papers

Publications (17)

astro-ph.CO2014

The Mutual Interaction Between Population III Stars and Self-Annihilating Dark Matter

Athena Stacy, Andreas H. Pawlik, Volker Bromm +1

We use cosmological simulations of high-redshift minihalos to investigate the effect of dark matter annihilation (DMA) on the collapse of primordial gas. We numerically investigate…

astro-ph.GA2020

Modeling the survival of Population III stars till present day

Jayanta Dutta, Sharanya Sur, Athena Stacy +1

Recent numerical simulations have suggested the probability of a fraction of the primordial stars being ejected from the cluster of their origin. We explore the possibility that so…

astro-ph.GA2016

Gravitational Waves from the Remnants of the First Stars

Tilman Hartwig, Marta Volonteri, Volker Bromm +4

Gravitational waves (GWs) provide a revolutionary tool to investigate yet unobserved astrophysical objects. Especially the first stars, which are believed to be more massive than p…

astro-ph.CO2012

Effect of Population III Multiplicity on Dark Star Formation

Athena Stacy, Andreas H. Pawlik, Volker Bromm +1

We numerically study the mutual interaction between dark matter (DM) and Population III (Pop III) stellar systems in order to explore the possibility of Pop III dark stars within t…

astro-ph.GA2016

The First Stars: formation under cosmic ray feedback

Jacob A. Hummel, Athena Stacy, Volker Bromm

We explore the impact of a cosmic ray (CR) background generated by supernova explosions from the first stars on star-forming metal-free gas in a minihalo at . Starting fro…

astro-ph2009

The formation of the first galaxies and the transition to low-mass star formation

Thomas H. Greif, Dominik R. G. Schleicher, Jarrett L. Johnson +6

The formation of the first galaxies at redshifts z ~ 10-15 signaled the transition from the simple initial state of the universe to one of ever increasing complexity. We here revie…

astro-ph.CO2022

Magnetic fields in the formation of the first stars.--II Results

Athena Stacy, Christopher F. McKee, Aaron T. Lee +2

Beginning with cosmological initial conditions at z=100, we simulate the effects of magnetic fields on the formation of Population III stars and compare our results with the predic…

astro-ph.GA2019

Modeling the survival of Population III stars till present day

Jayanta Dutta, Sharanya Sur, Athena Stacy +1

Recent numerical simulations have suggested the probability of a fraction of the primordial stars to be ejected from the cluster of their origin. We explore the possibility that so…

astro-ph2007

Impact of Cosmic Rays on Population III Star Formation

Athena Stacy, Volker Bromm

We explore the implications of a possible cosmic ray (CR) background generated during the first supernova explosions that end the brief lives of massive Population III stars. We sh…

astro-ph.GA2016

Building up the Population III initial mass function from cosmological initial conditions

Athena Stacy, Volker Bromm, Aaron T. Lee

We simulate the growth of a Population III stellar system, starting from cosmological initial conditions at z=100. We follow the formation of a minihalo and the subsequent collapse…

astro-ph.CO2010

Rotation Speed of the First Stars

Athena Stacy, Volker Bromm, Abraham Loeb

We estimate the rotation speed of Population III (Pop III) stars within a minihalo at z ~ 20 using a smoothed particle hydrodynamics (SPH) simulation, beginning from cosmological i…

astro-ph.CO2013

Constraining the Statistics of Population III Binaries

Athena Stacy, Volker Bromm

We perform a cosmological simulation in order to model the growth and evolution of Population III (Pop III) stellar systems in a range of host minihalo environments. A Pop III mult…

astro-ph.GA2015

The First Stars: formation under X-ray feedback

Jacob A. Hummel, Athena Stacy, Myoungwon Jeon +2

We investigate the impact of a cosmic X-ray background (CXB) on Population III stars forming in a minihalo at . Using the smoothed particle hydrodynamics code GADGET-2,…

astro-ph.CO2014

The First Stars: A Low-Mass Formation Mode

Athena Stacy, Volker Bromm

We perform numerical simulations of the growth of a Population III stellar system under photodissociating feedback. We start from cosmological initial conditions at z = 100, self-c…

astro-ph.CO2011

Effect of Streaming Motion of Baryons Relative to Dark Matter on the Formation of the First Stars

Athena Stacy, Volker Bromm, Abraham Loeb

We evaluate the effect of a supersonic relative velocity between the baryons and dark matter on the thermal and density evolution of the first gas clouds at z < 50. Through a serie…

astro-ph.CO2012

Probing Pre-galactic Metal Enrichment with High-Redshift Gamma-Ray Bursts

F. Y. Wang, Volker Bromm, Thomas H. Greif +4

We explore high-redshift gamma-ray bursts (GRBs) as promising tools to probe pre-galactic metal enrichment. We utilize the bright afterglow of a Pop III GRB exploding in a primordi…

astro-ph.GA2020

Magnetic Fields in the Formation of the First Stars. I. Theory vs. Simulation

Christopher F. McKee, Athena Stacy, Pak Shing Li

While magnetic fields are important in contemporary star formation, their role in primordial star formation is unknown. Magnetic fields of order 10^-16 G are produced by the Bierma…