The phase transition from nuclear matter to quark matter during proto-neutron star evolution
Open Access
- 7 April 1999
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 304 (2) , L25-L29
- https://doi.org/10.1046/j.1365-8711.1999.02458.x
Abstract
No abstract availableKeywords
This publication has 14 references indexed in Scilit:
- Can We See the Hadron‐Quark Transition Happening in Neutron Stars?The Astrophysical Journal, 1998
- Burning of Two‐Flavor Quark Matter into Strange Matter in Neutron Stars and in Supernova CoresThe Astrophysical Journal, 1997
- The Conversion of Two-Flavor to Three-Flavor Quark Matter in a Supernova CoreThe Astrophysical Journal, 1995
- First-order phase transitions with more than one conserved charge: Consequences for neutron starsPhysical Review D, 1992
- STRANGE-PULSAR MODELSInternational Journal of Modern Physics A, 1991
- Evidence for strange matter in supernovae?Physical Review Letters, 1989
- Exotic Phases of Hadronic Matter and their Astrophysical ApplicationAnnual Review of Nuclear and Particle Science, 1988
- Statistical analysis of the time structure of the neutrinos from supernova 1987AThe Astrophysical Journal, 1988
- The birth of neutron starsThe Astrophysical Journal, 1986
- Neutron stars are giant hypernuclei?The Astrophysical Journal, 1985