A minimal Length Uncertainty Approach to Cosmological Constant Problem

Abstract

Based on quantum mechanical framework for the minimal length uncertainty, we demonstrate that the generalized uncertainty principle (GUP) parameter could be best constrained by recent gravitational waves observations on one hand. On other hand this suggests modified dispersion relations (MDRs) enabling an estimation for the difference between the group velocity of gravitons and that of photons. Utilizing features of the UV/IR correspondence and the obvious similarities between GUP (including non-gravitating and gravitating impacts on Heisenberg uncertainty principle) and the discrepancy between the theoretical and the observed cosmological constant (apparently manifesting gravitational influences on the vacuum energy density), we suggest a possible solution for the cosmological constant problem.

5 pages, 0 figures, an invited talk given at the int. Workshop on Astronomy and Relativistic Astrophysics (IWARA $2020$ Video Conference), accepted for publication in Astronomische Nachrichten

References in corpus (5)

• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Universality of Quantum Gravity Corrections
• Constraining the generalized uncertainty principle with the gravitational wave event GW150914
• Statistical physics in deformed spaces with minimal length
• Minimal-supersymmetric extended inflation field in Horava-Lifshitz gravity