J 2010

Observational Tests of Neutron Star Relativistic Mean Field Equations of State

BĚTÁK, Emil, Zdeněk STUCHLÍK and Martin URBANEC

Basic information

Original name

Observational Tests of Neutron Star Relativistic Mean Field Equations of State

Authors

BĚTÁK, Emil, Zdeněk STUCHLÍK and Martin URBANEC

Edition

Acta Astronomica, PL - Polská republika, 2010, 0001-5237

Other information

Language

English

Type of outcome

Článek v odborném periodiku

Field of Study

10308 Astronomy

Confidentiality degree

není předmětem státního či obchodního tajemství

Organization unit

Faculty of Philosophy and Science in Opava

UT WoS

000280180500005

Keywords in English

Stars: neutron, Equation of state, Dense matter

Tags

, LC06014, MSM4781305903

Tags

International impact, Reviewed

Links

LC06014, research and development project. MSM4781305903, plan (intention).
Změněno: 8/12/2020 09:23, Mgr. Pavlína Jalůvková

Abstract

V originále

Set of neutron star observational results is used to test some selected equations of state of dense nuclear matter. The first observational result comes from the mass-baryon number relation for pulsar B of the double pulsar system J0737-3039. The secondone is based on the mass radius relation coming from observation of the thermal radiation of the neutron star RX J1856.35-3754. The third one follows the population analysis of isolated neutron star thermal radiation sources. The last one is the test ofmaximum mass. The equation of state of asymmetric nuclear matter is given by the parametrized form of the relativistic Brueckner-Hartree-Fock mean held, and we test selected parametrization that represent fits of full relativistic mean field calculation.We show that only one of them is capable to pass the observational tests.
Displayed: 25/12/2024 17:27