The Structure of the Solar Core
| dc.creator | Manuel, O. | |
| dc.date | 2004-11-24 | |
| dc.date.accessioned | 2026-07-07T02:16:00Z | |
| dc.date.available | 2026-07-07T02:16:00Z | |
| dc.description | Data from the Galileo mission to Jupiter and the Apollo mission to the Moon show isotopically distinct types of xenon in Jupiter and in the Sun and evidence of a mass separation process that selectively moves lighter elements and the lighter isotopes of each element to the solar surface. Understanding the source of solar luminosity, solar neutrinos, and mono-isotopic H-1 pouring from the solar surface depends on measurements of anti-neutrinos coming from neutron decay in the Sun and on the development of a better theoretical basis for the empirical evidence of a.) Repulsive interactions between like nucleons; b.) Clustering of nucleons; and c.) Neutron penetration of the gravitational barrier surrounding a neutron star. | |
| dc.description | 9 pages with 5 figures, Proceedings of the Fourth International Conference on Beyond Standard Model Physics - BEYOND 2003 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0411658 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0411658 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/8623 | |
| dc.subject | Astrophysics | |
| dc.title | The Structure of the Solar Core | |
| dc.type | text |