Coupling Constant Corrections in a Holographic Model of Heavy Ion Collisions

We initiate a holographic study of coupling-dependent heavy ion collisions by analyzing, for the first time, the effects of leading-order, inverse coupling constant corrections. In the dual description, this amounts to colliding gravitational shock waves in a theory with curvature-squared terms. We...

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Main Authors: Grozdanov, Sašo, van der Schee, Wilke
Other Authors: Massachusetts Institute of Technology. Center for Theoretical Physics
Format: Article
Published: American Physical Society 2018
Online Access:http://hdl.handle.net/1721.1/118168
https://orcid.org/0000-0003-2477-6623
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author Grozdanov, Sašo
van der Schee, Wilke
author2 Massachusetts Institute of Technology. Center for Theoretical Physics
author_facet Massachusetts Institute of Technology. Center for Theoretical Physics
Grozdanov, Sašo
van der Schee, Wilke
author_sort Grozdanov, Sašo
collection MIT
description We initiate a holographic study of coupling-dependent heavy ion collisions by analyzing, for the first time, the effects of leading-order, inverse coupling constant corrections. In the dual description, this amounts to colliding gravitational shock waves in a theory with curvature-squared terms. We find that, at intermediate coupling, nuclei experience less stopping and have more energy deposited near the light cone. When the decreased coupling results in an 80% larger shear viscosity, the time at which hydrodynamics becomes a good description of the plasma created from high energy collisions increases by 25%. The hydrodynamic phase of the evolution starts with a wider rapidity profile and smaller entropy.
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spelling mit-1721.1/1181682022-10-01T03:47:25Z Coupling Constant Corrections in a Holographic Model of Heavy Ion Collisions Grozdanov, Sašo van der Schee, Wilke Massachusetts Institute of Technology. Center for Theoretical Physics van der Schee, Wilke We initiate a holographic study of coupling-dependent heavy ion collisions by analyzing, for the first time, the effects of leading-order, inverse coupling constant corrections. In the dual description, this amounts to colliding gravitational shock waves in a theory with curvature-squared terms. We find that, at intermediate coupling, nuclei experience less stopping and have more energy deposited near the light cone. When the decreased coupling results in an 80% larger shear viscosity, the time at which hydrodynamics becomes a good description of the plasma created from high energy collisions increases by 25%. The hydrodynamic phase of the evolution starts with a wider rapidity profile and smaller entropy. United States. Department of Energy (Grant DE-SC0011090) 2018-09-25T16:11:34Z 2018-09-25T16:11:34Z 2017-07 2017-05 2018-09-20T12:27:30Z Article http://purl.org/eprint/type/JournalArticle 0031-9007 1079-7114 http://hdl.handle.net/1721.1/118168 Grozdanov, Sašo, and Wilke van der Schee. “Coupling Constant Corrections in a Holographic Model of Heavy Ion Collisions.” Physical Review Letters 119, 1 (July 2017): 011601 © 2017 American Physical Society https://orcid.org/0000-0003-2477-6623 http://dx.doi.org/10.1103/PhysRevLett.119.011601 Physical Review Letters Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf American Physical Society APS
spellingShingle Grozdanov, Sašo
van der Schee, Wilke
Coupling Constant Corrections in a Holographic Model of Heavy Ion Collisions
title Coupling Constant Corrections in a Holographic Model of Heavy Ion Collisions
title_full Coupling Constant Corrections in a Holographic Model of Heavy Ion Collisions
title_fullStr Coupling Constant Corrections in a Holographic Model of Heavy Ion Collisions
title_full_unstemmed Coupling Constant Corrections in a Holographic Model of Heavy Ion Collisions
title_short Coupling Constant Corrections in a Holographic Model of Heavy Ion Collisions
title_sort coupling constant corrections in a holographic model of heavy ion collisions
url http://hdl.handle.net/1721.1/118168
https://orcid.org/0000-0003-2477-6623
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