Cosmological model with fermion and tachyon fields interacting via Yukawa-type potential
From MaRDI portal
Publication:2800896
DOI10.1142/S0217732316500395zbMath1334.83082arXiv1602.06874MaRDI QIDQ2800896
F. P. Devecchi, Marlos O. Ribas, Gilberto Medeiros Kremer
Publication date: 19 April 2016
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1602.06874
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (9)
Cosmology of fermionic dark energy coupled to curvature ⋮ Fermionic and bosonic fields in the Einstein–Cartan theory ⋮ Dirac spinors and their application to Bianchi-I space-times in 5 dimensions ⋮ On Einstein-non linear-Maxwell-Yukawa de-Sitter black hole thermodynamics ⋮ Einstein-nonlinear Maxwell–Yukawa black hole ⋮ Topologically nontrivial solution in Einstein-Dirac gravity on the Hopf bundle ⋮ Classical and quantum cosmological solutions in Bianchi type-I metric with fermionic field and relativistic fluid in Schutz’s formalism ⋮ Cosmology with fermionic sources and relativistic fluid in Schutz’s formalism: Classical and quantum solutions ⋮ Non minimally coupled condensate cosmologies: matching observational data with phase space
Cites Work
This page was built for publication: Cosmological model with fermion and tachyon fields interacting via Yukawa-type potential
