Quick Search:
Prog. Theor. Phys. Vol. 47 No. 2 (1972) pp. 416-443
Non-Linear Theory of Gravitational Instability in the Expanding Universe. III
Kenji Tomita
Research Institute for Theoretical Physics, Hiroshima University, Takehara, Hiroshima-ken
(Received August 7, 1971)
Abstract:
First it is indicated that, at the radiation-dominated stage of the expanding universe, two ways should be distinguished for the evolution of the second-order density waves most naturally associated with the first-order rotational and gravitational waves, and the behavior of an isolated eddy is examined for a comparison with those of periodically distributed eddies.
Next the second-order waves associated with rotational, density and their mixed waves at the intermediate stage (before and after the decoupling epoch tD) are analyzed and the rapidity of compression due to the inertial force appearing soon after tD is calculated.
Finally the possibility of galaxy formation is examined on the basis of the above analysis. Moreover a possibility for comparatively small galaxies to be formed through the cascade due to non-linear process is considered.
URL :
http://ptp.ipap.jp/link?PTP/47/416/
DOI : 10.1143/PTP.47.416
References:
- K. Tomita, Prog. Theor. Phys. 37 (1967), 831[PTP].
- K. Tomita, Prog. Theor. Phys. 45 (1971), 1747[PTP].
- E. M. Lifshitz, J. Phys. USSR 10 (1946), 116.
E. M. Lifshitz and I. M. Khalatnikov, Adv. Phys. 12 (1963), 185; Sov. Phys.-Uspekhi 6 (1964), 495.
- L. M. Ozernoi and A. D. Chernin, Sov. Astron. -AJ 11 (1968), 907; ibid. 12 (1969), 901.
- L. M. Ozernoi and G. V. Chibisov, Astrophys. Lett. 7 (1971), 201; Sov. Astron. -AJ 14 (1971), 615.
- H. Satō, T. Matsuda and H. Takeda, Prog. Theor. Phys. 43 (1970), 1115[PTP].
- H. Satō, Prog. Theor. Phys. 45 (1971), 370[PTP].
- K. Tomita, H. Nariai, H. Satō, T. Matsuda and H. Takeda, Prog. Theor. Phys. 43 (1970), 1511[PTP].
- L. M. Ozernoi, Sov. Phys. -JETP Lett. 10 (1969), 251.
-
C. F. von Weizsäcker, Astrophys. J. 114 (1951), 165[CrossRef].
-
J. Kristian and R. K. Sachs, Astrophys. J. 143 (1966), 379[CrossRef].
H. Satō, Prog. Theor. Phys. 40 (1968), 781[PTP].
-
E. K. Conklin and R. N. Bracewell, Nature 216 (1967), 777[CrossRef];
Phys. Rev. Lett. 18 (1967), 614[APS].
D. T. Wilkinson and R. B. Partridge, Nature 215 (1967), 719.
- H. Nariai, K. Tomita and S. Kato, Prog. Theor. Phys. 37 (1967), 60[PTP].
Citing Article(s) :
-
Progress of Theoretical Physics Vol. 48 No. 5 (1972) pp. 1503-1516
:
-
Primordial Irregularities in the Early Universe
-
Kenji Tomita
-
Progress of Theoretical Physics Vol. 49 No. 5 (1973) pp. 1770-1772
:
-
The Sound Generated by Cosmic Turbulence and the Origin of Galaxies
-
Takuya Matsuda, Hidenori Takeda and Humitaka Sato
-
Progress of Theoretical Physics Vol. 50 No. 2 (1973) pp. 472-487
:
-
On the Generatin of Sound from the Primordial Turbulence in an Expanding Universe
-
Hidekazu Nariai
-
Progress of Theoretical Physics Vol. 50 No. 4 (1973) pp. 1285-1301
:
-
Element Formation in a Chaotic Early Universe
-
Kenji Tomita
-
Progress of Theoretical Physics Vol. 54 No. 3 (1975) pp. 719-729
:
-
On the Acoustic Decay of Primordial Cosmic Turbulence
-
Kenji Tanabe, Hidekazu Nariai, Takuya Matsuda and Hidenori Takeda
-
Progress of Theoretical Physics Vol. 59 No. 4 (1978) pp. 1150-1169
:
-
On Inhomogeneous Cosmological Models Containing Space-Like and Time-Like Singularities Alternately
-
Kenji Tomita
-
Progress of Theoretical Physics Vol. 67 No. 4 (1982) pp. 1093-1106
:
-
Galaxy Formation in the Neutrino Dominated Universe
-
Kenji Tomita
-
Progress of Theoretical Physics Vol. 69 No. 3 (1983) pp. 828-841
:
-
Large-Scale Anisotropy of the Cosmic Background Radiation Due to Primordial Density and Gravitational-Wave Perturbations
-
Kenji Tomita and Kenji Tanabe
-
Progress of Theoretical Physics Vol. 117 No. 1 (2007) pp. 17-74
:
-
Second-Order Gauge Invariant Cosmological Perturbation Theory
-
Kouji Nakamura