On the quantum Bousso bound in JT gravity

Abstract

We prove the Strominger-Thompson quantum Bousso bound in the infinite class of conformal vacua in semiclassical JT gravity, with postive or negative cosmological constant. The Bousso-Fisher-Leichenauer-Wall quantum Bousso bound follows from an analogous derivation, requiring only initial quantum non-expansion. In this process, we show that the quantity \\documentclass[12pt]{minimal} \\usepackage{amsmath} \\usepackage{wasysym} \\usepackage{amsfonts} \\usepackage{amssymb} \\usepackage{amsbsy} \\usepackage{mathrsfs} \\usepackage{upgreek} \\setlength{\\oddsidemargin}{-69pt} \\begin{document}$$2\\pi {k}^{\\mu }{k}^{\ u }\\langle :{T}_{\\mu \ u }:\\rangle -{S}^{{\\prime}{\\prime}}-\\frac{6}{c}{\\left({S}{\\prime}\\right)}^{2}$$\\end{document} vanishes in any vacuum state, entailing a stronger version of Wall’s quantum null energy condition. We derive an entropy formula in the presence of a generic class of two reflecting boundaries, in order to apply our argument to the half reduction model of de Sitter JT gravity.