activity
19982026
most citedA dynamical collective calculation of supernova neutrino signals

131 citations · 663 across the 18 of their papers we have counts for

collaborators

18 papers

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.,…

hep-ph2024★ 8 cited

Quantum maximum entropy closure for small flavor coherence

Julien Froustey, James P. Kneller, Gail C. McLaughlin

Quantum angular moment transport schemes are an important avenue toward describing neutrino flavor mixing phenomena in dense astrophysical environments such as supernovae and mergi…

astro-ph.HE2024★ 2 cited

Neutrino flavor transformation with moments: application to fast flavor instabilities in neutron star mergers

Julien Froustey, Sherwood Richers, Evan Grohs +4

Neutrino evolution, of great importance in environments such as neutron star mergers (NSMs) because of their impact on explosive nucleosynthesis, is still poorly understood due to…