Learning physics from the cosmic microwave background

Nuclear Physics B - Proceedings Supplements

Volumn 78, Issue 1-3, 1999, Pages 3-13

  Ellis, J ^a  

^a CERN   (Switzerland)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0033236987     PISSN: 09205632     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0920-5632(99)00515-0     Document Type: Article

References (68)

1. G.F. Smoot, astro-ph/9902027.
2. Particle Data Group, C. Caso et al., Eur.Phys.J., C3 (1998) 1.
3. For a review with a constructively critical attitude, see: G.F.R. Ellis, gr-qc/9812046.
4. A great scientific check of this interpretation is to compute successfully the dipole anisotropy using knowledge of the local distribution of matter. see, e.g., M. Hudson, A. Dekel, S. Courteau, S. Faber and J.A. Willick, Mon.Not.Roy.Astron.Soc., 274 (1995) 305.
5. for a recent compilation, see: M. Tegmark, http://www.sns.ias.edu/~max/r_frames.html.
6. A.A. Starobinsky, Phys.Lett., 91B (1980) 99; D. Kazanas, Astrophys.J., 241 (1980) L59; A. Guth, Phys.Rev., D23 (1981) 347.
7. A.A. Starobinsky, Phys.Lett., 91B (1980) 99; D. Kazanas, Astrophys.J., 241 (1980) L59; A. Guth, Phys.Rev., D23 (1981) 347.
8. A.A. Starobinsky, Phys.Lett., 91B (1980) 99; D. Kazanas, Astrophys.J., 241 (1980) L59; A. Guth, Phys.Rev., D23 (1981) 347.
9. J. Preskill, Phys.Rev.Lett., 43 (1979) 1365; Ya. Zel'dovich and M. Khlopov, Phys.Lett., 79B (1979) 239.
10. J. Preskill, Phys.Rev.Lett., 43 (1979) 1365; Ya. Zel'dovich and M. Khlopov, Phys.Lett., 79B (1979) 239.
11. J. Bardeen, P.J. Steinhardt and M.S. Turner, Phys.Rev., D28 (1983) 679; A.H. Guth and S.-Y. Pi, Phys.Rev.Lett., 49 (1982) 1110; A.A. Starobinsky, Phys.Lett., 117B (1982) 175; S.W. Hawking, Phys.Lett., 115B (1982) 295
12. J. Bardeen, P.J. Steinhardt and M.S. Turner, Phys.Rev., D28 (1983) 679; A.H. Guth and S.-Y. Pi, Phys.Rev.Lett., 49 (1982) 1110; A.A. Starobinsky, Phys.Lett., 117B (1982) 175; S.W. Hawking, Phys.Lett., 115B (1982) 295
13. J. Bardeen, P.J. Steinhardt and M.S. Turner, Phys.Rev., D28 (1983) 679; A.H. Guth and S.-Y. Pi, Phys.Rev.Lett., 49 (1982) 1110; A.A. Starobinsky, Phys.Lett., 117B (1982) 175; S.W. Hawking, Phys.Lett., 115B (1982) 295
14. J. Bardeen, P.J. Steinhardt and M.S. Turner, Phys.Rev., D28 (1983) 679; A.H. Guth and S.-Y. Pi, Phys.Rev.Lett., 49 (1982) 1110; A.A. Starobinsky, Phys.Lett., 117B (1982) 175; S.W. Hawking, Phys.Lett., 115B (1982) 295
15. J. Ellis, S. Kelley and D.V. Nanopoulos, Phys.Lett., B249 (1990) 441 and Phys.Lett., B260 (1991) 131; U. Amaldi, W. de Boer and H. Furstenau, Phys.Lett., B260 (1991) 447; P. Langacker and M. Luo, Phys.Rev., D44 (1991) 817.
16. J. Ellis, S. Kelley and D.V. Nanopoulos, Phys.Lett., B249 (1990) 441 and Phys.Lett., B260 (1991) 131; U. Amaldi, W. de Boer and H. Furstenau, Phys.Lett., B260 (1991) 447; P. Langacker and M. Luo, Phys.Rev., D44 (1991) 817.
17. J. Ellis, S. Kelley and D.V. Nanopoulos, Phys.Lett., B249 (1990) 441 and Phys.Lett., B260 (1991) 131; U. Amaldi, W. de Boer and H. Furstenau, Phys.Lett., B260 (1991) 447; P. Langacker and M. Luo, Phys.Rev., D44 (1991) 817.
18. J. Ellis, S. Kelley and D.V. Nanopoulos, Phys.Lett., B249 (1990) 441 and Phys.Lett., B260 (1991) 131; U. Amaldi, W. de Boer and H. Furstenau, Phys.Lett., B260 (1991) 447; P. Langacker and M. Luo, Phys.Rev., D44 (1991) 817.
19. G. Veneziano, hep-th/9902097 and references therein.
20. A.G. Riess et al., astro-ph/9805201; S. Perlmutter et al., astro-ph/9812133.
21. A.G. Riess et al., astro-ph/9805201; S. Perlmutter et al., astro-ph/9812133.
22. S. Kachru and E. Silverstein, hep-th/9810129.
23. P.M. Garnavich et al., astro-ph/9806396; S. Perlmutter, M.S. Turner and M. White, astro-ph/9901052.
24. P.M. Garnavich et al., astro-ph/9806396; S. Perlmutter, M.S. Turner and M. White, astro-ph/9901052.
25. I. Zlatev, L.-M. Wang and P.J. Steinhardt, astro-ph/9807002; P.J. Steinhardt, L.-M. Wang and I. Zlatev, astro-ph/9812313.
26. I. Zlatev, L.-M. Wang and P.J. Steinhardt, astro-ph/9807002; P.J. Steinhardt, L.-M. Wang and I. Zlatev, astro-ph/9812313.
27. J. Ellis, N. Mavromatos and D. Nanopoulos, gr-qc/9810086.
28. T. Yanagida, Proc. Workshop on the Unified Theory and the Baryon Number in the Universe (KEK, Japan, 1979); R. Slansky, Talk at the Sanibel Symposium, Caltech preprint CALT-68-709 (1979).
29. T. Yanagida, Proc. Workshop on the Unified Theory and the Baryon Number in the Universe (KEK, Japan, 1979); R. Slansky, Talk at the Sanibel Symposium, Caltech preprint CALT-68-709 (1979).
30. Super-Kamiokande collaboration, Y. Fukuda et al., Phys.Rev.Lett., 81 (1998) 1562.
31. Y. Oyama, for the K2K collaboration, hep-ex/9803014; MINOS collaboration, E. Ables et al., Fermilab proposal P-875 (1995); G. Acquistapace et al., CERN report 98-02 (1998).
32. Y. Oyama, for the K2K collaboration, hep-ex/9803014; MINOS collaboration, E. Ables et al., Fermilab proposal P-875 (1995); G. Acquistapace et al., CERN report 98-02 (1998).
33. Y. Oyama, for the K2K collaboration, hep-ex/9803014; MINOS collaboration, E. Ables et al., Fermilab proposal P-875 (1995); G. Acquistapace et al., CERN report 98-02 (1998).
34. J.N. Bahcall, astro-ph/9808162.
35. J.M. Cline, hep-ph/9902328.
36. P. Fayet and S. Ferrara, Phys.Rep., 32, 251 (1977); H.E. Haber and G.L. Kane, Phys.Rep., 117, 75 (1985).
37. P. Fayet and S. Ferrara, Phys.Rep., 32, 251 (1977); H.E. Haber and G.L. Kane, Phys.Rep., 117, 75 (1985).
38. L. Maiani, Proc. Summer School on Particle Physics, Gif-sur-Yvette, 1979 (IN2P3, Paris, 1980) p. 3; G 't Hooft, in: G 't Hooft et al., eds., Recent Developments in Field Theories (Plenum Press, New York, 1980); E. Witten, Nucl.Phys., B188 513 (1981); R.K. Kaul, Phys.Lett., 109B 19 (1982).
39. L. Maiani, Proc. Summer School on Particle Physics, Gif-sur-Yvette, 1979 (IN2P3, Paris, 1980) p. 3; G 't Hooft, in: G 't Hooft et al., eds., Recent Developments in Field Theories (Plenum Press, New York, 1980); E. Witten, Nucl.Phys., B188 513 (1981); R.K. Kaul, Phys.Lett., 109B 19 (1982).
40. L. Maiani, Proc. Summer School on Particle Physics, Gif-sur-Yvette, 1979 (IN2P3, Paris, 1980) p. 3; G 't Hooft, in: G 't Hooft et al., eds., Recent Developments in Field Theories (Plenum Press, New York, 1980); E. Witten, Nucl.Phys., B188 513 (1981); R.K. Kaul, Phys.Lett., 109B 19 (1982).
41. L. Maiani, Proc. Summer School on Particle Physics, Gif-sur-Yvette, 1979 (IN2P3, Paris, 1980) p. 3; G 't Hooft, in: G 't Hooft et al., eds., Recent Developments in Field Theories (Plenum Press, New York, 1980); E. Witten, Nucl.Phys., B188 513 (1981); R.K. Kaul, Phys.Lett., 109B 19 (1982).
42. S. Abdullin and F. Charles, hep-ph/9811402.
43. J. Ellis, J.S. Hagelin, D.V. Nanopoulos, K.A. Olive and M. Srednicki, Nucl.Phys., B238, 453 (1984).
44. A. Linde, Phys.Rev., D59 (1999) 023503.
45. A. Linde, M. Sasaki and T. Tanaka, astro-ph/9901135.
46. D. Tytler, S. Burles, L.-M. Wu, X.-M. Fan, A. Wolfe and B.D. Savage, astro-ph/9810217.
47. S. Burles, K.M. Nollett, J.N. Truran and M.S. Turner, astro-ph/9901157.
48. N.A. Bahcall, astro-ph/9901076.
49. Any charged or strongly-interacting sparticle, including the gluino, is probably excluded as a cosmological relic by the stringent experimental upper limits on the abundances of anomalous heavy isotopes [24].
50. J. Ellis, T. Falk, K. Olive and M. Schmitt, Phys.Lett., B388 (1996) 97 and Phys.Lett., B413, 355 (1997).
51. J. Ellis, T. Falk, K. Olive and M. Schmitt, Phys.Lett., B388 (1996) 97 and Phys.Lett., B413, 355 (1997).
52. J. Ellis, T. Falk, G. Ganis, K.A. Olive and M. Schmitt, Phys.Rev., D58 (1998) 095002.
53. P.H. Chankowski, J. Ellis, K.A. Olive and S. Pokorski, hep-ph/9811284.
54. S. Dodelson, E.I. Gates and M.S. Turner, Science, 274 (1996) 69; M.S. Turner, astro-ph/9901168.
55. S. Dodelson, E.I. Gates and M.S. Turner, Science, 274 (1996) 69; M.S. Turner, astro-ph/9901168.
56. W. Hu, D.J. Eisenstein and M. Tegmark, Phys.Rev.Lett., 80 (1998) 5255 and http://www.sns.ias.edu/~whu/pub.html.
57. e∼ 0.2 eV, where the neutrino masses are weighted by their couplings to electrons: L. Baudis et al., hep-ex/9902014.
58. U.-L. Pen, U. Seljak and N.G. Turok, Phys.Rev.Lett., 79 (1997) 1611.
59. However, defect models based on local symmetries are surviving: see C. Contaldi, M. Hindmarsh and J. Magueijo, Phys.Rev.Lett., 82 (1999) 679; and interesting models combining inflation and strings have been proposed: C. Contaldi, M. Hindmarsh and J. Magueijo, astro-ph/9809053; P.P. Avelino, R.R. Caldwell and C.J.A.P. Martins, astro-ph/9809130; R.A. Battye and J. Weller, astro-ph/9810203.
60. However, defect models based on local symmetries are surviving: see C. Contaldi, M. Hindmarsh and J. Magueijo, Phys.Rev.Lett., 82 (1999) 679; and interesting models combining inflation and strings have been proposed: C. Contaldi, M. Hindmarsh and J. Magueijo, astro-ph/9809053; P.P. Avelino, R.R. Caldwell and C.J.A.P. Martins, astro-ph/9809130; R.A. Battye and J. Weller, astro-ph/9810203.
61. However, defect models based on local symmetries are surviving: see C. Contaldi, M. Hindmarsh and J. Magueijo, Phys.Rev.Lett., 82 (1999) 679; and interesting models combining inflation and strings have been proposed: C. Contaldi, M. Hindmarsh and J. Magueijo, astro-ph/9809053; P.P. Avelino, R.R. Caldwell and C.J.A.P. Martins, astro-ph/9809130; R.A. Battye and J. Weller, astro-ph/9810203.
62. However, defect models based on local symmetries are surviving: see C. Contaldi, M. Hindmarsh and J. Magueijo, Phys.Rev.Lett., 82 (1999) 679; and interesting models combining inflation and strings have been proposed: C. Contaldi, M. Hindmarsh and J. Magueijo, astro-ph/9809053; P.P. Avelino, R.R. Caldwell and C.J.A.P. Martins, astro-ph/9809130; R.A. Battye and J. Weller, astro-ph/9810203.
63. A.N. Lasenby, S.L. Bridle and M.P. Hobson, astro-ph/9901303.
64. R.E. Lopez, S. Dodelson, A. Heckler and M.S. Turner, astro-ph/9803095.
65. M. Grünewald and D. Karlen, talks at International Conference on High-energy Physics, Vancouver 1998, http://www.cern.ch/LEPEWWG/misc.
66. R.E. Lopez, S. Dodelson, R.J. Scherrer and M.S. Turner, Phys.Rev.Lett., 81 (1998) 3075, and references therein.
67. E.J. Copeland, I.J. Grivell, E.W. Kolb and A.R. Liddle, Phys.Rev., D58 (1998) 043002, and references therein.
68. W.H. Kinney, Phys.Rev., D58 (1998) 12350.