Solar - Nuclear Fusion Flashcards

1
Q

Where does solar energy come from?

A

Nuclear Fusion

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2
Q

Nuclear Fusion

A

Fusion of hydrogen to helium

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3
Q

Sun composition

A

74% hydrogen, 24% helium

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4
Q

First step of nuclear fusion

A

Fusion of two protons by weak interactions, forming deuterium, releasing an electron neutrino, a positron and 1.43mev of energy

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5
Q

Coulomb Repulsion Barrier

A

An energy barrier due to electrostatic interactions that tow nuclei must overcome to get close enough for nuclear reaction

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6
Q

What is thermal barrier of coloumb?

A

0.2MeV and 1.4x10^9K, 100 times greater than core of sun

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7
Q

What two processes allow nuclear fusion?

A

Quantum Tunneling
Boltzmann Distribution

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8
Q

Centre of Mass Frame

A

An inertial frame where centre of mass remains at the origin

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9
Q

What is fusion rate a product of?

A

Probability of finding two particles with energy E in their centre of mass frame
Probability these two particles get close to interact, depending on quantum tunneling
Reaction rate factor, describing likelihood of a fusion event

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10
Q

Quantum Tunneling

A

Passage of minute particles through seemingly impassable force barriers

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11
Q

Boltzmann Distribution

A

Describes probability of finding a particle in a certain state, in a gas at a particular temperature

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12
Q

Maxwell Boltzmann Distribution

A

Concerns distribution of amount of energy between identifcal but distinguishable particles.

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13
Q

What does MBD suggest?

A

Hot gases have assumed constant energies as energy is realtively closs regardless

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14
Q

Prediction of MBD

A

There are many molecules with energies higher than the average

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15
Q

How many MBD particles are there in one mole?

A

10^8 with 10 times mean energy, not enough to overcome the barrier

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16
Q

What determines barrier penetration factor?

A

Resilience of the barrier and energy of the particle

17
Q

What is probability of tunneling described by?

A

Gammow factor

18
Q

Gammow factor

A

This is a probability of the boltzmann factor and the barrier penetration factor

19
Q

When is fusion possible?

A

When a gamow window opens

20
Q

When does tunneling probabiltiy become significant?

A

When boltzmann distribution is below coloumb barrier energy of 0.2MeV

21
Q

What are the reactions of Nuclear Fusion?

A

Two deuterium merge forming helium, or interact with protons forming He-3, where two He-3 can fuse to make Be-6, which can break forming He-4 and two protons

22
Q

How are photons produced?

A

Interplay of nuclear force and coulomb force, or positron and electron annihiliation.