Axion hair and dynamical torsion from anomalies

1992/11/01 by M. J. Duncan, M.J Duncan, Nemanja Kaloper +3 · 1 voice · 3 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Pulsars and Gravitational Waves Research

paper · doi:10.1016/0550-3213(92)90052-d

crossref issued 1992/11/01 · crossref published 1992/11/01 · crossref published-print 1992/11/01 · openalex publication_date 1992/11/01 · crossref created 2002/11/12 · crossref deposited 2019/04/03 · openalex created_date 2025/10/10 · crossref indexed 2026/06/16 · openalex updated_date 2026/06/17

Cited by

• Beautiful Gauge Field Equations in Clifforms
• Dynamical-System analysis of single-axion monodromy inflation with periodically-modulated potentials
• A Photon Cloud Induced from an Axion Cloud

Discussions

• The traceless part of the torsion tensor is not arbitrarily set to zero, but is found to vanish through the equations of motion. In Einstein-Cartan theory, the gravitational action is given as $$ S_{G [stackexchange, 2 points]