Topic 7: Atomic and nuclear physics Flashcards

You may prefer our related Brainscape-certified flashcards:
1
Q

Describe a model of the atom that features a small nucleus surrounded by electrons

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

How are electrons kept in orbit?

A

Electrons are kept in orbit around the nucleus as a result of the electrostatic attraction between the electrons and the nucleus.

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

Describe the Geiger-Marsden experiment

A
  1. Beam of alpha particles aimed at thin gold foil
  2. Passage through foil detected
  3. Expected that particles would pass straight through
  4. Some of the particles emerged at different angles and some reflected back
  5. It was realised that the positively charged alpha particles were being repelled and deflected by a tiny concentration of negative charge in the atom
  6. As a result, the plum pudding model was replaced by the nuclear model
  7. Rutherford concluded that the atom must have a tiny nucleus with electrons whizzing around it and that the nucleus had a positive charge to balance the negative charge of the electrons
  8. He thought that almost the whole mass of an atom was concentrated in the nucleus, so it must be incredibly dense
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

Outline one limitation of the simple model of the nuclear atom

A

Accelerating charges are known to lose energy. If the orbiting electrons were to lose energy they would spiral into the nucleus. The Rutherford model cannot explain how atoms are stable.

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

Outline evidence for the existence of atomic energy levels.

A
  1. Rutherford model was developed further by Niels Bohr who suggested that the electrons orbit the nucleus rather like a planet orbits the sun
  2. Radius of Bohr’s electrons depended on the energy they had
  3. He also suggested that they could only move in certain orbits: when the electrons moved from a high energy state to a lower energy state they emitted a photon of light and the frequency of the light depends on the difference between the energy levels
  4. As there are a fixed number of energy levels only a few wavelengths of light are given out, resulting in a line spectrum
  5. Each individual element has distinct energy levels and therefore the emission spectra can be used to identify them
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

Define: nuclide

A

An atom characterised by its proton number and atomic number:

AZX

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

Define: isotope

A

Nuclei with the same atomic number but different mass number (due to a different number of neutrons)

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

Define: nucleon

A

A proton or a neutron making up a nucleus

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

Define: nucleon/mass number, A

A

The number of nucleons in a nucleus

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

Define: proton/atomic number, Z

A

The number of protons in a nucleus.

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

Define: neutron number, N

A

The number of neutrons in a nucleus

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

Describe the interactions in a nucleus

A
  • According to our knowledge of electrostatics a nucleus should not be stable; protons are positive charges so should repel each other and so there must be another force in the nucleus that overcomes the electrostatic repulsion and hold the nucleus together
  • This force is called the strong nuclear force
  • Strong nuclear forces must be very strong to overcome the electrostatic forces and must also have a very small range as they are not observed outside of the nucleus
  • Neutrons have some involvement in strong nuclear forces: small nuclei have equal numbers of protons and neutrons, but larger nuclei, which are harder to hold together, have a greater ratio of neutrons to protons
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

Describe the phenomenon of alpha decay.

A
  • Alpha decay is one process that unstable atoms can use to become more stable. During alpha decay, an atom’s nucleus sheds two protons and two neutrons in an alpha particle.
  • Since an atom loses two protons during alpha decay, it changes from one element to another.
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

Describe the phenomenon of beta decay.

A

Beta particles are electrons emitted from the nucleus. The electron is formed when a neutron decays. At the same time, another particle is emitted called an antineutrino.

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

Describe the phenomenon of gamma decay.

A

Gamma rays are unlike the other two radiations in that they are part of the electromagnetic spectrum. After their emission, the nucleus has less energy but its mass number and its atomic number have not changed. It is said to have changed from an excited state to a lower energy state.

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

Effect on photographic film of alpha, beta and gamma radiation

A

Alpha - yes

Beta - yes

Gamma - yes

17
Q

Approximate number of ion pairs produced in air for alpha, beta and gamma radiation.

A

Alpha - 104 per mm travelled

Beta - 102 per mm travelled

Gamma - 1 per mm travelled

18
Q

Typical material needed to absorb alpha, beta and gamma radiation.

A

Alpha - 10-2 mm aluminium; piece of paper

Beta - a few mm aluminium

Gamma - 10 cm lead

19
Q

Penetration ability of alpha, beta and gamma radiation

A

Alpha - low

Beta - medium

Gamma - high

20
Q

Typical path length in air of alpha, beta and gamma radiation

A

Alpha - a few cm

Beta - less than one m

Gamma - infinite

21
Q

Speed of alpha, beta and gamma radiation

A

Alpha - about 107 m s-1

Beta - about 108 m s-1, very variable

Gamma - 3 X 108 m s-1

22
Q

Outline the biological effects of ionising radiation.

A

At the molecular level, an ionisation could cause damage directly to a biologically important molecule such as DNA or RNA. This could cause it to cease functioning. Alternatively, an ionisation in the surrounding medium is enough to interfere with the complex chemical reactions called metabolic pathways taking place.

Molecular damage can result in a disruption to the functions that are taking place within the cells that make up the organism. As well as potentially causing the cell to die, this could just prevent cells from dividing and multiplying. On top of this, it could be the cause of the transformation of the cell into a malignant form.

As all body tissues are built up of cells, damage to these can result in damage to the body systems that have been affected. The non-functioning of these systems can result in death. If malignant cells continue to grow, then this is called cancer.

23
Q

Explain why some nuclei are stable while others are unstable.

A
  • The stability of a particular nuclide depends greatly on the numbers of neutrons present.
  • For small nuclei, the number of neutrons tends to equal the number of protons.
  • For large nuclei there are more neutrons than protons.
  • Nuclides above the band of stability have too many neutrons and will decay with either alpha or beta decay.
  • Nuclides below the band of stability have too few neutrons and will tend to emit positrons
24
Q

Describe the process of radioactive decay

A

Radioactive decay is a random process and is not affected by external conditions. For example, increasing the temperature of a sample of radioactive material does not affect the rate of decay. This means that there is no way of knowing whether or not a particular nucleus is going to decay within a certain period of time. All we know is the chances of a decay happening in that time.

Although the process is random, the large numbers of atoms involved allows us to make some accurate predictions. If we start with a given number of atoms, then we can expect a certain number to decay within the next minute. If there were more atoms in the sample, we would expect the number decaying to be larger. On average, the rate of decay of a sample is proportional to the number of atoms in the sample. This proportionality means that radioactive decay is an exponential process. The number of atoms of a certain element, N, decreases exponentially over time.

25
Q

Define: radioactive half life

A

The time taken for half the number of nuclides present in a sample to decay. The time taken for the rate of decay of a particular sample of nuclides to halve.

26
Q

Define: artificial transmutation

A

The conversion of one isotope to another. This can be done through a nuclear reaction whereby a nucleus is bombarded with a nucleon, an alpha particle or another small nucleus.

27
Q

Define: unified atomic mass unit

A

One twelfth the mass of a carbon-12 atom.

28
Q

Define: mass defect

A

The difference between the mass of a nucleus and the mass of its component nucleons

29
Q

Define: binding energy

A

The amount of energy that is released when a nucleus is assembled from its component nucleons.

30
Q

Define: binding energy per nucleon

A

Total binding energy for the nucleus divided by the total number of nucleons

31
Q
A