Future of Nuclear Fission Theory
Michael Bender, Remi Bernard, George Bertsch, Satoshi Chiba, Jacek, Dobaczewski, Noel Dubray, Samuel Giuliani, Kouichi Hagino, Denis Lacroix,, Zhipan Li, Piotr Magierski, Joachim Maruhn, Witold Nazarewicz, Junchen Pei,, Sophie Peru, Nathalie Pillet, Jorgen Randrup, David Regnier

TL;DR
This paper reviews recent advances in nuclear fission theory, highlighting new conceptual and computational developments, and discusses their implications for astrophysics, superheavy elements, and neutrino physics.
Contribution
It summarizes key findings and recommendations from a 2019 workshop on innovative theoretical approaches to nuclear fission.
Findings
New theoretical avenues identified
Enhanced computational methods developed
Implications for astrophysics and fundamental physics discussed
Abstract
There has been much recent interest in nuclear fission, due in part to a new appreciation of its relevance to astrophysics, stability of superheavy elements, and fundamental theory of neutrino interactions. At the same time, there have been important developments on a conceptual and computational level for the theory. The promising new theoretical avenues were the subject of a workshop held at the University of York in October 2019; this report summarises its findings and recommendations.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
