activity
20042026
most citedNeutrino Interactions in the Outflow from Gamma-Ray Burst Accretion Disks

43 citations · 115 across the 12 of their papers we have counts for

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Showing astro-ph.HEShow all

9 papers · 1 filter

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

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★ 10 cited

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…

astro-ph.HE2024

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.HE2024

The time evolution of fast flavor crossings in post-merger disks around a black hole remnant

Payel Mukhopadhyay, Jonah Miller, Gail C. McLaughlin

We postprocess a three-dimensional general relativistic, full transport neutrino radiation magnetohydrodynamics simulation of the black hole--accretion disk--wind system thought to…

astro-ph.HE2024

Nuclear uncertainties associated with the ejecta of a neutron-star black-hole accretion disk

M. R. Mumpower, T. M. Sprouse, J. M. Miller +5

The simulation of heavy element nucleosynthesis requires input from yet-to-be-measured nuclear properties. The uncertainty in the values of these off-stability nuclear properties p…

astro-ph.HE2023★ 2 cited

Emergent nucleosynthesis from a 1.2 second long simulation of a black-hole accretion disk

T. M. Sprouse, K. A. Lund, J. M. Miller +2

We simulate a black-hole accretion disk system with full-transport general relativistic neutrino radiation magnetohydrodynamics (GRRMHD) for 1.2 seconds. This system is likely t…

astro-ph.HE2011★ 36 cited

Nucleosynthesis of Nickel-56 from Gamma-Ray Burst Accretion Disks

R. Surman, G. C. McLaughlin, N. Sabbatino

We examine the prospects for producing Nickel-56 from black hole accretion disks, by examining a range of steady state disk models. We focus on relatively slowly accreting disks in…