GRBs from the First Stars
Conference
·
OSTI ID:902481
We present an estimate of the Gamma Ray Bursts which should be expected from metal-free, elusive first generation of stars known as PopulationIII (PopIII). We derive the GRB rate from these stars from the Stellar Formation Rate obtained in several Reionization scenarios available in the literature. In all of the analyzed models we find that GRBs from PopIII are subdominant with respect to the ''standard'' (PopII) ones up to z {approx} 10.
- Research Organization:
- SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Sponsoring Organization:
- USDOE
- DOE Contract Number:
- AC02-76SF00515
- OSTI ID:
- 902481
- Report Number(s):
- SLAC-PUB-12457; TRN: US200717%%321
- Resource Relation:
- Conference: Presented at 1st GLAST Symposium, Stanford, Palo Alto, 5-8 Feb 2007
- Country of Publication:
- United States
- Language:
- English
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