In the wormhole-dominant phase of a two-dimensional matrix model, the continuum disk amplitude matches pure 2D quantum gravity, and a renormalized wormhole coupling shifts the effective bulk cosmological constant.
Non-Perturbative Solution of Matrix Models Modified by Trace-Squared Terms
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abstract
We present a non-perturbative solution of large $N$ matrix models modified by terms of the form $ g(\Tr\Phi^4)^2$, which add microscopic wormholes to the random surface geometry. For $g<g_t$ the sum over surfaces is in the same universality class as the $g=0$ theory, and the string susceptibility exponent is reproduced by the conventional Liouville interaction $\sim e^{\alpha_+ \phi}$. For $g=g_t$ we find a different universality class, and the string susceptibility exponent agrees for any genus with Liouville theory where the interaction term is dressed by the other branch, $e^{\alpha_- \phi}$. This allows us to define a double-scaling limit of the $g=g_t$ theory. We also consider matrix models modified by terms of the form $g O^2$, where $O$ is a scaling operator. A fine-tuning of $g$ produces a change in this operator's gravitational dimension which is, again, in accord with the change in the branch of the Liouville dressing.
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Properties of the wormhole-dominant phase in two-dimensional quantum gravity
In the wormhole-dominant phase of a two-dimensional matrix model, the continuum disk amplitude matches pure 2D quantum gravity, and a renormalized wormhole coupling shifts the effective bulk cosmological constant.