The role of an invariant IR cutoff in late time cosmological dynamics

Abstract

We study the role of an invariant infra-red cutoff in the late time cosmological dynamics. This low energy cutoff originates from the existence of a minimal measurable uncertainty as a result of the curvature of background manifold, and can be encoded in an extended uncertainty relation. Inspired by black hole entropy-area relation, we extend the analysis to the thermodynamics of apparent horizon of the universe. By treating both the Newtonian and general relativistic cosmologies, we show that the contribution of infra-red cutoff in the equations of dynamics can be interpreted as an effective fluid which is capable of explaining late time cosmic speed up and even transition to a phantom phase of expansion. We use the latest observational data from PLANCK2018 to constrain the parameter of an extended uncertainty relation.

arXiv comment13 pages, one figure, accepted for publication in Phys. Lett. B

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Cited by in corpus (4)

• Investigating bounds on the extended uncertainty principle metric through astrophysical tests
• Thermostatistics with an Invariant Infrared Cutoff
• Behavior of a Free Quantum Particle in the Poincaré Upper Half-Plane Geometry
• IR-deformed thermodynamics of quantum bouncers and the issue of dimensional reduction