Missing Parameters in the CMB Physics

  • Pavel D. Naselsky
Conference paper
Part of the NATO Science Series book series (NAII, volume 130)

Abstract

The lecture is devoted to the comparison of a few models of cosmic recombination kinetics with recent CMB anisotropy data and to corresponding predictions for the upcoming PLANCK mission. The influence of additional sources of ionized photons at the epoch of hydrogen recombination may restrict our possibility to estimate the density of baryonic fraction of matter when using PLANCK data. This new source of degeneracy of the cosmological parameters which can be estimated from the CMB anisotropy data can mimic the distortion of the CMB power spectrum for different models of baryonic matter. I would like to point out that realistic values of the cosmological parameters can not be obtained without PLANCK polarization data.

Keywords

Cosmological Model Cosmic Microwave Background Cosmological Parameter High Redshift Primordial Black Hole 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Abu-Zayyad et al., 2001, ApJ, 557, 686ADSCrossRefGoogle Scholar
  2. Adams, J.A., Sarkar, S. & Sciama D.W., 1998, MNRAS, 301, 210ADSCrossRefGoogle Scholar
  3. Ave, M.,et al., Phys. Rev. Lett., 85, 2244, 2000ADSCrossRefGoogle Scholar
  4. Avelino, P., Martins, C, Rocha, G., & Viana, P., 2000, Phys. Rev. D, 62, 123508ADSCrossRefGoogle Scholar
  5. Battye, R., Crittenden, R., & Weiler, J., 2001, Phys. Rev. D, 63, 043505ADSCrossRefGoogle Scholar
  6. Bhattacharjee P. & Sigl, G. 2000, Phys. Rept., 327, 109ADSCrossRefGoogle Scholar
  7. Berezinsky, V. S., Bulanov, S. V., Dogel, V. A., Ginzburg, V. L. and V. S. Ptuskin, Astrophysics of Cosmic Rays, (North Holland, Amsterdam, 1990)Google Scholar
  8. Berezinsky, V. S., Kashelrieß, M. & A. Vilenkin, 1997, Phys. Rev. Lett, 79, 4302ADSCrossRefGoogle Scholar
  9. Berezinsky, V.S., Blasi, P. and A. Vilenkin, 1998, Phys. Rev. D, 58, 103515ADSCrossRefGoogle Scholar
  10. Birkel M. and Sarkar, S. 1998, Astropart. Phys., 9, 297ADSCrossRefGoogle Scholar
  11. de Bernardis, P., et al., 2000, Nature, 404, 955ADSCrossRefGoogle Scholar
  12. Blasi, P.,1999, Phys.Rev.D, 60, 023514,.Google Scholar
  13. Doroshkevich A. G., & Naselsky, P. D., 2002, Phys. Rev. D, 65, 123517ADSCrossRefGoogle Scholar
  14. Doroshkevich A. G., Naselsky, LP., Naselsky, P. D. & Novikov, L,D., 2002, astro-ph/0208114Google Scholar
  15. Ellis, J., Gelmini, G., Lopez, J., Nanopoulos, D., & Sarkar, S., 1992, Nucl. Phys. B, 373, 399ADSCrossRefGoogle Scholar
  16. Halverson, N. W., 2002, ApJ, 568, 38ADSCrossRefGoogle Scholar
  17. Hayashida, N., et al, 1994, Phys. Rev. Lett, 73, 3491.ADSCrossRefGoogle Scholar
  18. Hanany, S., et al., 2000, ApJ, 545, L5ADSCrossRefGoogle Scholar
  19. Greisen, K. 1966, Phys. Rev. Lett., 16, 748.ADSCrossRefGoogle Scholar
  20. Jones, B. J. T., & Wyse R., 1985, A&A, 149, 144ADSGoogle Scholar
  21. Yoshida, S. & H. Dai, 1998., J. Phys.G, 24, 905.ADSCrossRefGoogle Scholar
  22. Ivanov, P.B., Naselsky, P.D. and Novikov, I.D., 1994, Phys. Rev.D, 50, 7173.ADSCrossRefGoogle Scholar
  23. Kotok, E.V. and Naselsky, P.D.,1998, Phys. Rev.D, 58,103517.ADSCrossRefGoogle Scholar
  24. Kovac, J., et al., 2002, astro-ph 0209478.Google Scholar
  25. Kuzmin, V.A., & V.A. Rubakov, 1998, Yader.Fiz., 61, 1122Google Scholar
  26. Landau, S., Harari, D., & Zaldarriaga, M., 2001, Phys. Rev.D, 63, 3505Google Scholar
  27. Lawrence, M. A., Reid, R. J. O. & Watson, A. A., 1991, J. Phys. G., Nucl.Part.Phys., 17, 733ADSCrossRefGoogle Scholar
  28. Mason, B. S., et al., 2002, astro-ph/0205384Google Scholar
  29. Naselsky, P. D., 1978, Sov. Astron. Lett., 344, 4Google Scholar
  30. Naselsky, P. D., & Polnarev, a. G., 1987, Sov. Astron. Lett., 13, 67ADSGoogle Scholar
  31. Naselsky, P.D., & Novikov, I.,D., 2002, MNRAS, 334, 137ADSCrossRefGoogle Scholar
  32. Peebles, P., 1968, ApJ, 153, 1ADSCrossRefGoogle Scholar
  33. Peebles, P., Seager, S., & Hu, W., 2000, ApJ, 539, L1ADSCrossRefGoogle Scholar
  34. Protheroe, R.J., & Biermann, P. L., 1996, Astrop. Physics, 6, 45ADSCrossRefGoogle Scholar
  35. Protheroe, R.J., Stanev, T., and V.S. Berezinsky, 1995, astro-ph/9409004Google Scholar
  36. Rybicki, G. B and Lightman, A. P., 1979, Radiative processes in astrophysics, A Wiley-Interscience publicationGoogle Scholar
  37. Sarkar, S., and Toldra, R., 2002, Nucí. Phys., B621, 495ADSCrossRefGoogle Scholar
  38. Sarkar, S., & Cooper, a., 1983, Phys. Lett. B, 148, 347ADSGoogle Scholar
  39. Scott, D., Rees, M.,J., & Sciama, D., W., 1991, A&A, 250, 295ADSGoogle Scholar
  40. Seager, S., Sasselov, D., & Scott, D., 1999, ApJ, 523, L1ADSCrossRefGoogle Scholar
  41. Seljak, U., & Zaldarriaga, M., 1966, ApJ, 469, 437ADSCrossRefGoogle Scholar
  42. Sigl, G., 2001, hep-ph/0109202Google Scholar
  43. Tegmark, M., 2001, A&AS, 199, 3407Google Scholar
  44. Zabotin, N. A., & Naselsky, P. D., 1982, Sov. Astron., 26, 272ADSGoogle Scholar
  45. Zatsepin G.T., and Kuzmin, V.A.,1966, Pis’ma Zh. Eksp.Theor.Fiz., 4, 114,; JETP. Lett., 4, 78, 1966. Zel’dovich, Ya. B., Kurt, V.,& Sunuyaev, R.A., 1968, Zh. Eksp. Theor. Phys., 55, 278 Watson, R. A., et al., 2002, astro-ph/0205378Google Scholar

Copyright information

© Springer Science+Business Media Dordrecht 2003

Authors and Affiliations

  • Pavel D. Naselsky
    • 1
    • 2
    • 3
  1. 1.Theoretical Astrophysics CenterCopenhagenDenmark
  2. 2.Niels Bohr InstituteCopenhagenDenmark
  3. 3.Rostov State UniversityRostov-DonRussia

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