Quantum closures for neutrino moment transport
Year: 2025
Type: article
Abstract: A computationally efficient method for calculating the transport of neutrino flavor in simulations is to use angular moments of the neutrino one-body reduced density matrix, i.e., “quantum moments.” As with any moment-based radiation transport method, a closure is needed if the infinite tower of moment evolution equations is truncated. We derive a general parametrization of a quantum closure and the limits the parameters must satisfy in order for the closure to be physical. We then derive from multiangle calculations the evolution of the closure parameters in two test cases which we then progressively insert into a moment evolution code and show how the parameters affect the moment results until the full multiangle results are reproduced. This parametrization paves the way to setting prescriptions for genuine quantum closures adapted to neutrino transport in a range of situations.
Language: English
Topic: Neutrino Physics Research
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: hybrid
Awards: G1286236842, G1632040200, G1863003419, G222768804, Collaborative Research: NSF-BSF: WoU-MMA: RUI: Crossing the Chasm: From Compact Object Mergers to Cosmic Fireworks, G2821925151, PHYSICS OF SUPERNOVAE AND GAMMA RAY BURSTS: WEAK INTERACTIONS AND ELEMENT SYNTHESIS, G3083819904, G3210496953, G419881185, G4259852868, G42916606, G4501827968, G479440474, Modern Neutrino Physics in Neutron Star Merger Models, G498139845, Network for Neutrinos, Nuclear Astrophysics, and Symmetries, G7911000663, NEUTRINOS AND NUCLEOSYNTHESIS: SUPERNOVAE, GAMMA RAY BURSTS, AND LOW ENERGY BETA BEAMS, G969889393
OpenAlex ID: W4408505234
