伽玛暴(Gamma-Ray Burst)笔记。记录有关伽玛暴的新文章,另外也包括看的老文章、自己的想法、以及跟天文相关的一些东西。 Feel free to leave me a message by comments or by email.

星期三, 七月 15, 2009

Abbasi 2009 IceCube对伽玛暴的mu中微子观测的上限

主要内容:
观测了41个, 都只能给出上限.

精彩摘抄:


文章信息:

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· arXiv e-print (arXiv:0907.2227)
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Title:
Search for muon neutrinos from Gamma-Ray Bursts with the IceCube neutrino telescope
Authors:
IceCube Collaboration: R. U. Abbasi
Publication:
eprint arXiv:0907.2227
Publication Date:
07/2009
Origin:
ARXIV
Keywords:
Astrophysics - High Energy Astrophysical Phenomena
Comment:
32 pages, 8 figures, submitted to ApJ
Bibliographic Code:
2009arXiv0907.2227I

Abstract

We present the results of searches for high-energy muon neutrinos from 41 gamma-ray bursts (GRBs) in the northern sky with the IceCube detector in its 22-string configuration active in 2007/08. The searches cover both the prompt and a possible precursor emission as well as a model-independent, wide time window of -1 h to +3 h around each GRB. In contrast to previous searches with a large GRB population, we do not utilize a standard Waxman-Bahcall GRB flux for the prompt emission but calculate individual neutrino spectra for all 41 GRBs from the burst parameters measured by satellites. In none of the three time windows do we find a deviation from the background-only hypothesis. Therefore, we place 90% CL upper limits on the fluence from the prompt phase of 3.7x10^-3 erg cm^-2 (72 TeV - 6.5 PeV) and on the fluence from the precursor phase of 2.3x10^-3 erg cm^-2 (2.2 TeV - 55 TeV), where the quoted energy ranges contain 90% of the expected signal events in the detector. The 90% CL upper limit for the wide time window is 2.7x10^-3 erg cm^-2 (3 TeV - 2.8 PeV) assuming an E^-2 flux.
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