… observer falling into a black hole using the AdS/CFT correspondence. In order to do this, we
reconstruct the local bulk operators measured by the observer … , the observer would need to …

… by the AdS/CFT correspondence. This motivates us to consider accelerating observers not
… on” and “switching off” processes of our infalling source, we will see that the CFT can tell …

… 24 and 28 but the AdS-CFT correspondence … observer. It is also important to determine at
what point the outside measurements begin to have significant influence on infalling observers …

… a source to the CFT to create an infalling observer. The C = A … available to the infalling
observer, allowing her free infall. Since the … ) systems giving universal free infall. We discuss the …

… For sufficiently large but finite R=fðmÞ, the infalling observer … description of an infalling
observer requires a quantum … its application to the infalling observer relies on semiclassical bulk …

… If we do so, the future boundary of the shaded region is a horizon, but only because the
infalling observer is forced to leave through a copy of the original asymptotic region. The physics …

… observer sees its slow approach to the horizon at late time. … What the observer sees as the
shell falls is dual to the evolution of … of the ratio between the infalling and outfalling waves, we …

… to cover all applications of AdS/CFT. This is because … infalling photon, but one can consider
the outgoing photon. In this case, t → ∞ until the light from the horizon reaches the observer …

… If we in addition take the large A limit and use the AdS/CFT correspondence, the expectation
value of the Wilson loop in the fundamental representation can be computed as [36, 37] …

… how infalling matter in a pure state forms a Schwarzschild black hole that appears to be at
nonzero temperature is discussed in the context of the AdS/CFT … to the outside observer. In this …