Ab initio calculation of charge symmetry breaking in and -hypernuclei
arXiv:2210.03387 · doi:10.1103/PhysRevC.107.024002
Abstract
The separation energies of the isospin triplet , , Be, and the doublet Li, Be are investigated within the no-core shell model. Calculations are performed based on a hyperon-nucleon potential derived from chiral effective field theory at next-to-leading order. The potential includes the leading charge-symmetry breaking (CSB) interaction in the N channel, whose strength has been fixed to the experimentally known difference of the separation energies of the mirror hypernuclei and . It turns out that the CSB predicted for the systems is small and agrees with the splittings deduced from the empirical binding energies within the experimental uncertainty. In case of the doublet, the computed CSB is somewhat larger than the available experimental value. Using other experimental input for can change this prediction moving it closer to experiment.
11 pages, 4 tables
References in corpus (8)
- Observation of Lambda H-4 hyperhydrogen by decay-pion spectroscopy in electron scattering
- Charge symmetry breaking in hypernuclei revisited
- Nuclear properties with semilocal momentum-space regularized chiral interactions beyond N2LO
- Structure of Be and B hypernuclei studied with the four-body cluster model
- Jacobi no-core shell model for -shell hypernuclei
- Constraints on the -neutron interaction from charge symmetry breaking in the -- hypernuclei
- Nuclear physics uncertainties in light hypernuclei
- Measurement of and binding energy in Au+Au collisions at = 3 GeV
Cited by in corpus (4)
- Thermal behavior as indicator for hyperons in binary neutron star merger remnants
- First measurement of A = 4 (anti)hypernuclei at the LHC
- Charge symmetry breaking in hypernuclei within RMF model
- Properties of hyperons in nuclear matter from chiral hyperon-nucleon interactions at next-to-next-to-leading order