Chaotic new inflation and primordial spectrum of adiabatic fluctuations

1999 ◽  
Vol 59 (10) ◽  
Author(s):  
Jun’ichi Yokoyama
1983 ◽  
Vol 104 ◽  
pp. 219-221
Author(s):  
S. A. Bonometto ◽  
F. Lucchin

The isothermal theories of galaxy formation encounter serious difficulties in accounting for the existence of large voids (see, e.g., Aarseth and Saslow 1982). The alternative picture of adiabatic fluctuations and pancake collapse (see, e.g., Doroshkevich et al. 1978 and references therein) faces difficulties due to: i) observed correlation functions, and ii) the absence of small-scale fluctuations in the microwave background.


1992 ◽  
Vol 9 ◽  
pp. 319-321
Author(s):  
J. Richard Bond

Constraints on models of cosmic structure formation that can be drawn from current limits on large angle microwave background anisotropies are now competitive with those from recent small and intermediate angle experiments and are relatively insensitive to the reheating history of the Universe. Here I give limits on Gaussian scale invariant adiabatic fluctuations and describe the role that the large angle results play in constraining models with enhanced large distance galaxy clustering power inferred from correlation function measurements is described.


2009 ◽  
Vol 2009 (07) ◽  
pp. 015-015 ◽  
Author(s):  
Robert H Brandenberger ◽  
Tomo Takahashi ◽  
Masahide Yamaguchi

1978 ◽  
Vol 79 ◽  
pp. 448-449
Author(s):  
J. Jaaniste ◽  
E. Saar

The cosmological turbulence theory and the theory of adiabatic fluctuations predict different orientations of galaxies in clusters and superclusters. the first theory favours the alignment of the planes of galaxies with the supergalactic plane, whereas the planes of spiral galaxies formed according to the second theory are perpendicular to the plane of a supergalaxy.


1998 ◽  
Vol 31 (36) ◽  
pp. 7301-7313
Author(s):  
Suman Kumar Banik ◽  
Jyotipratim Ray Chaudhuri ◽  
Deb Shankar Ray

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