KM
About
Nuclear physics for neutron stars, supernovae, neutron star mergers, and heavy-ion collisions
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Publications (19)
- Relativistic mean-field model with density- and isospin-density-dependent couplings Save
- Effect of mesonic off-shell correlations in the PNJL equation of state Save
- Confining density functional approach for color superconducting quark matter and mesonic correlations Save
- Hybrid equation of state with pasta phases, and third family of compact stars Save
- Quark-hadron pasta in neutron stars Save
- RMF models with σ -scaled hadron masses and couplings for the description of heavy-ion collisions below 2 A GeV Save
- Charged ρ meson condensate in neutron stars within RMF models Save
- Charged ρ-meson condensation in neutron stars Save
- Cooling of neutron stars in “nuclear medium cooling scenario” with stiff equation of state including hyperons Save
- Hyperons, Δ resonances and condensate of charged ρ mesons within relativistic mean-field models with scaled hadron masses and couplings Save
- On cooling of neutron stars with a stiff equation of state including hyperons Save
- Robustness of third family solutions for hybrid stars against mixed phase effects Save
- Delta isobars in relativistic mean-field models with σ-scaled hadron masses and couplings Save
- The effect of inclusion of Δ resonances in relativistic mean-field model with scaled hadron masses and coupling constants Save
- Δ resonances and charged ρ mesons in neutron stars Save
- Hyperon puzzle and the RMF model with scaled hadron masses and coupling constants Save
- Relativistic mean-field models with scaled hadron masses and couplings: Hyperons and maximum neutron star mass Save
- Making a soft relativistic mean-field equation of state stiffer at high density Save
- Solution of the hyperon puzzle within a relativistic mean-field model Save