TeV Neutrinos from Companion Stars of Rapid-Rotating Neutron Stars
| dc.creator | Nagataki, S. | |
| dc.date | 2002-02-26 | |
| dc.date | 2002-06-29 | |
| dc.date.accessioned | 2026-07-07T03:46:34Z | |
| dc.date.available | 2026-07-07T03:46:34Z | |
| dc.description | We have estimated the number flux of of mu-neutrinos which are produced due to the hadronic interactions between the cosmic rays coming from a neutron star and the matter in a companion star. The event rate at 1 km^2 detectors of high-energy neutrinos such as ICECUBE, ANTARES and NESTOR is also estimated to be 2.7 \times 10^4 events yr^-1 when the source is located at 10 kpc away from the Earth. We have estimated the number of such a system and concluded that there will be several candidates in our galaxy. Taking these results into consideration, this scenario is promising and will be confirmed by the future observations. | |
| dc.description | 4 pages, using REVTeX. Some comments are added | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0202243 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0202243 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/41336 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | Astrophysics | |
| dc.title | TeV Neutrinos from Companion Stars of Rapid-Rotating Neutron Stars | |
| dc.type | text |