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Article: Maximum mass and radius of strange stars in the linear approximation of the EOS
Title | Maximum mass and radius of strange stars in the linear approximation of the EOS |
---|---|
Authors | |
Keywords | Dense matter Equation of state Stars: fundamental parameters |
Issue Date | 2002 |
Publisher | E D P Sciences. The Journal's web site is located at http://www.aanda.org |
Citation | Astronomy And Astrophysics, 2002, v. 385 n. 3, p. 947-950 How to Cite? |
Abstract | The Chandrasekhar limit for strange stars described by a linear equation of state (describing quark matter with density-dependent quark masses) is evaluated. The maximum mass and radius of the star depend on the fundamental constants and on the energy density of the quark matter at zero pressure. By comparing the expression for the mass of the star with the limiting mass formula for a relativistic degenerate stellar configuration one can obtain an estimate of the mass of the strange quark. |
Persistent Identifier | http://hdl.handle.net/10722/91875 |
ISSN | 2023 Impact Factor: 5.4 2023 SCImago Journal Rankings: 1.896 |
ISI Accession Number ID | |
References |
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Harko, T | en_HK |
dc.contributor.author | Cheng, KS | en_HK |
dc.date.accessioned | 2010-09-17T10:29:09Z | - |
dc.date.available | 2010-09-17T10:29:09Z | - |
dc.date.issued | 2002 | en_HK |
dc.identifier.citation | Astronomy And Astrophysics, 2002, v. 385 n. 3, p. 947-950 | en_HK |
dc.identifier.issn | 0004-6361 | en_HK |
dc.identifier.uri | http://hdl.handle.net/10722/91875 | - |
dc.description.abstract | The Chandrasekhar limit for strange stars described by a linear equation of state (describing quark matter with density-dependent quark masses) is evaluated. The maximum mass and radius of the star depend on the fundamental constants and on the energy density of the quark matter at zero pressure. By comparing the expression for the mass of the star with the limiting mass formula for a relativistic degenerate stellar configuration one can obtain an estimate of the mass of the strange quark. | en_HK |
dc.language | eng | en_HK |
dc.publisher | E D P Sciences. The Journal's web site is located at http://www.aanda.org | en_HK |
dc.relation.ispartof | Astronomy and Astrophysics | en_HK |
dc.subject | Dense matter | en_HK |
dc.subject | Equation of state | en_HK |
dc.subject | Stars: fundamental parameters | en_HK |
dc.title | Maximum mass and radius of strange stars in the linear approximation of the EOS | en_HK |
dc.type | Article | en_HK |
dc.identifier.email | Harko, T: harko@hkucc.hku.hk | en_HK |
dc.identifier.email | Cheng, KS: hrspksc@hkucc.hku.hk | en_HK |
dc.identifier.authority | Harko, T=rp01333 | en_HK |
dc.identifier.authority | Cheng, KS=rp00675 | en_HK |
dc.description.nature | link_to_subscribed_fulltext | - |
dc.identifier.scopus | eid_2-s2.0-0036531542 | en_HK |
dc.relation.references | http://www.scopus.com/mlt/select.url?eid=2-s2.0-0036531542&selection=ref&src=s&origin=recordpage | en_HK |
dc.identifier.volume | 385 | en_HK |
dc.identifier.issue | 3 | en_HK |
dc.identifier.spage | 947 | en_HK |
dc.identifier.epage | 950 | en_HK |
dc.identifier.isi | WOS:000174901700024 | - |
dc.publisher.place | France | en_HK |
dc.identifier.scopusauthorid | Harko, T=7006485783 | en_HK |
dc.identifier.scopusauthorid | Cheng, KS=9745798500 | en_HK |
dc.identifier.issnl | 0004-6361 | - |