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GRB as luminosity indicator

Published online by Cambridge University Press:  29 January 2014

Rupal Basak
Affiliation:
Tata Institute of Fundamental Research, Mumbai
A. R. Rao
Affiliation:
Tata Institute of Fundamental Research, Mumbai
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Abstract

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Gamma Ray Bursts (GRBs) are found at much higher redshifts (z > 6) than Supernova Ia (z ~ 1), and hence, they can be used to probe very primitive universe. However, radiation mechanism of GRB remains a puzzle, unlike Supernova Ia. Through comprehensive description, both empirical and physical, we shall discuss the most likely way to use the constituent pulses of a GRB to find the radiation mechanism as well as using the pulses as luminosity indicators.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2014 

References

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