Estimating Microscopic Nuclear Data by Compact Star Observations

We studied recent observation data of pulsar masses and radii of PSR J0740+6620, PSR J0348+0432, and PSR J1614–2230 from different measurements, based on the extended version of σ-ω model. Throughout our analysis, we assumed that these pulsars are maximal-mass compact stars, thus we applied the core...

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Bibliographic Details
Published in:EPJ Web of conferences Vol. 259; p. 13011
Main Authors: Szigeti, Balázs Endre, Barnaföldi, Gergely Gábor, Pósfay, Péter, Jakovác, Antal
Format: Journal Article Conference Proceeding
Language:English
Published: Les Ulis EDP Sciences 2022
Subjects:
Compressibility
Pulsars
ISSN:2100-014X, 2101-6275, 2100-014X
Online Access:Get full text
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Summary:We studied recent observation data of pulsar masses and radii of PSR J0740+6620, PSR J0348+0432, and PSR J1614–2230 from different measurements, based on the extended version of σ-ω model. Throughout our analysis, we assumed that these pulsars are maximal-mass compact stars, thus we applied the core approximation. Based on the linear relation between the microscopic and macroscopic parameters of compact stars evaluated by our model, we estimated the average Landau mass m L = 752.46 - 42.5 + 49.1 MeV and compressibility K = 261.7 - 28.0 + 57.2 MeV.
Bibliography:ObjectType-Conference Proceeding-1
SourceType-Conference Papers & Proceedings-1
content type line 21
ISSN:2100-014X
2101-6275
2100-014X
DOI:10.1051/epjconf/202225913011