A5101727768- Pulsars and Gravitational Waves Research
- Gamma-ray bursts and supernovae
- Geophysics and Gravity Measurements
- High-Energy Particle Collisions Research
Saha Institute of Nuclear Physics
2024
Homi Bhabha National Institute
2024
Background: The equations of state (EoSs) which determine the properties neutron stars (NSs) are often characterized by isoscalar and isovector nuclear matter parameters (NMPs). Recent attempts to relate radius tidal deformability a NS individual NMPs have been inconclusive. These display strong correlations with pressure depends on several NMPs. It may be necessary map NMPs.Purpose: To identify important required describe star for astrophysically relevant range their gravitational masses...
Background: The equations of state (EoSs) which determine the properties neutron stars (NSs) are often characterized by iso-scalar and iso-vector nuclear matter parameters (NMPs). Recent attempts to relate radius tidal deformability a NS individual NMPs have been inconclusive. These display strong correlations with pressure depends on several NMPs. knowledge minimal that will be necessary address any connection between (e.g., deformability) finite nuclei. Purpose: To identify important...