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SUMMARY:Sayantani Bhattacharyya (NISER\, India)
DTSTART:20201208T150000Z
DTEND:20201208T160000Z
DTSTAMP:20260423T022932Z
UID:HoloTube/29
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/HoloTube/29/
 ">Entropy current for higher derivative theories of gravity</a>\nby Sayant
 ani Bhattacharyya (NISER\, India) as part of HoloTube: Applied holography 
 webinars\n\n\nAbstract\nWe know that black holes could be viewed as thermo
 dynamic ensemble of large number of microstates and therefore we could ass
 ociate some entropy with these objects. For Einstein gravity\, the local a
 rea element around any point of the black hole horizon plays the role of e
 ntropy density\, that satisfies the second law of thermodynamics locally a
 t every point on the horizon. However\, any UV complete theory of gravity\
 , in its low energy limit\, will typically have higher derivative correcti
 ons to Einstein gravity. Black holes continue to exist for such higher der
 ivative theories. In this talk\, we shall show that for such theories we c
 ould still satisfy the second law locally on every point of the horizon\, 
 at least when the dynamics of the black hole is of small amplitude. To see
  this\, we need to add a spatial entropy current to the equilibrium constr
 uction of Wald entropy density. This method also fixes some of the ambigui
 ties that arise in Wald’s construction\, for the entropy of a dynamical 
 black hole in higher derivative theories.\n
LOCATION:https://researchseminars.org/talk/HoloTube/29/
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