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Numerical simulations of host galaxies of gamma-ray bursts

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

In this project we addresses the nature of host galaxies of gamma-ray bursts (GRBs) through numerical simulations of galaxy formation. GRBs are the most energetic events in the universe and those longer than about 2 seconds are thought to result from the core collapse and explosion of massive stars [1][Pir05]. Because of the cosmologically short lifetime of the massive progenitors, GRBs are generally considered to be powerful tracers of the massive star formation history of the universe. They can therefore also be expected to provide useful insights into the understanding of the galaxy formation process. The current interest in GRB research started in 1997 with the discovery of their optical afterglow emission. To date over 40 optical detections have been made, but the number of GRB host galaxy observations is still rather limited with only about 20 positive detections.

Original languageEnglish
Title of host publicationHigh Performance Computing in Science and Engineering 2005 - Transactions of the High Performance Computing Center Stuttgart, HLRS 2005
PublisherSpringer Verlag
Pages15-23
Number of pages9
ISBN (Print)3540283773, 9783540283775
DOIs
Publication statusPublished - 2006
Event8th Results and Review Workshop on High Performance Computing in Science and Engineering, HLRS 2005 - Stuttgart, Germany
Duration: 13 Oct 200514 Oct 2005

Publication series

NameHigh Performance Computing in Science and Engineering 2005 - Transactions of the High Performance Computing Center Stuttgart, HLRS 2005

Conference

Conference8th Results and Review Workshop on High Performance Computing in Science and Engineering, HLRS 2005
Country/TerritoryGermany
CityStuttgart
Period13/10/0514/10/05

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