2009/08/31 by Takaharu Otsuka, Toshio Suzuki, Jason D. Holt +5 · 486 citations
Physics and Astronomy · #Anomaly (physics) #Astro and Planetary Science #Astronomical and nuclear sciences #Atomic physics #Condensed matter physics #Isotope #Isotopes of oxygen #Line (geometry) #Materials science #Neutron #Nuclear drip line #Nuclear force #Nuclear physics #Nuclear physics research studies #Nucleon #Oxygen #Physics #Quantum mechanics #Shell (structure) #astro-ph.SR #hep-ph #nucl-ex #nucl-th
paper · pdf · doi:10.1103/physrevlett.105.032501
published in Physical Review Letters 105(3), 032501 (American Physical Society) · 4 pages, 4 figures, to be published in PRL
arxiv created 2010/06/19 · openalex publication_date 2010/07/13 · arxiv updated 2013/01/04 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/06
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)O to the experimentally observed (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.