Cosmological dark matter amplification through dark torsion
From MaRDI portal
Publication:5162052
DOI10.1088/1361-6382/abb2d2zbMath1479.83272arXiv2004.06058OpenAlexW3015548514MaRDI QIDQ5162052
Fernando Izaurieta, Samuel Lepe
Publication date: 1 November 2021
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2004.06058
Relativistic cosmology (83F05) Simple homotopy type, Whitehead torsion, Reidemeister-Franz torsion, etc. (57Q10) Dark matter and dark energy (83C56)
Cites Work
- Unnamed Item
- On Poincaré gauge theory of gravity, its equations of motion, and Gravity Probe B
- Gravity-induced four-fermion contact interaction implies gravitational intermediate W and Z type gauge bosons
- The theory of local mass dimension one fermions of spin one half
- Cosmology with scalar–Euler form coupling
- Chern–Simons forms in gravitation theories
- The observable universe inside a black hole
- Lorentz Invariance and the Gravitational Field
- The Weyssenhoff fluid in Einstein-Cartan theory
- Non-minimally coupled scalar field cosmology with torsion
- Prospects of detecting spacetime torsion
- Elko and mass dimension one field of spin one-half: Causality and Fermi statistics
- General relativity with spin and torsion: Foundations and prospects
- Multivalued Fields
- Chern–Simons (Super)Gravity
- Supergravity
- Physical aspects of the space-time torsion
