Quantum torsion with non-zero standard deviation: non-perturbative approach for cosmology

DOI10.1016/j.physletb.2013.01.008zbMath1370.83114arXiv1210.5878OpenAlexW2042498207MaRDI QIDQ2404999

Burkhard Kleihaus, Jutta Kunz, Vladimir Folomeev, Vladimir Dzhunushaliev

Publication date: 21 September 2017

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1210.5878

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Methods of quantum field theory in general relativity and gravitational theory (83C47)

Related Items

Neutrino oscillations in cosmological spacetime

Cites Work

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• Curvature phase transition in \(\mathbb{R}^ 2\) quantum gravity and induction of Einstein gravity
• SOME PROPERTIES OF THE "STRING GAS" WITH THE EQUATION OF STATE $p = -\frac{1}{3} \rho$
• Physical aspects of the space-time torsion

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