scholarly journals On creation of scalar particles with Gauss-Bonnet type coupling to curvature in Friedmann cosmological models

2014 ◽  
Vol 20 (1) ◽  
pp. 21-25
Author(s):  
Yu. V. Pavlov
1974 ◽  
Vol 63 ◽  
pp. 273-282
Author(s):  
I. D. Novikov

Observations primarily of the microwave background radiation show that the Universe expands isotropically with a high degree of accuracy at the present time and that the matter distribution is homogeneous on a large scale. Thus, the Friedmann cosmological models are a good approximation today for the expanding Universe. This is valid for at least some period of time in the past too. But how did the Universe expand and what was the matter distribution close to the starting point, near the cosmological singularity?


1980 ◽  
Vol 23 (7) ◽  
pp. 545-548
Author(s):  
I. L. Bukhbinder

1996 ◽  
Vol 472 (1) ◽  
pp. 25-33 ◽  
Author(s):  
John M. Horack ◽  
Thomas M. Koshut ◽  
Robert S. Mallozzi ◽  
A. Gordon Emslie ◽  
Charles A. Meegan

1987 ◽  
Vol 36 (4) ◽  
pp. 1032-1035 ◽  
Author(s):  
M. Rosenbaum ◽  
M. Ryan ◽  
L. Urrutia ◽  
Richard Matzner

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