09:30 to 10:30 |
Amos Yarom (Technion institute of technology Haifa, Israel) |
New constraints on transport from Schwinger Keldysh theory After a brief review, I will discuss how a new formulation of a low energy Schwinger Keldysh effective action gives rise to the appearance of an entropy current, Onsager relations, and further constraints on hydrodynamics which are not implied by the either
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10:30 to 11:00 |
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Tea break |
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11:00 to 12:00 |
Suvrat Raju (ICTS, India) |
A Critique of the Fuzzball Program We explore the viability of fuzzballs as candidate microstate geometries for the black hole, and their possible role in resolutions of the information paradox. We argue that if fuzzballs provide a description of black-hole microstates, then the typical fuzzball geometry can only differ significantly from the conventional black-hole geometry at a Planck-scale-distance from the horizon. However, precisely in this region, quantum fluctuations in the fuzzball geometry become large and the fuzzball geometry becomes unreliable. We verify these expectations through a detailed calculation of quantum expectation values and quantum fluctuations in the two-charge fuzzball geometries. We then examine some of the solutions discovered in arXiv:1607.03908. We show, based on a calculation of a probe two-point function in this background, that these solutions, and others in their class, violate robust expectations about the gap in energies between successive energy eigenstates, and differ too much from the conventional black hole to represent viable microstates. We conclude that while fuzzballs are interesting star-like solutions in string theory, they do not appear to be relevant for resolving the information paradox, and cannot be used to make valid inferences about black-hole interiors.
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12:00 to 14:00 |
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Lunch |
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14:00 to 16:00 |
Shivaji Sondhi (Princeton University, USA) |
Two variations on the theme of operator spreading Operator spreading refers to the growth of local operators in spatial support and complexity under unitary dynamics. I will discuss some exact results on operator spreading under local random unitary circuits, how they tie into more general beliefs about how operators spread in different settings, and finally how these beliefs constrain the phase space for finding examples of time translation symmetry breaking.
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16:00 to 17:00 |
Juan Maldacena (IAS, NJ, USA) |
Black Holes and the Structure of Spacetime (Public Lecture) Black holes are fascinating objects predicted by Einstein's theory of general relativity. Though they were initially viewed as pathological and unphysical solutions, they were later understood to be a solid and generic outcome of the theory. They are objects where the distortion of space and time is so extreme that it defies imagination. Black holes give rise to paradoxes whose resolution requires us to modify our conception of spacetime. We will review how black holes went from being an apparently unphysical solutions to a central tool for discovering new perspectives on the nature of spacetime.
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