Resolution of the cosmological constant problem by unimodular gravity and signature reversal symmetry
Recai Erdem

TL;DR
This paper proposes that unimodular gravity, combined with signature reversal symmetry in a higher-dimensional bulk, can potentially resolve both aspects of the cosmological constant problem.
Contribution
It introduces a novel approach using brane-world scenarios and symmetry principles to address the smallness and specific value of the cosmological constant.
Findings
Unimodular gravity solves the discrepancy between observed and theoretical cosmological constant values.
Signature reversal symmetry in higher dimensions constrains the cosmological constant.
The approach offers a unified resolution to both problems of the cosmological constant.
Abstract
The (old) cosmological constant problem consists of two different problems. The first is the huge discrepancy between the value of the cosmological constant deduced from observations and its value expected from cosmological constant-like theoretical contributions (such as vacuum expectation value of Higgs potential). The second problem is why the value of the cosmological constant has its particular (very small) value. It is well-known that unimodular gravity solves the first problem while it leaves the second problem unsolved. In this paper I show that the second problem may also be resolved in the context of unimodular gravity by letting our 4-dimensional spacetime be a brane in a D = 2(2n + 1) dimensional bulk and imposing the signature reversal symmetry
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