Results 41 to 50 of about 79,313 (303)
HOLOGRAPHIC MODIFIED GRAVITY [PDF]
In this paper, we investigate cosmological application of holographic dark energy density in the modified gravity framework. We employ the holographic model of dark energy to obtain the equation of state for the holographic energy density in a spatially flat universe. Our calculation shows that, taking ΩΛ = 0.73 for the present time, it is possible to
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PhD thesis : Compact objects in modified theories of gravity [PDF]
The formulation of General Relativity by Albert Einstein in 1915 revolutionised our understanding of the gravitational interaction. However, despite its tremendous successes, this theory struggle to explain certain important phenomena such as the ...
Ducobu, Ludovic
core
Reissner–Nordström Anti-de Sitter Black Holes in Mimetic F(R) Gravity
In this paper, we study under which conditions the Reissner–Nordström anti-de Sitter black hole can be a solution of the vacuum mimetic F ( R ) gravity with Lagrange multiplier and mimetic scalar potential.
V. K. Oikonomou
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Constraining f(T,T) gravity with gravitational baryogenesis
Gravitational baryogenesis is one of the mechanisms which help us to explore more about our early universe, especially baryon-anti-baryon asymmetry.
Sai Swagat Mishra +2 more
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Exact rotating black hole solutions for f(R) gravity by modified Newman Janis algorithm
We show that the f(R)-gravity theories with constant Ricci scalar in the Jordan/Einstein frame can be described by Einstein or Einstein–Maxwell gravity with a cosmological term and a modified gravitational constant.
Pankaj Chaturvedi +3 more
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Critical gravity in the Chern–Simons modified gravity [PDF]
13 pages, 1 figure, version to appear in ...
Moon, Taeyoon, Myung, Yun Soo
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Rastall gravity is equivalent to Einstein gravity
Rastall gravity, originally developed in 1972, is currently undergoing a significant surge in popularity. Rastall gravity purports to be a modified theory of gravity, with a non-conserved stress–energy tensor, and an unusual non-minimal coupling between ...
Matt Visser
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ON EXPONENTIAL MODIFIED GRAVITY [PDF]
A modified theory of gravity with the function F(R) = R exp (αR) instead of Ricci scalar R in the Einstein–Hilbert action is considered and analyzed. The action of the model is converted into Einstein–Hilbert action at small value of the parameter α. From local tests we obtain a bound on the parameter α ≤ 10-6 cm 2.
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The P-V phase transition of the FRW universe
We define thermodynamic pressure P by work density W as the conjugate quantity of thermodynamic volume V from field equation. We derive the equations of state P=P(V, T) for the Friedmann–Robertson–Walker (FRW) universe in Einstein gravity and a modified ...
Shi-Bei Kong +4 more
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added references; made some clarifications; 8 ...
Dimitrijevic, Ivan +3 more
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