Published August 1, 2008 | Version v1
Journal article

Skyrmion semiclassical quantization in the presence of an isospin chemical potential

  • 1. CONICET, Rivadavia 1917, 1033 Buenos Aires (Argentina) and Universidad Favaloro, Solis 453, 1078 Buenos Aires (Argentina)
  • 2. Physics Department, Comision Nacional de Energia Atomica, 1429 Buenos Aires (Argentina)
  • 3. Department of Physics, University of Maryland, College Park, Maryland 20742-4111 (United States) and CEFIMAS, Aveniada Santa Fe 1145, 1059 Buenos Aires (Argentina) and CONICET, Rivadavia 1917, 1033 Buenos Aires (Argentina) and Universidad Nacional de La Plata, C.C. 67, 1900 La Plata (Argentina)

Description

The semiclassical description of Skyrmions at small isospin chemical potential μI is carefully analyzed. We show that when the calculation of the energy of a nucleon is performed using the straightforward generalization of the vacuum sector techniques (μI=0), together with the 'natural' assumption μI=O(Nc0), the proton and neutron masses are nonlinear in μI in the regime |μI|<mπ. Although these nonlinearities turn out to be numerically quite small, such a result fails to strictly agree with the very robust prediction that for those values of μI the energy excitations above the vacuum are linear in μI. The resolution of this paradox is achieved by studying the realization of the large Nc limit of QCD in the Skyrme model at finite μI. This is done in a simplified context devoid of the technical complications present in the Skyrme model but which fully displays the general scaling behavior with Nc. The analysis shows that the paradoxical result appears as a symptom of using the semiclassical approach beyond its regime of validity and that, at a formal level, the standard methods for dealing with the Skyrme model are only strictly justified for states of high isospin, I∼Nc.

Additional details

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
78
Journal Issue
3
Journal Page Range
p. 034040-034040.10
ISSN
0556-2821
CODEN
PRVDAQ

Optional Information

Notes
(c) 2008 The American Physical Society