CHEM 1310 A/B Fall 2006 Chapter 16: Quantum Mechanics and the Hydrogen Atom

Quantum Mechanics and the Hydrogen Atom

Overview

  • Waves and Light
  • Paradoxes in Classical Physics
  • Planck, Einstein, and Bohr
  • Waves, Particles, and the Schrödinger equation
  • The Hydrogen Atom

Questions Addressed

  • What is quantum mechanics?
  • When do we need it?
  • What does it do?
  • How does it apply to the H atom?

Quantum Mechanics (QM) Defined

  • QM is the set of rules obeyed by small systems (molecules, atoms, and subatomic particles).
  • It's one of the two greatest achievements of 20th-century physics.
  • QM is the basis for new research into smaller electronic devices (e.g., quantum dots).
  • It is required to understand chemistry.

The Two-Slit Experiment

  • Firing small particles at a barrier with two tiny slits:

    • Classical expectation: Particles go through one slit or the other, resulting in two distinct bands.
    • Actual Result: An interference pattern is observed, indicating wave-like properties.
  • Even stranger, the wave-like interference pattern happens even when sending one electron through at a time.

  • If we watch to see which slit a particle goes through, the interference pattern disappears, and we see the expected pattern!

  • Richard Feynman: "I think it is safe to say that no one understands quantum mechanics."

Historical Background of QM

  • Near the end of the 19th century, physicists thought they knew everything.
  • Several key experiments showed something really unknown was going on.
  • QM developed to explain these unusual experiments in the early 1900s (~1900-1930s).
  • Developed around same time as theory of relativity.

Electromagnetic Spectrum

  • Illustrates the range of electromagnetic radiation, from radio waves to gamma rays.
  • Visible light is a small portion of the spectrum.
  • Wavelength and frequency are inversely proportional.

The Ultraviolet Catastrophe

  • Classical physics predicted that blackbodies should emit infinite energy at high frequencies (short wavelengths), which was not observed.
  • This discrepancy was known as the "ultraviolet catastrophe."

Planck's Solution

  • In 1900, Planck postulated that the blackbody is made of tiny oscillators with energies proportional to the frequency of oscillation.
  • E=nhνE = nhν, where:
    • EE is the energy.
    • nn is an integer.
    • hh is Planck’s constant (6.626×10346.626 \times 10^{-34} J s).
    • νν is the frequency.
  • Energy is quantized; only certain values are allowed.
  • Using this hypothesis, blackbody radiation curves can be predicted accurately.

The Photoelectric Effect

  • Light can cause electrons to be ejected from a metal surface.
  • Problem: KE of electrons does not depend on intensity, but does depend on frequency νν.

Einstein's Explanation

  • Borrowed Planck’s “quantum” idea --- maybe light might have quantized energy levels, too!
  • Light comes in “packets” of energy E=hνE = hν, called “photons.”
  • Explains the photoelectric effect --- higher νν, more energy in each light packet (photon), kicks out electron with more KE.

Photoelectric Effect Explained

  • Minimum energy to remove an electron is hν0hν_0, the “work function” of the metal.

Atomic/Molecular Spectra

  • Emission Spectrum: Excited sample emits light and pass through prism, resulting in individual lines.
  • Absorption Spectrum: White light source shines through an absorbing sample and then through a prism, it results in dark lines.

H Atom Spectrum

  • The lines follow a particular pattern.
  • Lines fit the “Rydberg formula” ν=(1/n21/m2)(3.29×1015s1)ν = (1/n^2 – 1/m^2)(3.29 \times 10^{15} s^{-1}) where n and m are integers. Amazing!

Bohr's Explanation of H Atom Spectrum

  • Bohr(1913) borrowed ideas of quantization from Planck and Einstein and explained the H atom spectrum.
  • Bohr argued that angular momentum was quantized, leads to quantization of H atom energy levels.
  • Bohr frequency condition: ΔE=hν\Delta E = hν
  • Equations match the Rydberg formula to an accuracy not seen previously in all of science.

Bohr’s Solution

  • Quantization of angular momentum.
  • Leads to quantization of radii (“Bohr orbits”).
  • Leads to quantization of energies.
  • Assume the “Bohr frequency condition”.
  • Yields the same “Rydberg formula” for allowed energy levels!!!
  • Constants: a<em>0=1a<em>0 = 1 bohr (0.5290.529 Å), R</em>y=1R</em>y = 1 Rydberg = 2.17987×10182.17987 \times 10^{-18} J

H Atom Spectrum Explained

  • Energy-level diagram for the hydrogen atom, showing how transitions from higher states into some particular state lead to the observed spectral series for hydrogen.

“New Quantum Theory”

  • The “quantization” idea was groundbreaking, but it did not have a firm foundation.
  • De Broglie (1924) realized that if light can act as a wave and a particle, then maybe particles like electrons can also act like waves!
  • “Wave/particle duality” also works for matter!
  • Can relate momentum (particle property) to wavelength (wave property) via the de Broglie relation λ=h/p\lambda = h / p (p=mvp = mv)

The Schrödinger Equation

  • 1925: Schrödinger developed new mechanics for “matter waves” shown by de Broglie. Quantum mechanics!

The Schrödinger Equation (Components)

  • Nuclear kinetic energy
  • Electron kinetic energy
  • Nuclear/electron attraction
  • Nuclear/nuclear repulsion
  • Electron/electron repulsion

The Schrödinger Equation (Wave Function)

  • Ψ\Psi is the wave function. It gives the amplitude of the matter wave at any position in space (for more than 1 electron; need the coordinates x<em>i=x</em>i,y<em>i,z</em>ix<em>i = {x</em>i, y<em>i, z</em>i} for each particle i)
  • Ψ(x<em>1,x</em>2,,xn)\Psi(x<em>1, x</em>2, …, x_n) for n particles.
  • Focus on wave function for a single particle (like an electron) for now…

Classical Standing Waves

  • String tied to the wall at both ends (x=0x=0 and x=Lx=L).
  • Have to fit a half-integer number of wavelengths λ\lambda in the length L.
  • Number the standing waves n=1n=1, n=2n=2, …
  • Max amplitude for standing wave n is u<em>n(x)=A</em>nsin(nπx/L)u<em>n(x) = A</em>n \sin(nπx/L)
  • # of nodes increases with n; energy also increases with n (more nodes -> higher energy).
  • Just like u<em>n(x)u<em>n(x) gives amplitude of vibration at a given point x, Ψ</em>n(x)\Psi</em>n(x) gives the “amplitude” of the matter wave.

Interpretation of Ψ

  • Most commonly accepted interpretation due to Max Born.
  • Assume only one particle for now.
  • Ψ(x,y,z)Ψ(x,y,z)ΔxΔyΔz\Psi^*(x, y, z) \Psi(x, y, z) \Delta x \Delta y \Delta z is the probability that the particle will be found in a box of size ΔxΔyΔz\Delta x \Delta y \Delta z centered at point x,y,z.
  • Seems crazy--we never actually know where the particle is, only the probability of finding it there. Even worse – these “probability waves” can interfere constructively/destructively!

Wave Picture Justifies Bohr’s Assumption for H Atom!

  • To avoid destructive interference, an electron in a Bohr orbit must have its wavefunction match itself after going around once.
  • 2πr=nλ2 πr = n \lambda
  • But also λ=h/mv\lambda = h / mv
  • … and so 2πr=nh/mv2 πr = nh / mv, or mvr=nh/2πmvr = nh / 2 π, as Bohr assumed!

Schrödinger Equation for H Atom

  • Can solve and obtain the same energy equation as Bohr found. But now we also get the wave functionΨnlm(x,y,z)\Psi_{nlm}(x, y, z), depending on three integers n, l, and m
    • n = “principal quantum number” (the same n in energies EnE_n), starts counting from 1
    • l = “angular quantum number” l = 0, 1, …, n-1
    • m = “magnetic quantum number” m = -l, -l+1, …, 0, 1, …, l
  • Actually there’s also a 4th quantum number, ms, giving the spin (12\frac{1}{2} for “up” spin α, -12\frac{1}{2} for “down” spin β)

Wave functions for H atom

  • Energy depends only on n for H atom, not on l or m
  • Shape of wave function depends on n, l, and m
  • A function of one particle is called an “orbital”
    • l=0 is an s orbital
    • l=1 is a p orbital (m=-1, 0, 1 => px, py, pz)
    • l=2 is a d orbital (m=-2, -1, 0, 1, 2 => dxy, dxz, dyz, dx2-y2, dz2)
    • l=3 is an f orbital (7 of these)… etc…
  • All these functions are 3D functions; hard to plot…

Summary of H atom orbitals

  • Energy depends only on n.
  • For a given l, increasing n increases the average distance of electrons from the nucleus (& the size of the orbital). 3s larger than 2s.
  • Ψnlm\Psi_{nlm} has l angular nodes and n-l-1 radial nodes (total of n-1 nodes).
  • Only for s orbitals does Ψnlm\Psi_{nlm} remain nonzero as r→0. Only s orbitals “penetrate to the nucleus”.
  • Note: orbitals are only rigorous for H atom or other 1-electron atoms! For multiple electrons, need molecular orbital theory (even for atoms). Solve multi-electron Schrödinger equation.

Heisenberg Uncertainty Principle

  • “Bohr orbit” idea violates the uncertainty principle!
  • Certain pairs of variables (e.g., x and px; E and t; r and L) can’t be known exactly at the same time
  • E.g., (Δx)(Δpx)h4π(\Delta x)(\Delta p_x) ≥ \frac{h}{4π}, whereΔx\Delta x denotes an uncertainty in x, etc. Clearly both uncertainties can’t be zero if RHS is nonzero…
  • Deep result, NOT a mere technical problem with measurement.