Understanding the strong coupling limit of massive type IIA string theory is a longstanding problem. We argue that perhaps this problem does not exist; namely, there may be no strongly coupled solutions of the massive theory. We show explicitly that massive type IIA string theory can never be strongly coupled in a weakly curved region of space-time. We illustrate our general claim with two classes of massive solutions in extAd extS4 ×mathbbCmathbbP3 { ext{Ad}}{{ ext{S}}_4} imes mathbb{C}{mathbb{P}^3} : one, previously known, with N = 1 mathcal{N} = 1 supersymmetry, and a new one with N = 2 mathcal{N} = 2 supersymmetry. Both solutions are dual to d = 3 Chern-Simons-matter theories. In both these massive examples, as the rank N of the gauge group is increased, the dilaton initially increases in the same way as in the corresponding massless case; before it can reach the M-theory regime, however, it enters a second regime, in which the dilaton decreases even as N increases. In the N = 2 mathcal{N} = 2 case, we find supersymmetry-preserving gauge-invariant monopole operators whose mass is independent of N. This predicts the existence of branes which stay light even when the dilaton decreases. We show that, on the gravity side, these states originate from D2-D0 bound states wrapping the vanishing two-cycle of a conifold singularity that develops at large N.
Aharony, O., Jafferis, D., Tomasiello, A., Zaffaroni, A. (2010). Massive type IIA string theory cannot be strongly coupled. JOURNAL OF HIGH ENERGY PHYSICS, 2010(11), 1-40 [10.1007/JHEP11(2010)047].
Massive type IIA string theory cannot be strongly coupled
TOMASIELLO, ALESSANDRO;ZAFFARONI, ALBERTO
2010
Abstract
Understanding the strong coupling limit of massive type IIA string theory is a longstanding problem. We argue that perhaps this problem does not exist; namely, there may be no strongly coupled solutions of the massive theory. We show explicitly that massive type IIA string theory can never be strongly coupled in a weakly curved region of space-time. We illustrate our general claim with two classes of massive solutions in extAd extS4 ×mathbbCmathbbP3 { ext{Ad}}{{ ext{S}}_4} imes mathbb{C}{mathbb{P}^3} : one, previously known, with N = 1 mathcal{N} = 1 supersymmetry, and a new one with N = 2 mathcal{N} = 2 supersymmetry. Both solutions are dual to d = 3 Chern-Simons-matter theories. In both these massive examples, as the rank N of the gauge group is increased, the dilaton initially increases in the same way as in the corresponding massless case; before it can reach the M-theory regime, however, it enters a second regime, in which the dilaton decreases even as N increases. In the N = 2 mathcal{N} = 2 case, we find supersymmetry-preserving gauge-invariant monopole operators whose mass is independent of N. This predicts the existence of branes which stay light even when the dilaton decreases. We show that, on the gravity side, these states originate from D2-D0 bound states wrapping the vanishing two-cycle of a conifold singularity that develops at large N.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.