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Phenomenological Model of Multiphase Cosmological Scenario in Theory of Induced Gravity that can both match with the solutions of the standard theory of gravity as well as can differ from it
The realistic models of relativistic stars in f (R) = R + α R2 gravity© 2017 IOP Publishing Ltd. In the context of f (R) = R + αR 2 gravity, we study the existence
ON THE PROBLEM OF GRAVITY QUANTIZATION IN GRAVITATION THEORY of both geometry as a whole and space-time. Quantum mechanics and quantum field theory may be considered
Cosmological Solutions in the Tensor-Multi-Scalar Theory of Gravity with the Higgs Potential on cosmology of general relativity (GR), to the case of a two-field model of the tensor-multiscalar theory
Cosmological attractor inflation from the RG-improved Higgs sector of finite gauge theory which sums all leading logs of perturbation theory is essential for a successful realization
Brane world corrections to Newton's law by most of alternative theories of gravity and unified models of physical interactions. After giving a
Yang-Baxter deformations beyond coset spaces (a slick way to do TsT)Classical Theories of Gravity
The screening Horndeski cosmologies, but it may acquire ghost in more general versions of the Horndeski theory.
Big bounce with finite-time singularity: The F (R) gravity description occurring at the bouncing point in the context of F(R) modified gravity. We investigate the evolution
Einstein-aether theory with a Maxwell field: General formalismWe extend the Einstein-aether theory to include the Maxwell field in a nontrivial manner by taking
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