The equation of state (EOS) of cold and dense strongly interacting matter is crucial for better research of compact stars, i.e., neutron stars and quark stars. We generalize our improved quasi-particle model from finite temperature and zero chemical potential [Phys. Lett. B 711 (2012) 65] to the case of zero temperature and finite chemical potential to obtain an EOS of our improved quasi-particle model and then apply this EOS to study the structure of a quark star. The results are consistent with the most recent astronomical observational data.


    Zugriff

    Zugriff über TIB

    Verfügbarkeit in meiner Bibliothek prüfen

    Bestellung bei Subito €


    Exportieren, teilen und zitieren



    Titel :

    Quark Stars Investigated using an Improved Quasi-Particle Model


    Beteiligte:
    Yan, Yan (Autor:in) / Cao, Jing (Autor:in) / Luo, Xin-Lian (Autor:in) / Sun, Wei-Min (Autor:in) / Zong, Hong-Shi (Autor:in)

    Erschienen in:

    Chinese Physics Letters ; 29 , 10 ; 101201/1-101201/4


    Erscheinungsdatum :

    2012


    Format / Umfang :

    4 Seiten, 25 Quellen




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Print


    Sprache :

    Englisch




    AXPs-SGRs: Magnetars or quark-stars?

    Xu, Renxin | Online Contents | 2007


    AXPs/SGRs: Magnetars or quark-stars?

    Xu, Renxin | Elsevier | 2007



    Helicopter Rotor Ground Effect and Frigate Interaction Investigated by Particle Image Velocimetry

    Bardera Mora, Rafael / Matías García, Juan Carlos | AIAA | 2021


    comparison of measured and predicted combustion characteristics using an improved quasi-dimensional model

    Mugele, M. / Worret, R. / Spicher, U. et al. | SAE Technical Papers | 1999