Wormholes in -gravity within the formalism
arXiv:1709.07774 · doi:10.1140/epjc/s10052-018-5538-1
Abstract
We propose, as a novelty in the literature, the modelling of wormholes within the particular case of the gravity, namely , with and being the Ricci scalar and trace of the energy-momentum tensor, respectively, while and are constants. Although such a functional form application can be found in the literature, those concern to compact astrophysical objects, such that no wormhole analysis has been done so far. The quadratic geometric and linear material corrections of this theory make the matter content of the wormhole to remarkably be able to obey the energy conditions.
Published version
References in corpus (24)
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Shapiro delay measurement of a two solar mass neutron star
- A Massive Pulsar in a Compact Relativistic Binary
- f(R,T) gravity
- Disappearing cosmological constant in f(R) gravity
- Low surface brightness galaxies rotation curves in the low energy limit of gravity : no need for dark matter?
- Nonminimal coupling of perfect fluids to curvature
- Modelling wormholes in gravity
- Can we distinguish between black holes and wormholes by their Einstein-ring systems?
- Wormhole geometries supported by a nonminimal curvature-matter coupling
- Static Spherically Symmetric Wormholes in Gravity
- Nonminimal curvature-matter coupled wormholes with matter satisfying the null energy condition
- The simplest non-minimal matter-geometry coupling in the cosmology
- Wormholes in viable modified theories of gravity and Weak Energy Condition
- New asymptotically flat phantom wormhole solutions
- Dynamical Instability and Expansion-free Condition in Gravity
- Evolution of Axially Symmetric Anisotropic Sources in Gravity
- Neutron stars with hyperon cores: stellar radii and EOS near nuclear density
- Distinguishing black holes and wormholes with orbiting hot spots
- N-dimensional static and evolving Lorentzian wormholes with cosmological constant
- Tolman-Oppenheimer-Volkoff equations in non-local gravity
- The growth factor of matter perturbations in an f(R) gravity
- Non-minimal Coupling of Torsion-matter Satisfying Null Energy Condition for Wormhole Solutions
- Scalaron production in contracting astrophysical objects