quantum mechanics Flashcards

1
Q

what is the rydberg equation?

A

v(frequency) = Rh [1/n (initial) ^2 - 1/n (final)^2 ]

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

what is the rydeberg equation used for?

A

to calculate the frequency of light when an electron moves form one orbital to another.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

what does n (initial) equal in the Balmer series

A

2

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

what does n (initial) equal in the Paschen series

A

3

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

what does n (initial) equal in the Lyman series

A

1

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

what type of light is used for the Lyman series

A

ultra violet

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

what type of light is used for the Balmer series

A

visible

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

what type of light is used for the paschen series

A

infrared

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

what happens if you are able to fully remove an electron from an atom (move it up an infinite number of shells.)

A

the n (final) becomes infinity, any number over infinity is 0. (this is the same thing as ionisation energy.)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

when the Rydberg equation to calculate the ionisation energy, the infinity should go _____ and the second value should be ______

A

first, stated in the question

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

what is the de Broglie equation?

A

wavelength = h/mv (velocity)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

when would you use the de Broglie equation ?

A

when calculating the wavelength of a moving object

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

what does the Heisenberg uncertainty principle state ?

A

it is impossible to predict both the precise position and momentum of an object. - the more precise that we know the of the location, the more uncertain the momentum will become and vice versa.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

what is the equation for the Heisenberg uncertainty principle?

A

delta p . delta q >= h/4pi

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

how do you calculate the change in momentum ?

A

since p=mv
delta = m . deltav

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

what element is the schrodinger equation used for and why?

A

hydrogen, as it only has 1 electron.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
17
Q

what does H^ stand for and what does it hold?

A

the Hamiltonian operator, and it holds all the info on the conditions of the atom.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
18
Q

what is the Schrödinger equation

A

H^ Y(wave function symbol) = E Y( wave function symbol)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
19
Q

what is the equation (linked to the Schrödinger equation), which helps us find the energy for the different hydrogen orbitals?

A

En = - hR/n^2

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
20
Q

what is an orbital?

A

an orbital is the region of space defined by the wave function

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
21
Q

what does the radial wavefuntion describe ? [R(r)]

A

the distance of an electron from the nucleus of an atom

22
Q

what does R(r)^2 stand for

A

the radial probability density

23
Q

what does the radial probability density show us ? [R(r)^2]

A

The probability of finding the electron at a point located distance r from the proton.

(This is important to use as a square number can never be negative. )

24
Q

what is the equation for the radial distribution function?

A

4pi(r)^2R(r)^2

25
Q

draw the graph of R(r) for a 1s orbital

A

exponential decay from 1

26
Q

draw the graph of R(r) for a 2s orbital

A

exponential decay from 1 and a dip below the x axis.

27
Q

draw the graph of R(r) for a 2p orbital

A

starting from 0 straight up to 1, then an exponential decay back to 0.

28
Q

draw the graph of R(r) for a 3s orbital

A

exponential decay from, a dip below the x axis and a hump above the x axis.

29
Q

draw the graph of R(r) for a 3p orbital

A

starting from 0 straight up to 1, then an exponential decay back to 0, with an dip below the x axis

30
Q

draw the graph of R(r) for a 3d orbital

A

same as 2p, but a less steep line up to 1 from the origin.

31
Q

what do the graphs look like for R(r)^2

A

in tetxbook

  • s starts from 1
    never drops below 0
32
Q

draw the graphs for the radial distribution function against r

A

in textbook

  • all start from origin
  • extra waves are smaller before the big wave
  • never drops below 0
33
Q

when does a node exist?

A

where there is a 0% chance of finding an electron.

where R(r)=0

34
Q

what helps you determine the number of radial nodes?

A

n - l - 1 = number of radial nodes

35
Q

where there is no nodes there is ….

A

0 probability of finding an electron

36
Q

what helps you determine the number of angular nodes?

A

It is equal to the value of l

37
Q

draw the d xy orbital

A

in between the x and y axis

38
Q

draw the d yz orbital

A

in between the z and y axis

39
Q

draw the d xz orbital

A

inbetween the x and z axis

40
Q

draw the x^2 - y^2 orbital

A

lies on the x and y axis

41
Q

draw the z^2 orbital

A

p orbital along the z axis and a ring around the centre

42
Q

what is the Pauli exclusion principle

A

No 2 electrons in the same atom can have the same 4 quantum numbers.

43
Q

what is aufbaus principle

A

orbitals much be filled in order of increasing energy

44
Q

what is hunds rule

A

When filling a set of degenerate orbitals, electrons are added with parallel spins to different orbitals.

45
Q

for what elements is hunds rule broken

A

chromium and copper

46
Q

what is the order of better shielding

A

s>p>d>f

47
Q

how do you find the total nuclear charge on a nucleus

A

the number of protons

48
Q

draw a 3p orbital

A
49
Q

draw a Pz orbital

A

only side on one

50
Q

strong s-p mixing occurs when s and p have ____

A

similar energies - elements bonding up to carbon is normally considered to have strong s-p mixing