Neutron stars properties viewed by the ENU model
| dc.creator | Sukenik, Miroslav | |
| dc.creator | Sima, Jozef | |
| dc.date | 2002-03-25 | |
| dc.date.accessioned | 2026-07-07T02:03:15Z | |
| dc.date.available | 2026-07-07T02:03:15Z | |
| dc.description | Up-to-now known characteristics of radio pulsars, such as mass limits, magnetic field intensity, rotational period, and maximum radiation are mainly of empirical nature. Applying the Expansive Nondecelerative Universe model (ENU) into the issue allows to offer a deeper theoretical explanation of the known parameters and to estimate their limits. Using the ENU approach the following values related to synchrotron radiation emitting radio pulsars were estimated: the lower and upper limits of magnetic field intensity are B(min) = 8.6 x 10^6 T, and B(max) = 9.4 x 10^8 T, respectively, the maximum rotation period reaches 3.9 s, the maximum radiation output of a pulsar is P(max) = 5.6 x 10^29 W (all the values relate to radio pulsars with 1.4 solar masses and radius 1.0 x 10^4 m and are mass and radius dependent). These values are in accordance with the experimental observations. | |
| dc.description | 5 pages, LaTeX, submitted to Spacetime & Substance | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0203426 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0203426 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/4321 | |
| dc.subject | Astrophysics | |
| dc.title | Neutron stars properties viewed by the ENU model | |
| dc.type | text |