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.

星期四, 二月 09, 2012

Smale, Peter R. 2011 用伽马暴来区分timescape cosmology和lambda CDM模型

主要内容:
说timescape cosmology更好一点儿。

(八字还没有一撇呢,就用来区分宇宙学模型了?)

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Title:
Gamma-ray burst distances and the timescape cosmology
Authors:
Smale, Peter R.
Affiliation:
AA(Department of Physics and Astronomy, University of Canterbury, Private Bag 4800, Christchurch 8140, New Zealand)
Publication:
Monthly Notices of the Royal Astronomical Society, Volume 418, Issue 4, pp. 2779-2784. (MNRAS Homepage)
Publication Date:
12/2011
Origin:
WILEY
Astronomy Keywords:
cosmological parameters, cosmology: observations, cosmology: theory
Abstract Copyright:
© 2011 The Author Monthly Notices of the Royal Astronomical Society © 2011 RAS
DOI:
10.1111/j.1365-2966.2011.19678.x
Bibliographic Code:
2011MNRAS.418.2779S

Abstract

Gamma-ray bursts can potentially be used as distance indicators, providing the possibility of extending the Hubble diagram to redshifts ˜7. Here we follow the GRB analysis of Schaefer, with the aim of distinguishing the timescape cosmological model from the Λ cold dark matter (ΛCDM) model by means of the additional leverage provided by Gamma-ray bursts (GRBs) in the range 2 ≲z≲ 7. We find that the timescape model fits the GRB sample slightly better than the ΛCDM model, but that the systematic uncertainties are still too little understood to distinguish the models.
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