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

Authors

URBANEC, Martin, John MILLER and J. RIKOVSKA STONE

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

Language

English

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

ISBN

80-7248-334-X

Keywords in English

neutron stars, equations of state

Tags

International impact

Links

MSM4781305903, plan (intention).
Změněno: 8/12/2020 09:04, Mgr. Pavlína Jalůvková

Abstract

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.