Fusion and Fission
The wiki articles for these two topics contain a lot of great information, written in complex English and giving textbook vibes. Let’s break down their highlights to understand them!
Nuclear Fusion (Wikipedia link)
- Usually deuterium and tritium (hydrogen variants) or helium (variants?)
- The mass changes from reactants to products
- Observed as energy absorbing or being released during reaction
- Exothermic: reactions releasing energy
- Usually what occurs when producing nuclei lighter than iron-56 or nickel-62 (presumably the same mass)
- Endothermic: reactions absorbing energy
- Usually what occurs when the resulting product nuclei are very large
- In a supernova, nuclei are formed heavier than iron
Fusion History
- First self-sustaining fusion in November 1052 hydrogen bomb (H-bomb / thermonuclear bomb)
- Reaction must be self-sustained and also controlled to use fusion as an energy source
- US Dept of Energy in December 2022: first fusion reaction reported where energy succeeded in breaking even during human-caused fusion (2.05 megajoules 15 MJ)
- Private fusion companies funded with $2.1B during 2021
Fusion Process
- Caused by interaction of nuclear force and Coulomb force
- Nuclear force: holds protons and neutrons together in nucleus (due to strong interaction)
- Most effective at short distances
- Coulomb force: positively-charged protons in nucleus repel each other
- When lighter atomic nuclei are pushed closely together, the Nuclear force overwhelms the Coulomb force, and all excess energy is released
- Less effective as nuclei get larger, as Coulomb force starts to match or overwhelm Nuclear force (due to Nuclear force decreasing)
- Nucleosynthesis is when (most) elements are produced by fusion in stars
- Our sun is a “main-sequence star”
- Fuses hydrogen nuclei into helium
- 6% of mass is exerted using alpha particles or EM radiation or other energy
- Energy released is much larger than exothermic chemical reactions, because binding energy of nucleus is much more than energy holding electrons to a nucleus (different by factor of ~1 million)
- Sounds like overall fusion reactions produce more energy per unit mass, while the individual fission reactions produce more energy
- Fusion in stars
- Mostly fusion of hydrogen to form helium (proton-proton chain reaction)
- Fuses four protons into one alpha particle, with release of two positirons and two neutrinos (also two protons are turned into two neutrons?) and releases energy
- In heavier stars, other processes such as the Carbon-Nitrogen-Oxygen cycle are important
- As fraction of hydrogen remaining is reduced, heavier elements begin to be produced
- Heaviest produced in a giant supernova at end of a star’s life
- Artificial fusion
- Thermonuclear
- Beam-beam (beam-target)
- Muon-catalyzed
- At ordinary temps
- High energy required to create muons, so likely will not produce net energy increase
- Mostly fusion of hydrogen to form helium (proton-proton chain reaction)
- Our sun is a “main-sequence star”
- Nuclear force: holds protons and neutrons together in nucleus (due to strong interaction)
- Otto Hahn and Fritz Strassman discovered in 1938
- Usually uses heavier elements (uranium, thorium, and plutonium) as inputs
- In comparison with fusion, where atoms are fused together, in fission we see large atoms split up into smaller ones
- In addition to smaller atoms, fission produces gamma photons and energy (kinetic energy of particles and EM radiation both produced) (exothermic)
- A form of “nuclear transmutation”: resulting fragments different elements from original parent atoms
- Most fissions produce 2 charged fragments, occasionally 3
- “Unpredictable composition”: nuclear power and nuclear weapons (“self-sustaining nuclear chain reactions”) do not break apart in a perfectly predictable way
- Lots more energy released per atom and per mass and per reaction than methane and fossil fuels.
- Products: some products are more radioactive than products in other reactions, which are dangerous in the long-term
- Some strategies to reduce their harm
- Mechanism
- Radioactive decay: random, happens “spontaneously”, but at generally consistent rates over time
- Used in isotopic geochemistry, which I will discuss in a future article
- Nuclear reactions
- An incident particle fuses with a target, which forms a “compound system”
- One of a few types of fission reactions occur
- Usually binary fission, where 2 atoms (plus neutrons) are produced
- Assuming that atoms are what is referred to as fragments
- 2-4% of time we get ternary fission, where 3 fragments are produced
- Usually binary fission, where 2 atoms (plus neutrons) are produced
- Radioactive decay: random, happens “spontaneously”, but at generally consistent rates over time
Nuclear Fission (Wikipedia link)
- Nuclear fuels: chemical element isotopes which can sustain a fission chain reaction
- “Fissile”
- Most common fuels: Uranium-235 and Plutonium-239
- These two fuels and U-233 can be used as both fissile nuclear fuels and can undergo spontaneous fission (radioactive decay)
- Most neutrons usually escape rapidly from fuel, becoming a “free neutron” in the air, and decay into protons and beta particles in ~15 minutes
- If, instead of escaping, those neutrons hit other fuel atoms, they can continue inducing other reactions
- This will happen if there is a lot of fuel in one place, or if the neutrons are adequately contained (physically)
- Fun fact: freshly created neutrons from fission move ~7% the speed of light
- Critical mass: a mass of an element which could support a sustained nuclear chain reaction
- Critical assembly: an assembly of an element which could support a sustained nuclear chain reaction
- Fission reactors
- Usually only built with of 1 of 3 goals:
- Power reactors: produce heat for nuclear power
- Either in a generating station or a nuclear submarine
- Research reactors: produce neutrons / activate radioactive sources for scientific / research purposes
- Breeder reactors: produce nuclear fuels in bulk
- Fission bombs
- One class of nuclear weapons (different from fusion bombs)
- Generates as much energy as possible from before reactor explodes, which stops the chain reaction
- Fundamental physics same as those in the chain reactions of reactors
- But goals are different: fission bombs release all their energy at once, while fission reactors want to release energy slowly and steadily for power generation
- Overheating of a reactor can and has led to metdowns
- Will never have as much destructive power as a weapon because of “low Uranium enrichment”
- But goals are different: fission bombs release all their energy at once, while fission reactors want to release energy slowly and steadily for power generation
- Fission bombs