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Abstract:

The operator structures that can contribute to three-nucleon forces are classified in the 1/Nc expansion. At leading order in 1/Nc a spin-flavor-independent term is present, as are the spin-flavor structures associated with the Fujita-Miyazawa three-nucleon force. Modern phenomenological three-nucleon forces are thus consistent with this O(Nc) leading force, corrections to which are suppressed by a power series in 1/Nc2. A complete basis of operators for the three-nucleon force, including all independent momentum structures, is given explicitly up to next-to-leading order in the 1/Nc expansion. © 2013 American Physical Society.

Registro:

Documento: Artículo
Título:Three-nucleon forces in the 1/Nc expansion
Autor:Phillips, D.R.; Schat, C.
Filiación:Institute of Nuclear and Particle Physics, Department of Physics and Astronomy, Ohio University, Athens, OH 45701, United States
Departamento de Física, FCEyN, Ciudad Universitaria, (1428) Buenos Aires, Argentina
Año:2013
Volumen:88
Número:3
DOI: http://dx.doi.org/10.1103/PhysRevC.88.034002
Título revista:Physical Review C - Nuclear Physics
Título revista abreviado:Phys. Rev. C Nucl. Phys.
ISSN:05562813
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562813_v88_n3_p_Phillips

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Citas:

---------- APA ----------
Phillips, D.R. & Schat, C. (2013) . Three-nucleon forces in the 1/Nc expansion. Physical Review C - Nuclear Physics, 88(3).
http://dx.doi.org/10.1103/PhysRevC.88.034002
---------- CHICAGO ----------
Phillips, D.R., Schat, C. "Three-nucleon forces in the 1/Nc expansion" . Physical Review C - Nuclear Physics 88, no. 3 (2013).
http://dx.doi.org/10.1103/PhysRevC.88.034002
---------- MLA ----------
Phillips, D.R., Schat, C. "Three-nucleon forces in the 1/Nc expansion" . Physical Review C - Nuclear Physics, vol. 88, no. 3, 2013.
http://dx.doi.org/10.1103/PhysRevC.88.034002
---------- VANCOUVER ----------
Phillips, D.R., Schat, C. Three-nucleon forces in the 1/Nc expansion. Phys. Rev. C Nucl. Phys. 2013;88(3).
http://dx.doi.org/10.1103/PhysRevC.88.034002