Gamma-ray bursts and dark energy-dark matter interaction

被引：6
|
作者：
Barreiro, T. [1 ,3 ]
Bertolami, O. [2 ,3 ]
Torres, P. [2 ,4 ]
机构：
[1] Univ Lusofona Humanidades & Tecnol, Dept Matemat, P-1749024 Lisbon, Portugal
[2] Inst Super Tecn, Dept Fis, P-1049001 Lisbon, Portugal
[3] Inst Super Tecn, Inst Plasmas & Fusao Nucl, P-1049001 Lisbon, Portugal
[4] Inst Super Tecn, Ctr Fis Teor & Particulas, P-1049001 Lisbon, Portugal
来源：
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2010年 / 409卷 / 02期
关键词：
gamma-ray burst: general; cosmological parameters; dark energy; dark matter; CHAPLYGIN-GAS MODEL; E-P; E-I-E-ISO CORRELATION; COSMOLOGICAL PARAMETERS; CONSTRAINTS; EMISSION;
D O I：
10.1111/j.1365-2966.2010.17344.x
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this work, gamma-ray burst (GRB) data are used to place constraints on a putative coupling between dark energy and dark matter. Type Ia supernovae constraints from the Sloan Digital Sky Survey II (SDSS-II) first-year results, the cosmic microwave background radiation shift parameter from Wilkinson Microwave Anisotropy Probe seven year results and the baryon acoustic oscillation peak from the SDSS are also discussed. The prospects for the field are assessed, as more GRB events become available.
引用
收藏
页码：750 / 754
页数：5
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