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Impact of r-modes on the cooling of neutron stars

dc.contributor.authorMahmoodifar, Simin
dc.contributor.authorSchwenzer, Kaı Olıver
dc.contributor.authorAlford, Mark G.
dc.date.accessioned2021-03-05T17:43:56Z
dc.date.available2021-03-05T17:43:56Z
dc.identifier.citationAlford M. G. , Mahmoodifar S., Schwenzer K. O. , "Impact of r-modes on the cooling of neutron stars", International Workshop on Quantum Chromodynamics - Theory and Experiment (QCD at Work), Lecce, İtalya, 18 - 21 Haziran 2012, cilt.1492, ss.257-263
dc.identifier.othervv_1032021
dc.identifier.otherav_c6f68f87-7870-45ca-887c-e327773465f1
dc.identifier.urihttp://hdl.handle.net/20.500.12627/131879
dc.identifier.urihttps://doi.org/10.1063/1.4763528
dc.description.abstractStudying the frequency and temperature evolution of a compact star can give us valuable information about the microscopic properties of the matter inside the star. In this paper we study the effect of dissipative reheating of a neutron star due to r-mode oscillations on its temperature evolution. We find that there is still an impact of an r-mode phase on the temperature long after the star has left the instability region and the r-mode is damped completely. With accurate temperature measurements it may be possible to detect this trace of a previous r-mode phase in observed pulsars.
dc.language.isoeng
dc.subjectFİZİK, UYGULAMALI
dc.subjectFizik
dc.subjectBilgisayar Bilimleri
dc.subjectTemel Bilimler
dc.subjectMühendislik ve Teknoloji
dc.subjectMühendislik
dc.subjectMühendislik, Bilişim ve Teknoloji (ENG)
dc.subjectMEKANİK
dc.subjectTemel Bilimler (SCI)
dc.subjectMatematik
dc.subjectMATEMATİK, UYGULAMALI
dc.titleImpact of r-modes on the cooling of neutron stars
dc.typeBildiri
dc.contributor.departmentWashington University (WUSTL) , ,
dc.identifier.volume1492
dc.contributor.firstauthorID728516


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