Effective relativistic mean field model for finite nuclei and neutron stars
Bharat Kumar, B. K. Agrawal, and S. K. Patra
TL;DR
This paper introduces the IOPB-I parameter set for the relativistic mean field model, enhancing the theoretical tools for studying finite nuclei and neutron stars.
Contribution
Development of the new IOPB-I parameter set improves the accuracy of relativistic mean field models for nuclear and astrophysical applications.
Findings
Enhanced modeling of finite nuclei properties
Improved predictions for neutron star characteristics
Validation against experimental data
Abstract
New Relativistic mean field parameter set IOPB-I has been developed.
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Gamma-ray bursts and supernovae · Astrophysical Phenomena and Observations