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Delve into the origins of neutrons from spallation physics at the WNR Facility, studying moderators, thermalization, diffusion, and scattering processes. Explore the intricacies of nuclear evaporation models, Fermi gases, and moderator functions.
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? ? ? ? ? Where are the neutrons coming from? Spallation Physics 101
Linear Accelerator Cockroft-Walton Injector WNR Facility Proton Storage Ring
Central Control Room ER1/2 Lujan Center 1L Target
1L-Target Proton beam Bulk Shield Window Moderators W-targets Reflector
Proton beam Window Moderators W-targets Reflector
Lower Tier Moderators LQD SPEAR Asterix FP8/LAPTRON Pharos FDS NPDF SMARTS SCD FP5 HIPD HIPPO
Upper Tier Moderators NPD-g IN500 DANSCE PCS
p+ Spallation Process
Statistical Thermodynamics Nuclear Evaporation Model Fermi gas of free particles in a collective potential
cold neutrons epi-thermal neutrons thermal neutrons Moderator functions Moderation and Slowing Down Thermalization and Diffusion
Moderation/Slowing Down (incoherent inelastic scattering) #01 Neutron wavelength shorter than lattice parameters Moderator Atoms Epi-thermal neutron
Moderation/Slowing Down (incoherent inelastic scattering) #02
Neutron wavelength of the same order as the lattice constants Coherent elastic scattering (Bragg-reflection) • Scattering on vibrational modes of polyatomic molecules Discrete oscillators Thermalization and Diffusion • Absorption
Maxwell Distribution: Thermal Spectrum
Diffusion equation: Simplified form: Storage Time #01
HIPPO instrument 1L Target Thermal neutrons Sample Location
Do you know where the neutrons are coming from? If not, please fill free to ask questions!