Supergravity models for (3+1)-dimensional QCD
The most general black M5-brane solution of eleven-dimensional supergravity (with a flat R4 spacetime in the brane and a regular horizon) is characterized by charge, mass and two angular momenta. We use this metric to construct general dual models of large-N QCD (at strong coupling) that depend on t...
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todo:paper_05562821_v60_n4_p1_Csaki2023-10-03T15:35:38Z Supergravity models for (3+1)-dimensional QCD Csáki, C. Russo, J. Sfetsos, K. Terning, J. The most general black M5-brane solution of eleven-dimensional supergravity (with a flat R4 spacetime in the brane and a regular horizon) is characterized by charge, mass and two angular momenta. We use this metric to construct general dual models of large-N QCD (at strong coupling) that depend on two free parameters. The mass spectrum of scalar particles is determined analytically (in the WKB approximation) and numerically in the whole two-dimensional parameter space. We compare the mass spectrum with analogous results from lattice calculations, and find that the supergravity predictions are close to the lattice results everywhere on the two dimensional parameter space except along a special line. We also examine the mass spectrum of the supergravity Kaluza-Klein (KK) modes and find that the KK modes along the compact D-brane coordinate decouple from the spectrum for large angular momenta. There are however KK modes charged under a U(1)XU(1) global symmetry which do not decouple anywhere on the parameter space. General formulas for the string tension and action are also given. ©1999 The American Physical Society. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_05562821_v60_n4_p1_Csaki |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
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Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
description |
The most general black M5-brane solution of eleven-dimensional supergravity (with a flat R4 spacetime in the brane and a regular horizon) is characterized by charge, mass and two angular momenta. We use this metric to construct general dual models of large-N QCD (at strong coupling) that depend on two free parameters. The mass spectrum of scalar particles is determined analytically (in the WKB approximation) and numerically in the whole two-dimensional parameter space. We compare the mass spectrum with analogous results from lattice calculations, and find that the supergravity predictions are close to the lattice results everywhere on the two dimensional parameter space except along a special line. We also examine the mass spectrum of the supergravity Kaluza-Klein (KK) modes and find that the KK modes along the compact D-brane coordinate decouple from the spectrum for large angular momenta. There are however KK modes charged under a U(1)XU(1) global symmetry which do not decouple anywhere on the parameter space. General formulas for the string tension and action are also given. ©1999 The American Physical Society. |
format |
JOUR |
author |
Csáki, C. Russo, J. Sfetsos, K. Terning, J. |
spellingShingle |
Csáki, C. Russo, J. Sfetsos, K. Terning, J. Supergravity models for (3+1)-dimensional QCD |
author_facet |
Csáki, C. Russo, J. Sfetsos, K. Terning, J. |
author_sort |
Csáki, C. |
title |
Supergravity models for (3+1)-dimensional QCD |
title_short |
Supergravity models for (3+1)-dimensional QCD |
title_full |
Supergravity models for (3+1)-dimensional QCD |
title_fullStr |
Supergravity models for (3+1)-dimensional QCD |
title_full_unstemmed |
Supergravity models for (3+1)-dimensional QCD |
title_sort |
supergravity models for (3+1)-dimensional qcd |
url |
http://hdl.handle.net/20.500.12110/paper_05562821_v60_n4_p1_Csaki |
work_keys_str_mv |
AT csakic supergravitymodelsfor31dimensionalqcd AT russoj supergravitymodelsfor31dimensionalqcd AT sfetsosk supergravitymodelsfor31dimensionalqcd AT terningj supergravitymodelsfor31dimensionalqcd |
_version_ |
1807322591386402816 |