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U(1) Breakdown in Super Yang-Mills and Cascade of Gregory-Laflamme Transitions Masanori Hanada (RIKEN) With Tatsuma Nishioka (Kyoto U., D1 ) Weizmann inst. ( Israel ) Oct. ~ arXiv: 0706.0188[hep-th]
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Outline Phase structure of bosonic YM on torus SYM on torus Supergravity AdS/CFT (gauge/gravity) High Temrerature Hint for phase str. Confirm it in gravity side.
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1.Phase structure of bosonic YM on torus (simulation by Narayanan et.al.) 2.SYM at high temperature 3.Relation to gravity side: Cascade of Gregory-Laflamme transitions
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3d pure bosonic U(N) YM on torus (1) LμLμ Global U(1) 3 symmetry Spatial Wilson loop
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All nonzero 3d pure bosonic U(N) YM on torus (2) When L μ becomes small, becomes nonzero. If we take all L μ to be the same, L, then… Narayanan-Neuberger-Reynoso, arXiv:0704.2591[hep-lat] L 0 L (1) =0 for all directions 1 nonzero 2 nonzero L (2) L (3)
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YM on torus with adjoint scalars If we take L 3 → 0 first, then we obtain 2d YM on torus with 1 adjoint scalars. L 0 L (1) =0 for all directions 1 nonzero L (2) All nonzero YM on T 4 has the same pattern. We may expect that in YM on p -torus with m adjoint scalars U (1) p breaks down one-by-one.
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1.Phase structure of bosonic YM on torus 2.SYM at high temperature 3.Relation to gravity side: Cascade of Gregory-Laflamme transitions
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Bosonic YM as High Temp. limit of SYM Consider SYM on T p+1 with (9-p) adjoint scalars. (In this talk, p=0,1,2,3.) Finite temperature → ・ size of temporal circle = β= 1/ T ・ antiperiodic b.c. for fermion Fermions decouple at high temperature Bosonic YM on T p
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Temporal KK decouple bosonic YM Spatial KK decouple One-by-one breakdown of U(1) At weak coupling and high-temperature, bosonic YM can be used. One-by-one breakdown of U(1) exist also in SYM.
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1.Phase structure of bosonic YM on torus 2.SYM at high temperature 3.Relation to gravity side : Cascade of Gregory-Laflamme transitions
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Assume (or believe) that one-by-one breakdown of U(1) in SYM persists to strong coupling. AdS/CFT [gauge/gravity] correspondence SYM at strong coupling can be described using supergravity. U(1) breakdown Gregory-Laflamme Susskind, Barbon-Kogan-Rabinovici, Li-Martinec-Sahakian, Aharony-Marsano-Minwalla-Wiseman, Harmark-Obers, …
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Gregory-Laflamme transition Black string winding on S 1 is unstable if S 1 is large.
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Phase of spatial Wilson loop Position of D-brane T-dual Taking T-dual along all directions of torus, we have a system of D0-branes. Then, condensation of spatial Wilson loop Condensation of D0-branes “ Gregory-Laflamme ”
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Simulation result of Narayanan et.al. suggests a cascade of Gregory-Laflamme transitions: Smeared D0 ’ s on T 2 on S 1 localized Check it.
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Metric for Dp-brane, etc. Cf) Itzhaki-Maldacena- Sonnenschein-Yankieloewicz
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T-dual picture: D0-branes
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When SUGRA approximation is good? Winding mode along torus and massive tower of string oscillation should be heavier than KK mode along S 8-p. Dp-brane picture: D0-brane picture:
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Comparison of free energies (1) Compare free energies for D p -brane with the same temperature T H. Exact metric for D p in T n is not known. Approximate compact directions transvers to brane by noncompact ones.
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Comparison of free energies (2) 02.402.672.87 0-brane1-brane2-brane3-brane
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Comparison of free energies (3) t>2.87/λ’ 1/2 3-brane 2-brane ? t<2.87/λ’ 1/2 t=2.87/λ’ 1/2
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Remarks Transition takes place where D0-brane picture is valid. In D0-picture, small t ⇔ large 1/L. internal space large internal space large low dim.object favored. low dim.object favored.
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Schwarzschild case
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Schwarzschild-type black brane Schwarzschild BH Torus (flat)
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t C(1) t C(2) t C(3) 1.28 1.17 1.04 Critical temp. for R 7 × T 3
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t<t C(3) 3-brane 2-brane 1-brane 0-brane ? t=t GL(3) t=t C(3) t>t C(3)
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t C(1) t C(2) t C(3) 1.28 1.17 1.04 Critical temp. for R 7 × T 3 t GL(1) t GL(2) t GL(3) 1.30 1.20 1.08
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Cascade of first order transitions: 3-brane→ 2-brane→ 1-brane→ 0-brane 3 2 1 0 3-brane cannot decay to 1- or 0-brane
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Resolution of a puzzle “ 3-brane in R 7 ×T 3 cannot decay to 0-brane. ” 3-brane cannot decay to 0-brane directly, but it can decay as 3-brane→ 2-brane→ 1-brane→ 0-brane ! (Kol-Sorkin, 2004)
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Summary Black brane on torus goes through a cascade of Gregory-Laflamme transitions. This cascade is related to one-by-one breakdown of U(1) in Yang-Mills theory.
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おまけ
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Take it small. Condition for fermion decoupling(1)
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If spatial KK modes decouple first, then … Condition for fermion decoupling(2) Small ⇒ temporal KK decouple Especially, all fermions decouple.
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Small → ・ spatial KK decouple ・ U(1) breaks one-by-one (result from bosonic model) When U(1) p ? If temporal KK modes decouple first, then …
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