InChem foundation

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277 Terms

1
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What does the plum pudding model look like and consist of?

Positive mass with small, negative electrons embedded

2
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What does the Rutherford atom look like and consist of?

Positive nucleus with negative electrons orbiting nucleus

3
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What is the problem with the Rutherford atom?

All electrons are equal contradicting idea of atomic emission spectra

4
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What is the atomic emission spectra?

When atoms are given a lot of energy & light is emitted

5
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What is the Bohr atom?

Same as Rutherford atom but electrons are at different distances from the nucleus

6
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How much energy do electrons closer to the nucleus have?

More stable & lower energy since they are more tightly bound

7
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What are transitions?

When electrons absorb energy and it moves from a lower energy level (ground state) to a higher energy level (excited state)1

8
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What do emission lines represent?

Energy levels in atom

9
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What is the formula of showing energy in a quantum level?

En = k / n2

n = Quantum number e.g n=1 etc

k = Plancks constant

10
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What is the problem with the atomic emission spectra?

-Works for hydrogen, but not for heavy atoms

  • Doesn't explain periodic properties

-Bohr model doesn't explain everything

11
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What is the deviation for De Broglie's equation?

knowt flashcard image
12
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What is the wave particle duality?

Subatomic particles can act as both particles & waves (electrons can diffract)

13
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What is Heisenberg's uncertainty principle?

Uncertainty associated with momentum

14
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Why is uncertainty associated with momentum

To see electron, light waves reflect from spherical electron & meets eye

  • Light wave adds energy & changes momentum of electron

15
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What is the problem with Bohr's atom?

Shows orbit which gives electron well defined orbit, however electrons do not exist in orbits

16
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What is used instead of orbits?

Orbitals = Area of space around the nucleus where electrons are seen (probability distributions)

17
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Why must wavelengths be in integral number when electron moves in circular manner?

Destructive interference may occur (λ n = 2 pi r)

18
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What is schrodingers equation?

Describes how wave function evolves overtime?

19
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What does the wave function describe?

Amplitude of x, y or z (only applies to ELECTRONS)

20
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What does wave function^2 represent?

Probability density

21
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What are the components of wave function?

Wave function = Rn1 (r) x Y 1 m1

n1 & m1 = Quantum numbers

Y = Angular wave function (Direction)

22
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What is the n (principal) quantum number?

Includes positive integer values (0 not included)

e.g = n=1 ,2,3,4 etc

23
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What does n (principal) quantum number determine?

Size of orbital therefore energy

24
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What is L (Azimuthal) quantum number?

-Known as angular momentum

Includes positive integer values (0 included) up to a max of n -1

e.g = n=4 L can be 0,1,2 or 3

25
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What does L (Azimuthal) quantum number determine?

Affects shape so no changes in energy

26
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What is the mL quantum number?

-Known as magnetic quantum number

-Includes positive integer values (0 included) between -L & +L values

e.g = At L=2 can be -2,-1, 0 ,1,2

27
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What does mL quantum number determine?

Orientation of orbital

28
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How do you name orbitals?

L = 0 -> S

L = 1 -> p

L = 2 -> d

L= 3 -> f

L = 4 -> g

-Letter code preceded by principal quantum number e.g n=3 & L=1 so 3p orbital

29
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What is the radial wavefunction?

R = Function of distance from nucleus (r)

-R never goes to 0 as r -> infinity

30
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What is the Bohr radius?

Probable distance of electron from nucleus for H atom in ground state

31
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What is irrelevant for negative values of R?

-Electron probability as square of negative values give out positive

-Not relevant to electrostatic charges

32
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What is negative values of R important for?

Bonding

33
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What are radial distribution functions (RDF)?

Total probability electron will be found at given distances from nucleus regardless of electron

34
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What are the limitations of using wavefunction^2?

Only gives probability of finding electron at a single point

35
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How do you find RDF?

Probability of electron being at r x number of locations at r

36
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What happens if n (orbital size & energy) increases?

Area of max probability (density) increases

37
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What is boundary surface?

Where there is 90% probability of finding an electron.

38
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When is boundary surface used?

When there is a small probability of finding an electron far away from nucleus

39
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What are radial nodes?

Distances with 0 probability

40
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How do you find number of radial nodes?

n - L -1

41
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What is angular wavefunction dependent on?

L & ml only (no n)

42
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What shape do ns orbitals give off?

Spherical shape

43
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What is L=0 (ml 0) name?

ns (s orbitals)

44
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What is L=1 (ml can be -1,0,+1) name?

np orbitals (p orbitals)

45
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What shape do np orbitals give off?

Dumbell shape

46
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What is l=3 (ml -3,-2,-1,0,1,2,3) name?

nf (f orbitals)

47
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What shape is nf orbitals?

A lot more angular nodes

48
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What are angular nodes?

Planes with 0 electron probability

49
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What are orbital shapes independent of?

n (orbital size)

50
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What is l=2 (ml is -2,-1,0,1,2) name?

nd (d orbital)

51
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What shape is nd orbitals?

knowt flashcard image
52
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What does V (potential energy) in Schrodingers equation include?

Sum of electron attraction & repulsion

53
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Why can Schrodingers equation only be applied to the H atom and carbocations with 1 electron?

No electron repulsion in H atom (1 electron only)

54
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Why can't Schrodingers equation be applied to atoms with more than one atom?

Location of electrons must be seen for atoms with more than one electron

55
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How do you make it so Schrodingers equation can be used for atoms with more than one electron?

-Use H atom (or carbocations with one electron) as all orbitals have similar shapes

-Orbital energies vary depending on effective nuclear charge

56
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What quantum number(s) do orbital energies depend on now for atoms with more than one electron?

n & l (energy, size & shape)

57
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Why do electrons in orbitals with larger n quantum number have higher energy?

They have probability distribution further from the nucleus & experience less nuclear charge so are less tightly bound

58
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Why do electrons in orbitals with smaller n quantum number have lower energy?

Lower probability distribution from nucleus & experience greater nuclear charge so are more tightly bound

59
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What is the shielding effect?

When outer electrons feel lower effective nuclear charge so have higher energy

60
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Why is s<p<d<f in terms of energies?

-In RDF graph, 2s has a residual maximum (2 peaks)

-So 2s penetrates closer to nucleus than 2p electrons so experiences greater nuclear charge

61
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Why do orbital energies decrease with increasing Z (atomic number)?

Electrostatic attraction of electron increases

62
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Why does 4s become more penetrating for K & Ca?

As Z increases, 4s becomes more penetrating

-> Stronger nuclear charge = Energy decreases

63
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What is electron penetration?

How close an electron can get to the nucleus

64
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Why does 3d have lower energy than 4s from Sc onwards?

Sufficient electrons

65
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What is the Afbau principle?

"Add 1 proton, 1 electron & some neutrons to orbital of LOWEST ENERGY available"

66
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What is ms quantum number?

Spin quantum number

-> Have values of +1/2 or -1/2

67
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What is Pauli exclusion principle?

No 2 electrons in any system can have identical values for all FOUR quantum numbers

-> Values of ms must be different (Must have opposite spins)

68
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What is Hund's rule?

Most stable state is one with identical or parallel spins

->Otherwise repulsion between electrons may occur

69
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What are valence electrons?

Incomplete orbitals with higher energy & are affected by chemical reactions

70
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What are core electrons?

All orbitals with specific quantum number are full

-> e.g = 1s2 for He to F

71
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Why are full & half filled shells more stable in neutral atoms?

Electron repulsion is minmised

72
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What is periodicity?

Similar chemical properties

73
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Why does periodicity occur?

Valence orbitals

74
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How does electron fill for transition metals?

4s always empties before 3d

75
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Who first drafted the periodic table?

Mendeleev

76
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What did Mendeleev do?

Ordered periodic table by increasing atomic weights (relative atomic masses)

77
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What did Mosely discover?

Periodic table instead ordered by increasing atomic numbers -> Defines periodic table

78
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What is the structure of the periodic table?

ns2 np6 = Noble gases -> fully filled shells

ns1 = Group 1

ns2 = Group 2

ns2 np5 = Group 17 metals

ns2 np4 = Group 16 metals

ns2 np3 = Group 5 metals

79
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What are the main group elements?

  • s- block -> groups 1&2

-p- block -> groups 13-18

80
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What are transition elements?

Incomplete d-orbitals is either metal, compound or complex

81
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What are NOT transition metals?

Zn, Cd & Hs

82
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What are actinides or actinoids?

Partially filled 5f orbitals

83
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What are lathanides or lathanoids?

Partially filled 4f orbitals

84
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What are some multi-electron system rules?

-Same quantum numbers as hydrogen

-Same angular functions as hydrogen

-Radial functions similar to hydrogen, but contracted of increased nuclear charge

85
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Why are electrons placed far apart as possible?

Minimizes colombic (electrostatic) repulsion

86
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Are parallel spins in an electron more unstable or stable?

Stable

87
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What is the formula for electron energies in multi-electron systems?

E = -Rn hc Z^2 / n^2

88
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What is the effective nuclear charge?

Electron experiences less nuclear charge than full nuclear charge because of shielding

89
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What does shielding from other electrons depend on?

n (principal quantum number)

90
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What does penetration refer to?

Electron density. Electrons in orbitals have different wavefunctions and RDF

91
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Why does 2s get filled before 2p?

-2p has no radial node

-2s is less shielded of radial node so experiences greater nuclear charge & lower energy

So 1s shields 2p more than 2s

92
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Why is 4s filled before 3d?

-4s has 3 radial nodes (n-L-1)

-3d max closer to nucleus than 4s

93
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What does effective nuclear charge depend on?

Which shell electron is in -> Valence electrons in 3s experiences smaller nuclear charge than 1s of shielding

94
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What is Slater's rules?

Effective nuclear charge (Zeff) = Z - S

-Z = Actual nuclear charge

-S = Shielding constant

95
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Why doesn't perfect shielding exist?

-Electrons with same n contribute to 0.35 to s (shielding constant) ->Not much

-Electrons with 1 below n contribute to 0.85 to s -> Better shielding

-Electrons with low n contribute 1 to s -> Perfect shielding

96
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What is ionisation energy?

Sufficient energy required to detach one or more electrons from a gaseous atom, molecule or ion to form one gaseous ion

97
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Are ionisation energies always positive?

Yes

98
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What happens to energy required for second,third,fourth etc ionisation energies?

Increases each time

99
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What are the general trends for first ionisation energy?

-General increases across period

-General decreases down the group

100
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Why does first ionisation energy decrease down a group?

Increasing principal quantum number, energy required to remove electron decreases. However, no dramatic decrease of shielding