Cosmological dynamics in the model with nonminimal kinetic coupling of such potential on the dynamics of the model is found using the methods of the
theory of dynamical systems. Two
Modified equations in the theory of induced gravity. Solution to the cosmological constant problem are Einstein's
theory of
gravity and string
theory. This work is devoted to the formation of self
De Sitter vacua in ghost-free massive gravity theory Sitter solution in the ghost-free massive
gravity theory via applying the Gordon ansatz
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
Introduction to modified gravity in modified multidimensional
gravity.
On the stability of electrovacuum space-times in scalar–tensor gravity–tensor
theories (STT) of
gravity belonging to the Bergmann–Wagoner–Nordtvedt class, in the presence of an electric
Cosmology in modified f(R, T)-gravity cosmological equations for a few representations of the
theory and discuss main differences with conventional f(R, T)-
gravity