scholarly journals Spring and Asymptotic Boundary Condition Models for Study of Scattering by Thin Cylindrical Interphases

Author(s):  
W. Huang ◽  
S. I. Rokhlin
1991 ◽  
Vol 27 (6) ◽  
pp. 5013-5015 ◽  
Author(s):  
J.R. Brauer ◽  
S.M. Schaefer ◽  
J.-F. Lee ◽  
R. Mittra

2014 ◽  
Vol 2014 ◽  
pp. 1-12 ◽  
Author(s):  
Chanyong Park

The holographic renormalization of a charged black brane with or without a dilaton field, whose dual field theory describes a dense medium at finite temperature, is investigated in this paper. In a dense medium, two different thermodynamic descriptions are possible due to an additional conserved charge. These two different thermodynamic ensembles are classified by the asymptotic boundary condition of the bulk gauge field. It is also shown that in the holographic renormalization regularity of all bulk fields can reproduce consistent thermodynamic quantities and that the Bekenstein-Hawking entropy is nothing but the renormalized thermal entropy of the dual field theory. Furthermore, we find that the Reissner-Nordström AdS black brane is dual to a theory with conformal matter as expected, whereas a charged black brane with a nontrivial dilaton profile is mapped to a theory with nonconformal matter although its leading asymptotic geometry still remains as AdS space.


2021 ◽  
Vol 2021 (4) ◽  
Author(s):  
Andreas Karch ◽  
Zhu-Xi Luo ◽  
Hao-Yu Sun

Abstract We extend the holographic duality between 3d pure gravity and 2d Ising CFT proposed in ref. [1] to CFTs with boundaries. Besides the usual asymptotic boundary, the dual bulk spacetime now has a real cutoff, on which live branes with finite tension, giving Neumann boundary condition on the metric tensor. The strongly coupled bulk theory requires that we dress the well-known semiclassical AdS/BCFT answer with boundary gravitons, turning the partition function into the form of Virasoro characters. Using this duality, we relate the brane tensions to the modular S-matrix elements of the dual BCFT and derive the transformation between gravitational solutions with different brane tensions under modular S action.


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