Symmetry energy effects on the quark deconfinement phase transition
Περίληψη
The nuclear symmetry energy plays an important role on the structure of finite nuclei, as well as on the bulk properties of neutron stars. In the present study we study the effects of the symmetry energy on some properties of hybrid stars, which consist mainly of hadron and quark matter. To this end, for the hadron matter of hybrid stars, we parameterize the equation of state which describes the asymmetric and symmetric nuclear matter with the help of the parameter η = (K0L2)1/3, where K0 is the incompressibility and L is the slope parameter.
Λεπτομέρειες άρθρου
- Πώς να δημιουργήσετε Αναφορές
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Divaris, M., & Moustakidis, C. (2025). Symmetry energy effects on the quark deconfinement phase transition. Annual Symposium of the Hellenic Nuclear Physics Society, 31, 27–33. https://doi.org/10.12681/hnpsanp.8164
- Τεύχος
- Τόμ. 31 (2025): HNPS2024
- Ενότητα
- Oral contributions
Αυτή η εργασία είναι αδειοδοτημένη υπό το CC Αναφορά Δημιουργού – Μη Εμπορική Χρήση – Όχι Παράγωγα Έργα 4.0 4.0.
Αναφορές
D. Blaschke, et al., Phys. Rev. C 105, 035804 (2022); doi: 10.1103/PhysRevC.105.035804
DOI: https://doi.org/10.1103/PhysRevD.105.084069
L.L. Lopes, et al., Phys. Rev. C 109, 045801 (2024); doi: 10.1103/PhysRevC.109.045801
DOI: https://doi.org/10.1103/PhysRevC.109.045801
M. Divaris, et al., Phys. Rev. C 109, 055805 (2024); doi: 10.1103/PhysRevC.109.055805
DOI: https://doi.org/10.1103/PhysRevC.109.055805
