On the Electron Energy Distribution Index of Swift Gamma-ray Burst Afterglows
dc.contributor.author | Curran, Peter | |
dc.contributor.author | Evans, P. | |
dc.contributor.author | De Pasqualea, M. | |
dc.contributor.author | Page, M. | |
dc.contributor.author | van der Horst, A. | |
dc.date.accessioned | 2017-01-30T14:10:54Z | |
dc.date.available | 2017-01-30T14:10:54Z | |
dc.date.created | 2014-11-19T01:13:33Z | |
dc.date.issued | 2010 | |
dc.identifier.citation | Curran, P. and Evans, P. and De Pasqualea, M. and Page, M. and van der Horst, A. 2010. On the Electron Energy Distribution Index of Swift Gamma-ray Burst Afterglows. The Astrophysical Journal Letters. 716: pp. L135-L139. | |
dc.identifier.uri | http://hdl.handle.net/20.500.11937/38025 | |
dc.description.abstract |
The electron energy distribution index, p, is a fundamental parameter of the synchrotron emission from a rangeof astronomical sources. Here we examine one such source of synchrotron emission, gamma-ray burst (GRB)afterglows observed by the Swift satellite. Within the framework of the blast wave model, we examine theconstraints placed on the distribution of p by the observed X-ray spectral indices and parameterize the distribution.We find that the observed distribution of spectral indices are inconsistent with an underlying distribution ofp composed of a single discrete value but consistent with a Gaussian distribution centered at p = 2.36 andhaving a width of 0.59. Furthermore, accepting that the underlying distribution is a Gaussian, we find that themajority ( 94%) of GRB afterglows in our sample have cooling break frequencies less than the X-ray frequency. | |
dc.publisher | Institute of Physics Publishing Ltd. | |
dc.relation.uri | http://iopscience.iop.org/2041-8205/716/2/L135/pdf/apjl_716_2_135.pdf | |
dc.subject | shock waves | |
dc.subject | radiation mechanisms: - non-thermal | |
dc.subject | acceleration of particles | |
dc.subject | gamma-ray burst: general | |
dc.subject | methods: statistical | |
dc.title | On the Electron Energy Distribution Index of Swift Gamma-ray Burst Afterglows | |
dc.type | Journal Article | |
dcterms.source.volume | 716 | |
dcterms.source.startPage | L135 | |
dcterms.source.endPage | L139 | |
dcterms.source.issn | 2041-8205 | |
dcterms.source.title | The Astrophysical Journal Letters | |
curtin.accessStatus | Fulltext not available |