Instability of brane cosmological solutions with flux compactifications
Masato Minamitsuji

TL;DR
This paper analyzes the stability of higher-dimensional de Sitter brane solutions with flux compactifications, revealing that instabilities in scalar perturbations correspond to thermodynamic instability and influence cosmological evolution.
Contribution
It demonstrates the connection between dynamical and thermodynamic stability of flux compactified brane solutions and explores their implications for cosmological evolution.
Findings
Unstable solutions are thermodynamically unstable.
Unstable solutions evolve towards stable configurations or decompactify.
Higher-dimensional instabilities relate to four-dimensional cosmological transitions.
Abstract
We discuss the stability of the higher-dimensional de Sitter (dS) brane solutions with two-dimensional internal space in the Einstein-Maxwel theory. We show that an instability appears in the scalar-type perturbations with respect to the dS spacetime. We derive a differential relation which has the very similar structure to the ordinary laws of thermodynamics as an extension of the work for the six-dimensional model [20]. In this relation, the area of dS horizon (integrated over the two internal dimensions) exactly behaves as the thermodynamical entropy. The dynamically unstable solutions are in the thermodynamically unstable branch. An unstable dS compactification either evolves toward a stable configuration or two-dimensional internal space is decompactified. These dS brane solutions are equivalent to the accelerating cosmological solutions in the six-dimensional…
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