activity
20112026
most citedMagnetorotational Core-Collapse Supernovae in Three Dimensions

280 citations · 1.4k across the 35 of their papers we have counts for

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Showing 2024Show all

6 papers · 1 filter

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.HE2024★ 23 cited

Asymptotic-state prediction for fast flavor transformation in neutron star mergers

Sherwood Richers, Julien Froustey, Somdutta Ghosh +2

Neutrino flavor instabilities appear to be omnipresent in dense astrophysical environments, thus presenting a challenge to large-scale simulations of core-collapse supernovae and n…

astro-ph.HE2024

Inspecting neutrino flavor instabilities during proto-neutron star cooling phase in supernova: I. Spherically symmetric model

Masamichi Zaizen, Sherwood Richers, Hiroki Nagakura +2

In the standard model of core-collapse supernova (CCSN), all neutrinos are assumed to be in pure flavor eigenstates in CCSN cores, but the assumption becomes invalid if neutrino di…

astro-ph.HE2024★ 3 cited

Three-flavor, Full Momentum Space Neutrino Spin Oscillations in Neutron Star Mergers

Henry Purcell, Sherwood Richers, Amol V. Patwardhan +1

In the presence of anisotropic neutrino and antineutrino fluxes, the quantum kinetic equations drive coherent oscillations in neutrino helicity, frequently referred to as spin osci…

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…

astro-ph.HE2024★ 9 cited

Chaos in Inhomogeneous Neutrino Fast Flavor Instability

Erick Urquilla, Sherwood Richers

In dense neutrino gases, the neutrino-neutrino coherent forward scattering gives rise to a complex flavor oscillation phenomenon not fully incorporated in simulations of neutron st…