Abstract

Canonical forms of positive geometries play an important role in revealing hidden structures of scattering amplitudes, from amplituhedra to associahedra. In this paper, we introduce “stringy canonical forms”, which provide a natural definition and extension of canonical forms for general polytopes, deformed by a parameter α′. They are defined by real or complex integrals regulated with polynomials with exponents, and are meromorphic functions of the exponents, sharing various properties of string amplitudes. As α′→ 0, they reduce to the usual canonical form of a polytope given by the Minkowski sum of the Newton polytopes of the regulating polynomials, or equivalently the volume of the dual of this polytope, naturally determined by tropical functions. At finite α′, they have simple poles corresponding to the facets of the polytope, with the residue on the pole given by the stringy canonical form of the facet. There is the remarkable connection between the α′→ 0 limit of tree-level string amplitudes, and scattering equations that appear when studying the α′→ ∞ limit. We show that there is a simple conceptual understanding of this phenomenon for any stringy canonical form: the saddle-point equations provide a diffeomorphism from the integration domain to the interior of the polytope, and thus the canonical form can be obtained as a pushforward via summing over saddle points. When the stringy canonical form is applied to the ABHY associahedron in kinematic space, it produces the usual Koba-Nielsen string integral, giving a direct path from particle to string amplitudes without an a priori reference to the string worldsheet. We also discuss a number of other examples, including stringy canonical forms for finite-type cluster algebras (with type A corresponding to usual string amplitudes), and other natural integrals over the positive Grassmannian.

Highlights

  • Tree level n-point open superstring amplitudes are defined as integrals over a componentM+0,n of the real points of the moduli space of n-points z1, z2, . . . , zn on the Riemann sphere, associated with the Koba-Nielsen factor [1]:1In({s}) = (α )n−3 dn−3z M+0,n z1,2 · · · zn,1(za,b)α sa,b, a 0 for a < b

  • We find that our stringy canonical forms/integrals have properties analogous to those of open string amplitudes

  • With the string amplitude in the new form (1.6) as our motivating example, we show that its remarkable properties mentioned above generalize to all stringy canonical forms (1.3)

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Summary

Introduction

Tree level n-point open superstring amplitudes are defined as integrals over a component. We find that our stringy canonical forms/integrals have properties analogous to those of open string amplitudes. The stringy canonical form associated with this presentation precisely yields (1.6) with Koba-Nielsen factor, giving a path from kinematic space to string amplitudes, making no reference either to bulk spacetime nor the string worldsheet as auxiliary constructs (see section 5). The cluster string integrals IΦ, defined for any cluster algebra A(Φ) of finite type, are stringy canonical forms for the generalized associahedron of the dual Dynkin diagram, P(Φ∨) [22, 23].3.

Stringy canonical forms and Newton polytopes
Newton polytopes and stringy integrals
Volumes of dual polytopes as limits of stringy integrals
Stringy canonical forms at finite α
Recurrence relations and residues at massless poles
Stringy properties
Stringy integrals with many polynomials
Tropical functions
Applications to positive parametrizations
From kinematic associahedra to open-string integrals
Further examples
Cluster string integrals
Grassmannian string integrals
Scattering equations and pushforward
Saddle point equations as a diffeomorphism
Dimension of the space of integral functions
Mod-squared stringy canonical forms
Volumes of duals of unbounded polyhedra
Complex stringy integrals
Closed-string amplitudes
Big polyhedron and dual u-variables
Big polyhedron and u-variables
The u-variables for the open-string amplitude
Example
Big polyhedron from tropical functions
Simple polytopes and complete integrands
10 Tropical compactification
10.3 The cluster configuration space
Y 12 Y 23 Y 34 Y 41
Full Text
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