Quantum mechanics Flashcards

(45 cards)

1
Q

What is the equation for kinetic energy?

A

K = 1/2 mv^2 = p^2/2m
where p = (h bar) x a

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2
Q

Equation for average kinetic energy of a monoatomic gas i.e. argon

A

1/2 kB T
where kB = Boltzmann constant
T = absolute temperature
kBT = thermal energy

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3
Q

What is potential energy?

A

Energy required to place particles of system in given position i.e. energy associated to position of such particles

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4
Q

Give examples of potential energy and any laws used to give potential energy (give equations)

A

Example: Potential energy between two charges q1 and q2 at distance r given by Coulomb Law
Vc(r) = e^2/(4piε0) x q1q2/r
where e = elementary charge
ε0 = 8.854 x10^-12 F.m-1

Example 2: Potential energy between 2 atoms that can form chemical bond

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5
Q

Compute thermal energy at T = 300K and express in J and eV

A

kBT = 1.381 x10^-23 JK-1 x 300K = 4.143 x10^-21 J –> 0.02586 eV = 25.85 meV
J/1.602 x10^-19 = eV

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6
Q

Compute linear momentum of argon atom (m=40 u) or an electron (m = 9.1 x10^-31 kg) if their kinetic energy is equal to thermal energy computed in previous question (4.413 x10^-21 J)

A

p = mv
m = 40 x 1.661 x10^-27 kg = 6.644 x10^-26 kg
K = p^2/2m
For argon atom:
p = sqrt(K x 2m) = sqrt(4.413x10^-21 x 2(6.644x10^-26)) = 2.422 x10^-23 kg m/s

For electron:
p = sqrt(4.413x10^-21 x 2(9.1x10^-31)) = 8.962 x10^-26 kg m/s

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7
Q

Description of a classical system of N particles (Law involved)

A
  • Position and velocity at initial time
  • Forces or potential energy between particles
  • Mass of all particles (m1, m2, …)
  • Newton’s Law (Fi = miai)
  • System fully descirbed by {r1(t), r2(t), …, rN(t), v1(t), v2(t), …, vN(t)}
    where rN(t) = position of all particles as a function of time
    vN(t) = velocity of all particles as a function of time
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8
Q

Description of a quantum system of N particles (equation involved, requirements of wavefunction)

A
  • Wavefunction at an initial time
  • Potential energy of a system
  • Mass of all particles (m1, m2, …)
  • Schroedinger equation
  • System fully described by wavefunction ψ(r,t)
    where r = coordinates of all particles and t = time
  • Wavefunction must be continuous (no jumps) and differentiable (no corners)
  • Values of wavefunction can be complex (with real and imaginary part)
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9
Q

Where are the particles at a given time in a quantum system? (probability of finding)

A
  • System with 1 particle in 1 dimension (1 coordinate x) has wavefunction: ψ(x,t)
  • Probability of finding particle in vicinity of certain value of x is: |ψ(x,t)|^2
  • Quantum mechanics only predicts probability of finding particle in given position
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10
Q

Compare/contrast classical mechanics with quantum mechanics

A

Classical:
- Time evolution: trajectory (i.e. position and velocity as function of time)
- Info needed: Initial position/velocity at t = 0, potential energy V, mass of particles
- Position of particles: Known with certainty
- Other observables: Known with certainty

Quantum:
- Time evolution:wavefunction (i.e. function of all coordinates and time)
- Info needed: Initial wavefunction at t = 0, potential energy V, mass of particles
- Position of particles: Known as a probability
- Other observables: Known as a probability (in general)

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11
Q

What is an operator?

A
  • A mathematical object (O hat) that transforms a function into another function
  • In O hat f = g, O hat transforms function f into new function g
  • Operator that transforms function into derivative written as O hat 1 = d/dx
  • Operator that transforms function into same function multiplied by x written as O hat 2 = x
  • Operators can be summed or multiplied
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12
Q

What is the de Broglie relation?

A

lambda = 2 pi h bar/p = h/p

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13
Q

Describe the particle in a box theory (give equation for free particle wavefunction)

A
  • Particle of mass m in 1 dimension can only occupy positions between x = 0 and x = L
  • Wavefunction must = 0 for x<0 and x>L (particle is never there)
  • Wavefunction will also be 0 at edge of box as it must be continuous
  • In region 0<x<L particle is free and free particle wavefunction can be used ψ(x) = Acos(ax) + Bsin(ax)
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14
Q

What is the normalisation of a wavefunction?

A

Multiplying the wavefunctions by a factor such that the integral over all space is 1

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15
Q

What are observables? Give examples. When are they used/cannot be used?

A

Everything you can actually measure (classical):
- Position (x)
- Linear momentum (p(x))
- Kinetic energy (K)
- Angular momentum (L)

  • Wavefunction cannot be measured (quantum mechanics).
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16
Q

How are observables and operators related and give examples.

A
  • Correspondence between everything you can measure and a mathematical operator
  • Operators can be seen as variables that multiply by function to give different function

Operators:
- Position x: x hat –> x
- Linear momentum p(x): p(x) hat –> -ih bar d/dx
- Kinetic energy: K hat = -(h bar)^2/2m x d^2/dx^2

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17
Q

What is expectation value? Give equation

A
  • If system in generic state psi (not eigenfunction of A hat) and one measures quantity of A, measure gives one of eigenvalues of A with certain probability
  • Expectation value = average of many measures
  • <a> = (integral of psi * A hat psi d tau)/(integral of psi * psi d tau)</a>
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18
Q

What is the Heisenberg Uncertainty Principle?

A
  • Different operators/observables have different eigenfunctions
  • It is not possible to measure both quantities with arbitrary accuracy
  • Uncertainty set by quantum mechanics
  • For position and momentum: delta(x)delta(px) is greater than or equal to 1/2h bar
  • For smaller boxes (decreasing L), become more sure of position (delta x decreases) and more unsure about momentum (delta p increases)
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19
Q

What is the lowest energy level in the harmonic oscillator and why (give equation)?

A
  • 1/2 h bar omega
  • Can’t be 0 (bottom of potential energy curve) because equation Ev = h bar omega (1/2 + v)
  • Would mean position and momentum of particle known with arbitrary precision which is forbidden by Heisenberg principle
20
Q

Describe harmonic oscillator energy graph - how are the energy levels spaced and what is the space between them?

A
  • Evenly distributed
  • h bar omega between each energy level Ev (v = 0,1,2, etc)
  • v starts from 0, whereas in particle in box they start from 1
21
Q

Equation for wavelength

A

lamda = c/v
c = speed of light
v = frequency

22
Q

Equation for angular frequency

A

omega = 2.pi.v

23
Q

How is radiation absorption measured? (3 equations)

A

Transmittance: T = I/I0 (transmitted light/incident light)
Absorbance: A = -logT
Beer-Lambert Law: Av = 𝜀v.cL

24
Q

What is rate of light absorption proportional to? Which transitions are allowed/forbidden?

A

proportional to |𝜇(ij)|^2
transition dipole moment 𝜇(ij) = integral of 𝜓(𝑖)∗𝜇𝜓(𝑗) 𝑑𝜏
where 𝜇 = dipole moment operator
𝜇(ij) = 0, transitions FORBIDDEN
𝜇(ij) ≠ 0, transitions ALLOWED

25
What are selection rules?
Conditions that need to be satisfied for transition to be allowed
26
What are the selection rules for the Harmonic Oscillator? (3)
1. Must have permanent dipole moment (HF, HLi, CO, etc) 2. Only allowed transitions have 𝛥v = ±1 3. Only radiation absorbed has energy ℏ𝜔
27
What does intensity of transition depend on? (1)
Fraction of molecules found in initial state (population)
28
What does population depend on and what law does it follow? Give equation (given in equation sheet)
- Depends on T - Follows Boltzmann distribution law: - P(i) ∝ exp(−𝐸(𝑖)/𝑘(B)𝑇) - If at energy level Ei, there are g(i) degenerate (same energy) states: P(i) ∝ 𝑔(𝑖)exp(−𝐸𝑖/𝑘𝐵𝑇)
29
What is the Anharmonic Oscillator (Morse Oscillator) model used best for? Give an equation for energy levels (given in eq. sheet). Which transitions are allowed? What is transition 1 --> 2 called?
- Better model for vibration in biatomic molecules - Includes dissociation - Energy levels get closer at higher energy: - Ev = ℏ𝜔(𝑣 + 1/2) − (ℏ𝜔)^2/4𝐷(𝑒) x (𝑣 + 1/2)^2 - Transitions 𝛥𝑣 = 2, 3 allowed (overtones) - 1 --> 2 = hot band (transition between 2 excited vibrational states, neither is ground state)
30
What are the 2 ways of emitting radiation?
- Spontaneous emission: excited atom/molecule transitions to lower energy state and emits photon of energy without external influence - Stimulated emission: incoming photon triggers excited atom to release photon of same energy/phase/direction, transitions to lower energy with external influence
31
What 2 other things can happen when radiation hits molecule? How does this help to compute energy levels? Which type of molecules are Raman active?
- Rayleigh scattering: molecule will scatter elastically (change direction of motion of radiation without losing energy). Scatter radiation is same frequency as incoming radiation - Raman scattering: molecule will absorb some of the radiation and scatter inelastically (radiation scattered but some energy lost to molecule). Scatter radiation is lower frequency than incoming radiation - Energy levels measured by computing how much energy lost in process of plasma scattering - Biatomic molecules without permanent dipole (H2, F2) = Raman active
32
What is a rigid rotor and what are the energy levels (equations given in eq. sheet)?
Rigid rotor = object formed by 2 point-like particles rotating freely in space Each state of rigid rotor defined by 2 quantum numbers: J = angular momentum quantum number (0,1,2,...) m(J) = magnetic quantum number (-J, ..., +J) not affecting energy so energy is only a function of J: (Energy levels) E(J) = ℏ^2/2I x J(J+1) where I (moment of inertia) = 𝜇R^2 R = internuclear distance ℏ^2/2I = constant B, same for all states
33
What are the selection rules of the rigid rotor?
- 𝛥𝐽 = ± 1 (are the transitions allowed) - Molecules must have net dipole moment - In general, majority of transitions not allowed
34
What is the equation for energy levels if a molecule rotates and vibrates?
E(T) = Evib + Erot = ℏ𝜔(𝑣 + 1/2) + BJ(J + 1)
35
Electron angular momentum (What is electron spin?)
- Electron spin = measurable natural/essential angular momentum of electron (observed experimentally), 2 observables and operators, 2 spin wavefunctions per electron - All electrons have same total angular momentum and 2 possible orientations (never seen for macroscopic/non-microscopic particles) - Since observable, corresponding operator: - (S hat)^2 x sigma = s(s + 1)x (h hat)^2 sigma where s = angular quantum number for spin - (S hat)^2 sigma = m(s) x h hat x sigma where m(s) = magnetic quantum number for spin - Only possible values of quantum numbers are: s = 1/2 and m(s) = 1/2, -1/2 - Only 2 possible spin wavefunctions: spin up (alpha) or spin down (beta)
36
What are the consequences of existence of electron spin?
- Extra magnetic dipole affects energy of atom under magnetic field, important only if 1 is interested in magnetic properties - Angular momentum of electron and angular momentum of spin combine together in non-trivial way (total energy isn't exact sum of energies of 2 rotors) - Effect called spin orbit coupling, explains spectra of multi electron atoms - Spin orbit coupling small, important only for heavy atoms - Existence of spin completely changes behaviour of multi-electron systems
37
Helium atom Hamiltonian equation
H hat (He)(r1, r2) = K hat(1) + V hat(1n) + K hat(2) + V hat(2n) + V hat(1 2) K hat 1 and 2 = KE of 2 electrons V hat 1n and 2n = attraction to nucleus of 2 electrons V hat 12 = electron-electron repulsion (depends on r12/distance between electrons)
38
What is an orbital?
Single electron wavefunction - If more than 1 electron, electrons not rigorously described by orbital but good approximation
39
What is the wavefunction for two electrons? Include wrong examples and explain why they don't work
Wrong: - psi(A)(r1)psi(B)(r2) wrong because electrons also have spin - psi(A)(r1)alpha(1)psi(B)(r2)beta(2) wrong because electrons shouldn't be distinguishable Right: - |psi(r1,r2)|^2 = |psi(r2,r1)|^2 Common mistake: - psi(r1,r2) = +/- psi(r2,r1) wrong; sign is always minus, can't be explained therefore is a postulate
40
What is the only valid wavefunction for 2 electrons in 1 orbital?
[psi(A)r1)psi(A)r2][alpha(1)beta(2)-beta(1)alpha(2)] - electrons have opposite spin when in same orbital - not possible to write valid wavefunction with 2 or more electrons in same orbital (Pauli exclusion principle)
41
Which energy out of singlet or triplet configuration is smaller and why?
E singlet > E triplet Triplet: psi(A)(1)psi(B)(2) - psi(B)(1)psi(A)(2) Singlet: psi(A)(1)psi(B)(2) + psi(B)(1)psi(A)(2) psi(1,2) = psi(r1,r2) |psi(r1,r1)|^2 (prob. of e-s in same place) = 0 (for triplet so less repulsion) and not 0 (for singlet so more repulsion)
42
What is the most common approximation method for wavefunctions?
To express approx. wavefunction as linear combination of basis functions: psi = c1psi1 + c2psi2 + ... + c(n)psi(n) where coefficients {c1,c2,...,cn} determined to make psi best possible approx. of ground/excited wavefunction
43
What are molecular orbitals?
Linear combination of atomic orbitals (LCAO) Describe electrons in molecules Expressed as wavefunction approx. equation and {psi1,psi2, ..., psi(n)} = set of atomic orbitals Computing molecular orbital = determining coefficients of wavefunction approx. eq.
44
What's the best linear combo that solves Hpsi = Epsi ?
psi = c1psi1 + c2psi2 Sub into time-indepedent Schrodinger equation: H(c1psi1 + c2psi2) = E(c1psi1 + c2psi2) Multiply by psi1* and integrate: psi1*H(c1psi1 + c2psi2) = E(c1psi1*psi1 + c2psi1*psi2) [integration steps] c1H11 + c2H12 = E(c1S11 + c2S12) new symbols are just replacing integrals Multiplying subbed TI Schrodinger eq. by psi2* and repeating process gives: c1H21 + c2H22 = E(c1S21+c2S22)
45
What are elements H(ij) and S(ij) called?
H(ij) = matrix elements S(ij) = overlap matrix elements