Joel R. Primack (auth.), David B. Cline (eds.)'s Sources and Detection of Dark Matter and Dark Energy in the PDF

By Joel R. Primack (auth.), David B. Cline (eds.)

ISBN-10: 3642074464

ISBN-13: 9783642074462

ISBN-10: 3662045877

ISBN-13: 9783662045879

Dark subject study is without doubt one of the such a lot attention-grabbing and energetic fields between present high-profile clinical endeavors. It holds the main to all significant breakthroughs to come back within the fields of cosmology and astroparticle physics. the current quantity is very focused on the resources and the detection of darkish topic and darkish strength within the universe and should end up to be a useful learn software for all scientists who paintings during this field.

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H. P. Kirshner: ApJ 473, 88 (1996) 104. G. : AJ 116, 1009 (1998) 105. G. V. Filippenko, W. P. Schmidt: AJ 118, 2668 (1999) 106. G. Riess: astroph/0005229 (2000) 107. G. : ApJ 536, 62 (2000) 108. A. Rosenberg, I. Saviane, G. Piotto, A. Aparicio: AJ 118, 2306 (1999) 109. M. RowanRobinson: The Cosmological Distance Ladder (Freeman, New York 1985) 110. P. : ApJ 439, 60 (1995) 111. A. Saha, A. A. Tammann, L. D. Macchetto, N. Panagia: ApJ 522, 802 (1999) 112. D. : ApJ 464, L63 (1996) 113. P. : ApJ 475, L85 (1997) 114.

58, 689 (1986) 43. L. : ApJ 529, 745 (2000) 44. A. H. R. Primack: astroph/9909397 (1999) 45. W. : ApJ submitted (2000) 46. Y. : Phys. Rev. Lett. 81, 1562 (1998) 47. M. C. Liu, N. Sugiyama: hepph/9908450 (1999) 3. 4. 5. 6. 7. 8. 9. 10. 11. 12. 13. 14. 15. 16. 17. 18. 19. 20. 21. 16 48. 49. 50. 51. 52. 53. 54. 55. 56. 57. 58. 59. 60. 61. 62. 63. 64. 65. 66. 67. 68. 69. 70. 71. 72. 73. 74. 75. 76. 77. 78. 79. 80. 81. 82. 83. 84. 85. 86. 87. 88. 89. 90. 91. 92. 93. 94. 95. Primack P. : ApJ, 493, L53 (1998) E.

A particularly simple way to deduce a lower limit on Dm from the POTENT peculiar velocity data was proposed by [31], based on the fact that high-velocity outflows from voids are not expected in low-il models. L. Stronger constraints are available if we assume that the probability distribution function (PDF) of the primordial fluctuations was Gaussian. e. large Dm. , the PDF of the mass, if the POTENT reconstruction is reliable) is far from Gaussian today, with a long positive-fluctuation tail. 3 is ruled out at ~ 4a [87,10].

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Sources and Detection of Dark Matter and Dark Energy in the Universe: Fourth International Symposium Held at Marina del Rey, CA, USA February 23–25, 2000 by Joel R. Primack (auth.), David B. Cline (eds.)


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