Chiral symmetry breaking and pions in nonsupersymmetric gauge / gravity duals
By J. Babington, Johanna Erdmenger, N. Evans, Z. Guralnik, I. Kirsch. 2004
472 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/c8424258e11f94b1500bf3c1ba6012093de9990a
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Citations in the corpus
- Quarks in an External Electric Field in Finite Temperature Large N Gauge Theory (2007, background): “r3(~r) = 0 ; (13) which has solution: (~r) = m~ ~r + ~c r~3 : (14) The constants ~mand ~care related to the bare quark mass and the condensate respectively, in a manner that is by now very standard [6, 14, 15, 16]. In our notation, the exact relationship is given by: m q = bm~ 2ˇ0 ; h i= 8ˇ30VN fT ”
- Holographic phase transitions at finite baryon density (2006, background): “transport coefficients such as the shear viscosity [6]. 2 Initial studies include [ 10 , 11].”
- Holographic spectral functions and diffusion constants for fundamental matter (2007, methodology): “The thermal behaviour of the N = 2 gauge theory with fundamental matter has recently been actively studied [ 8 , 9, 7, 10].”
- Thermodynamics and instabilities of a strongly coupled anisotropic plasma (2011, background): “As we will see, the anisotropy in the SYM plasma that we will study can be thought of as resulting from a dissolved 2-brane charge.”
- Meson spectroscopy from holomorphic probes on the warped deformed conifold (2004, background): “m of mesons with arbitrary R-charge in N = 2 SYM was extracted from the masses of the probe fluctuations. It was shown that the spectrum is discrete with a mass gap. For related works, see [13], [14], [15], [16], [17], [18], [19], [20], [21]. The main purpose of this paper is to explore supersymmetri”
- Holographic chiral phase transition with chemical potential (2006, methodology): “the chiral symmetry breaking one considers condensations of quark bilinears ψψ¯ as an order parameter. The quark masses are sources of these operators. In fact, in other models of the holographic QCD [7, 8] the mechanism of the chiral symmetry breaking is different from that in the Sakai-Sugimoto mod”
- Probe branes, time-dependent couplings and thermalization in AdS/CFT (2010, methodology): “Such probe branes [44, 45] have been used to model flavor physics [46–53] and quantum critical phenomena : this ”top-down” approach [54–61] is complementary to the ”bottom-up” approach involving the physics of charged black holes in AdS [21, 22, 62–65].”
- Introduction to holographic superconductor models (2015, methodology): “It is referred as AdS/QCD or holographic QCD, which has been widely studied [222, 223, 224, 225, 226, 227, 228, 229, 230, 231, 232, 233, 234, 235].”
- Holographic phase transitions at finite chemical potential (2007, methodology): “ity [3, 4]. The holographic method provides a powerful framework to study a broad class of large Nc, strongly coupled gauge theories with a small number Nf of fields in the fundamental representations [9, 10, 11, 12, 13, 14]. The gravity dual of these gauge fields appear as Nf probe Dq-branes on the n”
- Light-Front Dynamics and AdS/QCD Correspondence: The Pion Form Factor in the Space- and Time-Like Regions (2007, methodology): “Recent applications to describe chiral symmetry breaking [26] and other meson and baryon properties, have also been carried out within the framework of a topbottom approach to AdS/CFT using higher dimensional branes [27, 28, 29, 30, 31].”
- Thermodynamics of the brane (2007, methodology): “f the embeddings near the critical solution for general Dp/Dq systems, as originally presented in [3]. In the subsequent detailed discussion of the thermodynamics, we focus our attention on the D3/D7 [4] and D4/D6 [5] cases for concreteness. In section 4, we compute the free energy, entropy and ener”
- Energy loss of a heavy quark moving through Script N = 4 supersymmetric Yang-Mills plasma (2006, background): “st energy M rest(T) which differs from its Lagrangian mass m. Determining this relation requires solving (numerically) for the change in the embedding of the D7-brane induced by the black hole horizon [41,42]. Asymptotically,7 M rest(T) = m ˆ 1 − ∆m(T) m + 1 8 ∆m(T) m 4 − 5 128 ∆m(T) m 8 +O ∆m(T) ”