Abstract
The Polchinski equations for the Wilsonian renormalization group in the D-dimensional matrix scalar field theory can be written at large N in a Hamiltonian form. The Hamiltonian defines evolution along one extra holographic dimension (energy scale) and can be found exactly for the subsector of Trϕn (for all n) operators. We show that at low energies independently of the dimensionality D the Hamiltonian system in question reduces to the integrable effective theory. The obtained Hamiltonian system describes large wavelength KdV type (Burger-Hopf) equation with an external potential and is related to the effective theory obtained by Das and Jevicki for the matrix quantum mechanics.
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References
J. M. Maldacena, Adv. Theor. Math. Phys. 2, 231 (1998); Int. J. Theor. Phys. 38, 1113 (1999), arXiv:hepth/9711200; S. S. Gubser, I. R. Klebanov, and A. M. Polyakov, Phys. Lett. B 428, 105 (1998), arXiv:hep-th/9802109; E. Witten, Adv. Theor. Math. Phys. 2, 253 (1998), arXiv:hep-th/9802150.
E. T. Akhmedov, Phys. At. Nucl. 72, 1574 (2009); arXiv:hep-th/9911095; Phys. Usp. 44, 955 (2001).
A. Gerasimov, unpublished; E. T. Akhmedov, Phys. Lett. B 442, 152 (1998), arXiv:hep-th/9806217.
V. Balasubramanian and P. Kraus, Phys. Rev. Lett. 83, 3605 (1999), arXiv:hep-th/9903190.
E. Alvarez and C. Gomez, Nucl. Phys. B 566, 363 (2000), arXiv:hep-th/9907158; Nucl. Phys. B 574, 153 (2000), arXiv:hep-th/9911215; arXiv:hep-th/9911202; Phys. Lett. B 476, 411 (2000), arXiv:hep-th/0001016; arXiv:hep-th/0009203.
J. de Boer, E. P. Verlinde, and H. L. Verlinde, J. High Energy Phys. 0008, 003 (2000), arXiv:hep-th/9912012; E. P. Verlinde and H. L. Verlinde, J. High Energy Phys. 0005, 034 (2000), arXiv:hep-th/9912018.
M. Fukuma and T. Sakai, Mod. Phys. Lett. A 15, 1703 (2000), arXiv:hep-th/0007200; M. Fukuma, S. Matsuura, and T. Sakai, Prog. Theor. Phys. 104, 1089 (2000), arXiv:hep-th/0007062.
A. Gorsky, A. Marshakov, A. Mironov, and A. Morozov, Nucl. Phys. B 527, 690 (1998), arXiv:hep-th/9802007.
C. Becchi, S. Giusto, and C. Imbimbo, Nucl. Phys. B 633, 250 (2002), arXiv:hep-th/0202155.
A. Mironov and A. Morozov, Phys. Lett. B 490, 173 (2000), arXiv:hep-th/0005280.
A. Gerasimov, unpublished; E. T. Akhmedov, arXiv:hep-th/0202055.
E. T. Akhmedov and E. T. Musaev, Phys. Rev. D 81, 085010 (2010), arXiv:hep-th/1001.4067.
J. Polchinski, Nucl. Phys. B 231, 269 (1984).
S. R. Das and A. Jevicki, Mod. Phys. Lett. A 5, 1639 (1990).
A. Jevicki, arXiv:hep-th/9309115.
J. Polchinski, arXiv:hep-th/9411028.
E. T. Akhmedov, JETP Lett. 81, 357 (2005), arXiv:hepth/0502174; JETP Lett. 80, 218 (2004), arXiv:hepth/0407018.
A. Morozov, A. J. Niemi, Nucl. Phys. B 666, 311 (2003), hep-th/0304178; D. B. Fairlie, J. Govaerts, and A. Morozov, Nucl. Phys. B 373, 214 (1992), hepth/9110022.
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Akhmedov, E.T., Gahramanov, I.B. & Musaev, E.T. Hints on integrability in the Wilsonian/holographic renormalization group. Jetp Lett. 93, 545–550 (2011). https://doi.org/10.1134/S0021364011090037
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DOI: https://doi.org/10.1134/S0021364011090037