collaborators

9 papers

astro-ph.SR2026

The Effect of Mass Loss and Convective Overshooting on the Pre-Collapse Structure, Composition, and Neutrino Emission of Red Supergiants

McKenzie A. Myers, Claire B. Campbell, Kelly M. Patton +6

Prior to core collapse, the neutrino emission from red supergiants (RSGs) is so large that a nearby (kpc) RSG will become visible in current and near-future neutrino det…

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

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.HE2026

Data-driven core collapse supernova multilateration with first neutrino events

Farrukh Azfar, Jeff Tseng, Marta Colomer Molla +8

A Galactic core-collapse supernova (CCSN) is likely to be observed in neutrino detectors around the world minutes to hours before the electromagnetic radiation arrives. The SNEWS2.…

astro-ph.HE2025

Turbulence in Core-Collapse Supernovae

David Calvert, Michael Redle, Bibek Gautam +4

It is understood in a general sense that turbulent fluid motion below the shock front in a core-collapse supernova stiffens the effective equation of state of the fluid and aids in…

astro-ph.HE2025

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…