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Article: GRB afterglows: Deep Newtonian phase and its application

TitleGRB afterglows: Deep Newtonian phase and its application
Authors
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?
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
2008 Impact Factor: 0.277
2015 SCImago Journal Rankings: 0.204
ISI Accession Number ID
References

 

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

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