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Cosmological constant from quarks and torsion

✍ Scribed by N.J. Popławski


Publisher
John Wiley and Sons
Year
2011
Tongue
English
Weight
124 KB
Volume
523
Category
Article
ISSN
0003-3804

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✦ Synopsis


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 vector 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.


📜 SIMILAR VOLUMES


Cosmological constant and vacuum energy
✍ G.E. Volovik 📂 Article 📅 2005 🏛 John Wiley and Sons 🌐 English ⚖ 127 KB

The general thermodynamic analysis of the quantum vacuum, which is based on our knowledge of the vacua in condensed-matter systems, is consistent with the Einstein earlier view on the cosmological constant. In the equilibrium Universes the value of the cosmological constant is regulated by matter. I