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Title: Naturalness of Nonlinear Scalar Self-Couplings in a Relativistic Mean Field Theory for Neutron Stars

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.1843632· OSTI ID:20630367
 [1]; ;  [2];  [3];  [4]
  1. Departamento de Fisica, Fundacao Universidade Federal de Rio Grande, CEP 96201-900 Rio Grande (Brazil)
  2. Instituto de Fisica, Universidade Federal do Rio Grande do Sul, CEP 91501-970 Porto Alegre, Rio Grande do Sul (Brazil)
  3. Institut fuer Theoretische Physik III, der Universitaet Erlangen-Nuernberg, D91058 Erlangen (Germany)
  4. Instituto de Fisica e Matematica, Universidade Federal de Pelotas, CEP 96010-900 Pelotas, Rio Grande do Sul (Brazil)

We investigate the role of naturalness in effective field theory. We focus on dense hadronic matter using a generalized relativistic multi-baryon lagrangian density mean field approach which contains nonlinear self-couplings of the {sigma}, {delta} meson fields and the fundamental baryon octet. We adjust the model parameters to describe bulk static properties of ordinary nuclear matter. Then, we show that our approach represents a natural modelling of nuclear matter under the extreme conditions of density as the ones found in the interior of neutron stars.

OSTI ID:
20630367
Journal Information:
AIP Conference Proceedings, Vol. 739, Issue 1; Conference: Joint meeting on QCD and QCP: 9. hadron physics and 7. relativistic aspects of nuclear physics, Rio de Janeiro (Brazil), 28 Mar - 3 Apr 2004; Other Information: DOI: 10.1063/1.1843632; (c) 2004 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
Country of Publication:
United States
Language:
English