Fine Tuning Free Paradigm of Two Measures Theory: K-Essence, Absence of Initial Singularity of the Curvature and Inflation with Graceful Exit to Zero Cosmological Constant State
E. I. Guendelman, A. B. Kaganovich

TL;DR
This paper explores a scale-invariant Two Measures Field Theory in cosmology, demonstrating it can naturally produce inflation, avoid initial singularities, and address the cosmological constant problem without fine tuning.
Contribution
It presents a novel, fine-tuning free TMT model that yields diverse cosmological scenarios, including singularity avoidance, inflation with graceful exit, and small cosmological constant solutions.
Findings
Absence of initial curvature singularity with a singular derivative.
Power law inflation with graceful exit to zero or small CC.
Resolution mechanisms for the old cosmological constant problem.
Abstract
The dilaton-gravity sector of the Two Measures Field Theory (TMT)is explored in detail in the context of cosmology. The model possesses scale invariance which is spontaneously broken due to the intrinsic features of the TMT dynamics. The effective model represents an explicit example of the effective k-essence resulting from first principles without any exotic term in the fundamental action. Depending of the choice of regions in the parameter space, TMT exhibits different possible outputs for cosmological dynamics: a) Absence of initial singularity of the curvature while its time derivative is singular. This is a sort of "sudden" singularities studied by Barrow on purely kinematic grounds. b) Power law inflation in the subsequent stage of evolution. Depending on the region in the parameter space (but without fine tuning) the inflation ends with a graceful exit either into the state with…
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