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Fundamental structure of string geometry theory

Published 4 Nov 2025 in hep-th, gr-qc, hep-ph, math.DG, and math.SG | (2511.02310v1)

Abstract: String geometry theory is one of the candidates of a non-perturbative formulation of string theory. In this theory, the classical'' action is almost uniquely determined by T-symmetry, which is a generalization of the T-duality, where the parameter ofquantum'' corrections $\beta$ in the path-integral of the theory is independent of that of quantum corrections $\hbar$ in the perturbative string theories. We distinguish the effects of $\beta$ and $\hbar$ by putting " " like "classical" and "loops" for tree level and loop corrections with respect to $\beta$, respectively, whereas by putting nothing like classical and loops for tree level and loop corrections with respect to $\hbar$, respectively. A non-renormalization theorem states that there is no loop'' correction. Thus, there is no problem of non-renormalizability, although the theory is defined by the path-integral over the fields including a metric on string geometry. Noloop'' correction is also the reason why the complete path-integrals of the all-order perturbative strings in general string backgrounds are derived from the tree''-level two-point correlation functions in the perturbative vacua, although string geometry includes information of genera of the world-sheets of the stings. Furthermore, a non-perturbative correction in string coupling with the order $e^{-1/g_s^2}$ is given by a transition amplitude representing a tunneling process between the semi-stable vacua in theclassical'' potential by an ``instanton'' in the theory. From this effect, a generic initial state will reach the minimum of the potential.

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