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.

星期日, 七月 13, 2008

Li 2008 GRB不能做标准烛光

主要内容:
指出了观测上对弱暴和强暴的选择效应。

精彩摘抄:


文章信息:

· Find Similar Abstracts (with default settings below)
· arXiv e-print (arXiv:0806.2770)
· References in the Article
· Also-Read Articles (Reads History)
·
· Translate This Page
Title:
Are Gamma-Ray Bursts a Standard Energy Reservoir?
Authors:
Li, Li-Xin
Publication:
eprint arXiv:0806.2770
Publication Date:
06/2008
Origin:
ARXIV
Keywords:
Astrophysics
Comment:
10 pages, 4 figures
Bibliographic Code:
2008arXiv0806.2770L

Abstract

One of the most important discoveries in the observation of gamma-ray bursts (GRBs) is that the total energy emitted by a GRB in gamma-rays has a very narrow distribution around 10^51 erg, which has led people to claim that GRBs are standard energy explosions. As people made the claim they have ignored the selection biases which must be important since GRB observations are strongly fluence or flux-limited. In this paper we show that, when the selection effects are considered, the intrinsic distribution of the GRB energy can be very broad. The number of faint GRBs has been significantly underestimated because of the fluence or flux limit. The bright part of the distribution has been affected by another important selection effect arising from the beaming of GRB jets, which is instrument-independent and caused by the fact that brighter GRBs tend to have smaller jet angles and hence smaller probabilities to be detected. Our finding indicates that GRBs are not a standard energy reservoir, and challenges the proposal that GRBs can be used as standard candles to probe cosmology.
Bibtex entry for this abstract Preferred format for this abstract (see Preferences)

没有评论: