<?xml version="1.0"?>
<rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:dc="http://purl.org/dc/elements/1.1/"><rdf:Description rdf:about="https://dirros.openscience.si/IzpisGradiva.php?id=28303"><dc:title>Symmetry in nuclear physics and astrophysics</dc:title><dc:creator>Vesić,	Jelena	(Avtor)
	</dc:creator><dc:subject>symmetry energy</dc:subject><dc:subject>isospin</dc:subject><dc:subject>nuclear symmetry</dc:subject><dc:description>Symmetry is a key principle in physics that links basic invariances to the structure of matter and the evolution of the universe. In this review, we use symmetry as a unifying thread connecting nuclear structure, nuclear reactions, and dense matter, and we highlight how symmetry-based arguments connect laboratory observables to astrophysical constraints. We present the essential concepts in a form accessible to a broad physics audience.</dc:description><dc:publisher>MDPI</dc:publisher><dc:date>2026</dc:date><dc:date>2026-03-13 11:30:21</dc:date><dc:type>Neznano</dc:type><dc:identifier>28303</dc:identifier><dc:source>Švica</dc:source><dc:language>sl</dc:language><dc:rights>© 2026 by the author.</dc:rights></rdf:Description></rdf:RDF>
