4–9 juin 2023
Palais des Papes - Avignon - France
Fuseau horaire Europe/Paris
Thanks to all for an outstanding conference - see you in Fukushima for ARIS 2026!

Possible Existence of Extremely Neutron-Rich Superheavy Nuclei in Neutron Star Crusts Under a Superstrong Magnetic Field

8 juin 2023, 14:30
15m
oral contribution astrophysics/nucleosynthesis parallel session

Orateur

Dr Kazuyuki Sekizawa (Tokyo Institute of Technology)

Description

We investigate outer crust compositions for a wide range of pressures (densities) and magnetic-field strengths, adopting the latest experimental masses (AME2020) supplemented with various theoretical mass models. By exploring the optimal composition of nuclei in the entire nuclear chart, we find emergence of neutron-rich heavy nuclei, which are much heavier than previously thought (that was at most $Z\approx50$), mainly because of the increasing electron density with the magnetic field strength, which allows nuclei to exist at higher densities without leakage of neutrons. We point out a clear manifestation of neutron magic numbers, e.g. $N=50, 82, 126$, as well as $184$, and possibly those around the next spherical magic number $N\approx 258$. Furthermore, surprisingly enough, for $B\geq4\times10^{18}$ G, we find that superheavy nuclei with $Z>110$, including the unknown element $119$, naturally emerge as optimal compositions that minimize the Gibbs energy. In this talk, we will explain the aforementioned findings and discuss possible consequences.

Author

Dr Kazuyuki Sekizawa (Tokyo Institute of Technology)

Co-auteur

M. Kentaro Kaba (Tokyo Institute of Technology)

Documents de présentation

Aucun document.