Gravitational Waves from a Pulsar Kick Caused by Neutrino Conversions
arXiv:astro-ph/0309362 · doi:10.1103/PhysRevD.69.024008
Abstract
It has been suggested that the observed pulsar velocities are caused by an asymmetric neutrino emission from a hot neutron star during the first seconds after the supernova collapse. We calculate the magnitude of gravitational waves produced by the asymmetries in the emission of neutrinos. The resulting periodic gravitational waves may be detectable by LIGO and LISA in the event of a nearby supernova explosion.
arXiv comment15 pages, 2 figures
References in corpus (17)
- On the Nature of Core Collapse Supernova Explosions
- Sterile Neutrino Hot, Warm, and Cold Dark Matter
- The Pulsar Kick Velocity Distribution
- Pulsar Recoil and Gravitational Radiation due to Asymmetrical Stellar Collapse and Explosion
- Neutron Star Population Dynamics.II: 3D Space Velocities of Young Pulsars
- Why pulsars rotate and move: kicks at birth
- Pulsar kicks from a dark-matter sterile neutrino
- Population Synthesis for Neutron Star Systems with Intrinsic Kicks
- Neutral current induced neutrino oscillations in a supernova
- Velocities of pulsars and neutrino oscillations
- Neutrino Conversions in a Polarized Medium
- Pulsar kicks from neutrino oscillations
- "Nucleosynthesis constraints on active-sterile neutrino conversions in the early universe with random magnetic field"
- Neutrino propagation in a medium with a magnetic field
- Neutrino oscillation mechanism for pulsar kicks reexamined
- Effect of magnetic field on electron neutrino sphere in pulsars
- New Supernova Constraints on active-sterile neutrino conversions
Cited by in corpus (17)
- Dark-matter sterile neutrinos in models with a gauge singlet in the Higgs sector
- Post-Newtonian corrections to the gravitational-wave memory for quasicircular, inspiralling compact binaries
- Effects of neutrino-driven kicks on the supernova explosion mechanism
- Gravitational Waves from Gravitational Collapse
- Heavy sterile neutrinos and supernova explosions
- Pulsar kicks from neutrino oscillations
- Active-sterile neutrino oscillations and pulsar kicks
- Flavour Mixing of Neutrinos and Baryon Asymmetry of the Universe
- Pulsar Kicks Induced by Spin Flavor Oscillations of Neutrinos in Gravitational Fields
- Delayed pulsar kicks from the emission of sterile neutrinos
- Neutrino mass spectrum from gravitational waves generated by double neutrino spin-flip in supernovae
- Snowmass-2013 Cosmic Frontier 3 (CF3) Working Group Summary: Non-WIMP dark matter
- Gravitational-wave astronomy: the high-frequency window
- Pulsar kicks and dark matter from a sterile neutrino
- Possible astrophysical clues of dark matter
- Neutrino oscillations, and the origin of pulsar velocities and dark matter
- Pulsar velocities and dark matter hint at a singlet neutrino