AbstractWe show that majoron emission from a hot nascent neutron star can be anisotropic in the presence of a strong magnetic field. If majorons carry a non-negligible fraction of the supernova energy, the resulting recoil velocity of a neutron star can explain the observed velocities of pulsars
We show that neutrino-driven pulsar kicks can increase the energy of the supernova shock. The observ...
Aims. We critically discuss a pulsar acceleration mechanism based on asymmetric neutrino emission fr...
AbstractObservations show that, at the beginning of their existence, neutron stars are accelerated b...
AbstractWe show that majoron emission from a hot nascent neutron star can be anisotropic in the pres...
We show that two long-standing astrophysical puzzles may have a simultaneous solution. Neutrino osci...
In proto-neutron stars with strong magnetic fields, the cross section for magnetic field strength du...
The collapse of a massive star’s core, followed by a neutrino-driven, asymmetric supernova explosion...
Refering to recent hydrodynamical computations (Herant et al. 1992, Janka and Mueller 1993a) it is a...
ABSTRACT: A convincing explanation for the observed pulsar large peculiar velocities is still missin...
We show that pulsar velocities may arise from anisotropic neutrino emission induced by resonant conv...
Observational advances over the last decade have left little doubt that neutron stars received a lar...
The neutron star formation during the collapse with the strong magnetic field may lead to a mirror s...
We have recently proposed an explanation for the birth velocities of pulsars as resulting from asymm...
In proto-neutron stars with strong magnetic fields, the neutrino-nucleon scattering/absorption cross...
If core collapse leads to the formation of a rapidly rotating bar-unstable proto-neutron star surrou...
We show that neutrino-driven pulsar kicks can increase the energy of the supernova shock. The observ...
Aims. We critically discuss a pulsar acceleration mechanism based on asymmetric neutrino emission fr...
AbstractObservations show that, at the beginning of their existence, neutron stars are accelerated b...
AbstractWe show that majoron emission from a hot nascent neutron star can be anisotropic in the pres...
We show that two long-standing astrophysical puzzles may have a simultaneous solution. Neutrino osci...
In proto-neutron stars with strong magnetic fields, the cross section for magnetic field strength du...
The collapse of a massive star’s core, followed by a neutrino-driven, asymmetric supernova explosion...
Refering to recent hydrodynamical computations (Herant et al. 1992, Janka and Mueller 1993a) it is a...
ABSTRACT: A convincing explanation for the observed pulsar large peculiar velocities is still missin...
We show that pulsar velocities may arise from anisotropic neutrino emission induced by resonant conv...
Observational advances over the last decade have left little doubt that neutron stars received a lar...
The neutron star formation during the collapse with the strong magnetic field may lead to a mirror s...
We have recently proposed an explanation for the birth velocities of pulsars as resulting from asymm...
In proto-neutron stars with strong magnetic fields, the neutrino-nucleon scattering/absorption cross...
If core collapse leads to the formation of a rapidly rotating bar-unstable proto-neutron star surrou...
We show that neutrino-driven pulsar kicks can increase the energy of the supernova shock. The observ...
Aims. We critically discuss a pulsar acceleration mechanism based on asymmetric neutrino emission fr...
AbstractObservations show that, at the beginning of their existence, neutron stars are accelerated b...
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