Published October 1, 2004
| Version v1
Journal article
Quantum anomalies in dense matter
Creators
- 1. Institute for Nuclear Theory, University of Washington, Seattle, Washington 98195-1550 (United States)
- 2. Department of Physics and Astronomy, University of British Columbia, Vancouver, BC, V6T 1Z1 (Canada)
Description
We consider the effects of quantum anomalies involving the baryon current for high-density matter. In the effective Lagrangian, the anomaly terms describe the interaction of three light fields: the electromagnetic photons Aμ, neutral light Nambu-Goldstone bosons (π, η, η'), and the superfluid phonon. The anomaly induced interactions lead to a number of interesting phenomena which may have phenomenological consequences observable in neutron stars
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.70.074018;
- arXiv
- arXiv:hep-ph/0405216v1;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 70
- Journal Issue
- 7
- Journal Page Range
- p. 074018-074018.5
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37020534
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- BARYONS; BASIC INTERACTIONS; GOLDSTONE BOSONS; LAGRANGIAN FIELD THEORY; LAGRANGIAN FUNCTION; NEUTRAL CURRENTS; NEUTRON STARS; NUCLEAR MATTER; PHONONS; PHOTONS; QUANTUM CHROMODYNAMICS; SUPERFLUIDITY
- Descriptors DEC
- ALGEBRAIC CURRENTS; BOSONS; CURRENTS; ELEMENTARY PARTICLES; FERMIONS; FIELD THEORIES; FUNCTIONS; HADRONS; INTERACTIONS; MASSLESS PARTICLES; MATTER; POSTULATED PARTICLES; QUANTUM FIELD THEORY; QUASI PARTICLES; STARS
Optional Information
- Notes
- (c) 2004 The American Physical Society