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- Publisher Website: 10.1016/j.physletb.2007.10.053
- Scopus: eid_2-s2.0-36849045223
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Article: Constraints on dark energy models including gamma ray bursts
Title | Constraints on dark energy models including gamma ray bursts |
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Authors | |
Issue Date | 2008 |
Citation | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, 2008, v. 658, n. 4, p. 95-100 How to Cite? |
Abstract | In this Letter we analyze the constraints on the property of dark energy from cosmological observations. Together with SNe Ia Gold sample, WMAP, SDSS and 2dFGRS data, we include 69 long Gamma-Ray Bursts (GRBs) data in our study and perform global fitting using Markov Chain Monte Carlo (MCMC) technique. Dark energy perturbations are explicitly considered. We pay particular attention to the time evolution of the equation of state of dark energy parameterized as wDE = w0 + wa (1 - a) with a the scale factor of the universe, emphasizing the complementarity of high redshift GRBs to other cosmological probes. It is found that the constraints on dark energy become stringent by taking into account high redshift GRBs, especially for wa, which delineates the evolution of dark energy. © 2007 Elsevier B.V. All rights reserved. |
Persistent Identifier | http://hdl.handle.net/10722/226682 |
ISSN | 2023 Impact Factor: 4.3 2023 SCImago Journal Rankings: 1.593 |
ISI Accession Number ID |
DC Field | Value | Language |
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dc.contributor.author | Li, Hong | - |
dc.contributor.author | Su, Meng | - |
dc.contributor.author | Fan, Zuhui | - |
dc.contributor.author | Dai, Zigao | - |
dc.contributor.author | Zhang, Xinmin | - |
dc.date.accessioned | 2016-06-29T01:58:17Z | - |
dc.date.available | 2016-06-29T01:58:17Z | - |
dc.date.issued | 2008 | - |
dc.identifier.citation | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, 2008, v. 658, n. 4, p. 95-100 | - |
dc.identifier.issn | 0370-2693 | - |
dc.identifier.uri | http://hdl.handle.net/10722/226682 | - |
dc.description.abstract | In this Letter we analyze the constraints on the property of dark energy from cosmological observations. Together with SNe Ia Gold sample, WMAP, SDSS and 2dFGRS data, we include 69 long Gamma-Ray Bursts (GRBs) data in our study and perform global fitting using Markov Chain Monte Carlo (MCMC) technique. Dark energy perturbations are explicitly considered. We pay particular attention to the time evolution of the equation of state of dark energy parameterized as wDE = w0 + wa (1 - a) with a the scale factor of the universe, emphasizing the complementarity of high redshift GRBs to other cosmological probes. It is found that the constraints on dark energy become stringent by taking into account high redshift GRBs, especially for wa, which delineates the evolution of dark energy. © 2007 Elsevier B.V. All rights reserved. | - |
dc.language | eng | - |
dc.relation.ispartof | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics | - |
dc.title | Constraints on dark energy models including gamma ray bursts | - |
dc.type | Article | - |
dc.description.nature | link_to_subscribed_fulltext | - |
dc.identifier.doi | 10.1016/j.physletb.2007.10.053 | - |
dc.identifier.scopus | eid_2-s2.0-36849045223 | - |
dc.identifier.volume | 658 | - |
dc.identifier.issue | 4 | - |
dc.identifier.spage | 95 | - |
dc.identifier.epage | 100 | - |
dc.identifier.isi | WOS:000252463600001 | - |
dc.identifier.issnl | 0370-2693 | - |