Home
For authors
Submission status

Archive
Archive (English)
Current
   Volumes 113-119
   Volumes 93-112
      Volume 112
      Volume 111
      Volume 110
      Volume 109
      Volume 108
      Volume 107
      Volume 106
      Volume 105
      Volume 104
      Volume 103
      Volume 102
      Volume 101
      Volume 100
      Volume 99
      Volume 98
      Volume 97
      Volume 96
      Volume 95
      Volume 94
      Volume 93
Search
VOLUME 96 (2012) | ISSUE 4 | PAGE 226
Neutron Rich Hypernuclei in Chiral Soliton Model
Abstract
The binding energies of neutron rich strangeness S=-1 hypernuclei are estimated in the chiral soliton approach using the bound state rigid oscillator version of the SU(3) quantization model. Additional binding of strange hypernuclei in comparison with nonstrange neutron rich nuclei takes place at not large values of atomic (baryon) numbers, A=B\leq\sim 10. This effect becomes stronger with increasing isospin of nuclides, and for the "nuclear variant" of the model with rescaled Skyrme constant e. Binding energies of 8Λ He and recently discovered 6Λ H satisfactorily agree with data. Hypernuclei 7ΛH, 9ΛHe are predicted to be bound stronger in comparison with their nonstrange analogues 7H, 9He; hypernuclei 10Λ Li, 11Λ Li, 12Λ Be, 13Λ Be etc. are bound stronger in the nuclear variant of the model.