2020/04/28 by Thomas Hartman, Edgar Shaghoulian, Andrew Strominger · 2 citations
Physics and Astronomy · #hep-th
paper · pdf · doi:10.1007/jhep07(2020)022
30 pages
arxiv created 2020/04/28 · arxiv updated 2020/08/26
The large-N limit of asymptotically flat two-dimensional dilaton gravity coupled to N free matter fields provides a useful toy model for semiclassical black holes and the information paradox. Analyses of the asymptotic information flux as given by the entanglement entropy show that it follows the Hawking curve, indicating that information is destroyed in these models. Recently, motivated by developments in AdS/CFT, a semiclassical island rule for entropy has been proposed. We define and compute the island rule entropy for black hole formation and evaporation in the large-N RST model of dilaton gravity and show that, in contrast, it follows the unitary Page curve. The relation of these two observations, and interesting properties of the dilaton gravity island rule, are discussed.