Pulsar velocities and dark matter hint at a singlet neutrino
| dc.creator | Kusenko, Alexander | |
| dc.date | 2003-11-11 | |
| dc.date | 2003-11-12 | |
| dc.date.accessioned | 2026-07-07T02:11:09Z | |
| dc.date.available | 2026-07-07T02:11:09Z | |
| dc.description | Two astrophysical puzzles, the origin of pulsar velocities and that of dark matter, may have a simultaneous explanation if there exists a sterile neutrino with a mass in the 1-20 keV range and a small mixing (of order 10^{-4}) with the electron neutrino. Although the mixing is too small for direct detection, future observations of the X-ray telescopes, as well as the gravity waves detectors, such as LIGO and LISA, may be able to confirm or rule out the existence of such a neutrino. | |
| dc.description | 4 pages, 1 figure; talk presented at The 6th RESCEU International Symposium "Frontier in Astroparticle Physics and Cosmology", Tokyo, Japan, November 4 - 7, 2003 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0311240 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0311240 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6982 | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Pulsar velocities and dark matter hint at a singlet neutrino | |
| dc.type | text |