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Article: Gravitational waves from phase transitions of accreting neutron stars

TitleGravitational waves from phase transitions of accreting neutron stars
Authors
Cheng, KSDai, ZG
KeywordsDense matter
Gravitation
Pulsars: general
Stars: neutron
Stars: oscillations
Issue Date1998
PublisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205
Citation
Astrophysical Journal Letters, 1998, v. 492 n. 1 PART I, p. 281-285 How to Cite?
DOI: http://dx.doi.org/10.1086/305040
AbstractWe propose that when neutron stars in low-mass X-ray binaries accrete sufficient mass and become millisecond pulsars, the interiors of these stars may undergo phase transitions, exciting stellar radial oscillations. We show that the radial oscillations will be mainly damped by gravitational-wave radiation instead of internal viscosity. Such gravitational waves may be detected by the advanced Laser Interferometer Gravitational-wave Observatory. © 1998. The American Astronomical Society. All rights reserved.
Persistent Identifierhttp://hdl.handle.net/10722/43215
ISSN
2041-8205
2023 Impact Factor: 8.8
2023 SCImago Journal Rankings: 2.766
ISI Accession Number ID
WOS:000071389300025
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorCheng, KSen_HK
dc.contributor.authorDai, ZGen_HK
dc.date.accessioned2007-03-23T04:41:29Z-
dc.date.available2007-03-23T04:41:29Z-
dc.date.issued1998en_HK
dc.identifier.citationAstrophysical Journal Letters, 1998, v. 492 n. 1 PART I, p. 281-285en_HK
dc.identifier.issn2041-8205en_HK
dc.identifier.urihttp://hdl.handle.net/10722/43215-
dc.description.abstractWe propose that when neutron stars in low-mass X-ray binaries accrete sufficient mass and become millisecond pulsars, the interiors of these stars may undergo phase transitions, exciting stellar radial oscillations. We show that the radial oscillations will be mainly damped by gravitational-wave radiation instead of internal viscosity. Such gravitational waves may be detected by the advanced Laser Interferometer Gravitational-wave Observatory. © 1998. The American Astronomical Society. All rights reserved.en_HK
dc.format.extent232683 bytes-
dc.format.extent12158 bytes-
dc.format.mimetypeapplication/pdf-
dc.format.mimetypetext/plain-
dc.languageengen_HK
dc.publisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205en_HK
dc.relation.ispartofAstrophysical Journal Lettersen_HK
dc.rightsThe Astrophysical Journal. Copyright © University of Chicago Press.en_HK
dc.subjectDense matteren_HK
dc.subjectGravitationen_HK
dc.subjectPulsars: generalen_HK
dc.subjectStars: neutronen_HK
dc.subjectStars: oscillationsen_HK
dc.titleGravitational waves from phase transitions of accreting neutron starsen_HK
dc.typeArticleen_HK
dc.identifier.openurlhttp://library.hku.hk:4550/resserv?sid=HKU:IR&issn=0004-637X&volume=492&issue=pt 1&spage=281&epage=285&date=1998&atitle=Gravitational+Waves+from+Phase+Transitions+of+Accreting+Neutron+Starsen_HK
dc.identifier.emailCheng, KS: hrspksc@hkucc.hku.hken_HK
dc.identifier.authorityCheng, KS=rp00675en_HK
dc.description.naturepublished_or_final_versionen_HK
dc.identifier.doi10.1086/305040en_HK
dc.identifier.scopuseid_2-s2.0-13944275729en_HK
dc.identifier.hkuros29778-
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-13944275729&selection=ref&src=s&origin=recordpageen_HK
dc.identifier.volume492en_HK
dc.identifier.issue1 PART Ien_HK
dc.identifier.spage281en_HK
dc.identifier.epage285en_HK
dc.identifier.isiWOS:000071389300025-
dc.publisher.placeUnited Kingdomen_HK
dc.identifier.scopusauthoridCheng, KS=9745798500en_HK
dc.identifier.scopusauthoridDai, ZG=7201387760en_HK
dc.identifier.issnl2041-8205-

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