EPJ Web Conf.
Volume 113, 201621st International Conference on Few-Body Problems in Physics
|Number of page(s)||4|
|Section||Strangeness in Few-body Systems|
|Published online||25 March 2016|
Strangeness in nuclei and neutron stars: a challenging puzzle
1 Physics Division, Argonne National Laboratory, Lemont, Illinois 60439, USA
2 Theoretical Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
3 Department of Physics, University of Trento, Via Sommarive 14, I-38123 Trento, Italy
4 INFN-Trento Institute for Fundamental Physics and Application, Trento, Italy
Published online: 25 March 2016
The prediction of neutron stars properties is strictly connected to the employed nuclear interactions. The appearance of hyperons in the inner core of the star is strongly dependent on the details of the underlying hypernuclear force. We summarize our recent quantum Monte Carlo results on the development of realistic two- and threebody hyperon-nucleon interactions based on the available experimental data for light- and medium-heavy hypernuclei.
© Owned by the authors, published by EDP Sciences, 2016
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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