Cosmological models with the spinor and non-minimally interacting scalar field

DOI10.1142/S0217732315500157zbMath1307.83052arXiv1411.5445MaRDI QIDQ5178780

Yu. A. Rybalov, Andrey N. Makarenko, K. E. Osetrin

Publication date: 17 March 2015

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1411.5445

zbMATH Keywords

cosmological modelscalar fieldnon-minimally interactions

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Spinor and twistor methods in general relativity and gravitational theory; Newman-Penrose formalism (83C60) Equations of motion in general relativity and gravitational theory (83C10)

Cites Work

• Exact solutions in modified gravity models
• Cosmological solution of the Einstein-Weyl equation
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae

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