Section 4 Flashcards

1
Q

The time evolution of a quantum state of definite energy is

A

Ψ(t) = exp[-iEt/ℏ] Ψ(0)

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2
Q

Unitary evolution

A

|Ψ(t)|^2 = |Ψ(0)|^2 : a stationary state

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3
Q

The eigenvectors of stationary states are also

A

time-invariant

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4
Q

Time-dependent state evolution

A

iℏ ∂Ψ(r,t)/∂t = H(hat)Ψ(r,t)

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5
Q

eigenstate of the Hamiltonian

A

A stationary state has definite energy

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6
Q

The Hamiltonian governs

A

the time-evolution of the state, and hence the expectation values

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7
Q

Ehrenfest’s Theorem

A

is an example of the correspondence principle: QM limits to classical physics for large systems

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8
Q

Newtonian momentum derivation

A

[x(hat),H(hat)] = [x(hat),p(hat)^2/2m + V(x)]

since x(hat) commutes with V(x(hat))

d<x>/dt = 1/2iℏm <[x(hat),p(hat)^2]></x>

=> <p> = m d<r>/dt</r>

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9
Q

similarly derivation gives, [p(hat),H(hat)] =>

A

d<p>/dt = -<ΔV></ΔV>

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10
Q

Stationary states are

A

super-important solutions of time-invarient probability density; time-evolution

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11
Q

eigenvalue equation

A

H(hat) Ψi(x) = EiΨi(x)

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12
Q

The time-independent schrodinger equation

A

[ -ℏ^2/2m d^2/dx^2 + V(x) ]Ψ(x) = EΨ(x)

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13
Q

Probability conservation

A

dPtot(t)/dt = 0

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14
Q

Schrodinger equation links

A

wave-function time evolution and spatial curvature

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15
Q

The flux is a probability current

A

J(r,t) = ℏ/2im [Ψ∇Ψ - Ψ∇Ψ]

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16
Q

Conservation equation

A

dP(r,t)/dt = -∇ . J(r,t)

17
Q

Any change in probability density at a point is

A

balanced by a flow of probability current into or out of that region

18
Q

∇Ψ(x) in definition of J

A

spatial wave-functions must be continuous, to avoid delta-function spikes in flux

19
Q

∇ . J in probability conservation

A

wave-functions must be differentiable everywhere, i.e. ∂Ψ/∂x must be continuous.