Asymmetric shockwave collisions in AdS5
- 1. University of Regensburg, Institute for Theoretical Physics (Germany)
- 2. University of Washington, Department of Physics (United States)
Description
Collisions of asymmetric planar shocks in maximally supersymmetric Yang-Mills theory are studied via their dual gravitational formulation in asymptotically anti-de Sitter spacetime. The post-collision hydrodynamic flow is found to be very well described by appropriate means of the results of symmetric shock collisions. This study extends, to asymmetric collisions, previous work of Chesler, Kilbertus, and van der Schee examining the special case of symmetric collisions [1]. Given the universal description of hydrodynamic flow produced by asymmetric planar collisions one can model, quantitatively, non-planar, non-central collisions of highly Lorentz contracted projectiles without the need for computing, holographically, collisions of finite size projectiles with very large aspect ratios. This paper also contains a pedagogical description of the computational methods and software used to compute shockwave collisions using pseudo-spectral methods, supplementing the earlier overview of Chesler and Yaffe [2].
Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of High Energy Physics (Online)
- Journal Volume
- 2019
- Journal Issue
- 8
- Journal Page Range
- p. 1-43
- ISSN
- 1029-8479
INIS
- Country of Publication
- Germany
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 54069986
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- ANTI DE SITTER GROUP; ANTI DE SITTER SPACE; ASPECT RATIO; ASYMMETRY; COLLISIONS; COMPUTER CODES; GRAVITATION; HYDRODYNAMICS; QUARK MATTER; SHOCK WAVES; SPACE-TIME; SUPERSYMMETRY; YANG-MILLS THEORY
- Descriptors DEC
- DIMENSIONLESS NUMBERS; FLUID MECHANICS; LIE GROUPS; MATHEMATICAL SPACE; MATTER; MECHANICS; SPACE; SYMMETRY; SYMMETRY GROUPS
Optional Information
- Copyright
- Copyright (c) 2019 The Author(s)