Abstract

The full two-loop amplitudes for five massless states in Type II and Heterotic superstrings are constructed in terms of convergent integrals over the genus-two moduli space of compact Riemann surfaces and integrals of Green functions and Abelian differentials on the surface. The construction combines elements from the BRST cohomology of the pure spinor formulation and from chiral splitting with the help of loop momenta and homology invariance. The α′ → 0 limit of the resulting superstring amplitude is shown to be in perfect agreement with the previously known amplitude computed in Type II supergravity. Investigations of the α′ expansion of the Type II amplitude and comparisons with predictions from S-duality are relegated to a first companion paper. A construction from first principles in the RNS formulation of the genus-two amplitude with five external NS states is relegated to a second companion paper.

Highlights

  • The perturbative evaluation of superstring amplitudes in the Ramond-Neveu-Schwarz (RNS) formulation proceeds systematically from first principles

  • Various identities for the Clifford-Dirac algebra and pure spinors are collected in appendix A; basics ingredients of Riemann surfaces and their function theory are summarized in appendix B; a detailed derivation of the chiral splitting procedure suitable for the pure spinor formulation is presented in appendix C; and the operator product expansions of the pure spinor worldsheet fields are gathered in appendix D

  • We have proposed a spacetime supersymmetric expression for the chiral twoloop five-point amplitude relevant to massless states of Type II, Heterotic, and Type I superstring theories

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Summary

Introduction

The perturbative evaluation of superstring amplitudes in the Ramond-Neveu-Schwarz (RNS) formulation proceeds systematically from first principles (see for example [1,2,3,4] and references therein). Our key result is the construction of the chiral amplitude K(5) which is a function of external momenta, chiral polarization vectors and spinors, loop momenta, and a complex analytic dependence on vertex operator points and moduli of the underlying compact Riemann surface Σ. The integration of the pairing of left and right chiral amplitudes over loop momenta, vertex operator points, and moduli gives the physical amplitude for five external states in the supergravity multiplet. The kinematic factors T1m,2,3|4,5, T23,1|4,5, S2;4|5|1,2 in pure spinor superspace will be developed below, giving access to arbitrary combinations of external states from the massless supersymmetry multiplets These kinematic factors are independent of moduli, vertex points, and loop momenta. Various identities for the Clifford-Dirac algebra and pure spinors are collected in appendix A; basics ingredients of Riemann surfaces and their function theory are summarized in appendix B; a detailed derivation of the chiral splitting procedure suitable for the pure spinor formulation is presented in appendix C; and the operator product expansions of the pure spinor worldsheet fields are gathered in appendix D

Pure spinors and chiral splitting
Gauge symmetry of the ghost fields and gauge invariant composites
Chiral splitting
Homology invariance
BRST transformations
Vertex operators
The b-ghost
Basics of genus-two amplitudes
Genus-two correlators in the pure spinor formalism
Partition functions
The zero-mode regulator
Wick contractions of non-zero-mode fields
Zero mode counting
Zero modes absorbed by the b-ghosts
The chiral amplitude for four external states
Genus-two amplitudes for five massless states
Structure of the chiral amplitude for five external states
Four d-zero modes and one loop momentum from vertex operators
Four d-zero modes and one Wick contraction from vertex operators
The vector block for the amplitude of five external states
Worldsheet dependence of the vector block
Construction of the scalar block
Scalar block in terms of two-particle superfields
Preamble
Two-particle superfield formalism
Two-particle superfields for the five-point function
The scalar block in terms of two-particle superfields
Structure of the chiral amplitude
The supergravity limit
Findings
Conclusion and future directions
Full Text
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