Holographic duals of evaporating black holes

<!--HTML--><p><span style="background-color:rgb(255,255,255);color:rgb(29,29,29);"><span style="-webkit-text-size-adjust:auto;-webkit-text-stroke-width:0px;caret-color:rgb(29, 29, 29);display:inline !important;float:none;font-family:Calibri;font-size:16px;font-style:normal;font-variant-caps:normal;font-weight:400;letter-spacing:normal;orphans:auto;text-align:start;text-decoration:none;text-indent:0px;text-transform:none;white-space:normal;widows:auto;word-spacing:0px;">We describe the dynamical evaporation of a black hole as the classical evolution in time of a black hole in an Anti-de Sitter braneworld. A bulk black hole whose horizon intersects the brane yields the classical bulk dual of a black hole coupled to quantum conformal fields. The evaporation of this black hole happens when the bulk horizon slides off the brane, making the horizon on the brane shrink. We use a large-D effective theory of the bulk Einstein equations to solve the time evolution of these systems. With this method, we study the dual evaporation of a variety of black holes interacting with colder radiation baths. We also obtain the dual of the collapse of holographic radiation to form a black hole on the brane.</span></span></p>