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Article: GRB afterglows: Deep Newtonian phase and its application

TitleGRB afterglows: Deep Newtonian phase and its application
Authors
Huang, YFLu, TCheng, KS
Issue Date2005
PublisherSocieta Italiana di Fisica.
Citation
Nuovo Cimento Della Societa Italiana Di Fisica C, 2005, v. 28 n. 3, p. 415-418 How to Cite?
DOI: http://dx.doi.org/10.1393/ncc/i2005-10141-2
AbstractGamma-ray burst afterglows have been observed for months or even years in a few cases. It is worth noting that at such late stages, the remnants should have entered the deep Newtonian phase, during which the majority of shock-accelerated electrons will no longer be highly relativistic. To calculate the afterglows, we must assume that the electrons obey a power law distribution according to their kinetic energy, not simply the Lorentz factor. © Società Italiana di Fisica.
Persistent Identifierhttp://hdl.handle.net/10722/80871
ISSN
1124-1896
ISI Accession Number ID
WOS:000233646000038
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorHuang, YFen_HK
dc.contributor.authorLu, Ten_HK
dc.contributor.authorCheng, KSen_HK
dc.date.accessioned2010-09-06T08:11:11Z-
dc.date.available2010-09-06T08:11:11Z-
dc.date.issued2005en_HK
dc.identifier.citationNuovo Cimento Della Societa Italiana Di Fisica C, 2005, v. 28 n. 3, p. 415-418en_HK
dc.identifier.issn1124-1896en_HK
dc.identifier.urihttp://hdl.handle.net/10722/80871-
dc.description.abstractGamma-ray burst afterglows have been observed for months or even years in a few cases. It is worth noting that at such late stages, the remnants should have entered the deep Newtonian phase, during which the majority of shock-accelerated electrons will no longer be highly relativistic. To calculate the afterglows, we must assume that the electrons obey a power law distribution according to their kinetic energy, not simply the Lorentz factor. © Società Italiana di Fisica.en_HK
dc.languageengen_HK
dc.publisherSocieta Italiana di Fisica.en_HK
dc.relation.ispartofNuovo Cimento della Societa Italiana di Fisica Cen_HK
dc.titleGRB afterglows: Deep Newtonian phase and its applicationen_HK
dc.typeArticleen_HK
dc.identifier.emailCheng, KS: hrspksc@hkucc.hku.hken_HK
dc.identifier.authorityCheng, KS=rp00675en_HK
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1393/ncc/i2005-10141-2en_HK
dc.identifier.scopuseid_2-s2.0-28744435662en_HK
dc.identifier.hkuros113167en_HK
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-28744435662&selection=ref&src=s&origin=recordpageen_HK
dc.identifier.volume28en_HK
dc.identifier.issue3en_HK
dc.identifier.spage415en_HK
dc.identifier.epage418en_HK
dc.identifier.isiWOS:000233646000038-
dc.identifier.scopusauthoridHuang, YF=7501574835en_HK
dc.identifier.scopusauthoridLu, T=7402684810en_HK
dc.identifier.scopusauthoridCheng, KS=9745798500en_HK
dc.identifier.issnl1124-1896-

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