Description of isospin mixing by a generator coordinate method
arXiv:2108.07592 · doi:10.1103/PhysRevC.105.014311
Abstract
Background: The isospin mixing is an interesting feature of atomic nuclei. It plays a crucial role in astrophysical nuclear reactions. However, it is not straightforward for variational nuclear structure models to describe it. Purpose: We propose a tractable method to describe the isospin mixing within a framework of the generator coordinate method and demonstrate its usability. Method: We generate the basis wave functions by applying the Fermi transition operator to the wave functions of isobars. The superposition of these basis wave functions and variationally obtained wave functions quantitatively describes the isospin mixing. Results: Using 14N as an example, we demonstrate that our method reasonably describes both T = 0 and 1 states and their mixing. Energy spectrum and E1 transition strengths are compared with the experimental data to confirm isospin mixing. Conclusion: The proposed method is effective enough to describe isospin mixing and is useful, for example, when we discuss α capture reactions of N = Z nuclei.
arXiv comment14 pages, 3 figures
References in corpus (12)
- The 12C(a,g)16O reaction and its implications for stellar helium burning
- Deformed Base Antisymmetrized Molecular Dynamics and its Application to ^{20}Ne
- Cluster structures of excited states in C
- Rotations in isospace: a doorway to the understanding of neutron-proton superfluidity in N=Z nuclei
- Isospin-symmetry breaking in masses of nuclei
- Structure and decay pattern of linear-chain state in 14C
- Isospin-symmetry restoration within the nuclear density functional theory: formalism and applications
- Energy-density-functional calculations including the proton-neutron mixing
- Structure and decay of the pygmy dipole resonance in 26Ne
- Proton and neutron correlations in B
- Isospin Projected Antisymmetrized Molecular Dynamics and its Application to B
- New determinations of gamma-ray line intensities of the Ep = 550 keV and Ep = 1747 keV resonances of the 13-C(p,gamma)14-N reaction