4: Electrons in atoms Flashcards

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1
Q

the wave equation

A

c=fλ

speed of light = frequency * wavelength
note frequency often written as v rather than f

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2
Q

equation for energy of photons

A

E = hf or hv
h is Planck’s constant

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3
Q

equation relating energy of photons to wavelength

A

combine c=fλ and E=hf
E = h (c/λ)
inversely proportional

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4
Q

define atomic orbital

A

energy levels which electrons occupy

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5
Q

each orbital can accommodate …

A

two electrons
spin up / spin down

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6
Q

names of shells in order

A

K (1s)
L (2s, three 2p)
M (3s, five 3d, three 3p)

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7
Q

describe photoelectron spectroscopy

A

measure energy levels of e- in atoms/molecules

photons (fixed frequency) ionise e- from sample, energy of these e- measured

energy of photon = energy of ionised e- + ionisation energy of e-

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8
Q

how does quantum mechanics model an energy level?

A

as a wavefunction predicted by theory

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9
Q

what is the Born interpretation of a wave function?

A

small box hovering in space - probability of finding an e- in here proportional to the SQUARE of wavefunction at this point
(greater value, greater prob)

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10
Q

what is the square of the wave function known as?

A

the probability density

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11
Q

probability of e- being in box = (eqn)

A

(wave function)^2 x volume of box

hence why wf^2 known as prob DENSITY
mass = density x volume

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12
Q

what are spherical polar coordinates?

A

coordinates expressing position in space relative to nucleus
r (radius), θ (angle from z axis) and φ (angle from x axis)
angles are like latitude / longitude

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13
Q

method to calculate the total probability of finding the e- at a set distance from the nucleus

A

image a thin spherical shell radius r

use probability eqn (prob in shell = wf^2 x vol shell)

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14
Q

what is the radial distribution function (RDF)?

A

RDF = wf^2 x 4πr^2

where 4πr^2 is the eqn for the surface area of the sphere shell

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15
Q

eqn prob e- in shell using RDF

A

prob = RDF x thickness of shell

bc shell assumed to be thin, so volume of shell = surface area x thickness
RDF = wf^2 x surface area

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16
Q

what is the Bohr radius?

A

plot RDF vs radius for 1s orbital
from zero, peak at 53pm, tail to the right
maximum is the Bohr radius, the same as the lowest energy orbit in the Bohr model

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17
Q

three quantum numbers

A

principle (n)
orbital angular momentum (l)
magnetic (ml)

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18
Q

what does the principle quantum number determine, what values can it take?

A

positive integers n = 1, 2…
determines the ENERGY of the orbital

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19
Q

equation for energy of the orbital

A

En = -R/(n^2)
where R is the Rydberg constant

note that energy is NEGATIVE, measured from energy of ionised e-

20
Q

letters for n=1, 2, 3

A

K, L, M shells

21
Q

values the orbital angular momentum number (l) can take

A

integers from n-1 to 0

eg. n=2, l=1,0

22
Q

letters representing l=0, l=1, l=2

A

s, p, d respectively
hence 2p, 3d etc

23
Q

what do n and l tell us about the orbital

A

its three-dimensional shape

24
Q

values the magnetic quantum number can take

A

integers from +l to -l

eg. l=1, m=1,0,-1

25
Q

what does m tell us

A

the orientation of the orbital in space

26
Q

describe 1s orbital in terms of n, l, m

A

K shell n=1
hence l=0 and m=0
hence only one orbital, wave function is spherical, RDF has a single maximum at Bohr radius

27
Q

describe the 2s orbital in terms of n, l and m

A

in the L shell with n=2
l can be 0,1 so for 2s, l=0 and m=0

28
Q

define radial node in terms of wave function

A

a radial node occurs where the wave function is zero

so graph wf vs radius crosses the x axis

29
Q

where is the radial node of the 2s orbital located?

A

graph wave function vs Bohr radii shows curve crosses x-axis (so wf=0) at 2 Bohr radii

30
Q

describe the general shape of 1s and 2s orbitals (actually all s orbitals)

A

m=0 for both so shape doesn’t depend on θ or Φ
l=0 so no angular nodes
only depends on radius so spherical

31
Q

describe 2p orbitals in terms of quantum numbers

A

n=2, l=1 so m= -1, 0, 1
hence three possible orbitals which depend on angles θ and Φ

32
Q

define nodal plane / angular node

A

a plane in which the wf=0 at some angle

33
Q

the wf of an orbital is the product of two parts, called…

A

the angular part (with angle θ)
the radial part (generally ne^-mr)

34
Q

the n=2 orbital wave functions have the same ___ part but different ___ parts

A

the same radial part (2s and all 2p)
but different angular parts (2p)

35
Q

T or F: in hydrogen, the 2s and three 2p orbitals have exactly the same energy

A

T, because energy depends only of the value of principle quantum number, n

36
Q

define degenerate

A

distinct orbitals which have the same energy

37
Q

in what case will the 2s and 2p orbitals be degenerate?

A

In H which only has one e- present, the L shell has 4 degenerate orbitals
but in atoms w more than 1 e-, they are not

38
Q

the general rules for # of radial and angular nodes

A

number of angular nodes (nodal planes) = l
number of radial nodes = n - l - 1

hence total number of radial and angular nodes is n-1

39
Q

how many 3d orbitals are there?

A

five.
n=3, l=2 (l=0 is 3s, l=1 is 3p), so m= -2, -1, 0, 1, 2
hence five total

40
Q

what is orbital approximation?

A

make a multi-electron atom like a one-electron atom

multiple e-‘s mean e-e- repulsion
hence alter the nuclear charge to Z(eff) from actual value to “effective” value

41
Q

what two things does changing Z(eff) do?

A

affects energy of orbitals
affects SIZE of orbitals (inversely)

42
Q

what does the energy of an orbital depend on?

A
  1. Principle quantum number
  2. Effective nuclear charge (actual nuclear charge and e-e- repulsion)
43
Q

what is screening?

A

basically the inner electrons blocking the outer electrons and influencing the effective nuclear charge experienced

44
Q

what does it mean when the 2s is said to be more penetrating than the 2p?

A

higher probability of the 2s electron being inside the air occupied by 1s, hence penetrating the screen and experiencing a greater nuclear charge

45
Q

in general the ordering of the orbitals depends on …

A

the degree of penetration
with lower value of l being more penetrating and hence lower in energy

46
Q

generally, the polarity of a bond depends on …

A

the relative energies of the atomic orbitals of the two atoms involved

generally the lowest energy will end up with the partial negative charge, more electronegative

ELECTRONEGATIVITY IS A CONSEQUENCE OF ORBITAL ENERGIES

47
Q
A