Add to ORKGWe review the differences in first order phase transition of single and multi-component systems, and then discuss the crystalline structure expected to exist in the mixed confined deconfined phase of hadronic matter. The particular context of neutron stars is chosen for illustration. The qualitative results are general and apply for example to the vapor-liquid transition in subsaturated asymmetric nuclear matter
Deconfinement phase transition and condensation of Goldstone bosons in neutron star matter are inves...
The transition from hadronic matter to quark matter in the core of neutron stars is likely to be as...
The transition from hadronic matter to quark matter in the core of neutron stars is likely to be as...
We review the differences in first order phase transition of single and multi-component systems, and...
Phase transitions in neutron stars due to formation of quark matter, kaon condensates, etc. are disc...
We give a general thermodynamical argument showing that in neutron stars, the Coulomb structured mix...
We examine the present status of the theoretical calculations for the internal structure of neutron ...
We investigate 1st order phase transitions in a general way, if not the single particle numbers of t...
AbstractWe consider how the occurrence of first-order phase transitions in non-constant pressure dif...
A structured mixed phase consisting of quark and hadron phases is numerically studied with the Coulo...
From sixth Texas symposium on relativistic astrophysics; New York, New York, USA (18 Dec 1972). Resu...
We investigate the occurrence of exotic structures in the outermost layers of neutron stars within t...
Numerous theoretical studies using various equation of state models have shown that quark matter may...
We investigate the properties of mixed stars formed by hadronic and quark matter in $\beta$-equilibr...
Deconfinement phase transition and condensation of Goldstone bosons in neutron star matter are inves...
Deconfinement phase transition and condensation of Goldstone bosons in neutron star matter are inves...
The transition from hadronic matter to quark matter in the core of neutron stars is likely to be as...
The transition from hadronic matter to quark matter in the core of neutron stars is likely to be as...
We review the differences in first order phase transition of single and multi-component systems, and...
Phase transitions in neutron stars due to formation of quark matter, kaon condensates, etc. are disc...
We give a general thermodynamical argument showing that in neutron stars, the Coulomb structured mix...
We examine the present status of the theoretical calculations for the internal structure of neutron ...
We investigate 1st order phase transitions in a general way, if not the single particle numbers of t...
AbstractWe consider how the occurrence of first-order phase transitions in non-constant pressure dif...
A structured mixed phase consisting of quark and hadron phases is numerically studied with the Coulo...
From sixth Texas symposium on relativistic astrophysics; New York, New York, USA (18 Dec 1972). Resu...
We investigate the occurrence of exotic structures in the outermost layers of neutron stars within t...
Numerous theoretical studies using various equation of state models have shown that quark matter may...
We investigate the properties of mixed stars formed by hadronic and quark matter in $\beta$-equilibr...
Deconfinement phase transition and condensation of Goldstone bosons in neutron star matter are inves...
Deconfinement phase transition and condensation of Goldstone bosons in neutron star matter are inves...
The transition from hadronic matter to quark matter in the core of neutron stars is likely to be as...
The transition from hadronic matter to quark matter in the core of neutron stars is likely to be as...