Cosmological Evolution of Gamma-Ray Bursts

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Abstract/Contents

Abstract
Gamma-ray bursts (GRBs) are among the most powerful electromagnetic events in the universe, luminous enough to be detected across vast stretches of space and time. This makes them invaluable cosmological probes of the early universe. However, to use GRBs as probes, we must first determine the evolution of their characteristics, such as the co-moving density rate and the luminosity function. This process is complicated by an extensive collection of observational biases, truncations, and questionable assumptions about the parametric forms of the various functions. We apply non-parametric methods, developed by Efron & Petrosian for truncated data, directly to a sample of Swift long GRBs with known redshifts, and obtain the co-moving density rate evolution and luminosity function and evolution. Furthermore, we derive a GRB rate which is very different from star formation rate, particularly below redshift z~2, indicating perhaps a distinct class of low-z GRBs.

Description

Type of resource text
Date created June 15, 2013

Creators/Contributors

Author Kitanidis, Ellie
Primary advisor Petrosian, Vahe
Advisor Church, Sarah
Degree granting institution Stanford University, Department of Physics

Subjects

Subject gamma-ray bursts
Subject cosmology
Subject high-energy astrophysics
Genre Thesis

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User agrees that, where applicable, content will not be used to identify or to otherwise infringe the privacy or confidentiality rights of individuals. Content distributed via the Stanford Digital Repository may be subject to additional license and use restrictions applied by the depositor.
License
This work is licensed under a Creative Commons Attribution Non Commercial 3.0 Unported license (CC BY-NC).

Preferred citation

Preferred Citation
Kitanidis, Ellie. (2013). Cosmological Evolution of Gamma-Ray Bursts. Stanford Digital Repository. Available at: http://purl.stanford.edu/xp981bq5003

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Undergraduate Theses, Department of Physics

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