Quantum Mechanics Flashcards

1
Q

Classical Mechanics

A

E=1/2mv² + V = P²/2m + V
EK - due to momentum (P)
V - due to position (x)
Need to know starting position, P and V to predict the subsequent trajectory exactly.
Newtonian mechanics - any x and p (or E) is possible.

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2
Q

Rotations of bodies

A
p->J/L (angular momentum)
m-> I (moment of inertia)
v -> ω (angular velocity)
F -> T (torque)
Any rotational E/p possible, if suitable torque is applied
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3
Q

Vibrations of bodies

A

F=-kx
All E possible
Internal motion

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4
Q

Light

A

Classical view - light is a wave (reflection, refraction etc)
Modern view - wave-particle duality
EMR-light has different colours associated with a Δλ.
Continuous, all E and λ possible.

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5
Q

Blackbody radiation

A

Material that converts heat to light. Cavity with exit pin-hole for light to escape, emitted by hot body. Increase T results in increase in total output, shifting the maxima to a lower λ.
ρ = total E in region of EM field / V
- ρ is energy density

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6
Q

Wein’s law

A

Assumptions about absorption/emission of EMR.
ρ=c1/λ⁵.1/e(c2/λT), adjusting c1 and c2 to get best fit.
-really good at short λ
-not so good at long λ

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7
Q

Rayleigh Jean Law

A

Treat EM field as a lot of oscillators. Calculate the number with each E, predict a curve proportional to λ-⁴
Full and detailed thermodynamic treatment.
ρ=8πkT/λ⁴
-good at long λ
-terrible at short λ
Average of each oscillator is kT, regardless of frequency. Each wave mode has the same energy.
UV catastrophe - emissions due to ∞ at 0λ. High E’s even at low T (no darkness!). All bodies lose E fast - does not reflect reality.

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8
Q

Planck Distribution

A

Empirical modification of Wein’s law.
ρ=c1/λ⁵.1/e(c2/λT)-1
Essentially a perfect fit at all λ.
Each mode has a discrete amount of E (QM). Addition of the -1 term, so cannot have continuous values (as previously allowed)

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9
Q

Quantum Assumptions

A
Wall of blackbody radiator contains harmonic oscillator (HO), each with characteristic frequency. E of each HO quantised: E=nhv, where n=0,1,2... HOs emit and absorb E only in discrete amounts: E=hv. 
Assumptions:
c1=8πch
c2=ch/k(B)
ρ=8πch/λ⁵.1/e(ch/λKT)-1
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10
Q

Photoelectric Effect

A

Light is a particle.

When light is shone on some metals, electrons are emitted. EK of e-s remains the same. No e-s emitted for v

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11
Q

e- diffraction

A

e-s diffracted from metallic Ni. Gives a diffraction pattern exactly in accord with de Broglie’s λ. Cannot think of small objects in terms of trajectory (x and p) - Heisenberg uncertainty. Rather, a probability of being in any particular place, described by the wavefunction.

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12
Q

Wavefunctions Ψ

A

Mathematical function describing the probability distribution of a particle (e-). Ψ is a function of position and time.
Deal with time-independent systems -> only position (x,y,z)

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13
Q

Postulate 1 - Ψ

A

In 1D Ψ, Ψ(x), allows us to determine translational motion.
Ψ contains all the dynamical information about the system. Values have no physical meaning. Get information by manipulating Ψ to return real values relating to physical properties (E, x, p…).
Operator form of SWE: H^Ψ=EΨ

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14
Q

Postulate 2 - Born Interpretation

A

Wavefunction has value Ψ at some point r. Probability of finding the particle in a really small volume at r∝|Ψ²|dτ
|Ψ²| gives real, positive values (relating to where something is)

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15
Q

Postulate 3 - acceptable Ψ’s

A
  • continuous
  • single values
  • continuous first derivative
  • square integrate the function (not infinite)
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16
Q

Operators

A

Something you do to a function to get real information out. Different operators represent different properties (E, p, x…)

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17
Q

Postulate 4 - observables

A

Represented by operators (built from x or p operators).
-position operator (x^) is x multiplied by something (operator for position along x axis). Multiply Ψ by x.
-momentum operator (p^) = ℏ/i . d/dx
Satisfy commutation relation (relation between conjugate quantities - mutually exclusive). x^ and p^ in x-direction of a particle in 1D: x^1p^ = xP-Px
-communtator of reduced Planck’s constant and i: x^p^=iℏ

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18
Q

Postulate 5 - Heisenberg

A

Impossible to specify simultaneously both p and x of particle. Can relate any pair of observables with operators that do not commutate.
ΔpΔx>ℏ/x
px-xp=h/2πi
If x=0, Δp=infinity - complete uncertainity in momentum
If p=0, Δx=infinity - complete uncertainity in position

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19
Q

Time independent SWE

A

Interpretation of de Broglie (wave-particle duality)
-ℏ²/2m . d²Ψ/dx² + V(x)Ψ = EΨ
Gives real values
Solutions: Ψ=coskx + isinkx
-k can take any value, thus E should be able to take any value. But acceptable Ψ restricts E (quantised)

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20
Q

K(B)

A

Boltzmann Constant

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21
Q

H^

A

Hamiltonian Operator

22
Q

τ (tau)

A

Really small volume

dτ=dxdydz

23
Q

|Ψ²

A

Probability density

24
Q

i

A

Imaginary number = root(-1)

25
Q

A

Reduced Planck’s constant = h/2π (Js/rad)

26
Q

Simple model systems

A

Translational (movement in 1D), rotational (motion about an axis) and vibrational (internal motion).

27
Q

Translational motion

A

Description of motion in 1D

Particle in a box and at a barrier

28
Q

Particle in a box

A

Particle of mass m can lie anywhere along a line of length L, creating a box where you can find the e- (V=∞ at walls and V=0 at base). Probability of being where V=∞ is zero, Ψ=0 at x=0 and x=L.
-ℏ²/2m . d²Ψ/dx² = EΨ as V=0
General solutions: Ψ=Ae(ikx) + Be(-ikx)
E=ℏk²/2m describes Ψ and E of a free particle.
As the particle is confined to a region, the acceptable Ψ must satisfy boundary conditions.
Ψ=(A+B)coskx + (A-B)isinkx = Csin(kx) + Dcos(kx)
x=0, Ψ(0)=0.
-D=0, thus, Ψ = Csin(kx)
x=L, Ψ(L)=Csin(kx)=0.
-if C=0, then Ψ=0 for all values of x, conflicting with the Born Interpretation (particle is somewhere)
-sin(kL)=0 and kL=πn, n=1,2,3…
-Ψ(x)=Csin kπx/L = Csin nπx/L
E=n²h²/8mL²
C=root(L/2), thus, Ψ(x)=root(2/L)sin(nπx/L) for 0

29
Q

Vibrating string

A

Classical analogy: only certain wavelengths possible as the ends are fixed.
Ψ = sin 2πx/λ, λ restricted to 2L/n, n=1,2,3…
-quantisation forced by boundary conditions

30
Q

Energy levels - translational motion

A

E levels increase as n² increases, separation increases with n.
E(n)=n²h²/8mL², n=1,2,3…

31
Q

Zero-point energy (ZPE)

A

n cannot = 0, so E cannot = 0.
n=1, E(1)=h²/8mL² = ZPE (lowest E a particle can possess).
-must have non-zero kinetic energy (Heisenberg)
-Ψ=0 at walls, but smooth, continuous and non-zero everywhere else.

32
Q

Correspondence Principle

A

The behaviour of QM systems becomes more classical in the limit of large qns.
E(n+1)-E(n)=(2n+1)h²/8mL²
E will increase with decreasing m and L (L has a greater effect due to ²).
-As m tends to infinity, E tends to 0. Thus, E level separation becomes inseparable and is no longer quantised
Implications - atoms/molecules in beakers treated as if their translational motion is not quantised, impacting spectroscopy and material properties.

33
Q

Applications - predict dye colour

A

To be coloured, dyes must absorb in the visible region of the EM spectrum. Interaction of light with e-s. Absorption of light/photons (change of quantised E). Object absorbing certain λ or v of white light, reflects complementary colour. E=hv=hc/λ
π e-s in p-orbitals (conjugated systems - alternating single and double bounds).
Terminantor atoms - denote the end of the box, disrupt the flow of e-s along molecule (N)
1) box length: 1.39Å x #bond lengths
2)#e-s (lp and π) - for multiple e-s, assume no interaction between e-s apart from Pauli Exclusion Principle. Populate using Aufbau’s rule.
3) ΔE=(2n+1)h²/8mL² (should be E-19 J or kgm²/s²). Convert to kJ/mol by multiply by N(A)/1000.
4) λ = hc/E. Absorbs this λ and reflects complementary colour
5) v = E/h

34
Q

Particle at a Barrier

A

Tunnelling - particle penetrates through the walls to classically forbidden regions. Walls thin, enough E for e- to pass through.
E=ℏ²k²/2m
kℏ²=root(2mE)
V->infinity at barrier, but if it doesn’t, E A’e(ikx).
Particle has a probability of being beyond the barrier, and within the barrier. Ψ must be continuous and dΨ/dx must be continuous entering and leaving the barrier.
Tunnelling consequence of wave character behaviour of matter (ex: radio waves pass through walls). Matter can pass through walls on the quantum level. Probability decreases with increasing thickness of walls and m of particle (e->proton).

35
Q

Applications of particle at a barrier - Scanning Tunnelling Microscopy (STM)

A

STM - dependence of e- tunnelling on thickness of region between point and surface. Needle scans across surface of conducting solid and e-s tunnelled across space.
Constant current mode - fixed distance between surface and stylus -> map
Quantum biology - does tunnelling occur during mutations of DNA? - Life and cancer research.

36
Q

c=normalising constant

A

c=root(L/2)

37
Q

Vibrational motion

A

Two models, Harmonic oscillator (HO) and Anharmonic oscillator (AO)

38
Q

Harmonic Oscillator (HO)

A

Hooke’s law: F=-kx
K is force constant. Large K = narrow potential well = stiff spring (more F required to displace spring)
V=1/2kx² - parabolic shape. No displacement means particle is at eqm. Particle tends towards infinity, no sharp boundary (unlike particle in a box)
SWE: -ℏ²/2m . (1/2x²)Ψ = EΨ
-particle trapped by infinite walls, results in quantisation and boundary conditions. Ψ and Ψ² don’t equal 0 at any point (except infinity).
-particle can be anywhere, regardless of E (even chemically forbidden zone -> tunnelling).
E levels: E=(v+1/2)ℏω, where v=0,1,2… and ω=root(k/m)
E spacings are even (ΔE=ℏω). For large objects ℏω is negligible.
ZPE: lowest E level at 1/2ℏω (E cannot be 0 - always in motion and position restricted). Walls rise to infinity (curved).
X-H: heavy atom (x) is stationary and light atom (H) moves, vibrating as a simple harmonic oscillator. Bonds act like springs.

39
Q

HO for diatomics

A

Atoms with similar masses move relative to each other.
Push atoms together (e- repel, increase E) and pull apart (until bond breaks) when vibrating with respect to r(eq).
HO: models bottom of potential well well, but not at higher E.
Parabolic V: close to r(eq) can approx V by parabola (V=1/2kx²), x=r-r(eq). k is a measure of curvature of V close to eqm extension of bond. Steep walls = stiff bond = large k.
Frequency of oscillator depends on the two masses
-homonuclear (F2): m1=m2
-heteronuclear (NaCl): m1 doesn’t equal m2
SWE: -ℏ²/2m(eff) . (1/2x²)Ψ = EΨ
E=(v+1/2)ℏω, v=0,1,2… and ω=root(k/m(eff))
Curvature of walls leads to some Ψ extending outside of the parabola (tunnelling). ΔE=ℏω, so E level spacings are even.
Tunnelling - probability of being in a forbidden region, independent of k and m.
ex: inversion of NH3. Doesn’t go over E barrier of planar form (not superimposable). Absorption ~900cm-1 (barrier ~2000cm-1), corresponding to v0->v1 (lowest vibrational state).

40
Q

Effective mass (M(eff))

A

Measure of mass moved during vibration

m(eff)=m1m2/(m1+m2)

41
Q

Reduced mass

A

Emerges from separation of relative internal and overall translational motion. Meff and u are not the same overall (except have same values for diatomics).

42
Q

Vibrational term (G~)

A

Expresses E of vibrational states in terms of wavenumber (cm-1). E=hcG~(v)
G~(v)=(v+1/2)v~
v=ω/2π and v~=ω/2πc

43
Q

IR spectroscopy

A

Frequency of E level transition (v~10E14 Hz). Use IR to look at vibrations of molecules.
Molecular fingerprint
-k proportional to bond strength
-bond strength depends on molecular environment
-selection rule: for a vibration to be observed, the dipole must change (heterogeneous, asymmetric or bent)

44
Q

Anharmonic Oscillators (AO)

A

AOs can break bonds to make new bonds (limitation of HO - based on a parabola). HO describes the small changes in bond length well (parabola), but is wrong for increased E/Ψ.
At higher vibrational excitations, movement of atoms allows molecules to explore regions of V curve where parabolic approx. is poor. F no longer proportional to x.
Curve less confined than parabola. E levels less widely spaced at high excitations (weaker bond) - Morse potential

45
Q

Morse Potential

A

V=hcD(e){1-e(-a(r-r(e)))}²
-a=root(m(eff)ω²/2hcD~(e)) - width of potential
-r - internuclear separation
-D~(o) - dissociation energy from v=0 to highest occupied v
-D~(e) - dissociation energy from r(eq) to highest occupied v
D(e)-D(o) = ZPE
Near minimum vibration of v with displacement resembles a parabola. Allows for dissociation at large displacements.
Permitted E levels: G~(v)=(v+1/2)v~-(v+1/2)²X(e)v~
-X(e) = a²ℏ/2m(eff)ω = anharmonicity constant
-G~(v) becomes smaller, reaching v(max) at G~=0.
Δv=+/-1, so ΔG~(v+1/2)=G~(v+1)-G~(v) -> converge
Dissociation limit - point where v=v(max). The separation between E levels vanishes and ΔG(v+1/2)=0.
v(max)=(v~/2v~X(e))-1
D(o) - when several vibrational transitions are detectable, can determine D(o) of bond. Sum of successive intervals from v=0 to v(max).
Birge-Sponer Plot - plot ΔG~(v+1/2) against v+1/2. X-axis intercept will give v(max). Inaccessible part of spectrum estimated by linear extrapolation. Integrate to get D(o) - often overestimated as realistically not linear.

46
Q

HO vs MO

A

HO
+gives bond strength; apply to polynuclear systems
-doesn’t give D(o) and doesn’t fit experimental data well
MO
+gives bond strengths and D(o) and fits experimental data well
-cannot be applied to polyatomic molecules

47
Q

Particle on a sphere

A

Ψ must satisfy 2 cyclic boundary conditions, resulting in 2 quantum number’s for state of angular momentum. θ and ϕ. Ψ must match over the poles (θ) and round the equator (ϕ)
SWE: -ℏ²/2m . ∇² = EΨ
-∇² (laplacian) = d²/dx²+d²/dy²+d²/dz²
-Once object is set in motion in a vacuum, no E required to keep it spinning, so V=0.
Rotational qn’s: 2 orbits -> 2 qn’s
L=angular momentum qn, L=0,1,2..
m(l) = component of orbital angular momentum about the x-axis, +L to -L.
E particle: restricted to certain values due to boundary conditions, continuous Ψ around sphere. Independent of m(l).
E=L(L+1)ℏ²/2I, where I=mr²
Classical model - centre of mass depends on m1/m2
-homogenic diatomic - m1=m2
-heterogenic diatomic - m1r1=m2r2 and r=r1+r2

48
Q

Rigid Rotor

A

Fixed radius (rotation doesn’t result in stretching of the bond). Thus, a body does not distort under the stress of rotation, due to negligible centrifugal force.
Simplification, use μ to transform problem to that of a single mass rotating around the origin.
μ=m1m2/m1+m2 x 1.66o54E-27
I depends on masses of atoms present and molecular geometries. 3 I defined about 3 perpendicular axes: I(c)>I(b)>I(a)
Linear rotor - E quantised.
E(J)=J(J+1)ℏ²/2I, J=0,1,2…
E level ladder: E expressed in terms of a rotational constant (B~)
B~=ℏ/4πcI or hcB~=ℏ/2I
E(J)=hcB~J(J+1)=nBJ(J+1)
-E level spacings get further apart with increasing J.
-B expressed as frequency = B~c
E rotational state: rotational term F~(J)
F~(J)=B~J(J+1)=E(J)/hc
Frequency: E=hb=hv

49
Q

Rotational-Vibrational Spectrum

A

Heteronuclear diatomics in the gas phase.
Rotational and vibrational motion is not discrete and combine to give special spectral information. As the molecule vibrates, the bond length changes. Rotational E changes with bond length (longer bond = slower spin).
Bond spectrum - high resolution vibrational spectrum has bands. n peaks = 2 isotopes (more abundant = bigger)
Selection rule: ΔJ=+/-1 and sometimes ΔJ=0 during a vibrational transition.
Spectral branches - each vibrational E level has a series of rotational E levels associated with it. Appearance of S~.
S~=G~(v)+F~(J) = (v+1/2)v~+B~J(J+1)
Vibrational transition from V+1

50
Q

P Branch

A

ΔJ=-1

Transition: v+1

51
Q

Q Branch

A

ΔJ=0

Transition: v+1

52
Q

R Branch

A

ΔJ=+1

Transition: v+1