activity
20162026
most citedObserving intermediate-mass black holes and the upper--stellar-mass gap with LIGO and Virgo

86 citations · 297 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.SR2026

Benchmarking Machine Learning Emulators of Stellar Evolution for Precision Asteroseismology

Naomi Gluck, Earl P. Bellinger, Yan Liang +5

Fast and accurate stellar evolution emulators---surrogate models that approximate expensive simulation outputs with machine learning (ML)---are powerful tools for modern stellar ch…

astro-ph.SR2026

Solar-like oscillations in accreting pre-main sequence stars: Insights and prospects

Johannes Jørgensen, Konstanze Zwintz, Ebraheem Farag +2

We present theoretical predictions for solar-like oscillators in the pre-main sequence phase of stellar evolution. Our pre-main sequence models start from a stellar seed of 0.01 so…

astro-ph.GA2025★ 1 cited

Evolutionary Tracks and Spectral Properties of Quasi-stars and Their Correlation with Little Red Dots

Andrew D. Santarelli, Ebraheem Farag, Earl P. Bellinger +4

JWST has revealed a population of red, compact, high-redshift () objects referred to as ``Little Red Dots'' (LRDs). These objects exhibit unusual spectral features rem…

astro-ph.HE2025

MESA-QUEST: Tracing the formation of direct collapse black hole seeds via quasi-stars

Andrew D. Santarelli, Claire B. Campbell, Ebraheem Farag +3

The origin of the first supermassive black holes (SMBHs) observed at redshifts remains one of the most challenging open questions in astrophysics. Their rapid emergence s…

astro-ph.SR2025

Nuclear Neural Networks: Emulating Late Burning Stages in Core Collapse Supernova Progenitors

Aldana Grichener, Mathieu Renzo, Wolfgang E. Kerzendorf +7

One of the main challenges in modeling massive stars to the onset of core collapse is the computational bottleneck of nucleosynthesis during advanced burning stages. The number of…

astro-ph.SR2024★ 14 cited

An Expanded Set of Los Alamos OPLIB Tables in MESA: Type-1 Rosseland-mean Opacities and Solar Models

Ebraheem Farag, Christopher J. Fontes, F. X. Timmes +11

We present a set of 1194 Type-1 Rosseland-mean opacity tables for four different metallicity mixtures. These new Los Alamos OPLIB atomic radiative opacity tables are an order of ma…

astro-ph.HE2023

Photons from neutrinos: the gamma ray echo of a supernova neutrino burst

Cecilia Lunardini, Joshua Loeffler, Mainak Mukhopadhyay +3

When a star undergoes core collapse, a vast amount of energy is released in a ~10 s long burst of neutrinos of all species. Inverse beta decay in the star's hydrogen envelope cause…

astro-ph.SR2023★ 10 cited

Stellar Neutrino Emission Across The Mass-Metallicity Plane

Ebraheem Farag, F. X. Timmes, Morgan T. Chidester +2

We explore neutrino emission from nonrotating, single star models across six initial metallicities and seventy initial masses from the zero-age main sequence to the final fate. Ove…

astro-ph.SR2023

Seismic Signatures of the C(, )O Reaction Rate in White Dwarf Models with Overshooting

Morgan T. Chidester, F. X. Timmes, Ebraheem Farag

We consider the combined effects that overshooting and the C(, )O reaction rate have on variable white dwarf stellar models. We find that carbon-oxygen white dw…

astro-ph.HE2022★ 51 cited

Resolving The Peak Of The Black Hole Mass Spectrum

Ebraheem Farag, Mathieu Renzo, Robert Farmer +2

Gravitational wave (GW) detections of binary black hole (BH) mergers have begun to sample the cosmic BH mass distribution. The evolution of single stellar cores predicts a gap in t…

astro-ph.GA2022★ 70 cited

JWST Imaging of Earendel, the Extremely Magnified Star at Redshift

Brian Welch, Dan Coe, Erik Zackrisson +60

The gravitationally lensed star WHL0137-LS, nicknamed Earendel, was identified with a photometric redshift based on images taken with the Hubble Space Tele…

astro-ph.SR2022★ 22 cited

On Trapped Modes In Variable White Dwarfs As Probes Of The C()O Reaction Rate

Morgan T. Chidester, Ebraheem Farag, F. X. Timmes

We seek signatures of the current experimental CO reaction rate probability distribution function in the pulsation periods of carbon-oxygen white dwarf models. W…

gr-qc2021★ 86 cited

Observing intermediate-mass black holes and the upper--stellar-mass gap with LIGO and Virgo

Ajit Kumar Mehta, Alessandra Buonanno, Jonathan Gair +5

Using ground-based gravitational-wave detectors, we probe the mass function of intermediate-mass black holes (IMBHs) wherein we also include BHs in the upper mass gap $\sim 60-130~…

astro-ph.SR2021★ 18 cited

On The Impact Of 22Ne On The Pulsation Periods Of Carbon-Oxygen White Dwarfs With Helium Dominated Atmospheres

Morgan T. Chidester, F. X. Timmes, Josiah Schwab +6

We explore changes in the adiabatic low-order g-mode pulsation periods of 0.526, 0.560, and 0.729 M carbon-oxygen white dwarf models with helium-dominated envelopes due to…

astro-ph.SR2020★ 23 cited

On Stellar Evolution In A Neutrino Hertzsprung-Russell Diagram

Ebraheem Farag, F. X. Timmes, Morgan Taylor +2

We explore the evolution of a select grid of solar metallicity stellar models from their pre-main sequence phase to near their final fates in a neutrino Hertzsprung-Russell diagram…

astro-ph.SR2020★ 2 cited

Investigating Opacity Modifications and Reaction Rate Uncertainties to Resolve the Cepheid Mass Discrepancy

Joyce A. Guzik, Ebraheem Farag, Jakub Ostrowski +4

Cepheid masses derived from pulsations or binary dynamics are generally lower than those derived from stellar evolution models. Recent efforts have been dedicated to investigating…

astro-ph.SR2016

Sound speed and oscillation frequencies for solar models evolved with Los Alamos ATOMIC opacities

Joyce A. Guzik, C. J. Fontes, P. Walczak +3

Los Alamos National Laboratory has calculated a new generation of radiative opacities (OPLIB data using the ATOMIC code) for elements with atomic number Z=1-30 with improved physic…