Research

Theory Group

Stellar Astrophysics

Supernovae

Gamma-ray Bursts

White Dwarfs

Neutron Stars & Magnetars

Asteroseismology

Planetary Sciences

Astrobiology

Planet Formation

Cosmology

Early Universe

First Stars & Galaxies

Fundamental Physics

Cosmic Reionization

Structure Formation

Extragalactic Astrophysics

Active Galactic Nuclei

Clusters of Galaxies

Theoretical & Computational Astrophysics

Galactic Evolution

Milky Way Evolution

ISM and Star Formation

Theory Group : Extragalactic Astrophysics : Theoretical & Computational Astrophysics

Early Universe Computational Astrophysics Laboratory

Meghann Agarwal, Volker Bromm, Daniel Kagan, Chris Lindner, Milos Milosavljevic, Jeremy Ritter, Chalence Safranek-Shrader


ADS | astro-ph

Volker Bromm  

Associate Professor

website

Research Interests

Formation of the first stars and quasars; high-redshift supernovae and metal enrichment; supermassive black hole formation; gamma-ray bursts; reionization of the intergalactic medium; present-day star formation; computational astrophysics.

Group Areas

First Stars & Galaxies, ISM and Star Formation, Structure Formation


ADS | astro-ph

Milos Milosavljevic  

Associate Professor

website

Research Interests

Massive black holes; the Galactic center; galaxy formation; galaxy clusters; plasma astrophysics.

Group Areas

Clusters of Galaxies, Gamma-ray Bursts, Black Holes & AGN


Meghann Agarwal  

Graduate Student - Physics


ADS | astro-ph

Daniel Kagan  

Graduate Student

Group Areas

Supernovae


ADS | astro-ph

Chris Lindner  

Graduate Student

website

Group Areas

Gamma-ray Bursts, Supernovae


Jeremy Ritter  

Graduate Student

Research Interests

Computational Cosmology

Group Areas

First Stars & Galaxies


Chalence Safranek-Shrader  

Graduate Student

website

Research Interests

Star Formation in the First Galaxies; Chemical and Radiative Feedback from the First Stars and Galaxies; Near-field Cosmology

Group Areas

First Stars & Galaxies, ISM and Star Formation

Gas number density n (upper panels) and neutral fraction XH (lower panels) at two separate instances around t~4,000 yr. The left panels show the flow during a central accretion minimum; infalling gas is clearly visible at r~1.5 x 1016 cm. The right panels show the flow during a central accretion maximum. The structure near the central axis, in the conical region marked by dashed lines, is an artifact of our having set the optical depth to zero along the axis, for R/|z| < tan5°, to avoid numerical issues arising from the coordinate singularity.

from

Accretion onto Intermediate-Mass Black Holes in Dense Protogalactic Clouds astro-ph