Nuclear physics Flashcards

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1
Q

Nucleon

A

particle in the nucleus

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2
Q

Atomic number (Z)

A

number of protons

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3
Q

N

A

number of neutrons

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4
Q

Mass number

A

protons and neutrons

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5
Q

Nuclide

A

a particle with a particular mass number

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6
Q

Isotopes

A

nuclides of the same element, same number of protons but different neutrons

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7
Q

evidence for isotopes

A

bainbridge mass spectrometer;charged atoms are fired at a specific velocity passed by an opposite plate and landing at different places reveals having different isotopes

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8
Q

Interactions in a nucleus

A

Coulomb interactions and nuclear interactions

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9
Q

Coulomb interactions

A

A charged particle will never enter the nucleus because as the distance to it reached 0, then the repulsion would be infinitely large.

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10
Q

Nuclear interactions

A

Where the coulomb repulsion is overcome, as on sun, but much larger gravities.

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11
Q

Stability of nuclei

A

if strong force and coulomb repulsion are balanced; if not, unstable
for it to be stable neutrons must be ≥ number of protons (because coulomb force goes further than strong force)

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12
Q

unified atomic mass unit

A

1/12 of the mass of a carbon-12 atom

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13
Q

Energy-mass equivalence

A

mass and energy are equivalent in that a change in mass can also be regarded in the same change in energy
E=mc^2

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14
Q

MeVc^-2

A

equivalent to 1 atomic mass unit

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15
Q

mass defect

A

difference in mass between mass of nucleus and the mass of separate nucleons

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16
Q

nuclear binding energy

A

energy required to separate the nucleus into different components (MeV)
E=mc^2 (binding energy= mass defect* c^2)

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17
Q

radioactive decay

A

when an unstable nucleus emits an alpa or beta particle or gamma ray photon resulting in a daughter nucleus which is more stable

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18
Q

characteristics of radioactive decay

A

random and spontaneous (with less nuclei, probability does not change and the number of decays reduce)

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19
Q

half-life

A

time taken for the initial activity of the radioactive sample to halve

20
Q

radioactive decay law

A

the rate of decay is proportional to the number of undecayed nuclei (dN/dt=-λ(decay constant)*N(number of undecayed nuclei))
N=N0e^(-λt)

21
Q

Activity (rate of decay same)

A

A=-dN/dt=λN=λN0e^(-λt)

22
Q

Measuring the half-life of an isotope (long)

A

number of decays by time
mass of the sample and calculating the number of atoms N
using A=λN to calculate λ constant
using T1/2= ln2/λ

23
Q

carbon-14 dating

A

once an organism has died, the amount of carbon-14 will fall with decay, which can be used to tell how old it is

24
Q

why is C-14 dating possible

A

c14 is unstable, but c12(also present) is stable (proportion constant in living)
neither can be replenished after death
c14 decays

25
Q

limitations of Carbon-14 dating

A

after 5000 years, the activity is too small to be measured

26
Q

Measuring geological time

A

age of rocks can be determined by the decay of Uranium-238 to lead-206
(the rock must contain uranium as an impurity in its structure, but reject lead so all that is left is results of the decay)
the half life is approximately the age of the earth

27
Q

alpha decay

what, why, how

A

an alpha particle (2 protons+2 neutrons) (also described as the nucleus of a helium-4)
causes transmutation
tends to be emitted by nuclides with too many neutrons for stability

28
Q

transmutation

A

alpha decay causing a change in element

29
Q

properties of alpha particles

A

travel at about 10^7ms^-1
deflected by electric and magnetic fields (double positive charges)
low penetration
causes intense ionization (change of charge from e- changes)

30
Q

beta decay for a proton in a nucleus

A

beta + particles (positrons, or antimatter of an electron (same mass, opposite charge)) and neutrino (v)(neutral particle with little or no mass) are emitted

31
Q

beta decay for a neutron

A

beta particle (electron) and antineutrino

32
Q

beta decay

A

both types are transmutations
beta+ because of too few electrons
beta because of too many electrons

33
Q

properties of beta particles

A

typically at 10^8ms^-1
deflected by electric and magnetic fields as expected for a single negative
causes moderate ionization
medium penetration

34
Q

gamma decay

A
gamma ray (part of electromagnetic spectrum)
does not cause transmutation
after alpha or beta decay, the exited state may gamma decay to reduce energy
35
Q

properties of gamma rays

A

travel at 3*10^8
not deflected by electric and magnetic fields
cause little ionization
high penetration

36
Q

nuclear energy levels (evidence)

A

alpha particles always emitted at same speed from a nuclide. gamma rays always emitted with same energy.

37
Q

biological effects of ionizing radiation

A

may damage dna (can be repaired, but if not could cause cancerous cells)
short term: could cause burns in high dosage; could kill organs
long term: risks of cancer, but no link between dosage and type of cancer

38
Q

induced nuclear reactions

A

the reactions can be forced by by striking a stable nucleus with another nucleus, particle or gamma ray photon

39
Q

nuclear fission

A

when a stable nucleus absorbs a slow moving neutron making it unstable and causing a split into two large fragments and some neutrons
the importance of neutron emission is possible chain reactions

40
Q

estimation of the energy produced by fission/fusion

A

=the increase in binding energy (binding energy of mother nucleus is seen as negative)

41
Q

Nuclear fusion

A

combing of two nuclei, which results in high levels of energy emission

42
Q

evaluation of fusion

A

possible because the binding energies of two low mass nuclei can fuse to create a larger nuclei of higher binding energy.
coulomb repulsion prevents it working, and requires the collision to happen at high speeds causing the energy released to mainly be kinetic energy
attractive because of large quantities of deuterium and tritium (H-2+H-3) and much less radioactive waste, but extremely hard to make it happen and remain constant

43
Q

thermonuclear reactions

A

reactions that require immense heat to keep the reaction occurring, happens in a star.

44
Q

problems involving mass defect and binding energy

A

E=mc^2
Mass defect= total mass of separated nucleons- mass of nucleus
Sometimes given in atomic masses, so incorporate electrons
Atomic mass= nuclear mass+(Zmass of electron); therefore Mass defect= (Zmass of proton)+(Nmass of a neutron)- (Atomic mass-(Zmass of electron)

45
Q

Measuring a short half life

A

lnA by time

46
Q

beta energy spectra

A

continuous with a range of speeds (thus energy levels) up to a maximum. the anitneutrino takes remaing energy away