English

Three-body forces and the limit of oxygen isotopes

Nuclear Theory 2013-01-04 v3 Solar and Stellar Astrophysics High Energy Physics - Phenomenology Nuclear Experiment

Abstract

The limit of neutron-rich nuclei, the neutron drip-line, evolves regularly from light to medium-mass nuclei except for a striking anomaly in the oxygen isotopes. This anomaly is not reproduced in shell-model calculations derived from microscopic two-nucleon forces. Here, we present the first microscopic explanation of the oxygen anomaly based on three-nucleon forces that have been established in few-body systems. This leads to repulsive contributions to the interactions among excess neutrons that change the location of the neutron drip-line from 28^{28}O to the experimentally observed 24^{24}O. Since the mechanism is robust and general, our findings impact the prediction of the most neutron-rich nuclei and the synthesis of heavy elements in neutron-rich environments.

Keywords

Cite

@article{arxiv.0908.2607,
  title  = {Three-body forces and the limit of oxygen isotopes},
  author = {Takaharu Otsuka and Toshio Suzuki and Jason D. Holt and Achim Schwenk and Yoshinori Akaishi},
  journal= {arXiv preprint arXiv:0908.2607},
  year   = {2013}
}

Comments

4 pages, 4 figures, to be published in PRL