We report on the first results of self-consistent second order metric perturbations produced by a point particle moving in the Schwarzschild spacetime. The second order waveforms satisfy a wave equation with an effective source term build up from products of first order metric perturbations and its derivatives. We have explicitly regularized this source term at the particle location as well as at the horizon and at spatial infinity
We present approximate formulas for the tensor BB, EE, TT, and TE multipole coefficients for large m...
We generalize the Raychaudhuri equation for the evolution of a self gravitating fluid to include an ...
The spherically symmetric perturbations in the spatially flat Friedman models are considered. It is ...
The second order perturbations in Friedmann-Robertson-Walker universe filled with a perfect fluid ar...
We give a solution of the wave equation for massless, or massive spin-2 particles propagating in a g...
The influence of higher order - stringly inspired - curvature corrections to the classical General R...
Recently, we found that the correction for the Einstein–de Sitter (EdS) assumption on the one-loop m...
Semi-classical gravity combines classical treatment of the gravitational field with quantum mechanic...
In the standard methodology for evaluating the Hawking radiation emanating from a black hole, the ba...
A more rigorous treatment of the Schwarzschild metric by making use of the energy-momentum tensor of...
The usual equivalence between the Palalini and metric (or affinity and vielbein) formulations of Ein...
In this pedagogical note, we discuss obstacles to the usual Palatini formulations of gauge and gravi...
A solution of the linearized Einstein's equations for a spherically symmetric perturbation of the ul...
Charged, rotating black hole solutions of Einstein's gravitational equations are investigated in the...
An exact solution of the source-free Kaluza-Klein field equations is presented. It is a 5D generaliz...
We present approximate formulas for the tensor BB, EE, TT, and TE multipole coefficients for large m...
We generalize the Raychaudhuri equation for the evolution of a self gravitating fluid to include an ...
The spherically symmetric perturbations in the spatially flat Friedman models are considered. It is ...
The second order perturbations in Friedmann-Robertson-Walker universe filled with a perfect fluid ar...
We give a solution of the wave equation for massless, or massive spin-2 particles propagating in a g...
The influence of higher order - stringly inspired - curvature corrections to the classical General R...
Recently, we found that the correction for the Einstein–de Sitter (EdS) assumption on the one-loop m...
Semi-classical gravity combines classical treatment of the gravitational field with quantum mechanic...
In the standard methodology for evaluating the Hawking radiation emanating from a black hole, the ba...
A more rigorous treatment of the Schwarzschild metric by making use of the energy-momentum tensor of...
The usual equivalence between the Palalini and metric (or affinity and vielbein) formulations of Ein...
In this pedagogical note, we discuss obstacles to the usual Palatini formulations of gauge and gravi...
A solution of the linearized Einstein's equations for a spherically symmetric perturbation of the ul...
Charged, rotating black hole solutions of Einstein's gravitational equations are investigated in the...
An exact solution of the source-free Kaluza-Klein field equations is presented. It is a 5D generaliz...
We present approximate formulas for the tensor BB, EE, TT, and TE multipole coefficients for large m...
We generalize the Raychaudhuri equation for the evolution of a self gravitating fluid to include an ...
The spherically symmetric perturbations in the spatially flat Friedman models are considered. It is ...