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Lorentzian Regularization of the Type IIB Superstring Torus Vacuum

Published 16 Jun 2026 in hep-th and math-ph | (2606.17602v1)

Abstract: We study the one-loop torus vacuum of Type IIB Superstring theory through sector-resolved modular integrals. Building on the i\varepsilon-prescription and the E_s-regularized modular-integral framework of Manschot and Wang [1], we construct regularized sector functionals for the closed oriented torus before the final GSO projection. The construction keeps the unprojected spin-sector data explicit and fixes the compact-domain and cusp contributions within a single modular prescription. We also independently cross-check the result with the Lorentzian-inversion reconstruction of modular integrals by Baccianti et al. [2] This provides a first direct regularized construction of the unprojected sectors of the Type IIB Superstring torus vacuum.

Authors (1)

Summary

  • The paper develops a sector-resolved regularization framework using Lorentzian contour deformations and the E_s-prescription to compute the one-loop vacuum amplitude.
  • It systematically separates compact and non-compact regions of the modular space, validating the approach with Lorentzian inversion and Rademacher methodologies.
  • The detailed mode-block construction highlights the convergence between all-mode and zero-mode sectors, offering a blueprint for extending techniques to higher-point, dynamical string amplitudes.

Lorentzian Regularization of the Type IIB Superstring Torus Vacuum

Introduction and Context

The paper "Lorentzian Regularization of the Type IIB Superstring Torus Vacuum" (2606.17602) develops a sector-resolved, regularized calculation of the one-loop (genus one) vacuum amplitude in Type IIB superstring theory. The analysis focuses on the oriented closed-string torus prior to GSO (Gliozzi-Scherk-Olive) projection, implementing a modular-invariant regularization at the level of auxiliary spin sectors, rather than at the stage of the physically projected amplitude.

Central to this work is the explicit treatment of both compact and non-compact regions of the string worldsheet moduli space, separation and organization of the spin structures, and the systematic implementation of the iεi\varepsilon (Feynman) prescription via Lorentzian and EsE_s-regularized modular integrals. The framework is cross-validated against contemporary reconstructions from Lorentzian inversion and Rademacher-theoretic methods (Baccianti et al., 23 Jan 2025), ensuring compatibility with state-of-the-art modular and unitarity techniques.

Vacuum Amplitudes, Modular Integrals, and Cusp Regularization

The genus-one string amplitude is governed by an integral over modular space, specifically the fundamental domain F⊂H\mathcal{F}\subset \mathbb{H} of the torus moduli parameter τ=x+iy\tau = x + iy. For the vacuum (n=0n=0 punctures), the amplitude schematically is:

A1,0=∫Fdτ∧dτˉ y−sf(τ,τˉ),\mathcal{A}_{1,0} = \int_{\mathcal{F}} d\tau \wedge d\bar{\tau} \, y^{-s} f(\tau, \bar{\tau}),

with ff carrying the spin-structure and oscillator data.

Upon Fourier expanding f(τ,τˉ)f(\tau, \bar{\tau}) as ∑m,nF(m,n)qmqˉn\sum_{m,n} F(m,n) q^m \bar{q}^n, one can reorganize the modular integral as a double sum over regularized mode blocks, each of which isolates the analytic contribution from the modular cusp (y→∞y \to \infty). The measure in the Type IIB context sets EsE_s0 due to the light-cone gauge zero mode and modular weight conventions.

A critical step is the decomposition of the modular domain into a compact keyhole region and a cusp strip. The integral over the cusp region is divergent and requires regularization. Specifically, only the diagonal modes (i.e., EsE_s1) survive the horizontal integration due to Fourier orthogonality, and these modes are treated using Lorentzian contour deformations, which effectuate the physical EsE_s2 prescription required for causal string amplitudes (Witten, 2013).

Spin Sector Resolution, EsE_s3 Character Organization, and GSO Structure

Before the physical GSO projection, the Type IIB torus integrand is expanded into four auxiliary spin sectors: EsE_s4 denoting vector and spinor EsE_s5 characters for left- and right-moving sectors, respectively. The sector-resolved blocks are

  • EsE_s6,
  • EsE_s7,
  • EsE_s8,
  • EsE_s9,

given as left-right products of appropriately normalized character/eta combinations. Explicitly, the four sector integrands are

F⊂H\mathcal{F}\subset \mathbb{H}0

Supersymmetry enforces the celebrated Jacobi identity, F⊂H\mathcal{F}\subset \mathbb{H}1, which implies complete cancellation in the physical (GSO-projected) amplitude but leaves non-trivial content at the level of individual sectors.

The Fourier expansions of the holomorphic blocks, e.g., F⊂H\mathcal{F}\subset \mathbb{H}2, provide explicit integer degeneracies for the coefficients, which are in turn controlled by Rademacher and modular form theory (Cheng et al., 2012, Baccianti et al., 23 Jan 2025).

Lorentzian Regularization and F⊂H\mathcal{F}\subset \mathbb{H}3-Prescription: Mode-Block Construction

The principal technical innovation is encapsulated in the prescription for regularized mode integrals:

F⊂H\mathcal{F}\subset \mathbb{H}4

where F⊂H\mathcal{F}\subset \mathbb{H}5 is the compact keyhole subdomain, and F⊂H\mathcal{F}\subset \mathbb{H}6 denotes the generalized exponential integral, which encodes the Lorentzian tail prescribed by string perturbation theory.

The Lorentzian contour deformation replaces the naive Euclidean integration over F⊂H\mathcal{F}\subset \mathbb{H}7 (proper time) with a contour that proceeds up to a cutoff F⊂H\mathcal{F}\subset \mathbb{H}8 and then into the complex direction, ensuring causality and correct analytic continuation. All intermediate F⊂H\mathcal{F}\subset \mathbb{H}9-dependence cancels in the full regularized block.

Sector Functionals and Numerical Evaluation

Each sector amplitude is defined via a double sum:

Ï„=x+iy\tau = x + iy0

The structure of the vacuum and the character identities ensure that at every finite mode cutoff, all sector functionals coincide:

Ï„=x+iy\tau = x + iy1

The regularized all-mode sector value is given explicitly (at cutoff Ï„=x+iy\tau = x + iy2) by

Ï„=x+iy\tau = x + iy3

while the exact zero-mode sector value (i.e., from Ï„=x+iy\tau = x + iy4 only) evaluates to

Ï„=x+iy\tau = x + iy5

The small, finite difference between the all-mode and zero-mode values illustrates the highly convergent nature of the non-polar mode organization.

After performing the GSO projection, the final amplitude cancels identically, Ï„=x+iy\tau = x + iy6, at the level of Fourier coefficients and for the full modular-regularized sum, exemplifying the power of the sector-resolved, modular-invariant regularization.

Compatibility with Lorentzian Inversion and Rademacher Expansions

The construction is explicitly cross-checked by rephrasing the modular regularization in terms of Lorentzian inversion and Rademacher-contour sum formulas (Baccianti et al., 23 Jan 2025). These convergent rearrangements facilitate direct analytic continuation in the modular parameter, isolate cusp contributions, and establish consistency between worldsheet-based and modular-theoretic perspectives in string perturbation theory. The shared structure between the Ï„=x+iy\tau = x + iy7-regularized and Lorentzian-contour blocks is made manifest, and the functional identity between the diverse approaches is established.

Implications and Future Directions

The sector-resolved, Lorentzian-regularized approach to the Type IIB torus vacuum provides a blueprint for systematically isolating cusp and compact-sector contributions in more general settings. For physical, non-vacuum amplitudes—such as one-loop four-point graviton amplitudes—puncture integrations and Koba-Nielsen factors introduce genuine kinematic branch cuts and threshold/analytic structure. The present analysis makes it clear that the regularization framework presented can be elevated and adapted to those higher-point, dynamical settings, with direct implications for modular graph function expansions, unitarity decompositions, and the study of stringy analytic structure near thresholds.

The extension of these techniques to amplitudes with polar Fourier support, detailed cut and discontinuity structure, and exotic modular subgroups will further clarify the interplay between worldsheet geometry, modular invariance, and target space unitarity. The computational tractability of the sector-resolved approach, combined with its analytic rigor and cross-compatibility with recent inversion and Rademacher machinery, ensures enduring utility for perturbative string anomaly studies, nonperturbative completions, and the algebraic analysis of higher-genus modular integrals.

Conclusion

This work provides a comprehensive, explicit regularization prescription for the one-loop vacuum amplitude of Type IIB superstring theory, fully resolving modular, cusp, and sector structure prior to supersymmetric projection. The algebraic and analytic tools developed exhibit strong compatibility with modern approaches to modular integrals and worldsheet unitarity, setting a reference point for subsequent generalizations to nontrivial string scattering regimes and offering robust numerical and algebraic benchmarks for the analysis of modular integrals in string perturbation theory.

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