Viability of the Matter Bounce Scenario

Abstract

It is shown that teleparallel $F(\mathcal{T})$ theories of gravity combined with Loop Quantum Cosmology support a Matter Bounce Scenario which is an alternative to the inflation scenario in the Big Bang paradigm. It is checked thatthese bouncing models provide theoretical data that fits well with the current observational data, allowing the viability of the Matter Bounce Scenario.

Communication to the ERE2014, (Spanish Relativistic Meeting)

References in corpus (7)

• Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
• Dark torsion as the cosmic speed-up
• Are loop quantum cosmos never singular?
• Loop quantum gravity corrections to gravitational wave dispersion
• Consistency of holonomy-corrected scalar, vector and tensor perturbations in Loop Quantum Cosmology
• Matter creation in a nonsingular bouncing cosmology
• Single field inflation with modulated potential in light of the Planck and BICEP2

Cited by in corpus (4)

• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• $\Lambda$CDM Bounce Cosmology without $\Lambda$CDM: the case of modified gravity
• Phenomenological Reconstruction of $f(T)$ Teleparallel Gravity
• Myrzakulov $F(T,Q)$ gravity: cosmological implications and constraints