Argonne potential and multi-neutron systems
- Saint Petersburg State University, Uljanovskaja 1, 198504 St. Petersburg (Russian Federation)
- Frankfurt Institute of Advanced Studies, Ruth-Moufang Str. 1, 60438 Frankfurt (Germany)
Recently it was proved that the neutron matter interacting through Argonne V18 pair-potential plus modern variants of Urbana or Illinois three-body forces is unstable. For the energy of N neutrons E(N), which interact through these forces one has E(N) = −cN³⁺+O(N{sup 8/3}), where c > 0 is a constant. This means that: (i) the energy per particle and neutron density diverge rapidly for large neutron numbers; (ii) bound states of N neutrons exist for N large enough. The neutron matter collapse is possible due to the form of the repulsive core in three-body forces, which vanishes when three nucleons occupy the same site in space. The obtained results partly change the paradigm, in which the stability of neutron stars is attained through the Pauli principle; the strong repulsive core in the nucleon interactions is by no means less important.
- OSTI ID:
- 22306046
- Journal Information:
- AIP Conference Proceedings, Vol. 1606, Issue 1; Conference: 2. Russian-Spanish congress on particle and nuclear physics at all scales, astroparticle physics and cosmology, St. Petersburg (Russian Federation), 1-4 Oct 2013; Other Information: (c) 2014 AIP Publishing LLC; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
- Publisher:
- AIP
- Country of Publication:
- United States
- Language:
- English
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