Cosmological constant from quarks and torsion
arXiv:1005.0893 · doi:10.1002/andp.201000162
Abstract
We present a simple and natural way to derive the observed small, positive cosmological constant from the gravitational interaction of condensing fermions. In the Riemann-Cartan spacetime, torsion gives rise to the axial-axial four-fermion interaction term in the Dirac Lagrangian for spinor fields. We show that this nonlinear term acts like a cosmological constant if these fields have a nonzero vacuum expectation value. For quark fields in QCD, such a torsion-induced cosmological constant is positive and its energy scale is only about 8 times larger than the observed value. Adding leptons to this picture could lower this scale to the observed value.
4 pages; published version
References in corpus (23)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- Quantum Gravity, Torsion, Parity Violation and all that
- Physical effects of the Immirzi parameter
- The cosmological constant from the QCD Veneziano ghost
- The cosmological constant from the ghost. A toy model
- Why the cosmological constant is small and positive
- A cosmological constant from the QCD trace anomaly?
- The QCD nature of Dark Energy
- Self-tuning vacuum variable and cosmological constant
- Torsion Cosmology and the Accelerating Universe
- Dark spinor models in gravitation and cosmology
- Dark spinors with torsion in cosmology
- Dynamic vacuum variable and equilibrium approach in cosmology
- Gluonic vacuum, q-theory, and the cosmological constant
- Dark energy with dark spinors
- Nonsingular Dirac particles in spacetime with torsion
- Cosmological Bardeen-Cooper-Schrieffer condensate as dark energy
- The cosmological constant as a manifestation of the conformal anomaly?
- Torsion cosmological dynamics
- Vacuum energy density kicked by the electroweak crossover
- Neutrino Condensate as Origin of Dark Energy
Cited by in corpus (26)
- Nonsingular, big-bounce cosmology from spinor-torsion coupling
- Beyond Einstein-Cartan gravity: Quadratic torsion and curvature invariants with even and odd parity including all boundary terms
- Neutrino coupling to cosmological background: A review on gravitational Baryo/Leptogenesis
- Matter-antimatter asymmetry and dark matter from torsion
- Stability of the Einstein static universe in Einstein-Cartan theory
- Einstein-Cartan Cosmologies
- Dark Energy from graviton-mediated interactions in the QCD vacuum
- Dark spinor model with torsion and cosmology
- Einstein-Cartan Gravity with Torsion Field Serving as Origin for Cosmological Constant or Dark Energy Density
- Emergent scenario in the Einstein-Cartan theory
- Torsion, an alternative to dark matter?
- Four-fermion interaction from torsion as dark energy
- Quantum vacuum, dark matter, dark energy and spontaneous supersymmetry breaking
- Boson mixing and flavor vacuum in the expanding Universe: a possible candidate for the dark energy
- Dark matter and dark energy induced by condensates
- Analyzing Black Hole super-radiance Emission of Particles/Energy from a Black Hole as a Gedankenexperiment to get bounds on the mass of a Graviton
- Torsion gravity with non-minimally coupled fermionic field: some cosmological models
- Renormalizability of the Dirac Equation in Torsion-Gravity with Non-Minimal Coupling
- Torsion at different scales: from materials to the Universe
- On Dark Energy and Accelerated Reference Frames
- Einstein-Cartan-Dirac gravity with symmetry breaking
- Spinor fields in -gravity
- Cosmological bounces, cyclic universes, and effective cosmological constant in Einstein-Cartan-Dirac-Maxwell theory
- Beyond Einstein: A Polynomial Affine Model of Gravity
- Fermion condensate from torsion in the reheating era after inflation
- Torsional four-fermion interaction and the Raychaudhuri equation