Radioactivity Flashcards

(37 cards)

1
Q

What is the typical size of a nucleus?

A

About 10^-15 m (1 femtometre).

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2
Q

What range can nuclear half-lives span?

A

From 10^-20 seconds to longer than the age of the Universe.

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3
Q

What are the typical nuclear energy units?

A

MeV (mega-electronvolts).

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4
Q

Define radioactive decay.

A

The spontaneous emission of radiation(s) that changes the state of the nucleus to more stable.

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5
Q

What is the nuclear notation A_Z X?

A

A nucleus with atomic number Z (protons), mass number A (protons + neutrons), and symbol X.

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6
Q

What are isotopes?

A

Nuclei with the same number of protons (Z) but different numbers of neutrons (N).

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7
Q

What are the main types of decay and their emissions?

A

α decay: Helium nucleus (4/2 He); β decay: electron or positron; γ decay: photon.

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8
Q

Which nuclei tend to undergo α decay?

A

Heavier nuclei (large Z, number of protons).

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9
Q

Which nuclei tend to undergo β decay?

A

Lighter nuclei with neutron or proton imbalance.

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10
Q

Define activity.

A

Rate at which decay occurs. The number of radioactive decays per second.

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11
Q

What are the SI of activity?

A

SI: Becquerel (1 Bq = 1 decay/s)

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12
Q

Formula for activity?

A

A = λN

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13
Q

Differential equation describing decay?

A

dN/dt = -λN

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14
Q

Exponential decay law?

A

N = N0 e^(-λt)

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15
Q

Half-life formula?

A

t1/2 = ln(2)/λ

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16
Q

Mean lifetime formula?

17
Q

What is a decay chain?

A

A series of decays where one unstable nucleus transforms into another until stability.

18
Q

Example of decay sequence differential equations?

A

dNA/dt = -λA NA,
dNB/dt = λA NA - λB NB

B is produced at the rate A decays

19
Q

General equation for α decay?

A

^A_Z X → ^{A−4}_{Z−2} Y + ^4_2 He

20
Q

Energy released (Q value) formula?

A

Q = [ΣMreactants − ΣMproducts] c²

21
Q

Condition for spontaneous decay?

22
Q

Why α particles released rather than nucleus with say 1 proton and 2 neutrons?

A

They are highly stable and energetically favorable for emission.

23
Q

What is the Geiger-Nuttall rule?

A

Higher α-particle energy → shorter half-life.

24
Q

What are the three types of β decay?

A

β−: n→p+e−+ν̄e; β+: p→n+e++νe; Electron capture: p+e−→n+νe.

25
Why is the β spectrum continuous?
Because energy is shared between the electron/positron and neutrino. Emitted electrons/positrons have a range of energies
26
What is γ decay?
De-excitation of a nucleus by emission of a photon without changing A or Z.
27
what is e^2/(4,pi,epsilon0)
1.440MeV fm
28
what is hbar c
197
29
why does more neutrons mean more stable?
to overcome coulomb interaction. too many protons will repel, the strong nuclear force doesn't hold them as strongly as coulomb interaction repels them. larger nuclei need more neutrons as these have no repulsive forces
30
conversion between nuclear and atomic masses
Mn = Ma - Zm_e
31
what does the Geiger-Nuttall rule assume?
alpha particle preformed inside nucleus and moves in spherical potential well
32
Alpha decay potential V(r)
V = (Z_1 Z_2 e^2)/(4 pi epsilon0 r)
33
Define the potential well for alpha decay
classically confined to potential well (r < a) with depth -V_0 Region with a
34
Alpha decay potential B?
B = barrier height B= (1/4 pi epsilon_0)(2(Z-2)e^2/a) comes from normal V using Z_1 and 2 and Z_2 as Z-2 and r as a
35
Alpha decay potential b
b = (1/4 pi epsilon_0)(2(Z-2)e^2/Q)
36
How do we approximate the alpha decay potential
step potential (B-Q)/2 and (b-a)/2
37
what is orbital electron capture
inner shell electron is captured by a proton, turns into a neutron, releases neutrino occurs in proton rich nuclei