Some cosmological models coming from gravitational theories having torsional degrees of freedom
DOI10.1007/s10714-016-2113-7zbMath1387.83130arXiv1410.3152OpenAlexW3102367858MaRDI QIDQ682392
J. Lorca Espiro, Yerko Vásquez
Publication date: 2 February 2018
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1410.3152
Topological characterizations of particular spaces (54F65) Relativistic cosmology (83F05) Applications of differential geometry to physics (53Z05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) General geometric structures on low-dimensional manifolds (57M50) Exact solutions to problems in general relativity and gravitational theory (83C15) Astrophysical cosmology (85A40)
Related Items (4)
Cites Work
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- Relations among tautological classes revisited
- The dynamical structure of higher dimensional Chern-Simons theory
- Neutrino oscillations induced by spacetime torsion
- Cosmology with scalar–Euler form coupling
- Barbero–Immirzi parameter, manifold invariants and Euclidean path integrals
- The Immirzi parameter as an instanton angle
- Boundary terms, variational principles, and higher derivative modified gravity
- Beyond Einstein–Cartan gravity: quadratic torsion and curvature invariants with even and odd parity including all boundary terms
- Lovelock-Cartan theory of gravity
- A TORSIONAL TOPOLOGICAL INVARIANT
- Quantum realizations of Hilbert–Palatini second-class constraints
- A MINIMAL MODEL OF LORENTZ GAUGE GRAVITY WITH DYNAMICAL TORSION
- f(R) Cosmology with torsion
- An identity in Riemann–Cartan geometry
- The topological structure of Nieh-Yan form and the chiral anomaly in spaces with torsion
- Locally Weyl invariant massless bosonic and fermionic spin-1/2 action in the \((Y_4,g)\) space-time
- Physical aspects of the space-time torsion
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