2013/09/30 by D. N. Basu, D N BASU
Physics and Astronomy · #Elastic scattering #Equation of state #High-Energy Particle Collisions Research #Isospin #Neutron #Neutron star #Nuclear drip line #Nuclear matter #Nuclear physics research studies #Nuclear reaction #Pulsars and Gravitational Waves Research #Symmetry (geometry) #nucl-th
paper · pdf · doi:10.1007/s12043-014-0734-5
published in Pramana 82(5), 809-822 · 11 pages including 2 figures and 3 tables; Invited talk delivered at the National Conference on Nuclear Physics, March 01 - 03 2013, School of Physics, Sambalpur University, India
arxiv created 2014/04/11 · openalex publication_date 2014/04/29 · arxiv updated 2014/11/04 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
An equation of state (EoS) for symmetric nuclear matter is constructed using the density dependent M3Y effective interaction and extended for isospin asymmetric nuclear matter. Theoretically obtained values of symmetric nuclear matter incompressibility, isobaric incompressibility, symmetry energy and its slope agree well with experimentally extracted values. Folded microscopic potentials using this effective interaction, whose density dependence is determined from nuclear matter calculations, provide excellent descriptions for proton, alpha and cluster radioactivities, elastic and inelastic scattering. The nuclear deformation parameters extracted from inelastic scattering of protons agree well with other available results. The high density behavior of symmetric and asymmetric nuclear matter satisfies the constraints from the observed flow data of heavy-ion collisions. The neutron star properties studied using β-equilibrated neutron star matter obtained from this effective interaction reconcile with the recent observations of the massive compact stars.