depend only on nn. Wavefunctions split into radial and angular parts, giving the familiar orbital shapes and probability distributions of atomic physics.

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