Published December 15, 2011 | Version v1
Journal article

Number of Nambu-Goldstone bosons and its relation to charge densities

  • 1. Department of Physics, University of California, Berkeley, California 94720 (United States)
  • 2. Department of Physics, University of Tokyo, Hongo, Tokyo 113-0033 (Japan)
  • 3. Department of Theoretical Physics, Nuclear Physics Institute ASCR, 25068 Rez (Czech Republic)
  • 4. Faculty of Physics, University of Bielefeld, 33615 Bielefeld (Germany)

Description

The low-energy physics of systems with spontaneous symmetry breaking is governed by the associated Nambu-Goldstone (NG) bosons. While NG bosons in Lorentz-invariant systems are well understood, the precise characterization of their number and dispersion relations in a general quantum many-body system is still an open problem. An inequality relating the number of NG bosons and their dispersion relations to the number of broken symmetry generators was found by Nielsen and Chadha. In this paper, we give a presumably first example of a system in which the Nielsen-Chadha inequality is actually not saturated. We suggest that the number of NG bosons is exactly equal to the number of broken generators minus the number of pairs of broken generators whose commutator has a nonzero vacuum expectation value. This naturally leads us to a proposal for a different classification of NG bosons.

Additional details

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
84
Journal Issue
12
Journal Page Range
p. 125013-125013.9
ISSN
0556-2821
CODEN
PRVDAQ

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
43080483
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Descriptors DEI
CHARGE DENSITY; CLASSIFICATION; DISPERSION RELATIONS; EXPECTATION VALUE; GOLDSTONE BOSONS; LORENTZ INVARIANCE; MANY-BODY PROBLEM; SYMMETRY BREAKING
Descriptors DEC
BOSONS; ELEMENTARY PARTICLES; INVARIANCE PRINCIPLES; POSTULATED PARTICLES

Optional Information

Notes
(c) 2011 American Institute of Physics