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Few new concepts of nuclear physics in a neutron star environment
Vlasios Petousis
* 1 ,
Martin Veselský
2 ,
Jozef Leja
3 ,
Charalampos Moustakidis
4 ,
George Souliotis
5 ,
Aldo Bonasera
6, 7 ,
Laura Navarro
8
1  Institute of Experimental and Applied Physics - Czech Technical University in Prague
2  Institute of Experimental and Applied Physics – Czech Technical University in Prague
3  Faculty of Mechanical Engineering - Slovak University of Technology in Bratislava
4  Aristotle University of Thessaloniki, Greece
5  Laboratory of Physical Chemistry, Department of Chemistry - National and Kapodistrian University of Athens, Greece
6  Cyclotron Institute, Texas A&M University, College Station, Texas, USA
7  Laboratori Nazionali del Sud, INFN, Catania, Italy
8  Department of Physics and Mathematics, University of Zaragoza, Spain
Academic Editor: Nicolas Chamel
Published: 17 February 2023 by MDPI in 2nd Electronic Conference on Universe session Compact Objects
https://doi.org/10.3390/ECU2023-14051
Abstract:

Neutron stars are nuclear physics laboratories, providing a unique opportunity to apply and search for new physics. In that spirit, we explored few new concepts of nuclear physics studied in a neutron star environment: In the first concept, the reported 17 MeV boson, which has been proposed as an explanation to the 8Be ,4He and 12C reported anomalies, is investigated in the context of its possible influence in the neutron star structure, defining a universal Equation of State as well. In the second concept, the synthesis of hyper-heavy elements is investigated under conditions, simulating the neutron star environment.

Keywords: Nuclear Physics; Neutrons Stars; Equation of State
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