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Scalar-Tensor Theory of Gravitation in Minkowski Space–TimeIn Minkowski space–time we consider the scalar and tensor fields, which form together
the effective
Particle creation by a black hole as a consequence of the casimir effect between the energy-momentum tensors of scalar and electromagnetic fields near the horizon is discovered
Cosmology in modified f(R, T)-gravity(R, T)-gravity (where T is trace of the energy-momentum tensor) by introducing higher derivatives matter fields. We
An outline of approach linking black-hole-evaporation with quantum-field effects in flat spacetime the vacuum expectation values of the energy-momentum tensors of scalar and electromagnetic fields near
Symmetry properties of a charged fluid in the general theory of relativity definite group of motions, is considered. It is shown that if nonempty spacetime V4 with an energy-momentum
Nonlinear plane-symmetric perturbations of a spatial-plane Friedman universe filled with an ideal dustThe general solution of Einstein's equations with the energy-momentum tensor of an ideal dust
Generation of static solutions of the self-consistent system of Einstein-Maxwell equations with an arbitrary momentum-energy tensor in the right hand side there corresponds a static solution of the self
Collisional plasma relaxation in the field of a planar gravitational wave. These corrections are used in corrections to the energy-momentum tensor and in deriving the collisional
Quantum kinetic equations in curved space-time and thermal equilibrium of the energy-momentum tensor are obtained, which are the moments of the classical distribution function and its
Particle creation by a black hole as a consequence of the casimir effect between the energy-momentum tensors of scalar and electromagnetic fields near the horizon is discovered
Страница 5 из 2002
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