2008
Equation of state of dense matter in neutron stars
ČERNÝ, Slavomír; Stanislav HLEDÍK and Zdeněk STUCHLÍKBasic information
Original name
Equation of state of dense matter in neutron stars
Authors
ČERNÝ, Slavomír; Stanislav HLEDÍK and Zdeněk STUCHLÍK
Edition
Singapore, Eleventh Marcel Grossmann Meeting on General Relativity Berlin, 3 pp. 2008
Publisher
World Scientific
Other information
Language
English
Type of outcome
Proceedings paper
Field of Study
10308 Astronomy
Confidentiality degree
is not subject to a state or trade secret
Organization unit
Faculty of Philosophy and Science in Opava
ISBN
978-981-283-426-3
Keywords in English
Neutron star, Equation of state (EoS), Mean eld model, Kaon, Pion, Hyperon
Tags
International impact
Links
MSM4781305903, plan (intention).
Changed: 8/12/2020 14:11, Mgr. Pavlína Jalůvková
Abstract
In the original language
Interior of a neutron star consists of various types of matter; namely (from surface towards the centre): iron crust described by Feynman-Metropolis-Teller EoS, neutron rich nuclei described by Baym-Pethick-Sunderland EoS, neutron drip to dissolve nucleidescribed by Baym-Bethe-Pethick EoS, and the very centre of a neutron star described by various types of EoS with kaons, pions and hyperons.