Background instability of quintessence model in light of entropy and distance conjecture
Min-Seok Seo

TL;DR
This paper investigates the instability of quintessence models under entropy and distance conjectures, revealing that accelerating backgrounds with horizons are unstable due to entropy growth constraints, linking swampland conjectures with entropy bounds.
Contribution
It demonstrates the instability conditions of quintessence models using covariant entropy bounds and connects these conditions with the trans-Planckian censorship and AdS distance conjectures.
Findings
Accelerating quintessence backgrounds with horizons are unstable.
Instability conditions align with the trans-Planckian censorship bound.
Scale separation is achievable when entropy growth rates are bounded.
Abstract
We apply the covariant entropy bound argument supporting the de Sitter swampland conjecture to the quintessence model, to find out the condition for the background to be unstable. More concretely, the background is unstable when the matter entropy given by the species number of the effective field theory increases more rapidly than the geometrical entropy proportional to the apparent horizon area, since it contradicts the covariant entropy bound. The rapid increase in the matter entropy is proposed by the distance conjecture, which states that the time evolution of some scalar field along the geodesic in the field space brings about the descent of a tower of states from UV. From this, we find that for the quintessence model, the accelerating background having the event horizon is unstable, and the instability condition as well as the lifetime of the unstable background is equivalent to…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories · Cosmology and Gravitation Theories
