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Constraining the physics of the r‐mode instability in neutron stars with X‐ray and ultraviolet observations
dc.contributor.authorHaskell, Brynmoren_US
dc.contributor.authorDegenaar, Nathalieen_US
dc.contributor.authorHo, Wynn C. G.en_US
dc.date.accessioned2012-07-12T17:25:45Z
dc.date.available2013-09-03T15:38:27Zen_US
dc.date.issued2012-07-21en_US
dc.identifier.citationHaskell, Brynmor; Degenaar, Nathalie; Ho, Wynn C. G. (2012). "Constraining the physics of the r‐mode instability in neutron stars with X‐ray and ultraviolet observations." Monthly Notices of the Royal Astronomical Society 424(1). <http://hdl.handle.net/2027.42/92112>en_US
dc.identifier.issn0035-8711en_US
dc.identifier.issn1365-2966en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/92112
dc.description.abstractRapidly rotating neutron stars in low‐mass X‐ray binaries may be an interesting source of gravitational waves (GWs). In particular, several modes of stellar oscillation may be driven unstable by GW emission, and this can lead to a detectable signal. Here we illustrate how current X‐ray and ultraviolet observations can constrain the physics of the r‐mode instability. We show that the core temperatures inferred from the data would place many systems well inside the unstable region predicted by standard physical models. However, this is at odds with theoretical expectations. We discuss different mechanisms that could be at work in the stellar interior, and we show how they can modify the instability window and make it consistent with the inferred temperatures.en_US
dc.publisherWiley Periodicals, Inc.en_US
dc.publisherBlackwell Publishing Ltden_US
dc.subject.otherGravitational Wavesen_US
dc.subject.otherX‐Rays: Binariesen_US
dc.subject.otherStars: Neutronen_US
dc.titleConstraining the physics of the r‐mode instability in neutron stars with X‐ray and ultraviolet observationsen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelAstronomyen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI 48109, USAen_US
dc.contributor.affiliationotherSchool of Mathematics, University of Southampton, Southampton SO17 1BJen_US
dc.contributor.affiliationotherAstronomical Institute ‘Anton Pannekoek’, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, the Netherlandsen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/92112/1/j.1365-2966.2012.21171.x.pdf
dc.identifier.doi10.1111/j.1365-2966.2012.21171.xen_US
dc.identifier.sourceMonthly Notices of the Royal Astronomical Societyen_US
dc.identifier.citedreferenceOwen B. J., 1995, Phys. Rev. Lett., 95, 211101en_US
dc.identifier.citedreferencePapitto A., Riggio A., Burderi L., di Salvo T., D’Aí A., Iaria R., 2011, A&A, 528, A55en_US
dc.identifier.citedreferencePassamonti A., Haskell B., Andersson N., 2009, MNRAS, 396, 951en_US
dc.identifier.citedreferencePatruno A., 2010, ApJ, 722, 909en_US
dc.identifier.citedreferencePatruno A., Altamirano D., Messenger C., 2010, MNRAS, 403, 1426en_US
dc.identifier.citedreferencePatruno A., Haskell B., D’Angelo C., 2012, ApJ, 746, 9en_US
dc.identifier.citedreferencePethick C., Potekhin A. Y., 1998, Phys. Lett. B, 427, 7en_US
dc.identifier.citedreferencePizzochero P. M., 1991, Phys. Rev. Lett., 66, 2425en_US
dc.identifier.citedreferencePotekhin A. Y., Chabrier G., Yakovlev D. G., 1997, A&A, 323, 415en_US
dc.identifier.citedreferenceRadhakrishnan V., Srinivasan G., 1982, Curr. Sci., 51, 1096en_US
dc.identifier.citedreferenceRezzolla L., Lamb F. K., Shapiro S. L., 2000, ApJ, 531, L139en_US
dc.identifier.citedreferenceRezzolla L., Lamb F. K., Markovic D., Shapiro S. L., 2001a, Phys. Rev. D, 64, 104013en_US
dc.identifier.citedreferenceRezzolla L., Lamb F. K., Markovic D., Shapiro S. L., 2001b, Phys. Rev. D, 64, 104014en_US
dc.identifier.citedreferenceSedrakian A., 2005, Phys. Rev. D, 71, 083003en_US
dc.identifier.citedreferenceShapiro S. L., Teukolsky S. A., 1983, Black Holes, White Dwarfs, and Neutron Stars. John Wiley & Sons, New Yorken_US
dc.identifier.citedreferenceShternin P. S., Yakovlev D. G., Heinke C. O., Ho W. C. G., Patnaude D. J., 2011, MNRAS, 412, L108en_US
dc.identifier.citedreferenceStejner M., Madsen J., 2006, A&A, 458, 523en_US
dc.identifier.citedreferenceUshomirsky G., Cutler C., Bildsten L., 2000, MNRAS, 319, 902en_US
dc.identifier.citedreferenceWagoner R. V., 1984, ApJ, 278, 345en_US
dc.identifier.citedreferenceWatts A. L., Krishnan B., Bildsten L., Schutz B. F., 2008, MNRAS, 389, 839en_US
dc.identifier.citedreferenceWen D.‐H., Newton W. G., Li B.‐A., 2012, Phys. Rev. C, 85, 025801en_US
dc.identifier.citedreferenceWhite N., Zhang W., 1997, ApJ, 490, L87en_US
dc.identifier.citedreferenceWitten E., 1984, Phys. Rev. D, 30, 272en_US
dc.identifier.citedreferenceYakovlev D. G., Levenfish K. P., Potekhin A. Y., Gnedin O. Y., Chabrier G., 2004, A&A, 417, 169en_US
dc.identifier.citedreferenceAbbott B. P. et al., 2010, ApJ, 713, 671en_US
dc.identifier.citedreferenceAlcock C., Farhi E., Olinto A., 1986, ApJ, 310, 261en_US
dc.identifier.citedreferenceAlford M., Schmitt A., Rajagopal K., Schäfer T., 2008, Rev. Modern. Phys., 80, 1455en_US
dc.identifier.citedreferenceAlford M. G., Mahmoodifar S., Schwenzer K., 2012a, Phys. Rev. D, 85, 024007en_US
dc.identifier.citedreferenceAlford M. G., Mahmoodifar S., Schwenzer K., 2012b, Phys. Rev. D, 85, 044051en_US
dc.identifier.citedreferenceAlpar M. A., Cheng A. F., Ruderman M. A., Shaham J., 1982, Nat, 300, 728en_US
dc.identifier.citedreferenceAlpar M. A., Langer S. A., Sauls J. A., 1984, ApJ, 282, 533en_US
dc.identifier.citedreferenceAltamirano D. et al., 2010a, MNRAS, 401, 223en_US
dc.identifier.citedreferenceAltamirano D., Watts A., Linares M., Markwardt C. B., Strohmayer T., Patruno A., 2010b, MNRAS, 409, 1136en_US
dc.identifier.citedreferenceAltamirano D. et al., 2011, ApJ, 727, L18en_US
dc.identifier.citedreferenceAndersson N., 1998, ApJ, 502, 708en_US
dc.identifier.citedreferenceAndersson N., Kokkotas K. D., 2001, Int. J. Modern Phys. D, 10, 381en_US
dc.identifier.citedreferenceAndersson N., Kokkotas K. D., Stergioulas N., 1999, ApJ, 516, 307en_US
dc.identifier.citedreferenceAndersson N., Jones D. I., Kokkotas K. D., 2002, MNRAS, 337, 1224en_US
dc.identifier.citedreferenceAndersson N., Glampedakis K., Haskell B., Watts A. L., 2005, MNRAS, 361, 1153en_US
dc.identifier.citedreferenceAndersson N., Comer G. L., Sidery T. L., 2006, MNRAS, 368, 162en_US
dc.identifier.citedreferenceAndersson N., Glampedakis K., Haskell B., 2009, Phys. Rev. D, 79, 103009en_US
dc.identifier.citedreferenceAndersson N., Haskell B., Comer G. L., 2010, Phys. Rev. D, 82, 023007en_US
dc.identifier.citedreferenceArnaud K. A., 1996, in Jacoby G. H., Barnes J., eds, ASP Conf. Ser. Vol. 101, xspec: The First Ten Years. Astron. Soc. Pac., San Francisco, p. 17en_US
dc.identifier.citedreferenceBaym G., Pethick C. J., Pines D., 1969, Nat, 224, 673en_US
dc.identifier.citedreferenceBildsten L., 1998, ApJ, 501, L89en_US
dc.identifier.citedreferenceBildsten L., Ushomirsky G., 2000, ApJ, 529, L33en_US
dc.identifier.citedreferenceBondarescu R., Teukolsy S. A., Wasserman I., 2007, Phys. Rev. D, 76, 064019en_US
dc.identifier.citedreferenceBrown E. F., Cumming A., 2009, ApJ, 698, 1020en_US
dc.identifier.citedreferenceBrown E. F., Ushomirsky G., 2000, ApJ, 537, 915en_US
dc.identifier.citedreferenceBrown E. F., Bildsten L., Rutledge R. E., 1998, ApJ, 504, L95en_US
dc.identifier.citedreferenceCackett E. M., Wijnands R., Miller J. M., Brown E. F., Degenaar N., 2008, ApJ, 687, L87en_US
dc.identifier.citedreferenceCackett E. M., Brown E. F., Cumming A., Degenaar N., Miller J. M., Wijnands R., 2010, ApJ, 722, L137en_US
dc.identifier.citedreferenceChakrabarty D., Morgan E. H., Muno M. P., Galloway D. K., Wijnands R., van der Klis M., Markwardt C. B., 2003, Nat, 424, 42en_US
dc.identifier.citedreferenceChandrasekhar S., 1970, Phys. Rev. Lett., 24, 611en_US
dc.identifier.citedreferenceCook G. B., Shapiro S. L., Teukolsky S. A., 1994, ApJ, 423, L117en_US
dc.identifier.citedreferenceCuofano C., Drago A., 2010, Phys. Rev. D, 82, 084027en_US
dc.identifier.citedreferenceCutler C., 2002, Phys. Rev. D, 66, 084025en_US
dc.identifier.citedreferenceDegenaar N. D. et al., 2007a, Astron. Telegram, 1091en_US
dc.identifier.citedreferenceDegenaar N. D. et al., 2007b, Astron. Telegram, 1098en_US
dc.identifier.citedreferenceDegenaar N. et al., 2011, MNRAS, 412, 1409en_US
dc.identifier.citedreferenceDegenaar N., Patruno A., Wijnands R., 2012, ApJ, preprint (arXiv:1204.6059)en_US
dc.identifier.citedreferenceDemorest P. B., Penucci T., Ransom S. M., Roberts M. S. E., Hessels J. W. T., 2010, Nat, 467, 1081en_US
dc.identifier.citedreferenceEpstein R. I., Baym G., 1992, ApJ, 387, 276en_US
dc.identifier.citedreferenceFalanga M. et al., 2011, A&A, 529, 68en_US
dc.identifier.citedreferenceFriedman J. L., Morsink S. M., 1998, ApJ, 502, 714en_US
dc.identifier.citedreferenceFriedman J. L., Schutz B. F., 1978, ApJ, 221, 281en_US
dc.identifier.citedreferenceGalloway D. K., Muno M. P., Hartman J. M., Psaltis D., Chakrabarty D., 2008, ApJS, 179, 360en_US
dc.identifier.citedreferenceGearheart M., Newton W. G., Hooker J., Li B., 2011, MNRAS, 418, 2343en_US
dc.identifier.citedreferenceGlampedakis K., Andersson N., 2006, Phys. Rev. D, 74, 044040en_US
dc.identifier.citedreferenceGlendenning N. K., Weber F., 1992, ApJ, 400, 647en_US
dc.identifier.citedreferenceGudmundsson E. H., Pethick C. J., Epstein R. I., 1983, ApJ, 272, 286en_US
dc.identifier.citedreferenceHaensel P., Lasota J. P., Zdunik J. L., 1999, A&A, 344, 151en_US
dc.identifier.citedreferenceHartman J. M., Galloway D. K., Chakrabarty D., 2011, ApJ, 726, 26en_US
dc.identifier.citedreferenceHaskell B., Andersson N., 2010, MNRAS, 408, 1897en_US
dc.identifier.citedreferenceHaskell B., Patruno A., 2011, ApJ, 738, L14en_US
dc.identifier.citedreferenceHaskell B., Jones D. I., Andersson N., 2006, MNRAS, 373, 1423en_US
dc.identifier.citedreferenceHaskell B., Andersson N., Jones D. I., Samuelsson L., 2007, Phys. Rev. Lett., 99, 1101en_US
dc.identifier.citedreferenceHaskell B., Samuelsson L., Glampedakis K., Andersson N., 2008, MNRAS, 385, 531en_US
dc.identifier.citedreferenceHaskell B., Andersson N., Passamonti A., 2009, MNRAS, 397, 1464en_US
dc.identifier.citedreferenceHaskell B., Pizzochero P. M., Sidery T., 2012, MNRAS, 420, 658en_US
dc.identifier.citedreferenceHeinke C. O., Ho W. C. G., 2010, ApJ, 719, L167en_US
dc.identifier.citedreferenceHeinke C. O., Rybicki G. B., Narayan R., Grindlay J. E., 2006, ApJ, 644, 1090en_US
dc.identifier.citedreferenceHeinke C. O., Jonker P. G., Wijnands R., Taam R. E., 2007, ApJ, 660, 1424en_US
dc.identifier.citedreferenceHeinke C. O., Jonker P. G., Wijnands R., Deloye C. K., Taam R. E., 2009, ApJ, 691, 1035en_US
dc.identifier.citedreferenceHeinke C. O. et al., 2010, ApJ, 714, 894en_US
dc.identifier.citedreferenceHeyl J. S., 2002, ApJ, 574, L57en_US
dc.identifier.citedreferenceHo W. C. G., Andersson N., Haskell B., 2011a, Phys. Rev. Lett., 107, 101101en_US
dc.identifier.citedreferenceHo W. C. G., Maccarone T. J., Andersson N., 2011b, ApJ, 730, L36en_US
dc.identifier.citedreferenceHo W. C. G., Glampedakis K., Andersson N., 2012, MNRAS, 422, 2632en_US
dc.identifier.citedreferenceHorowitz C. J., Berry D. K., 2008, Phys. Rev. C, 78, 035806en_US
dc.identifier.citedreferenceItoh N., 1970, Progress Theor. Phys., 44, 291en_US
dc.identifier.citedreferenceJones P. B., 1992, MNRAS, 257, 501en_US
dc.identifier.citedreferenceJones P. B., 2006, MNRAS, 371, 1327en_US
dc.identifier.citedreferenceKargaltsev O., Pavlov G. G., Romani R. W., 2004, ApJ, 602, 327en_US
dc.identifier.citedreferenceLattimer J. M., Prakash M., 2010, preprint (arXiv:1012.3208)en_US
dc.identifier.citedreferenceLevin Y., 1999, ApJ, 517, 328en_US
dc.identifier.citedreferenceLevin Y., Ushomirsky G., 2001, MNRAS, 324, 917en_US
dc.identifier.citedreferenceLindblom L., Mendell G., 2000, Phys. Rev. D, 61, 104003en_US
dc.identifier.citedreferenceLindblom L., Owen B. J., Morsink S. M., 1998, Phys. Rev. Lett., 80, 4843en_US
dc.identifier.citedreferenceLink B., 2003, Phys. Rev. Lett., 91, 101101en_US
dc.identifier.citedreferenceLowell A. W. et al., 2012, ApJ, 749, 111en_US
dc.identifier.citedreferenceMadsen J., 1992, Phys. Rev. D, 46, 3290en_US
dc.identifier.citedreferenceMannarelli M., Manuel C., Sa’d B. A., 2008, Phys. Rev. Lett., 101, 241101en_US
dc.identifier.citedreferenceMelatos A., Payne D. J. B., 2005, ApJ, 623, 1044en_US
dc.identifier.citedreferenceNayyar M., Owen B. J., 2006, Phys. Rev. D, 73, 084001en_US
dc.identifier.citedreferenceOwen B. J., 2010, Phys. Rev. D, 82, 104002en_US
dc.identifier.citedreferenceOwen B. J., Lindblom L., Cutler C., Schutz B. F., Vecchio A., Andersson N., 1998, Phys. Rev. D, 58, 084020en_US
dc.identifier.citedreferencePage D., Usov V. V., 2002, Phys. Rev. Lett., 89, 131101en_US
dc.identifier.citedreferencePage D., Prakash M., Lattimer J. M., Steiner A. W., 2011, Phys. Rev. Lett., 106, 081101en_US
dc.identifier.citedreferencePapaloizou J., Pringle J. E., 1978, MNRAS, 184, 501en_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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