Inhomogeneous cosmological models - New exact solutions with dust, isotropic radiation, and electromagnetic field

1987 ◽  
Vol 317 ◽  
pp. 52 ◽  
Author(s):  
Nazira Tomimura ◽  
Ioav Waga
2011 ◽  
Vol 28 (16) ◽  
pp. 164002 ◽  
Author(s):  
Krzysztof Bolejko ◽  
Marie-Noëlle Célérier ◽  
Andrzej Krasiński

2014 ◽  
Vol 11 (05) ◽  
pp. 1450050
Author(s):  
Rafael M. Rubio ◽  
Juan J. Salamanca

A new approach for arbitrary dimension to the Friedmann cosmological models is presented. Taking suitable changes of the parameters of the spacetime the harmonic motion equations appear, where the curvature determines the angular frequency. Some physical interpretations are also explained. As a consequence of our approach, we give new exact solutions to the Einstein's equation when the observer is not comoving with the perfect fluid, as well as, when the pressure not vanishes, including a new procedure to acquire exact solutions for cases of universes at the dark energy-dominated stage.


Author(s):  
Sobia Younus

<span>Some new exact solutions to the equations governing the steady plane motion of an in compressible<span> fluid of variable viscosity for the chosen form of the vorticity distribution are determined by using<span> transformation technique. In this case the vorticity distribution is proportional to the stream function<span> perturbed by the product of a uniform stream and an exponential stream<br /><br class="Apple-interchange-newline" /></span></span></span></span>


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