Quantum theory Flashcards

1
Q

quantum mechanics definition

A

which is the theory neededto describe the behaviour of individual atoms, molecules and the electrons theycontain.

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2
Q

Atomic orbitals

A

follows the laws of quantum mechanics

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3
Q

quantized

A

energy cannot take any level. it is restricted to a certain set of values, usually called energy levels,

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4
Q

location and quantum mechanics

A

we so not know precisely where a particle is located – all we can do is give the probability that a particle will be at a particular position. Different positions (coordinates)have different probabilities associated with them, so as a result it appears that the particle is ‘spread out’ over a region of space,

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5
Q

wave fucntion

A

variable quantity that mathematically describes the wave characteristics of a particle

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6
Q

wave function symbol

A

psi.

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7
Q

atomic spectra

A

the spectrum of frequencies of electromagnetic radiation emitted or absorbed during transitions of electrons between energy levels within an atom.

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8
Q

The principal quantum number,

A

n, describes the energy of an electron and the most probable distance of the electron from the nucleus.
n =1,2,3,4

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9
Q

The azimuthal number L

A

The azimuthal quantum number describes the shape of a given orbital.

the symbol ‘l’.

A value of the azimuthal quantum number can indicate either an s, p, d, or f subshell which vary in shape.

n–1

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10
Q

§ Magnetic quantum number

A

how many orbitals are there in a type.

it describes a specific orbital amongst. a particular set.

n–1
l 0=1 0
l 1=3 -1, 0, 1
l 2= 5 ………
l 3 = 7…………………

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11
Q

Spin quantum number

A

0.5/-0.5

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12
Q

Spin quantum number

A

0.5/-0.5

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13
Q

orbitals that are further away from nucleus

A

have higher potential energy.

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14
Q

Pauli Principle

A

: No two electrons in an atom can have all four quantum
numbers the same. What this means is that any orbital (defined by n, l
and ml
) can have a maximum of two electrons, one with ms
= +1/2 and
one with ms
= –1/2.

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15
Q

Aufbau Principle:

A

Electrons are placed in the lowest energy orbitals
available. For a given value of n, s lower than p lower than d, i.e. 3s < 3p
< 3d except in the special case of hydrogen where energy depends only
on n.

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16
Q

Hund’s Rule:

A

For degenerate (same energy) orbitals, electrons start by
going one into each.

17
Q

why does 4s fill before 3d

A

We say that the 4s orbitals have a lower energy than the 3d, and so the 4s orbitals are filled first.

17
Q

why does 4s fill before 3d

A

We say that the 4s orbitals have a lower energy than the 3d, and so the 4s orbitals are filled first.

18
Q

orbitals

A

probabiltiy where an electrons is found

19
Q

1s

A

sphere

20
Q

2s

A

larger sphere

21
Q

valence electron

A

, feels a positive charge less
than the full nuclear charge.

22
Q

Effective Nuclear Charge,

A

Z*
where Z* = Z – S.
Z is the actual nuclear charge (the atomic number) and S is a shielding constant.

23
Q

effective nuclear change

A

Z* increases substantially across a row and increases down a group.

24
Q

ionisation energy

A

is a endothermic reaction. energy is needed to break bonds.

25
Q

why does effective nuclear charge increase along row

A

there are more protons

26
Q

why does effective nucleur charge decrease down group

A

greater shielding and distance

27
Q

why does effective nuclear charge decrease

A

‘Kinks’ in the graph at B/Al reflect change in orbital type: p instead of s

28
Q

hunds rule effective nuclear charge

A

‘Kinks’ in the graph at O/S reflect electrons now paired in an orbital.
Hund’s Rule.

29
Q

electronegativity

A

‘the ability of an atom to attract electron density
towards itself in a molecule’

30
Q

ionisation
energies

A

energyit takes to become 1+ cation ions gaseous

31
Q

,

A