We discuss the effects of strong gravity on the observable characteristics, light curves and spectral broadening; of the radiation emitted during a finite interval of time from a relativistically collapsing object. Using a simplified model of monochromatic radiation from a freely-falling spherical surface, we demonstrate that the polar cap emission from a collapsing surface can be characterized by two successive light packets with distinctively different frequency broadening
We model the spectra and surface brightness distributions for the Ly alpha radiation expected from p...
We ·investigate the energy flux of the Hawking radiation due to collapsing shells in two· dimensiona...
We present Monte Carlo calculations of Ly alpha radiative transfer through optically thick, spherica...
In this work, we discuss observable characteristics of the radiation emitted from a surface of a col...
We address the question of radiation emitted from a collapsing star. We consider the simple model of...
AbstractWe study radiation emitted during the gravitational collapse from two different types of she...
We discuss a counterintuitive phenomenon of classical general relativity, in which a significant fra...
AbstractWe discuss a counterintuitive phenomenon of classical general relativity, in which a signifi...
AbstractWe study quantum radiation emitted during the collapse of a quantized, gravitating, spherica...
AbstractHawking radiation explicitly depends only on the black hole's total mass, charge and angular...
Large light deflection angles are produced in the strong gravitational field regions around neutron ...
We generalise the continual gravitational collapse of a spherically symmetric radiation shell of mat...
International audienceAccording to current pulsar emission models, photons are produced within their...
Using the Sparling form and a geometric construction adapted to spacetimes with a 2-dimensional iso...
Dynamical evolution of test fields in background geometry with a naked singularity is an important p...
We model the spectra and surface brightness distributions for the Ly alpha radiation expected from p...
We ·investigate the energy flux of the Hawking radiation due to collapsing shells in two· dimensiona...
We present Monte Carlo calculations of Ly alpha radiative transfer through optically thick, spherica...
In this work, we discuss observable characteristics of the radiation emitted from a surface of a col...
We address the question of radiation emitted from a collapsing star. We consider the simple model of...
AbstractWe study radiation emitted during the gravitational collapse from two different types of she...
We discuss a counterintuitive phenomenon of classical general relativity, in which a significant fra...
AbstractWe discuss a counterintuitive phenomenon of classical general relativity, in which a signifi...
AbstractWe study quantum radiation emitted during the collapse of a quantized, gravitating, spherica...
AbstractHawking radiation explicitly depends only on the black hole's total mass, charge and angular...
Large light deflection angles are produced in the strong gravitational field regions around neutron ...
We generalise the continual gravitational collapse of a spherically symmetric radiation shell of mat...
International audienceAccording to current pulsar emission models, photons are produced within their...
Using the Sparling form and a geometric construction adapted to spacetimes with a 2-dimensional iso...
Dynamical evolution of test fields in background geometry with a naked singularity is an important p...
We model the spectra and surface brightness distributions for the Ly alpha radiation expected from p...
We ·investigate the energy flux of the Hawking radiation due to collapsing shells in two· dimensiona...
We present Monte Carlo calculations of Ly alpha radiative transfer through optically thick, spherica...