Self-tuning Horava-Lifshitz's Universe
D. Bazeia, F. A. Brito, and F. G. Costa

TL;DR
This paper proposes a modified Horava-Lifshitz gravity model that achieves self-tuning of the cosmological constant, effectively canceling its gravitational effect and allowing for accelerating universe scenarios with various fluids.
Contribution
It introduces a novel modification to Horava-Lifshitz gravity enabling self-tuning of the cosmological constant, removing its gravitational influence.
Findings
Cosmological constant's gravitational effect is canceled in the model.
Accelerating universe scenarios are achievable with different fluids.
The model provides a new approach to the cosmological constant problem.
Abstract
In this paper we show that by considering a slightly modified Horava-Lifshitz gravity one can find self-tuning cosmological scenarios. Since in the proposed model the cosmological constant cancels out, then regardless of its value it cannot produce any gravitational effect. As a consequence this removes the gravitational effect of the vacuum energy on the expansion of the Universe. Accelerating scenarios, however, can be found through the presence of conventional and non-conventional fluids.
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Taxonomy
TopicsCosmology and Gravitation Theories · Computational Physics and Python Applications · Geophysics and Gravity Measurements
