collaborators

5 papers

astro-ph.HE2026

Correlated and uncorrelated Monte Carlo neutron capture rate variations in weak -process simulations

Atul Kedia, Jeffrey M. Berryman, Jonathan Cabrera Garcia +7

Reliable predictions of weak rapid neutron capture (-process) abundances require a systematic treatment of nuclear physics uncertainties, especially neutron capture rat…

astro-ph.HE2026

Propagating Uncertainties from Nuclear Physics to Gamma-rays in Core Collapse Supernovae

Chris L Fryer, Hendrik Schatz, Samuel Jones +18

Nuclear yields are powerful probes of supernova explosions, their engines and their progenitors. In addition, as we improve our understanding of these explosions, we can use nuclea…

astro-ph.HE2025

Kilonova Emissions from Neutron Star Merger Remnants: Implications for Nuclear Equation of State

Kelsey A. Lund, Rahul Somasundaram, Gail C. McLaughlin +3

Multi-messenger observation of binary neutron-star mergers can provide valuable information on the nuclear equation of state (EoS). Here, we investigate to which extent electromagn…

astro-ph.HE2025

Gamma rays as a signature of r-process producing supernovae: remnants and future Galactic explosions

Zhenghai Liu, Evan Grohs, Kelsey A. Lund +5

We consider the question of whether core-collapse supernovae (CCSNe) can produce rapid neutron capture process (r-process) elements and how future MeV gamma-ray observations could…

astro-ph.HE2025

Angle-dependent in-situ fast flavor transformations in post-neutron star merger disks

Kelsey A. Lund, Payel Mukhopadhyay, Jonah M. Miller +1

The remnant black hole-accretion disk system resulting from binary neutron star mergers has proven to be a promising site for synthesizing the heaviest elements via rapid neutron c…