Pages that link to "Item:Q5156520"
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The following pages link to Effects of symmetry energy on the radius and tidal deformability of neutron stars in the relativistic mean-field model (Q5156520):
Displaying 8 items.
- Constraining the surface gravitational redshift of proto neutron stars with new nucleon coupling constants (Q763271) (← links)
- Neutron-star tidal deformability and equation-of-state constraints (Q828792) (← links)
- Symmetry energy and neutron star properties in the saturated Nambu-Jona-Lasinio model (Q2403599) (← links)
- Symmetry restoration in the vicinity of neutron stars with a nonminimal coupling (Q2698914) (← links)
- Tidal deformability of neutron stars with exotic particles within a density dependent relativistic mean field model in R-squared gravity (Q5070225) (← links)
- The relationship of the neutron skin thickness to the symmetry energy and its slope (Q5097487) (← links)
- Non-radial oscillation modes in hybrid stars: consequences of a mixed phase (Q5882735) (← links)
- Impacts of symmetry energy slope on the oscillation frequencies of neutron stars with short-range correlation and admixed dark matter (Q6107132) (← links)