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Article: Cosmic-ray positrons produced by pulsar winds from mature gamma-ray pulsars
Title | Cosmic-ray positrons produced by pulsar winds from mature gamma-ray pulsars |
---|---|
Authors | |
Issue Date | 2001 |
Publisher | Zhongguo Wuli Xuehui & Institute of Physics Publishing Ltd. The Journal's web site is located at http://www.iop.org/EJ/journal/CPL |
Citation | Chinese Physics Letters, 2001, v. 18 n. 5, p. 701-704 How to Cite? |
Abstract | In the frame of the γ-ray pulsar outer gap model, e± pairs in the pulsar magnetosphere are produced by the cascade of e± pairs through synchrotron radiation of the return current from the outer gap. These pairs are accelerated mono-energetically to relativistic energies in the pulsar wind driven by low-frequency electromagnetic waves. Using Monte Carlo simulations, we generate a sample of the mature γ-ray pulsars in our Galaxy and calculate the positron production rate from these pulsars. With a simple leaky box model, we calculate the ratio of cosmic-ray positron to total electrons. Our result indicates that the pulsar contribution to the cosmic-ray positron peaks at about 40 GeV and the observed e+/(e- + e+) ratio can be explained by this model. |
Persistent Identifier | http://hdl.handle.net/10722/80438 |
ISSN | 2023 Impact Factor: 3.5 2023 SCImago Journal Rankings: 0.815 |
References |
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Zhang, L | en_HK |
dc.contributor.author | Cheng, KS | en_HK |
dc.contributor.author | Mei, DC | en_HK |
dc.date.accessioned | 2010-09-06T08:06:27Z | - |
dc.date.available | 2010-09-06T08:06:27Z | - |
dc.date.issued | 2001 | en_HK |
dc.identifier.citation | Chinese Physics Letters, 2001, v. 18 n. 5, p. 701-704 | en_HK |
dc.identifier.issn | 0256-307X | en_HK |
dc.identifier.uri | http://hdl.handle.net/10722/80438 | - |
dc.description.abstract | In the frame of the γ-ray pulsar outer gap model, e± pairs in the pulsar magnetosphere are produced by the cascade of e± pairs through synchrotron radiation of the return current from the outer gap. These pairs are accelerated mono-energetically to relativistic energies in the pulsar wind driven by low-frequency electromagnetic waves. Using Monte Carlo simulations, we generate a sample of the mature γ-ray pulsars in our Galaxy and calculate the positron production rate from these pulsars. With a simple leaky box model, we calculate the ratio of cosmic-ray positron to total electrons. Our result indicates that the pulsar contribution to the cosmic-ray positron peaks at about 40 GeV and the observed e+/(e- + e+) ratio can be explained by this model. | en_HK |
dc.language | eng | en_HK |
dc.publisher | Zhongguo Wuli Xuehui & Institute of Physics Publishing Ltd. The Journal's web site is located at http://www.iop.org/EJ/journal/CPL | en_HK |
dc.relation.ispartof | Chinese Physics Letters | en_HK |
dc.title | Cosmic-ray positrons produced by pulsar winds from mature gamma-ray pulsars | en_HK |
dc.type | Article | en_HK |
dc.identifier.openurl | http://library.hku.hk:4550/resserv?sid=HKU:IR&issn=0256-307X&volume=18&spage=701&epage=704&date=2001&atitle=Cosmic-ray+positrons+produced+by+pulsar+winds+from+mature+gamma-ray+pulsars | en_HK |
dc.identifier.email | Cheng, KS: hrspksc@hkucc.hku.hk | en_HK |
dc.identifier.authority | Cheng, KS=rp00675 | en_HK |
dc.description.nature | link_to_subscribed_fulltext | - |
dc.identifier.doi | 10.1088/0256-307X/18/5/326 | en_HK |
dc.identifier.scopus | eid_2-s2.0-0035629221 | en_HK |
dc.identifier.hkuros | 77471 | en_HK |
dc.relation.references | http://www.scopus.com/mlt/select.url?eid=2-s2.0-0035629221&selection=ref&src=s&origin=recordpage | en_HK |
dc.identifier.volume | 18 | en_HK |
dc.identifier.issue | 5 | en_HK |
dc.identifier.spage | 701 | en_HK |
dc.identifier.epage | 704 | en_HK |
dc.publisher.place | China | en_HK |
dc.identifier.scopusauthorid | Zhang, L=9432987500 | en_HK |
dc.identifier.scopusauthorid | Cheng, KS=9745798500 | en_HK |
dc.identifier.scopusauthorid | Mei, DC=7005968649 | en_HK |
dc.identifier.issnl | 0256-307X | - |