W14 - Neutron Interactions I/II Flashcards
What is the definition of BE?
Mass defect is positive for all nuclei
If the nucleus could be pulled apart and separated into its constituent protons and neutrons, there would be an increase in mass equal to the mass defect
The equivalent amount of energy, the BE, would need to be expended to carry out this disassembly.
Define fissionable materials. Provide examples
Isotopes that are capable of undergoing nuclear fission after capturing either fast (~MeV) or thermal (~0.025eV) neutrons
E.g. U238, Pu240, U235, U233, Pu239, Pu241
Define fissile materials, provide examples
Isotopes that are capable of undergoing nuclear fission only after capturing a thermal neutron
E.g. U235, U233, Pu239, Pu241
Define Fertile Materials and provide examples
Isotopes that are not fissionable by thermal neutrons but can be converted into fissile isotopes (after neutron absorption and subsequent decay)
E.g. U238, Th232
What happens to the fission fragments post fission
Fission fragments (Daughter nuclei):
• highly charged
• High speeds they emerge from fission cause electrons to be ripped from their shells as they encounter surround atoms
• interaction with surround atoms creates ion pairs, which reduces the KE of fragments causing deceleration
• +ve ions and free electrons subsequently reunite, liberating energy in the form of heat
• range is a few microns
What happens the non-fission fragments post fission event
Alpha beta particles have much greater ranges than fission fragments
Neutrons, gamma rays, and neutrinos travel in straight lines until making a collision, at which point they’re scattered or absorbed
• straight lines due to zero charge
Neutrons are only scattered from nuclei whereas gamma rays are scattered by nuclei and electrons
(More than 80% of the energy released in fission appears as KE from fission fragments)
What is the K and L factors in neutron multiplication?
K (chain reaction multiplier)
“the ration of fission neutrons born in one generation to those born in the prior generation”
L = neutron lifetime
“Neutron emission from fission, progressing/aging through a succession of scattering collisions, and ending with absorption”
Derive the neutron multiplication equation
@ t=0 N(0) neutrons
Next generation will have k•N(0)
The i’th generation will have k^i•N(0)
t=i•l where t is time and l is neutron lifetime
Hence the number of neutrons present at N(t) = N(0)•k^(t/l)
x = exp(lnx)
N(t) = N(0)•exp[(t/l)•lnk]
If K is close to 1 —> |k-1| «_space;1 then ln(k) ~~ k-1
Final, N(t) = N(0)•exp[(k-1)*t/l]
Why are fission fragments unstable?
High neutron to proton ratio
N/Z increases for larger nuclei (larger A)
Fragments have smaller A but same N/Z ratio hence beta decay and gamma decay
The N/Z ratio for these fragments is much higher than the line of stability
Principle fuel types and energy gain (BE/A). How to calculate total BE gain
Th233 - 5.1MeV
U234 - 6.8MeV
U236 - 6.5MeV
U239 - 5.0MeV
Pu240 - 6.7MeV
Reactants(BE/A A) - products(BE/AA)
Min and max Z^2/A for spontaneous fission to occur
Min: > 18
Max: < ~66
Upper limit as this would be higher than the coulomb potential and just would exist for a fraction of a second.
Delta M > 0 for a decay to occur
What is the roughly timeline for decay heat of a fully running reactor?
1% of max power approx 6hours
0.1% of max power approx 1 month
1600MW reactor
1% = 16MW
0.1% = 1.6MW
How does the cross-section for x-ray as a function of Z^2 differ from neutrons?
X-Rays
• cross section increases as Z increases
Neutrons
• varies massively on size of Z
More likely to interact with nuclei of similar size, also more likely to interact if KE lower
How to calculate total cross-section, sigma_t and its constituents
Sigma_t = sigma_s + sigma_a
Sigma_s (scattering) = sigma_n (elastic) + sigma_n’ (inelastic)
•inelastic conserves momentum but not KE
Sigma_a (absorption) = sigma_n,Gamma (absorption and remission of a gamma/ capture) + sigma_f (fission cross-section)
Same summations and subscripts apply to macroscopic cross-sections
How come neutrons travel far in a material before interacting? Think size of atoms
Size of atom = 10^-8
Size of nucleus = 10^-12
Fraction of the cross-sectional area perpendicular to a neutrons flight path blocked by a single tightly packed layer of atoms would be roughly
(10^-12)2/(10-8)2 = 10^-8 (small probability)