C. A. Bertulani

1 ta ish

East Texas A&M University

1. Neutron stars in $$f(\mathtt {R,L_m})$$ gravity with realistic equations of state: joint-constrains with GW170817, massive pulsars, and the PSR J0030+0451 mass-radius from NICER data

   Ronaldo V. Lobato, G. A. Carvalho, C. A. Bertulani

   Maqola20215 iqtibos

   ABIABI:AkademIndex/2026.other.332063