7 Nuclear Physics Flashcards

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1
Q

when an electron moves from a higher energy state to a lower energy state…

A

photons are emitted

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2
Q

describe the emission spectra

A

an electron transfer to a lower energy level and emit photon

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3
Q

Isotopes tend to be more unstable because

A

they have an imbalance of protons and neutrons

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4
Q

state and define the two main characteristic of radioactive decay

A
  1. spontaneous: not influenced by external factors
  2. random: cannot predict the time of decay
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5
Q

Explain the relationship between penetrating power and ionizing ability.

A

Alpha = most ionising = lose energy quickly = least penetrating, can be stopped by paper/skin

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6
Q

explain this Z-N diagram

A

For Z<20, proton number = neutron number → stable

For Z>20, neutron-proton ratio increases because as proton number increases, the electrostatic repulsion becomes very strong and more neutron is required to ‘shield’ the protons from each other and bind the nucleons together → unstable

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7
Q

examples of radiation detectors

A
  • Photographic film
  • Geiger-Muller (GM) tubes
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8
Q

describe beta-minus decay

A

n → p + e-

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9
Q

describe beta-plus decay

A

p → n + e+

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10
Q

α particles are emitted by nuclei that

A

have too many nucleons

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11
Q

define half life

A

the time taken for the undecayed nuclei to halve

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12
Q

define mass defect (Δm)

A

the difference in mass between separated and combined nucleons
(mass ⇒ binding energy)

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13
Q

convert mass defect to binding energy

A

ΔE = Δm x 931.5 (MeV)

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14
Q

convert MeV to J

A

1 e = 1.6 x 10^-19 C
1 eV = 1.6 x 10^-19 J
1 MeV = 1.6 x 10^-13 J

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15
Q

define nuclear fission

A

an unstable atom absorbs neutrons and becomes unstable → the nucleus splits into two daughter nuclei; releases energy

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16
Q

What happens to the binding energy after fission/fusion
1) per nucleon
2) total

A

binding energy per nucleon increases as the nuclei becomes more stable.
→ total binding energy also increases

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17
Q

why do lighter nuclei undergo fusion while heavier nuclei undergo fission?

A

small mass → less protons → attractive nuclear forces between nucleons > repulsive electrostatic forces between protons → fuse
(vice-versa for large mass)

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18
Q

advantages of fusion

A

Reactants readily available in ocean; no harmful by-product

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19
Q

Moderator

A

slows down neutrons so they can be captured by a U-235 nucleus

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20
Q

Heat Exchanger

A

heat water to steam to be used to turn turbines and produce electricity

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21
Q

Chain reaction

A

A self-sustaining nuclear reaction where U-235 fission releases more neutrons and trigger more fissions… this is when the rate of neutron production ≥ the rate of neutron lost

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22
Q

what is quark?

A

fundamental particles that make up other subatomic particles such as protons and neutrons

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23
Q

define baryon

A

consists of 3 quarks;
baryon number = 1

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24
Q

what are the quark configurations of proton and neutron?

A

proton: uud
neutron: udd

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25
Q

why does proton have the longest half-life of all baryons?

A

lightest baryon → most stable

26
Q

list the 4 fundamental interaction forces in order of strengths

A

strong > electromagnetic > weak > gravity

27
Q

which interaction force is responsible for the radioactive decay of atoms?

A

weak

28
Q

define exchange particles

A

virtual particles that mediate the a fundamental force between interacting particles

29
Q

Explain how atomic spectra provide evidence for the quantisation of energy in atoms.

A

E=hf=h(c/λ), since atomic spectra consists of discrete wavelengths, atoms must contain discrete/quantised energy levels

30
Q

describe the absorption spectra

A
  1. Electrons absorb photons and become ‘excited’
  2. Electrons de-excite and re-emit the photons but in all directions, so these wavelengths appear black in the direction of the observer.
31
Q

define radioactive decay

A

an unstable atomic nucleus becomes more stable by emitting a particle (alpha, beta) or a wave (gamma)

32
Q

state the nature of the 3 radiation

A

alpha = He nucleus (2p, 2n)

beta = high speed electron

gamma = EM radiation

33
Q

what materials stop the 3 types of radiation

A

alpha = paper

beta = thin aluminum foil

gamma = thick lead

34
Q

define background radiation

A

low level of radiation in our surroundings at all times

35
Q

state the sources of background radiation

A

radon gas, rocks, food, cosmic rays

36
Q

determine the background radiation

A

where the line plateaus

37
Q

β- particles are emitted by nuclei that

A

have too many neutrons

38
Q

β+ particles are emitted by nuclei that

A

have too many protons

39
Q

γ particles are emitted by nuclei that

A

have too much energy

40
Q

define the activity of a redioactive substance

A

number of decays per second

A = dN/dt = - λN

41
Q

define binding energy (ΔE)

A

the energy to separate the nucleons in a nucleus

42
Q

Calculate the binding energy per nucleon, in MeV, for K-40 (19 protons)
Nuclear mass = 39.953548 u
Mass of one neutron = 1.008665 u
Mass of one proton = 1.007276 u

A
  1. ∆m = nuclear - (p+n)
  2. convert u to kg!!
  3. ∆E = ∆mc²
  4. ∆E per nucleon (divide by 40)
  5. convert J to MeV!!
    → ∆E per nucleon = 8.594 MeV
43
Q

Draw the graph of mass number against binding energy per nucleon, including the main features

A

mass

44
Q

define nuclear fusion

A

two small nuclei join to produce a larger nucleus; release energy

45
Q

In nuclear fission/fusion, how is the mass of the product compared to the mass of the reactant? Why?

A

mr > mp because part of the mass of the reactant is converted into energy.

46
Q

In the graph of mass number (A) against B.E. per nucleon, what does the steeper graident for smaller A show?

A

fusion releases more energy (B.E.per nucleon increases more)

47
Q

difficulty in making a fusion reactor

A

Very difficult to create heat and pressure that exists in the sun → need to input more energy than what comes out

48
Q

Control Rod

A

absorbs neutrons to control the rate of reaction

49
Q

Enrichment

A

increasing the % of U-235 ( more reactive/fissionable isotope) in a fuel used in a nuclear power station

50
Q

Critical Mass

A

the minimum mass of nuclear fuel needed to sustain a chain reaction

51
Q

why does nuclear fusion need high temperature?

A

need lots of energy to overcome the electrostatic repulsion between positively charged nuclei

52
Q

define meson

A

a quark and an antiquark pair

53
Q

what is lepton?

A

fundamental particles that cannot be broken down further (eg. electron)

54
Q

how do you determine whether a particle interaction can occur?

A

check if QBLS are conserved
Q = charge
B = baryon number
L = lepton number
S = strangeness

55
Q

The strong force applies only to particles made up of

A

quarks

56
Q

The electromagnetic force only applies tp

A

particles with charge

57
Q

The gravitational force only applies to

A

particles with mass

58
Q

quark confinement states…

A

it is impossible to observe a free quark in isolation because more particles will be created when you try to separate a pair of quarks

59
Q

draw the Feymann diagram for beta-plus decay

A
60
Q

Mg-27 nuclei decay by β- to form Al-27. Explain why there’s a difference between the energy released in the decay and the total kinetic energy of beta particles and gamma rays.

A

another particle (anti-nutrino) is emitted

61
Q

Fluorine (18,9) can be created when a proton traveling at high speed interacts with an oxygen nucleus (18,8). Explain why the proton must be traveling at high speed for this process to occur.

A

+ve nucleus repels proton;
proton must be close to nucleus for nuclear force to be effective (high electric potential energy);
so the proton needs high initial kinetic energy

62
Q

range of wavelength for visible light

A

380 to 700 nm