Matching of equations of state: Influence on calculated neutron star models

@inproceedings{43060,
   author = {Urbanec, Martin and Miller, John and Rikovska Stone, J.},
   address = {Opava},
   booktitle = {Proceedings of RAGtime 6/7: Workshops on black holes and neutron stars},
   keywords = {neutron stars, equations of state},
   language = {eng},
   location = {Opava},
   isbn = {80-7248-334-X},
   pages = {357-362},
   publisher = {Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, Ústav fyziky},
   title = {Matching of equations of state: Influence on calculated neutron star models},
   year = {2005}
}

TY  - JOUR
ID  - 43060
AU  - Urbanec, Martin - Miller, John - Rikovska Stone, J.
PY  - 2005
TI  - Matching of equations of state: Influence on calculated neutron star models
PB  - Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, Ústav fyziky
CY  - Opava
SN  - 807248334X
KW  - neutron stars, equations of state
N2  - Equations of state for neutron-star matter at densities above nuclear-matter density are usually joined onto an equation of state for matter at lower densities calculated using a different physical treatment. Since the way of making the join is not clearly defined, we have tested the sensitivity of derived neutron-star models to the way in which the matching is made. We consider the joining between Skyrme equations of state for the higher densities and the Baym--Bethe--Pethick equation of state for densities between the neutron-drip point and nuclear-matter density.
ER  - 

URBANEC, Martin, John MILLER a J. RIKOVSKA STONE. Matching of equations of state: Influence on calculated neutron star models. In \textit{Proceedings of RAGtime 6/7: Workshops on black holes and neutron stars}. Opava: Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, Ústav fyziky, 2005, s.~357-362, 5 s. ISBN~80-7248-334-X.