Studying the Landau mass parameter of the extended - model for neutron star matter
arXiv:2004.04210 · doi:10.1134/S1063779620040073
Abstract
We present a Bayesian analysis of the Landau mass within the extended - model for neutron star matter. To this purpose, we consider the mass measurement of the object PSR 0740+6620, the tidal deformability estimation from the GW170817 and the mass-radius estimate of PSR J0030+0451 by NICER. Using Landau mass as free parameter of the theory, we rely on the prediction power of the Bayesian method to find the best value for this nuclear quantity.
arXiv comment8 pages, 9 figures. Proceedings of The International Bogolyubov Conference on Problems of Theoretical and Mathematical Physics, MIRAN & JINR, September 9-13, 2019
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Cited by in corpus (9)
- A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy
- Was GW170817 a canonical neutron star merger? Bayesian analysis with a third family of compact stars
- Effect of hyperons on f-mode oscillations in Neutron Stars
- Studying the parameters of the extended - model for neutron star matter
- Constraints on the dense matter equation of state and neutron star properties from NICER's mass-radius estimate of PSR J0740+6620 and multimessenger observations
- Investigating the role of nuclear parameters in Neutron Star oscillations: a model comparison
- Application of Kaluza-Klein Theory in Modeling Compact Stars: Exploring Extra Dimensions
- Properties of the Object HESS J1731-347 as a Twin Compact Star
- The effect of multiple extra dimensions on the maximal mass of compact stars in Kaluza-Klein space-time