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Prog. Theor. Phys. Vol. 70 No. 6 (1983) pp. 1556-1568

[ Full Text PDF : FREE ACCESS (589K) ]

Super-Weakly Interacting Particles and the Formation of Galaxies and Clusters of Galaxies

Tetsuya Hara

Department of Physics, Kyoto Sangyo University, Kyoto 603

(Received July 4, 1983)

Abstract:

We investigate whether adiabatic perturbations of massive neutrinos grow enough, during the matter-dominated era before and after decoupling, to explain the formation of clusters of galaxies, using the upper bounds on the small scale temperature fluctuations of the cosmic background radiation. The results are negative and similar constraints are derived for other super-weakly interacting particles. If we assume that the initial perturbations scale as δ∼M-1/2-n/6, then no objects form before z=3.78 for n=1, constant curvature fluctuations, whatever super-weakly interacting particle is introduced.


URL : http://ptp.ipap.jp/link?PTP/70/1556/
DOI : 10.1143/PTP.70.1556

[ Full Text PDF : FREE ACCESS (589K) ] Citation:

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Citing Article(s) :

  1. Progress of Theoretical Physics Vol. 72 No. 2 (1984) pp. 216-232 :
    Nonlinear Growth of Density Contrast and Formation of Galaxies in a Neutrino-Dominated Universe
    Satoru Ikeuchi and Masayuki Umemura
  2. Progress of Theoretical Physics Vol. 77 No. 5 (1987) pp. 1152-1162 :
    Formation of the First Systems in the Wakes of Moving Cosmic Strings
    Tetsuya Hara and Shigeru Miyoshi
  3. Progress of Theoretical Physics Vol. 83 No. 4 (1990) pp. 660-665 :
    Decrease of Velocity Differences between Baryonic Objects and Cold Dark Matter
    Tetsuya Hara and Shigeru Miyoshi

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