Effective Electromagnetic Lagrangian at Finite Temperature and Density in the Electroweak Model
arXiv:1006.5067 · doi:10.2478/s11534-010-0140-7
Abstract
Using the exact propagators in a constant magnetic field, the effective electromagnetic Lagrangian at finite temperature and density is calculated to all orders in the field strength B within the framework of the complete electroweak model, in the weak coupling limit. The partition function and free energy are obtained explicitly and the finite temperature effective coupling is derived in closed form. Some implications of this result, potentially interesting to astrophysics and cosmology, are discussed.
14 pages, Revtex4
References in corpus (18)
- Magnetic Fields in the Early Universe
- Primordial Magnetic Fields, Right Electrons, and the Abelian Anomaly
- Large-scale magnetic fields from hydromagnetic turbulence in the very early universe
- Momentum signatures for Schwinger pair production in short laser pulses with a sub-cycle structure
- QED effective action at finite temperature and density
- The Electroweak Phase Transition in a Magnetic Field
- The Casimir Force in Randall Sundrum Models
- Real-Time Thermal Propagators and the QED Effective Action for an External Magnetic Field
- Finite temperature Casimir effect in spacetime with extra compactified dimensions
- Effective potential at finite temperature in a constant hypermagnetic field: Ring diagrams in the Standard Model
- Exact Effective Action for (1+1 Dimensional) Fermions in an Abelian Background at Finite Temperature
- Neutrino self-energy in external magnetic field
- Schwinger Pair Production at Finite Temperature in QED
- Thermal Versus Vacuum Magnetization in QED
- Casimir energy, dispersion, and the Lifshitz formula
- Finite Temperature Effective Actions
- Effective actions at finite temperature
- Exact Effective action for (1+1)-dimensional fermions in an Abelian background at finite temperature and chemical potential
Cited by in corpus (4)
- Finite temperature Casimir effect for charged massless scalars in a magnetic field
- Symmetry restoration at finite temperature with weak magnetic fields
- Finite temperature Casimir effect for massive scalars in a magnetic field
- Magnetic field corrections to the repulsive Casimir effect at finite temperature