Infrared Modified QCD Couplings and Bjorken Sum RuleWe test the recently proposed «Massive»
Perturbation Theory (MPT) for the description of the г1p
Scalar wormholes in a cosmological setting and their instabilityWe construct exact nonstatic nonhomogeneous
spherically symmetric solutions in the
theory On the stability of electrovacuum space-times in scalar–tensor gravityWe study the behavior of static,
spherically symmetric solutions to the field equations of scalar
Spherical wave-type solution in relativistic theory of gravitationIn relativistic
theory of gravitation the nonstatic
spherically-symmetrical solutions
Gravitational perturbations in the expanding universe in a coordinate representationGravitational
perturbations in the expanding universe are analyzed within the framework
Once again on thin-shell wormholes in scalar-tensor gravity,
spherically symmetric spacetimes have a negative shell surface energy density in any scalartensor
theory