Relativistic effects in the solar EOS
| dc.creator | Bonanno, A. | |
| dc.creator | Murabito, A. L. | |
| dc.creator | Paterno', L. | |
| dc.date | 2001-07-19 | |
| dc.date.accessioned | 2026-07-07T01:59:23Z | |
| dc.date.available | 2026-07-07T01:59:23Z | |
| dc.description | We study the sensitivity of the sound speed to relativistic corrections of the equation of state (EOS) in the standard solar model by means of a helioseismic forward analysis. We use the latest GOLF/SOHO data for $\ell = 0,1,2,3$ modes to confirm that the inclusion of the relativistic corrections to the adiabatic exponent $Γ_1$ computed from both OPAL and MHD EOS leads to a more reliable theoretical modelling of the innermost layers of the Sun. | |
| dc.description | 3 pages, 3 figures, aa.cls, to appear on Astronomy and Astrophysics | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0107381 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0107381 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/3088 | |
| dc.subject | Astrophysics | |
| dc.title | Relativistic effects in the solar EOS | |
| dc.type | text |