What do exotic equations of state have to offer?
| dc.creator | Horvath, J. E. | |
| dc.date | 2006-09-11 | |
| dc.date.accessioned | 2026-07-07T10:40:06Z | |
| dc.date.available | 2026-07-07T10:40:06Z | |
| dc.description | We present a short general overview of the main features of exotic models of neutron stars, focusing on the structural and dynamical predictions derived from them. In particular, we discuss the presence of ``normal'' quark matter and Color-Flavor Locked (CFL) states, including their possible self-bound versions, and mention some different proposals emerging from the study of QCD microphysics. A connection with actual observed data is the main goal to be addressed at this talk and along the meeting. It is demonstrated that exotic equations of state are {\it not} soft if the vacuum contributions are large enough, and argued that recent measurements of high pulsar masses ($M \geq 2 M_{\odot}$) create problems for {\it hadronic} models in which hyperons should be present. | |
| dc.description | 8 pages, 2 figures. To be published in the Proceedings of the conference "Isolated Neutron Stars: from the Interior to the Surface" (April 24-28, 2006, London, UK), eds. D. Page, R. Turolla, & S. Zane | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0609272 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0609272 | |
| dc.identifier | Astrophys.SpaceSci.308:431-434,2007 | |
| dc.identifier | doi:10.1007/s10509-007-9314-1 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/181246 | |
| dc.subject | Astrophysics | |
| dc.title | What do exotic equations of state have to offer? | |
| dc.type | text |