Nuclear hydrodynamics in the inner crust of neutron stars
| dc.creator | Magierski, Piotr | |
| dc.creator | Bulgac, Aurel | |
| dc.date | 2003-12-30 | |
| dc.date.accessioned | 2026-07-07T10:27:09Z | |
| dc.date.available | 2026-07-07T10:27:09Z | |
| dc.description | In the inner crust of a neutron star, due to the high density and pressure, nuclei which are still present, are immersed in a neutron superfluid. One then expects that the dynamical properties of nuclei are significantly affected. In order to estimate the magnitude of the effect associated with the presence of a superfluid medium, we formulate the hydrodynamical approach to the nuclear dynamics in the inner crust of neutron stars. We calculate the renormalized nuclear mass and the strength of the medium-induced interaction between nuclei. We argue that these effects noticeably modify the properties of the Coulomb crystal in the inner crust. | |
| dc.description | 11 pages, 1 figure. Presented at XXVIII Mazurian Lakes Conference on Physics: Atomic Nucleus as a Laboratory for Fundamental Processes, August 31-September 7, 2003, Krzyze, Poland | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0312644 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0312644 | |
| dc.identifier | ActaPhys.Polon.B35:1203-1214,2004 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/177070 | |
| dc.subject | Astrophysics | |
| dc.subject | Nuclear Theory | |
| dc.subject | Fluid Dynamics | |
| dc.title | Nuclear hydrodynamics in the inner crust of neutron stars | |
| dc.type | text |