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- W132550165 abstract "A large part of energy from space is coming from collapsing stars (SN, Hypernovae) and collapsed stars (black holes, neutron stars and white dwarfs). The peak of their energy release is the hard-X and gamma-ray wavelengths where photons are insensitive to absorption and can travel from the edge the Universe or the central core of the Galaxy without loosing the primordial information of energy, time signature and polarization. The most efficient process to produce energetic photons is gravitational accretion of matter from a normal star onto a collapsed companion (L~GxMcollxdMacc/dtx( 1Rdisc)-dMacc/dt x c2), exceeding by far the nuclear reaction capability to generate high energy quanta. Thus our natural laboratory for in situ investigations are collapsed objects which matter and radiation co-exist extreme conditions of temperature and density due to gravitationally bent geometry and magnetic fields. This is a unique opportunity to study the physics of accretion flows stellar mass and super-massive Black Holes (SMBHs), plasmoids generated relativistic jets galactic microQSOs and AGNs, ionised plasma interacting at the touching point of weakly magnetized NS surface, GRB/Supernovae connection, and the mysterious origins of dark GRB and X-ray flash." @default.
- W132550165 created "2016-06-24" @default.
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- W132550165 date "2005-01-01" @default.
- W132550165 modified "2023-09-27" @default.
- W132550165 title "Unveiling the High Energy Obscured Universe: Hunting Collapsed Objects Physics" @default.
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