Chiral anomaly in contorted spacetimes
From MaRDI portal
Publication:1807401
DOI10.1023/A:1026653314045zbMath0945.83022arXivgr-qc/9704051MaRDI QIDQ1807401
Dirk Kreimer, Eckehard W. Mielke
Publication date: 18 November 1999
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/gr-qc/9704051
Applications of global differential geometry to the sciences (53C80) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (4)
Einstein-Cartan gravity, asymptotic safety, and the running Immirzi parameter ⋮ TORSION, CHERN–SIMONS TERM AND DIFFEOMORPHISM INVARIANCE ⋮ Chern-Simons solutions of the chiral teleparallelism constraints of gravity ⋮ TRANSLATIONS AND DYNAMICS
Cites Work
- Unnamed Item
- Unnamed Item
- Unnamed Item
- A geometric formulation of the \(\mathrm{SO}(3,2)\) theory of gravity
- Hamiltonian interpretation of anomalies
- Quantum field theory techniques in graphical enumeration
- Fermionic zero-modes around string solitons
- Anomaly-free formulation of non-perturbative, four-dimensional Lorentzian quantum gravity
- Nonlinear gauge realization of spacetime symmetries including translations
- Quantized Gravitational Field
- An identity in Riemann–Cartan geometry
- Chern–Simons terms in metric-affine space-time: Bianchi identities as Euler–Lagrange equations
- Poincaré gauge invariance and gravitation in Minkowski spacetime
- Evaluation of the heat kernel in Riemann - Cartan space
This page was built for publication: Chiral anomaly in contorted spacetimes