A comment on an exact solution with a stiff equation of state

1990 ◽  
Vol 22 (6) ◽  
pp. 715-717 ◽  
Author(s):  
Henning Knutsen
2012 ◽  
Vol 21 (12) ◽  
pp. 1250085 ◽  
Author(s):  
ANTONIO ENEA ROMANO

We address some recent erroneous claim that H0 observations are difficult to accommodate with LTB cosmological models, showing how to construct solutions in agreement with an arbitrary value of H0 by rewriting the exact solution in terms of dimensionless parameters and functions. This approach can be applied to fully exploit LTB solutions in designing models alternative to dark energy without making any restrictive or implicit assumption about the inhomogeneity profile. The same solution can also be used to study structure formation in the regime in which perturbation theory is not enough and an exact solution of the Einstein's equation is required, or to estimate the effects of a local inhomogeneities on the apparent equation of state of dark energy.


2002 ◽  
Vol 580 (2) ◽  
pp. 1043-1047 ◽  
Author(s):  
Timothy M. Braje ◽  
Roger W. Romani

2021 ◽  
Vol 104 (12) ◽  
Author(s):  
Kazuo Ghoroku ◽  
Kouji Kashiwa ◽  
Yoshimasa Nakano ◽  
Motoi Tachibana ◽  
Fumihiko Toyoda

2008 ◽  
Vol 08 (02) ◽  
pp. L141-L153
Author(s):  
THEO M. NIEUWENHUIZEN

Within the Relativistic Theory of Gravitation it is shown that the equation of state p = ρ holds near the center of a black hole. For the stiff equation of state p = ρ − ρc the interior metric is solved exactly. It is matched with the Schwarzschild metric, which is deformed in a narrow range beyond the horizon. The solution is regular everywhere, with a specific shape at the origin. The gravitational redshift at the horizon remains finite but is large, z ~ 1023 M⊙/M. Time keeps its standard role also in the interior. The energy of the Schwarzschild metric, shown to be minus infinity in the General Theory of Relativity, is regularized in this setup, resulting in E = Mc2.


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