Andrew Benson

Senior Research Fellow in Theoretical Cosmology
Theoretical AstroPhysics Including Relativity
(TAPIR)
California Institute of Technology

Theoretical
AstroPhysics
Including
Relativity


I am a Senior Research Fellow in Theoretical Cosmology within the TAPIR group at Caltech and a member of the Moore Center for Theoretical Cosmology and Physics. My research is described in more detail here and my publications are available here. I'm actively looking for graduate and undergraduate students to work on galaxy formation-related projects. Current projects on which I'm working, together with available projects for prospective students and postdocs are listed here.
My research program centers around the process of galaxy formation, with a particular emphasis on formlating a coherent picture of the many different aspects of this problem. In my research, I frequently utilize the Galform semi-analytic model of galaxy formation, which has been developed extensively at Caltech. The approach blends both analytic understanding and significant number-crunching utilizing distributed resources such as TeraGrid and Amazon''s Elastic Compute Cloud.

Research Highlight

With Arif Babul, I am developing a more sophisticated model of black hole growth and jet production which is embedded within a hierarchically growing population of galaxies. As part of this work we have developed a relatively simple model to compute the rate of spin up (or down) of an accreting black hole and the power of the jets it produces while accreting. The figure shows the efficiency (measured relative to the accretion luminosity) of jets driven out of supermassive black hole plus accretion flow systems as a function of the spin (j) of the black hole. The jet efficiency is divided into contributions from winds driven from the accretion disk, and jets launched from close to the black hole horizon. Points show results from relativistic magnetohydrodynamics simulations, while the lines indicate the results from my model of jet efficiency. This model is simple to implement in analytic calculations but agrees extremely well with relativistic magneto-hydrodynamic calculations.


(c) Andrew Benson, 2006-9. All rights reserved. Accessible Website Menu by Brothercake Scrolling News Ticker by Mioplanet Page last updated Monday, September 14, 2009.