3 Cornell and the Rotating Universe

Vera Rubin ◽  
2021 ◽  
pp. 46-62
Keyword(s):  
2003 ◽  
Vol 46 (10) ◽  
pp. 999-1009 ◽  
Author(s):  
E. V. Kufshinova ◽  
V. F. Panov
Keyword(s):  

1978 ◽  
Vol 225 ◽  
pp. 719 ◽  
Author(s):  
M. Novello ◽  
M. J. Reboucas

Nature ◽  
1946 ◽  
Vol 158 (4016) ◽  
pp. 549-549 ◽  
Author(s):  
G. GAMOW
Keyword(s):  

1972 ◽  
Vol 25 (3) ◽  
pp. 233-244 ◽  
Author(s):  
M. Demiański ◽  
L. P. Grishchuk
Keyword(s):  

1979 ◽  
Vol 70 (3) ◽  
pp. 161-163 ◽  
Author(s):  
M.J. Rebouças
Keyword(s):  

2011 ◽  
Vol 20 (09) ◽  
pp. 1643-1673 ◽  
Author(s):  
WŁODZIMIERZ GODŁOWSKI

In this paper we discussed the observational aspects of rotation in the Universe on different scales. We show dependence between the angular momentum of the structures and their size. The presented observational situation is that the galaxies, their pairs and compact groups have a non-vanishing angular momentum. In the structures of mass corresponding to groups of galaxies, this feature has not been found, while in the clusters and superclusters, alignment of galaxy orientation has been actually found. Also we know that galaxies have net angular momentum due to the fact that we actually measure the rotation curves of galaxies. These facts lead to the conclusion that theories which connect galaxy angular momentum with its surrounding structure are at some extend favored by data. We show that in the light of scenarios of galaxy formations this result could be interpreted as an effect of tidal force's mechanism, but it is also consistent with Li's model, in which galaxies form in the rotating universe. The theoretical and observational aspects of possible global rotation of the Universe were discussed as well.


1982 ◽  
Vol 67 (1) ◽  
pp. 120-126 ◽  
Author(s):  
M. J. Rebouças

2018 ◽  
Vol 4 (1) ◽  
Author(s):  
Jean-Pierre Luminet

Discovered in 1949 by Kurt Gödel, the homogeneous rotating universe model contains closed timelike curves and therefore allows for travel into the past, accompanied by all its paradoxes.


1979 ◽  
Vol 19 (10) ◽  
pp. 2850-2852 ◽  
Author(s):  
M. Novello ◽  
M. J. Reboucas
Keyword(s):  

2002 ◽  
Vol 11 (05) ◽  
pp. 733-737
Author(s):  
L. C. GARCIA DE ANDRADE

A rotating universe represented by the Gödel metric in spacetimes with Cartan torsion is investigated. The spin–torsion coupling is shown to contribute to the structure formation in an apppreciable way only at the early stages of the universe. To demonstrate these conjectures, we have made use of a spinning fluid model in Einstein–Cartan gravity. We also show that autoparallel equation in Riemann–Cartan spacetime leads to the evolution equation of the cosmological perturbation where the spin-rotation coupling contributes to the growth of inhomogeneities through a constant term. From this idea, one is able to estimate that torsion in the Planck era is around 1015 s -1 where COBE constraint on temperature fluctuations is used in this computation. A spin density of the universe of 1053 g · cm -1 s -1 is also obtained in our framework.


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