D
2005
Matching of equations of state: Influence on calculated neutron star models
URBANEC, Martin, John MILLER and J. RIKOVSKA STONE
Basic information
Original name
Matching of equations of state: Influence on calculated neutron star models
Edition
Opava, Proceedings of RAGtime 6/7: Workshops on black holes and neutron stars, p. 357-362, 5 pp. 2005
Publisher
Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, Ústav fyziky
Other information
Type of outcome
Stať ve sborníku
Field of Study
10308 Astronomy
Country of publisher
Czech Republic
Confidentiality degree
není předmětem státního či obchodního tajemství
Organization unit
Faculty of Philosophy and Science in Opava
Keywords in English
neutron stars, equations of state
Tags
International impact
Links
MSM4781305903, plan (intention).
V originále
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.
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