Hydrogen-Like Atoms Flashcards

1
Q

What do the energy eigenvalues depend on in the absence of an external field?

A

Only depend on n.

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2
Q

What is meant by degeneracy?

A

Where several quantum states can share the same energy.

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3
Q

What are the labels for the quantum number l?

A

l=0: s-state, l=1: p-state, l=2: d-state, l=3: f-state, l=4: g-state, and then in alphabetical order after that.

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4
Q

How many different possible m(l) states are there for each (n,l) state? What is l less than or equal to?

A

2l+1 and l <= n-1

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5
Q

How do we show the notation for increasing n and changing l?

A

The n goes first and then the letter for l. So say n=3, l=1, it would be 3p

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6
Q

What is the shell called for n=1, 2, 3?

A

n=1: K shell, n=2: L shell, n=3: M shell

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7
Q

What does a higher n mean for the electron?

A

Higher n means it is found further from the nucleus.

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8
Q

What is the equation for the reduced mass μ? What is μ usually approximated to?

A

μ = mn*me/mn+me, where mn is the nuclear mass and me is the electron mass. mn&raquo_space; me, so μ ~ me

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9
Q

What is the equation for the hydrogenic atom potential?

A

V(r) = -Z*e^2/4πε0r

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10
Q

What do we do first to the radial part of the wavefunction: [-ћ^2/2m 1/r^2 * d/dr(r^2 d/dr) + l(l+1)ћ^2/(2mr^2) + V(r)]R(r) = E*R(r)?

A

Substitute R(r) = u(r)/r, find 1/r^2 * d/dr * r^2 *d/dr(u(r)/r) = 1/r^2 *d/dr *r^2(1/r du/dr - u/r^2), which can be simplified by putting r^2 inside brackets and find = 1/2 * d^2u/dr^2

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11
Q

What do we do second after simplifying the radial part of the wavefunction?

A

Sub it in and rearrange, find final equation of -4πε0/2m *d^2u/dr^2+ [V(r) + l(l+1)ћ^2/(2mr^2)]u = Eu

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12
Q

What does the part inside the square brackets represent?

A

The effective potential.

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13
Q

What form does this new equation have solutions in?

A

R(r) = C(n,l) * f(ρ)exp(-ρ), ρ = r/a(B), a(B) is Bohr radius = 4πε0ћ^2/me^2

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14
Q

What is meant by the probability function, PDF?

A

We want the chance of finding the electron in some volume dV.

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15
Q

What is the equation for |Ψ|^2 dV?

A

|Ψ|^2 dV = |Ψ|^2 * r^2 sinθ dθdФdr

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16
Q

What is |Ψ|^2 equal to?

A

|Ψ|^2 = |R(r)|^2 * |Θ(θ)|^2 * |ф(Ф)|^2

17
Q

What is |ф(Ф)|^2 equal to?

A

|ф(Ф)|^2 = AA* * exp(im(l)Ф) 8 exp(-im(l)Ф) = A^2

18
Q

What do we need to do to average over Θ and ф to get the probability that the electron is inside a shell of radius r and thickness dr?

A

P(r) dr = r^2 *|R(r)|^2 dr * integral from 0 to π of |Θ|^2 sinθ dθ * integral from 0 to 2π of |ф|^2 dФ -> both these integrals equal 1

19
Q

What are the energy eigenvalues?

A

En = -E1*z^2/n^2, n=1,2,3,…, E1 = Rydberg energy

20
Q

What is the main experimental evidence of all of this?

A

Main evidence is optical spectra -> transitions between different allowed quantum states by absorbing or emitting a photon.

21
Q

What is the Rydberg energy?

A

E1 = 13.6 eV

22
Q

How can we sketch the H atom energy levels?

A

Different lines for different energy level with E=0 at the top and goes more negative as you go down. Each line split into sections (like s, p, d etc)

23
Q

Which optical transitions are forbidden?

A

Ones where the quantum number l does not change (e.g. 2s -> 1s)

24
Q

Why are transitions where l = +/- 1 allowed?

A

Because photons have angular momentum, and to conserve this a photon must carry off or deliver some to/from the atom.