Cut-off free finite zero-point vacuum energy and the cosmological missing mass problem
N. Kumar (Raman Research Institute, Bangalore, India)

TL;DR
This paper proposes a self-consistent method to account for gravitational self-energy that results in a finite vacuum energy contribution, potentially resolving the cosmological missing mass problem without requiring an ultraviolet cutoff.
Contribution
It introduces a non-perturbative gravitational charging technique to derive a finite vacuum energy contribution, addressing the infinite zero-point energy issue in cosmology.
Findings
Derives a finite gravitational mass from infinite vacuum energy.
Predicts a cosmological density parameter close to unity.
Provides a cutoff-free explanation for vacuum energy's role in cosmology.
Abstract
As the mass-energy is universally self-gravitating, the gravitational binding energy must be subtracted self-consistently from its bare mass value so as to give the physical gravitational mass. Such a self-consistent gravitational self-energy correction can be made non-perturbatively by the use of a gravitational `charging' technique, where we calculate the incremental change of the physical mass of the cosmological object, of size due to the accretion of a bare mass , corresponding to the gravitational coupling-in of the successive zero-point vacuum modes, i.e., of the Casimir energy, whose bare value is infinite. Integrating the `charging' equation, , we get a gravitational mass for the cosmological object that remains finite even in the limit of the infinite zero-point vacuum energy, i.e., without any…
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Taxonomy
TopicsQuantum Electrodynamics and Casimir Effect · Noncommutative and Quantum Gravity Theories · Cosmology and Gravitation Theories
