Pairing Theory of the Wigner Cusp
K. Neerg{\aa}rd

TL;DR
This paper investigates the Wigner cusp in nuclear masses, showing that RPA corrections and shell effects are crucial for understanding the mass variation near N=Z, with implications for nuclear superfluidity and symmetry energy modeling.
Contribution
It introduces RPA corrections to BCS pairing in Nilsson-Strutinskij calculations, clarifying their role in the Wigner cusp and linking symmetry energy to nuclear superfluidity.
Findings
RPA correction accounts for mass variation near N=Z
Macroscopic symmetry energy proportional to T(T+1)
Shell effects dominate Wigner cusp shape
Abstract
Conclusions: (1) Calculations with an RPA correction added to the BCS pairing correction conventionally employed in Nilsson-Strutinskij calculations account well for the variation with A of the pattern of masses near N=Z. (2) The RPA correction is insignificant for reproducing the doubly even masses and hence for the shape of the Wigner cusp. (3) It is important, however, that the macroscopic (liquid drop) symmetry energy be proportional to T(T+1). (4) This form of the macroscopic symmetry energy is understood microscopically, in terms of the RPA, to result from the nuclear superfluidity. (5) The variation of the shape of the Wigner cusp is dominated by shell effects. (6) The RPA correction significally reduces the T=0 binding in doubly odd nuclei, thus reducing the required pair coupling constant.
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.
Taxonomy
Topicsadvanced mathematical theories · Advanced Algebra and Geometry · Spectral Theory in Mathematical Physics
