Reactor Physics Flashcards
WhTs the best moderator to fuel ratio for water?
2:1
Why is water a good moderator?
Largest slowing down power due to small mass and large scattering xs, but it has a large thermal absorption xs
How are leakage and dimension related?
The larger the medium the less leakage. For an infinite medium you can assume no leakage.for a sphere leakage increases as r^2 and fission increases as r^3
What is the conversion or breeding ratio?
The average number of fissile atoms produced in a reactor per fuel atom consumed either by fission or absorption
What does it mean when a reactor breeds?
More fuel is produced than consumed, measured by breeding gain g
What values of eta allow a reactor to breed?
Much larger than 2. Note that eta increases with energy, so breeding reactors are often fast reactors
why do heavy nuclei not make good moderators?
take a large number of collisions to slow down since they have larger inelastic scattering cross sections
reaction rate
phi Sigma = nvN sigma
mean free path
average distance a neutron travels between collisions d = 1/Sigma_t
neutron lethargy
ln(E_0/E) where E_0 is 10 MeV
gain in lethargy
ln (E/E’) = 1 + alpha/(1-alpha)ln(alpha)
neutron generation lifetime
l = n(t)/L(t)
two factor formula
f eta = (nu Sigma_f^F)/(Sigma_a^F + Sigma_a^other)
six factor formula
fast fission factor - thermal + fast neutrons/thermal neutrons
resonance escape probability
thermal neutron utilization factor
thermal neutron reproduction factor
fast neutron non leakage probability
thermal neutron non leakage probability
what causes reactivity feedback caused by?
doppler broadening of resonances, changes in moderator density and temperature, changes in fission product inventory, changes due to core expansion
probability of decay between t and (t + dt)
p(t)dt = lambda e^{-lambda t} dt
binding energy
c^2[Nm_n + Zm_p - M_nucleus(A, Z)] in words strong nuclear force - surface tension binding + spin pairing + shell binding - coulomb repulsion
mass excess
[M_at(Z, N) - A]c^2
simple reactor power formula
P = epsilon_f R_f V = epsilon_f Sigma_f phi V
macroscopic cross section
Sigma = N sigma
Reaction Rate
R = phi Sigma = n v N sigma
intensity
I = I_0 e^{-Sigma_t x}
mean free path
lambda = 1 / Sigma_t
first collision probability
p(x)dx = Sigma_t e^{-Sigma_t x}
probability of uncollided flight
P = e^{- Sigma_t x}
thermal disadvantage factor
PhiMod_th/ PhiFuel_th
in hour equation
rho_0 = sl/(sl + 1) + 1/(sl +1) SUM((s beta_i)/(s + lambda_i))
general solution of in hour equation
phi(t) = A_1 e^{s_1t} + A_2 e^{s_2t} rho = 0, s1 = 0; rho goes to 1, s1 goes to infinity; rho goes to -infinity, s1 goes to -lambda