Strange stars in low-mass binary pulsar systems

International Journal of Modern Physics D

Volumn 8, Issue 6, 1999, Pages 669-675

  Horvath, J E ^a,b  

^a UNIVERSITY OF SÃO PAULO   (Brazil)

^b UNIVERSITY OF ARIZONA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0033270897     PISSN: 02182718     EISSN: None     Source Type: Journal    
DOI: 10.1142/S021827189900047X     Document Type: Article

References (38)

1. D. Bhattacharya and E. P. J. van den Heuvel, Phys. Rep. 203, 1 (1991).
2. E. P. J. van den Heuvel and O. Bitzaraki, Astron. Astrophys. 297, L41 (1995).
3. D. J. Helfand, M. Ruderman and J. Shaham, Nature 304, 423 (1983).
4. E. Witten, Phys. Rev. D30, 272 (1984).
5. C. Alcock, E. Farhi and A. V. Olinto, Astrophys. J. 310, 261 (1986); P. Haensel, J. Zudnik and R. Schaeffer, Astron. Astrophys. 160, 121 (1986).
6. C. Alcock, E. Farhi and A. V. Olinto, Astrophys. J. 310, 261 (1986); P. Haensel, J. Zudnik and R. Schaeffer, Astron. Astrophys. 160, 121 (1986).
7. O. G. Benvenuto, J. E. Horvath and H. Vucetich, Int. J. Mod. Phys. A6, 4769 (1991).
8. A. Bodmer, Phys. Rev. D4, 1601 (1971), see also H. Terazawa, INS Report 338 (INS, Univ. of Tokyo, 1979) and S. A. Chin and A. K. Kerman, Phys. Rev. Lett. 43, 1292 (1979).
9. A. Bodmer, Phys. Rev. D4, 1601 (1971), see also H. Terazawa, INS Report 338 (INS, Univ. of Tokyo, 1979) and S. A. Chin and A. K. Kerman, Phys. Rev. Lett. 43, 1292 (1979).
10. A. Bodmer, Phys. Rev. D4, 1601 (1971), see also H. Terazawa, INS Report 338 (INS, Univ. of Tokyo, 1979) and S. A. Chin and A. K. Kerman, Phys. Rev. Lett. 43, 1292 (1979).
11. O. G. Benvenuto and J. E. Horvath, Phys. Rev. Lett. 63, 716 (1989).
12. M. A. Alpar, Phys. Rev. Lett. 58, 2152 (1987).
13. N. K. Glendenning and F. Weber, Astrophys. J. 400, 647 (1992).
14. O. G. Benvenuto, J. E. Horvath and H. Vucetich, Phys. Rev. Lett. 64, 713 (1990).
15. G. Baym, C. Pethick and P. Sutherland, Astrophys. J. 170, 299 (1971).
16. P. Haensel and J. L. Zdunik, Astron. Astrophys. 229, 117 (1990).
17. Y. F. Huang and T. Lu, Astron. Astrophys. 325, 189 (1997).
18. D. Bailin and A. Love, Phys. Rep. 107, 325 (1984).
19. J. E. Horvath, O. G. Benvenuto and H. Vucetich, Mod. Phys. Lett. A7, 995 (1992).
20. J. E. Horvath, O. G. Benvenuto and H. Vucetich, Phys. Rev. D44, 1147 (1991).
21. C. Schaab, B. Hermann, F. Weber and M. K. Wiegel, Astrophys. J. Lett. 480, 111 (1997).
22. P. Pizzochero, Phys. Rev. Lett. 66, 2425 (1991).
23. H. Heiselberg and C. J. Pethick, Phys. Rev. D48, 2916 (1993), note that this refined calculations give a different behavior than the Fermi liquid theory, e.g. P. Haensel and A. J. Jerzak, Acta Phys. Pol. B20, 141 (1989).
24. H. Heiselberg and C. J. Pethick, Phys. Rev. D48, 2916 (1993), note that this refined calculations give a different behavior than the Fermi liquid theory, e.g. P. Haensel and A. J. Jerzak, Acta Phys. Pol. B20, 141 (1989).
25. D. Bailin and A. Love op. cit., had in fact first speculated that very short expulsion timescales were possible, see also the detailed calculation by H. F. Chau (Astrophys. J. 479, 886 (1997)).
26. D. Bailin and A. Love op. cit., had in fact first speculated that very short expulsion timescales were possible, see also the detailed calculation by H. F. Chau (Astrophys. J. 479, 886 (1997)).
27. M. Ruderman, Astrophys. J. 382, 576 (1991).
28. C. Pethick and M. Sharling, Astrophys. J. 453, L29 (1995).
29. V. A. Urpin, Sov. Astron. 36, 393 (1992).
30. V. A. Urpin and D. G. Yakovlev, Sov. Astron. 24, 303 (1980).
31. E. Flowers and M. A. Ruderman, Astrophys. J. 215, 302 (1977).
32. E. H. Gudmunsson, C. J. Pethick and R. Epstein, Astrophys. J. 272, 286 (1983).
33. V. V. Usov, Astrophys. J. Lett. 481, L107 (1997).
34. M. de Kook and J. van Paradijs, Astron. Astrophys. 173, 279 (1987).
35. T. Schaefer and F. Wilczek, hep-ph/9906512; D. Blaschke, D. M. Sedrakian and K. M. Shahabasyan, astro-ph/9911349.
36. J. Madsen, Phys. Rev. Lett. 81, 3311 (1998).
37. N. Andersson, K. Kokkotas and B. F. Schutz, Astrophys. J. 510, 846 (1999).
38. P. B. Jones, Mon. Not. R.A.S. 246, 364 (1990).