activity
20182026
most citedQuantum Closures for Neutrino Moment Transport

8 citations · 14 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2026

Machine Learning Detection of Non-Axisymmetric Fast Flavor Instabilities in Compact Objects

Madhurima Chakraborty, Sajad Abbar, Meng-Ru Wu +2

Neutrinos in dense astrophysical environments such as core-collapse supernovae (CCSNe) and neutron star mergers (NSMs) can undergo FFCs, which could develop on extremely small scal…

astro-ph.HE2026

Neutrino transport and flavor instabilities in a post-merger disk

Erick Urquilla, Swapnil Shankar, Debraj Kundu +6

Neutron star mergers are multimessenger sources whose dynamics and signals depend critically on neutrinos and their flavor transformations. We investigate whether fast and collisio…

astro-ph.HE2026★ 1 cited

Neutrino flavor instabilities in neutron star mergers with moment transport: Slow, fast, and collisional modes

Julien Froustey, Francois Foucart, Christian Hall +5

Determining where, when, and how neutrino flavor oscillations must be included in large-scale simulations of hot and dense astrophysical environments is an enduring challenge that…

astro-ph.HE2025★ 5 cited

Advection Algorithms for Quantum Neutrino Moment Transport

Evan Grohs, Sherwood Richers, Julien Froustey +3

Neutrino transport in compact objects is an inherently challenging multi-dimensional problem. This difficulty is compounded if one includes flavor transformation -- an intrinsicall…

hep-ph2024★ 8 cited

Quantum Closures for Neutrino Moment Transport

James P. Kneller, Julien Froustey, Evan B. Grohs +3

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.,…

astro-ph.HE2018

Elastic Scattering in General Relativistic Ray Tracing for Neutrinos

M. Brett Deaton, Evan O'Connor, Y. L. Zhu +5

We present a covariant ray tracing algorithm for computing high-resolution neutrino distributions in general relativistic numerical spacetimes with hydrodynamical sources. Our form…