12. Reactioins, Fusion, Nucleosynthesis Flashcards

1
Q

State the equation for the reaction rate per unit time, and define the components of the equation

A

W = JNσ
J - Flux = n_b v_i where n_b is the number density of the particles in the incoming beam, v_i is the velocity of the beam
N - Number of nuclei in the target illuminated by beam
σ - Mean cross section

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2
Q

What is the motion of the target particle in nuclear physics

A

Always stationary

Consider non-relativistic mechanics

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3
Q

What are the two classes of reactions

A

Direct reactions and compound nuclear reactions

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4
Q

What is a direct reaction?

A

Occurs on a short time scale of 10^-22s

- Time in which the projectile passes the target nucleus

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5
Q

What is a nuclear compound reaction?

A

Longer timescale

- Projectile absorbed and a compound nucleus is created which later decays

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6
Q

What are the four types of direct reactions?

A
  1. Elastic
  2. Inelastic
  3. Pick up
  4. Stripping
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7
Q

State all the properties of an elastic direct reaction

A

a + A -> a + A

Target and projectile remain the same, just exchange of energy and momenta

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8
Q

State all the properties of an inelastic direct reaction

A

a + A -> a + A*

Target nucleus is excited, but remains as the same nuclide

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9
Q

State all the properties of an pick up direct reaction

A

A1 a + A2 A -> (A1 + n) b + (A2 - n) B

- Projectile picks up one or more target nucleons

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10
Q

State all the properties of an stripping direct reaction

A

A1 a + A2 A -> (A1 - n) b + (A2 + n) B

- Projectile loses one or more nucleons to the target

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11
Q

Describe the graph of cross-section neutron energy for neutron absorption

A
  • Low energy, X-sec falls as 1/v
  • Then get resonance peaks reflecting shell structure of nucleus with decreasing amplitude
  • At high energy, slow smooth decrease
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12
Q

State the equation for the PP chain

A

H + H -> 2H + e+ + electron neutrino + 0.42MeV
H + 2H -> 3He + photon + 5.49 MeV
3He 3He -> 4He + 2H + 12.86MeV

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13
Q

What type of temperature do we need for fusion, and what is the biggest problem with this?

A

Need to heat plasma to 10^7 - 10^8 K

- Difficult to confine

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14
Q

State the total released energy in the PP chain, and how much of it is carried away?

A

Used 4 protons to produce 1 He
E = 24.68 + 2.04 (Annihilation)
0.26 MeV carried away

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15
Q

What is another process for fusion?

A

CNO
Again 4p fuse to 4He with the same energy budget
12C acts as a catalyst of the reaction

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16
Q

How does fusion occur in the sun when the energy needed to overcome V_c is 10^10K?

A

Sun temp is 10^7K. Quantum tunneling due to the large size of the sun

17
Q

Describe and explain the cross section energy graph for fusion in our sun

A

Bell curve centered about E_0, FWHM = E_0
- At low E(velocity), fusion cross section is too small to contribute
- Large energy there are too few nuclei pairs to contribute significantly
Middle part contributes to fusion.

18
Q

When does nuclear burning continue until, and why?

A

Until Iron (A = 56) as it is the peak BE/nucleon

19
Q

Why do we need a different mechanism to go beyond A = 56 to form heavier nuclei, and what is this mechanism?

A

As when we increase A, we are now decreasing the binding energy per nucleon

  • Not energetically favourable
  • Need neutron or proton capture from a large flux of particles which is typically available in exploding stars
20
Q

What are the two types of neutron capture?

A

The s process and the r process

21
Q

Describe the neutron capture s process

A

When neutron capture is slow compared to beta decay, so the atomic number increases

22
Q

Describe the neutron capture r process

A

When neutron capture is fastcompared to beta decay, so we get an increase in the mass number while the atomic number stays the same