132 citations
- Centre National de la Recherche ScientifiqueFR12 papers
- Romanian AcademyRO10 papers
- Université Côte d'AzurFR8 papers
- IMAR - Institutul de Matematică „Simion Stoilow” al Academiei RomâneRO7 papers
- Institute of MathematicsPL6 papers
- National Academy of Sciences of UkraineUA6 papers
- Institut national de recherche en sciences et technologies du numériqueFR5 papers
- Laboratoire Jean-Alexandre DieudonnéFR5 papers
- University of Duisburg-EssenDE5 papers
- Academia Oamenilor de Știință din RomâniaRO3 papers
- Government College University, LahorePK3 papers
- Institut Universitaire de FranceFR3 papers
9 papers · 1 filter
Boundary stress tensors for spherically symmetric conformal Rindler observers
Hristu Culetu
The boundary energy - momentum tensors for a static observer in the conformally flat Rindler geometry are considered. We found the surface energy is positive far form the Planck wo…
Bjorken expansion in the isotropic Kasner spacetime
Hristu Culetu
An isotropic expansion for the QGP is proposed in curved Kasner spacetime for an experimental configuration with three dimensional set of beams. The fluid of relativistic particles…
The Milne spacetime and the hadronic Rindler horizon
Hristu Culetu
A direct relation between the time dependent Milne geometry and the Rindler spacetime is shown. Milne's metric corresponds to that one beyond Rindler's event horizon (in the region…
Boundary sources in the Doran - Lobo - Crawford spacetime
Hristu Culetu
We take a null hypersurface (the causal horizon) generated by a congruence of null geodesics as the boundary of the Doran-Lobo-Crawford spacetime, to be the place where the Brown-Y…
On The Black Hole Interior Spacetime
Hristu Culetu
A new version of the geometry inside a black hole is proposed, on the grounds of an idea given by Doran et al. The spacetime is still time dependent and is a solution of Einstein's…
Is the Rindler horizon energy nonvanishing ?
Hristu Culetu
A nonvanishing value for the Rindler horizon energy is proposed, by an analogy with the "near horizon" Schwarzschild metric. We show that the Rindler horizon energy is given by the…