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Colliding compact objects

AIP Conference Proceedings, 2009
We study the collisions of compact objects induced by neutron star (NS) birth kicks. If a binary system survives the first supernova (SN) explosion, in some cases the second SN may place the stellar remnants into bound highly eccentric orbits. The two compact objects will tidally interact and quickly spiral into each other. We expect such encounters to
E. Troja   +5 more
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Deformed Compact Objects

International Journal of Theoretical Physics
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Quartuccio, J. T.   +2 more
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Compact objects

2009
Abstract When a star is near the end of its lifetime, and all of its fuel is used up, there is no longer enough outwards pressure due to radiation to resist the inwards pull of gravity and the star starts to collapse again. However, there is another source of internal pressure.
Stephen J. Blundell   +1 more
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Compact Object Reconstruction

1999
In this chapter we first present a review of the methods for the tomographie reconstruction of a compact homogeneous object that lies in a homogeneous background. Then we focus on contour estimation and polyhedral shape reconstructions. We give some sufficient conditions to obain exact reconstructions from a complete set of projections in the 2.1) case
Ali Mohammad-Djafari, Charles Soussen
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Neutrinos in compact objects

Physical Review D, 1980
The trapping of neutrinos in strong gravitational fields is considered. The zero-mass Dirac equation for curved space-time is specialized to the case of a static spherically symmetric object of constant density. The WKB method is applied to obtain the energy spectrum of the semibound states of the neutrinos.
Ajit K. Kembhavi, C. V. Vishveshwara
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