Alternative approach to the galactic dark matter problem

Physical Review D

Volumn 63, Issue 12, 2001, Pages

  Nucamendi, Ulises ^a   Salgado, Marcelo ^a   Sudarsky, Daniel ^b  

^a UNIVERSITY OF SUSSEX   (United Kingdom)

^b UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; COSMOLOGICAL PHENOMENA; MATHEMATICAL ANALYSIS; MOLECULAR DYNAMICS; MOTION; QUANTUM MECHANICS; ROTATION; THEORY;

EID: 85037885745     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.63.125016     Document Type: Article

References (60)

1. V. C. Rubin, Science 220, 1339 (1983).
2. M. S. Turner, Phys. Scr. T36, 167 (1991).
3. J. R. Primack, in Elementary Particles, Proceedings of the International School of Physics "Enrico Fermi," Vol. 92, edited by N. Cabibbo (North Holland, Amsterdam, 1988), p. 137.
4. J. Wess and B. Zumino, Nucl. Phys. B70, 39 (1974).
5. E. W. Kolb and M. S. Turner, The Early Universe (Addison Wesley, Redwood City, CA, 1990).
6. B. J. Carr, J. R. Bond, and \V. D. Arnett, Astrophys. J. 277, 445 (1984)
7. C. Alcock et al., Astrophys. J. 486, 697 (1997).
8. P. J. E. Peebles, Principles of Physical Cosmology (Princeton University Press, Princeton, 1993).
9. Steven Weinberg, Gravitation and Cosmology: Principles and Applications of the General Theory of Relativity (Wiley, New York, 1972).
10. C. J. Copi, D. N. Schramm, and B. M. Tinsley, Science 267, 192 (1995)
11. J. A. Sellwood and A. Kosowsky, astro-ph/0009074.
12. A. Finzi, Mon. Not. R. Astron. Soc. 127, 21 (1963).
13. R. H. Sanders, Astron. Astrophys. 136, L21 (1984).
14. M. Milgrom, Astrophys. J. 270, 365 (1983).
15. P. D. Mannheim, Astrophys. J. 479, 659 (1997);
16. 419, 150 (1993).
17. M. Persic, P. Salucci, and F. Stel, Mon. Not. R. Astron. Soc. 281, 27 (1996).
18. V. C. Rubin, W. K. Ford, and N. Thonnard, Astrophys. J. 238, 471 (1980);
19. V. C. Rubin, W. K. Ford, N. Thonnard, and D urstein, ibid. 261, 439 (1982);
20. 289, 81 (1985).
21. V. B. Braginskii and V. I. Panov, Zh. Éksp. Teor. Fiz. 61, 873 (1971)
22. [Sov. Phys. JETP 34, 463 (1972)].
23. M. Heusler, J. Math. Phys. 33, 3497 (1992);
24. Class. Quantum Grav. 12, 779 (1995).
25. D. Sudarsky, Class. Quantum Grav. 12, 579 (1995).
26. J. D. Bekenstein, Phys. Rev. D 51, R6608 (1995).
27. T. Matos, F. S. Guzman, and Dario Nunez, Phys. Rev. D 62, 061301(R) (2000).
28. P. J. E. Peebles, astro-ph/0002495; A. Riotto and I. Tkachev, Phys. Lett. B 484, 177 (2000); J. Goodman, astro-ph/0003018.
29. T. Damour and G. Esposito-Farèse, Phys. Rev. Lett. 70, 2220 (1993);
30. Phys. Rev. D 54, 1474 (1996);
31. 58, 042001 (1998).
32. M. Salgado, D. Sudarky, and U. Nucamendi, Phys. Rev. D 58, 124003 (1998).
33. U. Nucamendi, M. Salgado, and D. Sudarsky, Phys. Rev. Lett. 84, 3037 (2000).
34. I. Pena and D. Sudarsky, Class. Quantum Grav. 14, 3131 (1997).
35. M. Barriola and A. Vilenkin, Phys. Rev. Lett. 63, 341 (1989).
36. D. Harari and C. Lousto, Phys. Rev. D 42, 2626 (1990).
37. A. Edery, Phys. Rev. Lett. 83, 3990 (1999).
38. J. D. Bekenstein, M. Milgrom, and R. H. Sanders, Phys. Rev. Lett. 85, 1346 (2000).
39. U. Nucamendi and D. Sudarsky, Class. Quantum Grav. 14, 1309 (1997).
40. D. Zaritsky, R. Smith, C. S. Frenk, and S. D. M. White, Astrophys. J. 405, 464 (1993);
41. D. Zaritsky and S. D. M. White, ibid. 435, 599 (1994).
42. T. Brainerd, R. Blanford, and I. Smail, Astrophys. J. 466, 623 (1996).
43. A. S. Kulessa and D. Lynden-Bell, Mon. Not. R. Astron. Soc. 255, 105 (1992);
44. C. S. Kochanek, Astrophys. J. 457, 228 (1996).
45. D. Zaritsky, R. Smith, C. S. Frenk, and S. D. M. White, Astrophys. J. 478, 39 (1997).
46. Those contributions are: that which is associated with the energy density of the scalar field and the other which is associated with the reduction of the negative binding energy due to the reduction of G due to a nonzero value of the scalar field: G- l/( 1 + \6nC2) with £>0.
47. F. E. Schunck, in Proceedings of the 8th Marcel Grossmann Meeting, edited by T. Piran (World Scientific, Singapore, 1999), p. 1447; F. E. Schunck, astro-ph/9802258.
48. M. Colpi, S. L. Shapiro, and I. Wasserman, Phys. Rev. Lett. 57, 2485 (1986).
49. I. Pena and D. Sudarsky, Class. Quantum Grav. 18, 1461 (2001).
50. W. A. Hiscock, Phys. Rev. Lett. 64, 344 (1990).
51. R. M. Wald (private communication).
52. W. Press, B. P. Flannery, S. A. Teukolsky, and W. T. Vetterling, Numerical Recipes: The Art of Scientific Computing (Cambridge University Press, Cambridge, England, 1986), p. 578.
53. R. B. Tully and J. R. Fisher, Astron. Astrophys. 54, 661 (1977).
54. T. Barreiro, E. J. Copeland, and N. J. Nunes, Phys. Rev. D 61, 127301 (2000).
55. P. de Berdarnis et al. Nature (London) 404, 955 (2000);
56. S. Hanany et al, Astrophys. J. Lett. 545, L5 (2000);
57. U. L. Pen, U. Seljak, and N. Turok, Phys. Rev. Lett. 79, 1611 (1997);
58. R. Durrer, M. Kunz, and A. Melchiorri, Phys. Rev. D 59, 123005 (1999).
59. A. G. Riess et al, Astron. J. 116, 1009 (1998);
60. S. Perlmutter et al, Astrophys. J. 517, 565 (1999).