| dc.creator | Benvenuto, Omar Gustavo | |
| dc.creator | Vucetich, Héctor | |
| dc.creator | Horvath, Jorge Ernesto | |
| dc.date | 1994-02-01 | |
| dc.date | 2022-11-02T17:59:44Z | |
| dc.date.accessioned | 2023-07-15T04:58:57Z | |
| dc.date.available | 2023-07-15T04:58:57Z | |
| dc.identifier | http://sedici.unlp.edu.ar/handle/10915/145043 | |
| dc.identifier | issn:0035-8711 | |
| dc.identifier | issn:1365-2966 | |
| dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/7471631 | |
| dc.description | We study the effects of the accretion of normal matter on to strange-matter pulsar models. It is assumed that, because of the high strangeness barrier, normal matter is inert in contact with Q α matter. For this reason, normal matter accretion is able to form a thick outer layer with densities far above neutron drip. Accretion can make the superfluid quark-alpha Q α a layer disappear by solidification but, for the same reason, a superfluid neutron layer is formed. The fractional moment of inertia of the latter is large enough to fulfil the vortex-creep glitch model requirements. The high rotational stability of millisecond pulsars is discussed in the framework of the strange-matter hypothesis | |
| dc.description | Facultad de Ciencias Astronómicas y Geofísicas | |
| dc.description | Facultad de Ciencias Exactas | |
| dc.format | application/pdf | |
| dc.format | 690-696 | |
| dc.language | en | |
| dc.rights | http://creativecommons.org/licenses/by-nc-sa/4.0/ | |
| dc.rights | Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) | |
| dc.subject | Astronomía | |
| dc.subject | accretion | |
| dc.subject | accretion discs | |
| dc.subject | dense matter | |
| dc.subject | equation of state | |
| dc.subject | stars: neutron | |
| dc.subject | pulsars: general | |
| dc.title | Accretion on to strange-matter pulsars | |
| dc.type | Articulo | |
| dc.type | Articulo | |
