Topic 2 Flashcards

1
Q

What is the letter for the principal quantum number?

A

n

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2
Q

What is the letter for the orbital angular momentum quantum number?

A

l

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3
Q

What is the letter for the magnetic quantum number?

A

ml

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4
Q

What is the letter for the spin quantum number?

A

s

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5
Q

What is the letter for the magnetic spin quantum number?

A

ms

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6
Q

In the absence of spin-orbital coupling the energy of an atomic orbital in a one-electron atom or ion, X, only depends on what?

A

On the principal quantum number, n.

Where Z is the nuclear charge, RX is the Rydberg constant for that atom.

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7
Q

What happens when n goes closer to infinity?

A

Energy and n has an inverse relationship. So the higher the n the closer to 0 energy we get as relationship is E=1/n2

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8
Q

Why the energy velue of energy levels is negative?

A

As n increases, electron moves further away from the nucleus until we get n value where electron is ionised from the atom. This energy is equal 0. And as electron moves down in n, it gets more stable so we move down in energy.

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9
Q

What is Rydberg constant?

A

This expression comes from solving the Schrodinger equation and getting the correct units. Note that c is in cm s-1. The value depends on the mass of the nucleus, and so there is a drifferent Rydberg constant for each atom.ion.

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10
Q

How to calculate energy difference between to energy levels?

A
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11
Q

What are selection rules for spectroscopy?

A

Δn (principal quantum number) unrestricted

(orbital angular momentum quantum number) Δl=±1 (Laporte selectrion rule)

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12
Q

Explain Laporte selection rule.

A

Δl=±1, meaning transitions can accur between s,p,d,f orbitals byt not within them

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13
Q

How to calculate Ionisation energy?

A

IE is the energy where n is equal to infinity which is 0, minus the energy of 1s orbital which is minus. Thus ionisation energy is equal to energy of 1s orbital.

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14
Q

What is atomic emission spectrometer?

A

It records emissions produced by different substances when it is burning and compares it with a known values.

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15
Q

How do we analyse spectra with more then one electron?

A

We look at orbital angular momentum of each of the electrons and see how those behave inside a particular atom.

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16
Q

What is the value of l for s orbital?

A

l=0

17
Q

What is the value of l for p orbital?

A

l=1

18
Q

Why adding up the angular momenta will lead to different energies?

A

Because the angular momenta of the different electrons in the atom can couple together in different ways.

19
Q

When considering spectra with more than one electron which quantum numbers we consider first and which last?

A

We will consider spin first, then orbital angular momenta, then finally the coupling between spin and orbital angular momenta.

20
Q

What is Russell-Saunders coupling?

A

Is where we allow the spins to couple together and the orbital angular momenta to couple together separately. And then only at the end to be coupled together.

21
Q

What is Clebsch-Gordan series for spin quantum number?

A

If S in the overall spin of the two-electron system, then the allowed values come from: S=s1+s2​, s1+s2​-1… |s1-s2​|.

So the allowed values of S are 1/2+1/2=1 and 1/2 - 1/2=0

22
Q

What are alowed values for l coupling considering Clebsch- Gordan series?

A

Values of l are integer, 0,1,2… If L is the total orbial angular momentum of the combined system, then allowed values are L=(l1+l2), (l1+l2​-1),…|l1-l2​|

So if l1=2 and l2=3, for example, then we have a highest value of 2+3=5, and the lowest value |2-3|=1.

Hence L=5, 4, 3, 2, 1

23
Q

What are the values of spin-orbital angular momentum, J?

A

We use Clebsch-Gordan series J=L+S, L+S-1,… |L-S|

So if both L and S are 1, then allowed values of J are 2, 1, 0.

24
Q

What are values of ML of atom with more than one electron?

A

ML=L, L-1…, -L

25
Q

What are values of MS of atom with more than one electron?

A

MS= S, S-1…, -S

26
Q

What atomic term symbols mean?

A
27
Q

What is the term sybol for all closed-shell atoms and ions?

A

1S0

28
Q

What is the term symbol for alkali metals?

A

2S1/2

29
Q

What determines the intensity of transitions?

A

Since the final level is the same, the intensity of the transition is mostly determined by the degeneracy (2J+1) of the upper levels. Hence, we expect ratio 2:1 of intensities.

30
Q

What is boson?

A

Something which has a spin of 0, 1 or 2

31
Q

What is Pauli principle?

A

Any acceptable wavefunction must be antisymmetric with respect to the exchange of two identical fermions (e.g. electrons) and totally symmetric with respect to the exchange of identical bosons.

32
Q

Waht is Pauli exclusion principle?

A

No two electrons in an atom/ ion can have all quantum numbers the same

33
Q

What are Hund’s rules?

A
  1. The term with largest S is lowest in energy
  2. For a given S the term with largest L is lowest in energy
  3. For a term with several levels:
  • If the sub-shell is less than half full the lowest J level is lowest in energy,
  • If the sub-shell is more than half full the highest J level is lowest in energy