Quantum fluctuations of axions

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 58, Issue 10, 1998, Pages

  Singh, Anupam ^b   Srednicki, Mark ^b  

^a NASA FERMILAB ASTROPHYSICS CENTER   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 1542629882     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.58.105004     Document Type: Article

References (62)

1. Particle Physics and Cosmology: Dark Matter, edited by M. Srednicki (Elsevier, New York, 1990).
2. E. W. Kolb and M. S. Turner, The Early Universe (Addison-Wesley, Reading, MA, 1990).
3. G. Jungman, M. Kamionkowski and K. Griest, Phys. Rep. 267, 195 (1996).
4. J. Preskill, M. Wise and F. Wilczek, Phys. Lett. 120B, 127 (1983).
5. L. Abbott and P. Sikivie, Phys. Lett. 120B, 133 (1983).
6. M. Dine and W. Fischler, Phys. Lett. 120B, 137 (1983).
7. R. Peccei and H. Quinn, Phys. Rev. Lett. 38, 1440 (1977);
8. Phys. Rev. Lett.S. Weinberg, 40, 223 (1978);
9. Phys. Rev. Lett.F. Wilczek, 40, 279 (1978);
10. M. Dine, W. Fischler, and M. Srednicki, Phys. Lett. 104B, 199 (1981).
11. T. Banks and M. Dine, Nucl. Phys. B505, 445 (1997);
12. K. Choi, E. Chun, and J. Kim, Phys. Lett. B 403, 209 (1997).
13. A. Guth and S.-Y. Pi, Phys. Rev. D 32, 1899 (1985).
14. E. Weinberg and A. Wu, Phys. Rev. D 36, 2474 (1987).
15. D. Boyanovsky and H. J. de Vega, Phys. Rev. D 47, 2343 (1993).
16. D. Boyanovsky, D-S Lee, and A. Singh, Phys. Rev. D 48, 800 (1993).
17. J. Traschen and R. Brandenberger, Phys. Rev. D 42, 2491 (1990);
18. Phys. Rev. DY. Shtanov, J. Traschen, and R. Brandenberger, 51, 5438 (1995).
19. L. A. Kofman, A. Linde, and A. Starobinksy, Phys. Rev. Lett. 73, 3195 (1994).
20. D. Boyanovsky, H. J. de Vega, R. Holman, D.-S. Lee, and A. Singh, Phys. Rev. D 51, 4419 (1995);
21. Phys. Rev. DD. Boyanovsky, M. D’Attanasio, H. J. de Vega, R. Holman, and D. S. Lee, 52, 6805 (1995).
22. David B. Kaplan, Nucl. Phys. B260, 215 (1985).
23. Mark Srednicki, Nucl. Phys. B260, 689 (1985).
24. D. Boyanovsky, H. J. de Vega, R. Holman, and J. F. J. Salgado, Phys. Rev. D 54, 7570 (1996).
25. F. Cooper and E. Mottola, Mod. Phys. Lett. A 2, 635 (1987);
26. F. Cooper, S. Habib, Y. Kluger, E. Mottola, J. P. Paz, and P. R. Anderson, Phys. Rev. D 50, 2848 (1994);
27. Phys. Rev. DF. Cooper, S. Habib, Y. Kluger, and E. Mottola, 55, 6471 (1997).
28. O. Eboli, R. Jackiw, and S.-Y. Pi, Phys. Rev. D 37, 3557 (1988);
29. Phys. Rev. DM. Samiullah, O. Eboli, and S-Y. Pi, 44, 2335 (1991).
30. L. A. Kofman, A. D. Linde, and A. A. Starobinsky, Phys. Rev. Lett. 76, 1011 (1996).
31. E. W. Kolb, A. D. Linde, and A. Riotto, Phys. Rev. Lett. 77, 4290 (1996).
32. G. W. Anderson, A. D. Linde, and A. Riotto, Phys. Rev. Lett. 77, 3716 (1996).
33. E. W. Kolb and A. Riotto, Phys. Rev. D 55, 3313 (1997);
34. A. Riotto and I. I. Tkachev, Phys. Lett. B 385, 57 (1996);
35. S. Yu. Khlebnikov and I. I. Tkachev, Phys. Rev. Lett. 77, 219 (1996);
36. S. Yu. Khlebnikov and I. I. Tkachev, Phys. Lett. B 390, 80 (1997).
37. D. T. Son, Phys. Rev. D 54, 3745 (1996).
38. D. I. Kaiser, Phys. Rev. D 53, 1776 (1996).
39. H. Fujisaki, K. Kumekawa, M. Yamaguchi, and M. Yoshimura, Phys. Rev. D 53, 6805 (1996);
40. M. Yoshimura, Prog. Theor. Phys. 94, 873 (1995).
41. D. Boyanovsky, D. Cormier, H. J. de Vega, R. Holman, A. Singh, and M. Srednicki, Phys. Rev. D 56, 1939 (1997).
42. J. Schwinger, J. Math. Phys. 2, 407 (1961);
43. J. Math. Phys.P. M. Bakshi and K. T. Mahanthappa, 4, 1 (1963);
44. J. Math. Phys.P. M. BakshiK. T. Mahanthappa4, 12 (1963);
45. L. V. Keldysh, Sov. Phys. JETP 20, 1018 (1965);
46. A. Niemi and G. Semenoff, Ann. Phys. (N.Y.) 152, 105 (1984);
47. A. NiemiG. SemenoffNucl. Phys.B230 [FS10], 181 (1984);
48. E. Calzetta, Ann. Phys. (N.Y.) 190, 32 (1989);
49. R. D. Jordan, Phys. Rev. D 33, 444 (1986);
50. N. P. Landsman and C. G. van Weert, Phys. Rep. 145, 141 (1987);
51. R. L. Kobes and K. L. Kowalski, Phys. Rev. D 34, 513 (1986);
52. R. L. Kobes, G. W. Semenoff, and N. Weiss, Z. Phys. C 29, 371 (1985).
53. For a thorough exposition of non-equilibrium methods in cosmology see, for example: E. Calzetta and B.-L. Hu, Phys. Rev. D 35, 495 (1988);
54. Phys. Rev. DE. CalzettaB.-L. Hu37, 2838 (1988);
55. Phys. Rev. DJ. P. Paz, 41, 1054 (1990);
56. Phys. Rev. DJ. P. Paz42, 529 (1990);B.-L. Hu, in Bannf/Cap Workshop on Thermal Field Theories: Proceedings, edited by F. C. Khanna, R. Kobes, G. Kunstatter, and H. Umezawa (World Scientific, Singapore, 1994), p. 309 andin the Proceedings of the Second Paris Cosmology Colloquium, Observatoire de Paris, edited by H. J. de Vega and N. Sánchez (World Scientific, Singapore, 1995), p. 111 and references therein.
57. D. Boyanovsky, H. J. de Vega, and R. Holman, Phys. Rev. D 49, 2769 (1994).
58. D. Gross, R. Pisarski, and L. Yaffe, Rev. Mod. Phys. 53, 43 (1981).
59. For a discussion of this point and related cosmological issues please see section 10.3 of Ref. 2.
60. K. Freese, J. Frieman, and A. Olinto, Phys. Rev. Lett. 65, 3233 (1990);
61. F. Adams, J. R. Bond, K. Freese, J. Frieman, and A. Olinto, Phys. Rev. D 47, 426 (1993).
62. D. Cormier, R. Holman, and S. P. Kumar (work in progress);and (private communication).