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A young cooling neutron star in the remnant of Supernova 1987A

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Abstract

We describe the cooling theory for isolated neutron stars that are several tens of years old. Their cooling differs greatly from the cooling of older stars that has been well studied in the literature. It is sensitive to the physics of the inner stellar crust and even to the thermal conductivity of the stellar core, which is never important at later cooling stages. The absence of observational evidence for the formation of a neutron star during the explosion of Supernova 1987A is consistent with the fact that the star was actually born there. It may still be hidden in the dense center of the supernova remnant. If, however, the star is not hidden, then it should have a low thermal luminosity (below ∼1034 erg s−1) and a short internal thermal relaxation time (shorter than 13 yr). This requires that the star undergo intense neutrino cooling (e.g., via the direct Urca process) and have a thin crust with strong superfluidity of free neutrons and/or an anomalously high thermal conductivity.

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References

  1. D. Arnett, Supernovae and Nucleosynthesis: An Investigation of the History of Matter, from the Big Bang to the Present (Princeton: Princeton Univ. Press, 1996).

    Google Scholar 

  2. D. A. Baiko, P. Haensel, and D. G. Yakovlev, Astron. Astrophys. 374, 151 (2001).

    Article  ADS  Google Scholar 

  3. M. Bejger, D. G. Yakovlev, and O. Y. Gnedin, Acta Physica Polonica B 34, 223 (2003).

    ADS  Google Scholar 

  4. D. N. Burrows, E. Michael, U. Hwang, et al., Astrophys. J. 543, L149 (2000).

    Article  ADS  Google Scholar 

  5. L. Dessart, A. Burrows, E. Livne, and C. D. Ott, Astrophys. J. 645, 534 (2006).

    Article  ADS  Google Scholar 

  6. E. Flowers and N. Itoh, Astrophys. J. 206, 218 (1976).

    Article  ADS  Google Scholar 

  7. E. Flowers and N. Itoh, Astrophys. J. 230, 847 (1979).

    Article  ADS  Google Scholar 

  8. C. Fransson and R. A. Chevalier, Astrophys. J. 322, L15 (1987).

    Article  ADS  Google Scholar 

  9. C. L. Fryer, S. A. Colgate, and P.A. Pinto, Astrophys. J. 511, 885 (1999).

    Article  ADS  Google Scholar 

  10. U. Geppert, D. Page, and T. Zannias, Astron. Astrophys. 345, 847 (1999).

    ADS  Google Scholar 

  11. O. Y. Gnedin, D. G. Yakovlev, and A. Y. Potekhin, Mon. Not. R. Astron. Soc. 324, 725 (2001).

    Article  ADS  Google Scholar 

  12. G. J. M. Graves, P. M. Challis, R. A. Chevalier, et al., Astrophys. J. 629, 944 (2005).

    Article  ADS  Google Scholar 

  13. F. Haberl, U. Geppert, B. Aschenbach, and G. Hasinger, Astron. Astrophys. 460, 811 (2006).

    Article  ADS  Google Scholar 

  14. P. Haensel, A. Y. Potekhin, and D. G. Yakovlev, Neutron Stars. 1. Equation of State and Structure (N.Y.: Springer, 2007).

    Google Scholar 

  15. H. Heiselberg and C. J. Pethick, Phys. Rev. D 48, 2916 (1993).

    Article  ADS  Google Scholar 

  16. S. Immler, K. Weiler, and R. McCray, Eds., Supernova 1987A: 20 Years after: Supernovae and Gamma-Ray Bursters, AIP Conf. Proc. 937 (2007).

  17. V. S. Imshennik and D. K. Nadyozhin, Usp. Fiz. Nauk 156, 561 (1988).

    Google Scholar 

  18. V. S. Imshennik and O. G. Ryazhskaya, Pis’ma Astron. Zh. 30, 17 (2004) [Astron. Lett. 30, 14 (2004)].

    Google Scholar 

  19. V. S. Imshennik and I. Yu. Litvinova, Yad. Fiz. 69, 660 (2006) [Phys. At. Nucl. 69, 636 (2006)].

    Google Scholar 

  20. A. D. Kaminker, D. G. Yakovlev, and O. Y. Gnedin, Astron. Astrophys. 383, 1076 (2002).

    Article  ADS  Google Scholar 

  21. J. M. Lattimer, C. J. Pethick, M. Prakash, and P. Haensel, Phys. Rev. Lett. 66, 2701 (1991).

    Article  ADS  Google Scholar 

  22. J. M. Lattimer, K. A. van Riper, M. Prakash, and M. Prakash, Astrophys. J. 425, 802 (1994).

    Article  ADS  Google Scholar 

  23. R. N. Manchester, AIP Conf. Proc. 937, 134 (2007).

    Article  ADS  Google Scholar 

  24. J. A. Miralles, V. Urpin, and K. Van Riper, Astrophys. J. 480, 358 (1997).

    Article  ADS  Google Scholar 

  25. A. Muslimov and D. Page, Astrophys. J. 440, 77 (1995).

    Article  ADS  Google Scholar 

  26. K. Nomoto and S. Tsuruta, Astrophys. J. 312, 711 (1987).

    Article  ADS  Google Scholar 

  27. D. Page, U. Geppert, and F. Weber, Nucl. Phys. A 777, 497 (2006).

    Article  ADS  Google Scholar 

  28. D. Page and J. H. Applegate, Astrophys. J. 394, L17 (1992).

    Article  ADS  Google Scholar 

  29. S. Park, S. A. Zhekov, D. N. Burrows, et al., Astrophys. J. 610, 275 (2004).

    Article  ADS  Google Scholar 

  30. J. W. Percival, P. T. Boyd, J. D. Biggs, et al., Astrophys. J. 446, 832 (1995).

    Article  ADS  Google Scholar 

  31. A. Y. Potekhin, G. Chabrier, and D. G. Yakovlev, Astron. Astrophys. 323, 415 (1997).

    ADS  Google Scholar 

  32. M. Prakash, T. L. Ainsworth, and J. M. Lattimer, Phys. Rev. Lett. 61, 2518 (1988).

    Article  ADS  Google Scholar 

  33. S. Shapiro and S. Teukolsky, Black Holes, White Dwarfs, and Neutron Stars: The Physics of Compact Objects (Wiley, New York, 1983; Mir, Moscow, 1985).

    Google Scholar 

  34. Yu. A. Shibanov, A. Y. Potekhin, D. G. Yakovlev, and V. E. Zavlin, The Many Faces of Neutron Stars (Dordrecht: Kluwer, 1998), p. 553.

    Google Scholar 

  35. P. S. Shternin and D. G. Yakovlev, Phys. Rev. D 74, 043004 (2006).

    Google Scholar 

  36. P. S. Shternin and D. G. Yakovlev, Phys. Rev. D 75, 103 004 (2007).

    Google Scholar 

  37. P. E. Shtykovskiy, A. A. Lutovinov, M. R. Gilianov, and R. A. Sunyaev, Pis’ma Astron. Zh. 31, 258 (2005) [Astron. Lett. 31, 258 (2005)].

    Google Scholar 

  38. K. S. Thorne, Astrophys. J. 212, 825 (1977).

    Article  ADS  Google Scholar 

  39. D. R. Tilley and J. Tilley, Superfluidity and Superconductivity (Bristol: IOP Publ., 1990).

    Google Scholar 

  40. S. E. Woosley and T. A. Weaver, Astrophys. J. Suppl. Ser. 101, 181 (1995).

    Article  ADS  Google Scholar 

  41. D. G. Yakovlev, A. D. Kaminker, O. Y. Gnedin, and P. Haensel, Phys. Rep. 354, 1 (2001).

    Article  ADS  Google Scholar 

  42. D. G. Yakovlev and C. J. Pethick, Annu. Rev. Astron. Astrophys. 42, 169 (2004).

    Article  ADS  Google Scholar 

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Authors and Affiliations

  1. Ioffe Physicotechnical Institute, Russian Academy of Sciences, ul. Politekhnicheskaya 26, St. Petersburg, 194021, Russia

    P. S. Shternin & D. G. Yakovlev

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  1. P. S. Shternin
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  2. D. G. Yakovlev
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Correspondence to D. G. Yakovlev.

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Original Russian Text © P.S. Shternin, D.G. Yakovlev, 2008, published in Pis’ma v Astronomicheskiĭ Zhurnal, 2008, Vol. 34, No. 10, pp. 746–756.

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Shternin, P.S., Yakovlev, D.G. A young cooling neutron star in the remnant of Supernova 1987A. Astron. Lett. 34, 675–685 (2008). https://doi.org/10.1134/S1063773708100034

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  • DOI: https://doi.org/10.1134/S1063773708100034

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