{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,9,15]],"date-time":"2026-09-15T12:59:40Z","timestamp":1789477180575,"version":"build-2803163510"},"reference-count":146,"publisher":"MDPI AG","issue":"2","license":[{"start":{"date-parts":[[2024,2,10]],"date-time":"2024-02-10T00:00:00Z","timestamp":1707523200000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/4.0\/"}],"funder":[{"name":"Spanish MCIN\/AEI\/10.13039\/501100011033","award":["PID2020-118758GB-I00"],"award-info":[{"award-number":["PID2020-118758GB-I00"]}]},{"name":"Spanish MCIN\/AEI\/10.13039\/501100011033","award":["CEX2019-000918-M"],"award-info":[{"award-number":["CEX2019-000918-M"]}]}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Symmetry"],"abstract":"<jats:p>The saturation properties of symmetric and asymmetric nuclear matter have been computed using the finite range simple effective interaction with Yukawa form factor. The results of higher-order derivatives of the energy per particle and the symmetry energy computed at saturation, namely, Q0, Ksym, K\u03c4, Qsym, are compared with the corresponding values extracted from studies involving theory, experiment and astrophysical observations. The overall uncertainty in the values of these quantities, which results from a wide spectrum of studies described in earlier literature, lies in the ranges \u22121200\u2272Q0\u2272400 MeV, \u2212400\u2272Ksym\u2272100 MeV, \u2212840\u2272K\u03c4\u2272\u2212126 MeV and \u2212200\u2272Qsym\u2272800 MeV, respectively. The ability of the equations of state computed with this simple effective interaction in predicting the threshold mass for prompt collapse in binary neutron star merger and gravitational redshift has been examined in terms of the compactness of the neutron star and the incompressibility at the central density of the maximum mass star. The correlations existing between neutron star properties and the nuclear matter saturation properties have been analyzed and compared with the predictions of other model calculations.<\/jats:p>","DOI":"10.3390\/sym16020215","type":"journal-article","created":{"date-parts":[[2024,2,12]],"date-time":"2024-02-12T03:50:27Z","timestamp":1707709827000},"page":"215","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":4,"title":["Nuclear Matter Properties and Neutron Star Phenomenology Using the Finite Range Simple Effective Interaction"],"prefix":"10.3390","volume":"16","author":[{"given":"Xavier","family":"Vi\u00f1as","sequence":"first","affiliation":[{"name":"Departament de F\u00edsica Qu\u00e0ntica i Astrof\u00edsica (FQA), Institut de Ci\u00e8ncies del Cosmos (ICCUB), Universitat de Barcelona (UB), Mart\u00ed i Franqu\u00e8s 1, E-08028 Barcelona, Spain"},{"name":"Institut Menorqu\u00ed d\u2019Estudis, Cam\u00ed des Castell 28, E-07702 Ma\u00f3, Spain"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0003-2099-2185","authenticated-orcid":false,"given":"Parveen","family":"Bano","sequence":"additional","affiliation":[{"name":"School of Physics, Sambalpur University, Jyotivihar, Burla, Sambalpur 768 019, India"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0001-6285-7964","authenticated-orcid":false,"given":"Zashmir","family":"Naik","sequence":"additional","affiliation":[{"name":"School of Physics, Sambalpur University, Jyotivihar, Burla, Sambalpur 768 019, India"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0001-7774-8760","authenticated-orcid":false,"given":"Tusar Ranjan","family":"Routray","sequence":"additional","affiliation":[{"name":"School of Physics, Sambalpur University, Jyotivihar, Burla, Sambalpur 768 019, India"}],"role":[{"vocabulary":"crossref","role":"author"}]}],"member":"1968","published-online":{"date-parts":[[2024,2,10]]},"reference":[{"key":"ref_1","doi-asserted-by":"crossref","first-page":"207","DOI":"10.1016\/0370-1573(87)90085-8","article-title":"Nucleons, mesons and deltas in nuclear matter a relativistic Dirac-Brueckner approach","volume":"149","author":"Haar","year":"1987","journal-title":"Phys. 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