Week 2 Flashcards

(40 cards)

1
Q

as you go further down the periodic table…

A

the elements will become increasingly radioactive, nucleus is too big

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

Electrostatic (Coulomb) repulsion

A

The repulsion between protons acts to push these nucleons apart over a long range

Intended to make a nucleus radioactive, unstable

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

The strong nuclear force

A

a short range attraction between all nucleons
Make stable

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

Radioactivity 1: In nuclides with too few neutrons…

A

the electrostatic repulsion overwhelms the strong nuclear attraction

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

Radioactivity 2: As the nucleus gets larger…

A

the long-range electrostatic repulsion between protons accumulates and eventually overwhelms the strong nuclear attraction.

Nuclides with M > 208 (e.g. Uranium) are unstable

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

Radioactivity 3: When there are too many neutrons…

A

the nucleus is also unstable.

This is explained by a nuclear form of quantum theory, the Nuclear Shell Model

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

Noble gases are very stable because…

A

they have a complete shell

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

alpha decay

A

lose 2 protons and 2 neutrons

α particle is simply a helium nucleus with mass number 4 and charge 2+

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

beta decay

A

1 neutron lost and 1 proton gained

β(or β−) is an electron ejected from the nucleus. One neutron is changed into a proton in this nuclear reaction to balance the charge.

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

positron decay

A

1 neutron gained and 1 proton lost

β+ is a positron ejected from the nucleus. One proton is changed into a neutron in this nuclear reaction to balance the charge

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

electron capture

A

1 neutron gained, protons the same

Electrons fall into lower energy states to fill the vacancy left by the captured electron. A proton combines with the electron, forming a neutron.
Mass number stays the same

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

neutron emission

A

Simple emission of a neutron, which changes M but leaves Z unchanged.

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

gamma emission

A

No change in M or Z is associated with γ-emission on its own.

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

nuclear stability depends on…

A

size of nucleus
(there are no stable nuclei heavier than Pb w/ A=208 and Z=82)

N:Z ratio
(near to 1, but “bends” towards more neutrons per proton as the nucleus gets larger)

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

bad uses of radiation

A

Radiation sickness/burns
Cancer
Weapons

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

good uses of radiation

A

Cancer therapy
Medical imaging

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

radiation is…

A

high energy and produced by radioactive decay and causes ionisation of matter by ejecting electron from atoms

18
Q

the ionisation of a single molecule needs

19
Q

how much energy in alpha radiation? (approx)

20
Q

how much energy in beta radiation? (approx)

A

1 to 0.05 MeV

21
Q

how much energy in gamma radiation? (approx)

22
Q

Why is radiation so bad for the body?

A

because the body is 50-70% water and reactions begin with water.

Water ionised to a cation and an electron

23
Q

Damage depends on 3 things…

A
  1. type of radiation
  2. length of exposure
  3. source of exposure
24
Q

internal exposure to radiation

A

Ingestion or inhalation. Alpha and beta are most dangerous. Most gamma radiation escapes the body

25
external exposure to radiation
alpha and beta **can't penetrate** through air and skin. **Gamma** radiation can penetrate skin - *more dangerous*
26
Sievert (Sv)
unit that measures **biological effect** of *radiation*
27
cancer therapy
*Focusing* ionising radiation onto the **tumour** OR Internal administration of a **radiopharmaceutical**
28
Radiation for imaging
Uses radiation (**gamma**) emitted from within the body to **map** the body Computer-assisted tomography can give **3D** reconstruction of the body
28
Technetium-99m imaging
Easily incorporated into many **drugs** Easily prepared from **Mo-99** Does **not** change its *chemistry* when it decays Emits only highly-penetrating **gamma** rays, not harmful alpha/beta particles
29
PET imaging
Uses radionuclide that emits positrons: positron emitters are proton rich Within the body, **positron** reacts with an **electron**, producing two high energy **gamma** rays, which are *detected* outside the body FDG is used to observe parts of the body that use high levels of glucose (tumours, brain etc.)
30
Light (photoelectric effect)
Light is electromagnetic radiation that has both **wave** and **particle** (photons) nature. The amount of **energy** (quantum) in each photon is determined by its **frequency**, ν (nu) or **wavelength**, λ (lambda).
31
Black-body radiation
Proposed that energy is **quantised**: **E = hν** (ν = frequency of oscillation, h = Planck’s constant)
32
Spectroscopic lines
**electrons** in *discrete* orbits Thus atom **cannot** lose energy continuously, but must do do in *quantum jumps* between different orbits Light emitted by an excited atomic gas consists of discrete wavelengths, not a continuous band.
33
Bohr model
postulated a set of **circular orbits** for electrons with specific, *discrete* **radii** and **energies** and that electrons could move in each orbit **without** radiating energy
34
Energies for H
values between −ER (n = 1) and −ER/4 (n = 2) **cannot** be observed as n *increases*, En approaches the energy of an unbound electron, or **0**
35
Problems with Bohr model
1. According to classical physics, revolving charged particles **radiate energy** 2. Bohr’s model could only explain the emission spectra of `single-electron` atoms. It failed to predict the spectra of multi-electron atoms. 3. Bohr could offer `no reason` why an electron should have discrete orbits or energies.
36
wavelength of a matter wave
**λ=h/mv** m is mass v is velocity h is Planck's constant
37
Planck's constant
**6.626** x 10^**-34** J s
38
Mechanics of waves
**Wave**-behaviour + **restricted motion** lead automatically to *discrete* energy levels or frequencies. Thus, the matter wave concept *explains* why electrons have **discrete energy levels**. No need for discrete orbits!
39
Classical vs. quantum
quantum - has **large scale** (goes to subatomic objects) - **wave** is particles (dual nature)