Quantum Mechanics Flashcards

1
Q

What is quantum mechanics?

A

Molecular energies or the orientations of nuclear spins can only take discrete values
It predicts that the energy of a particle, such as an electron, can only take a discrete set of values, often called energy levels.
The position of a particle cannot be precisely predicted, only the probability that a particle has a given position can be calculated

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2
Q

What is classical mechanics

A

Predicts that the energy of an object can take any value
Energy varies continuously.
Used to predict the position of an object at any given time

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3
Q

What is a main axium (starting position) of quantum mechanics

A

In quantum mechanics every particle has a wavefunction (Ψ)

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4
Q

What does wavefunction tell us?

A
  • Contains all the information about the particle. If Ψ is known we can calculate the energy of the particle
  • Is a mathematic function of variables which describes the position of the particle, x, y, z
  • Gives a recipe for calculating the probability that the particle is in a small volume dV at a particular position
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5
Q

What is the born interpretation of the wavefunction

A

│Ψ(x, y, z)│² dV
Probability density is work out through squaring the wavefunction

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6
Q

Another axiom of quantum mechanics is the Schrodinger equation
What is it

A

The Strodinger equation allows us to find both the wavefunction and the energy levels for particles (e.g. electrons) in a given situation

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7
Q

Why does the form of the Schrodinger equation for a particle change

A

For a particular situation depends on the way in which the potential energy of the particle varies with position

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8
Q

An exact solution to the Schrodinger equation can only be found in a very few simply cases
Give an example

A

One example is an atom with a single electron - the hydrogen atom

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9
Q

What are atomic orbitals wavefunctions

A

The name for the wavefunction (Ψ) found by solving the Schrodinger equation for an atom with a single electron

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10
Q

What is the potential energy of a hydrogen atom

A

The negatively-charged electron is attracted to the positively-charged atomic nucleus by an electrostatic interaction
Therefore, the potential energy of the electron is proportional to -1/r
Where r is the seperation between the nucleus and the electron

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11
Q

When does potential energy become zero

A

As the seperation between the nucleus and electron becomes very large, the potential energy become zero

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12
Q

The magnitude of the potential energy of the electron is inversely proportionate to…

A

The seperation (r) between the nucleus and the electron
As seperation decreases, the electrostatic interaction become more favourable, resulting in a decrease in potenetial energy

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13
Q

Why would you say the 1s wavefunction has spherical symmetry

A

The value of the 1s wavefunction varies only with the separation of the electron from the nucleus regardless of direction, and so has spherocal symmetry

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14
Q

The wavefunction corresponding to the lowest energy is the 1s orbtial
Ψ₁s (r)= A₁s exp (-r/a₀)
What is A₁s and a₀

A

A₁s is a normalisation constant which ensures that the probability of finding the electron somewhere is equal to 1 (the electron is certain to be somewhere)
a₀ is a constant called the Bohr radius (52.9 pm)

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15
Q

The isosurface of a 1s orbital looks like this
How does wavefunction change across the isosurface

A

The wavefunction takes the same value at any point on the isosurface
The size of the iso-surface depends on the value of the wavefunction

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16
Q

What is another way we can determine the position of an electron

A

Use the radial distribution function P(r) to calculate the probability of finding the electron in a thin shell of radium (r) and thickness (dr)
This gives the probability of finding the electron at a distance (r) from the nucleus, regardless of direction
P(r)= 4πr²│Ψ(r)│²

17
Q

For the 1s orbital, the maximum probability of finding an electron occurs where

A

At the Bohr radius, a₀

17
Q

For the 1s orbital, the maximum probability of finding an electron occurs where

A

At the Bohr radius, a₀

18
Q

For atomic orbitals (AOs) there are three quantum numbers
How do quantum numbers differ across types of atomic orbtials

A

n = principle quantum number
l = orbital quantum number
ml = magnetic quantum number
Each orbital has a unique set of these quantum numbers

19
Q

In an atomic orbital with only 1 electron (¹H)
The energy of an atomic orbital in the hydrogen atom depends on?
How is this worked out?

A

Only the principal quantum number (n)
n = difference in wavelength of light from transition between energy levels
RH = 2.18 x 10⁻¹⁸

20
Q

The orbital energy is measured on a scale which takes its zero point as…

A

The situtation where the electron is infintely seperated from the nucleus (ionisation)
In this situation the energy of the electrostatic interaction within the nucleus is zero

21
Q

if n has a value of 2
What are the possible values of l abd ml
What do these values of ml imply about orbitals present

A

l = 0, 1
ml = -1, 0, +1
There are shells of degenerate orbitals (they have the same energy as one another) with a common* n *
e.g. in this case there are three 2p orbtials and a 2s orbital
as the l vaue increases, a new shell containing a new types of orbital occurs

22
Q

Why do we write the wavefucntion of a hydrogen atom in polar co-ordinates (r, θ, φ) rather than Cartesian ones (x, y z)

A

Since the hydrogen atom and the potential are spherically symmetrical it is convenient
In spherical polar coordinates each wavefunction cab be written as a productnof a radial part R, which only depends on radius and an angular part Y which only depends on orientation of φ and θ

23
Q

In general, the radial distribution function depends only on the radial part of the wavefunction
This can be found for non spherically symmetric orbitals using

A

P(r)= r²[R(r)]²

24
Q

For the spherically symmetrical 1s orbital the angular part = 1, so for a 1s orbtial the wavefunction is equal to

A

The radial part alone

25
Q

What is the L-shell

A

L-shell : the second innermost shell of electrons surrounding an atomic nucleus

26
Q

For the Radial Wavefunction for a 2s orbital, where is the radial node

A

The radial part of the 2s orbital passes through zero when the electron is 2a₀ from the nucleus
The zero crossing is known as a radial node
The radial part of the 2p orbital is always positive, so these orbitals do not have a radial node

27
Q

What does this comparision of the 1s, 2s and 2p corresponding radial distribution functions demonstrate

A

The L-shell, (2s + 2p) wavefunctions decay more slowly than the 1s wavefunction, and so the 2s and 2p orbitals spread into a larger region of space (more diffuse)

28
Q

Describe the iso-surface of the 2p wavefunctions

A

Each has a posititve lobe and a negative lobe
The wavefunction passes through zero between the lobes (this is shown by the pz orientation where wavefunction passes through the xy plane)

29
Q

What is the Aufbau Principle

A

States that the electrons in a multi-electron atom occupy the orbitals in the order 1s, 2s, 2p, 3s, 3p etc

30
Q

What is the Pauli Exclusion Principle

A

No two electrons in any system can have identical values for all 4 quantum numbers
It restricts the number of electrons within an orbital to 2 (ms = ±1/2)
meaning values for n, l, and ml must be different
Hence the electron must also have opposite spins

31
Q

What is Hund’s Rule

A

Every orbital in a subshell is singllaryly occupied with one electron before any one orbital is doubly occupied