Neutron energy after one elastic collision

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SUMMARY

The discussion focuses on calculating the fraction of neutrons with energy less than 0.5 MeV after one elastic collision with various target materials: hydrogen, deuterium, carbon-12, and uranium-238. The primary equation used is n = (1/ζ) * ln(E₀/Eₙ), where ζ is dependent on the atomic mass of the target. The calculated energies after one collision are E₁ = 0.367E₀ for hydrogen, E₁ = 0.472E₀ for deuterium, E₁ = 0.0853E₀ for carbon-12, and E₁ = 0.9916E₀ for uranium-238. The discussion concludes that neutron cross-section tables should be utilized to determine scattering probabilities instead of relying solely on the initial equation.

PREREQUISITES
  • Understanding of elastic collisions in nuclear physics
  • Familiarity with neutron cross-section tables
  • Knowledge of classical mechanics and center of mass frame transformations
  • Basic proficiency in logarithmic equations and energy calculations
NEXT STEPS
  • Research neutron cross-section σ tables for hydrogen, deuterium, carbon-12, and uranium-238
  • Study the transformation of particles in elastic collisions in the center of mass frame
  • Learn how to calculate scattering angles and their impact on neutron energy
  • Explore the relationship between scattering probabilities and neutron energy levels
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Physicists, nuclear engineers, and students studying nuclear interactions and neutron behavior in various materials.

knoximator
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ok, this is the question:

neutrons scatter elastically at 1.0MeV. after one scattering collision, determine what fraction of neutrons will have energy of less than 0.5 MeV if they scatter from:

a. hydrogen
b. Deuterium
c. Carbon-12
d. Uranium-238


solution process...

the basic equation to be used: n=\frac{1}{ζ}*ln\frac{E_{0}}{E_{n}}
n= number of collisions
ζ=depends on atomic mass of target≈ \frac{2}{A+\frac{2}{3}} (A= atomic mass)
for A=1, ζ=1!
E_{0}= original energy of neutron before collision
E_{n}= energy of neutron after n collisions

so, inputting n=1, i get the equation E_{1}=E_{0}*e^{-ζ}

and subsequently, i get the following energies:

a. E_{1}=0.367*E_{0}
b. E_{1}=0.472*E_{0}
c. E_{1}=0.0853*E_{0}
d. E_{1}=0.9916*E_{0}

and that is where i get stuck, i have no clue on how to continue and get a fraction out of the information i got.
in the book, there's a probability equation presented, but i can't see any use of it to my question


Edit

ok, so after some deep book delving session, i might have found my problem.
basically, i don't think i need the equation above, but should rely more on the neutron cross section σ tables for the elements mention above and the specific energies.

for example: \frac{σ_{s}(E)}{σ_{t}(E)} is the probability of a neutron to scatter for a certain energy E

my question is, how to use this relation, and which energies to use?
 
Last edited:
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Your answer for c is incorrect, the leading 0 shouldn't be there.

General approach to the problem is basically a classical mechanics problem - for one collision. First transform the particles (neutron and stationary target) to the center of mass coordinate frame. Next assume the elastic collision is isotropic. Transform back to the lab frame, getting the velocity vector of the neutron.
Here you can calculate the neutron energy as a function of scattering angle. Find the angle where the energy is 0.5 Mev. and get the probability that the scattering angle will be greater.

Hint: for U-238 and C-12, the probability will be 0. For H1 (from what I remember) it will be ~ .5, while for H2 it will smaller - I don't remember exactly.
 

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