Conveners
Afternoon session - Parallel B
- Janusz Gil (University of Zielona Gora, Poland)
Dr
Shuta Tanaka
(Institute for Cosmic Ray Research, The University of Tokyo)
28/03/2014, 14:30
Pulsar winds have problems in energy conversion and pair-cascade processes which determine the magnetization, the pair multiplicity and the bulk Lorentz factor of the wind.
We study induced Compton scattering by a relativistically moving cold plasma to constrain wind properties by imposing that radio pulses from the pulsar itself are not scattered by the wind as was first studied by Wilson &...
Dr
Lubos Neslusan
(Astronomical Institute, Slovak Academy of Sciences)
28/03/2014, 15:15
Neutron stars (NSs) are the compact objects with the metrics detectably deviated from the flat spacetime. In the interior of every NS the metrics can be calculated from the model of its internal structure. In the surrounding empty space the metrics is described by the outer Schwarzschild solution (OSS) of Einstein field equations if a non-rotating NS is considered. In the linkup of both NS and...
Mr
Rodrigo Souza
(IAG - USP Sao Paulo)
28/03/2014, 15:30
Recently, it has been suggested that a critical electrical field arises during the gravitational collapse of massive stars leading to a vacuum polarization. This, in turn, leads to the necessity of a reexamination of the gravito-electrodynamical properties of compact stars of the class of neutron stars. Rotondo, Rueda, Ruffini and Xue claim to have proved the impossibility of local charge...