Separate the constant embedding coordinate from its nonzero modes. Its integral gives the momentum-conservation delta function; below this is understood and absorbed into the amplitude normalization on the momentum-conserving locus. For the nonzero modes the Euclidean Polyakov action is quadratic, with worldsheet Green function
Treat the tachyon vertex operators as normal ordered, removing coincident self-contractions. The Gaussian functional integral, or the same calculation by Wick's theorem, gives
All remaining determinants are independent of the insertion points and momenta and enter the overall constant. This derives the Koba-Nielsen factor and the requested position integral.
For the Möbius transformation , , one has
The transformed Koba-Nielsen factor contributes, at insertion , the power of . Four-momentum conservation makes this power . The complete differential integrand therefore transforms by
It is invariant when for every external tachyon. The correlator alone is covariant; the integration measures are necessary for invariance. The group acting faithfully on the sphere is , with the two elements of acting identically.
The apparent integral over all positions includes the residual conformal-group gauge volume. Divide by it and fix three distinct insertions. The Faddeev-Popov determinant, equivalently the three-point worldsheet ghost correlator and its conjugate, contributes
Set , , , then send to infinity on the sphere; the sign of the real direction is irrelevant. The factors involving behave as , while . They cancel, leaving as the one integration variable.
The remaining distance exponents are
For example and each individual squared momentum is . Also
Consequently the reduced amplitude is proportional to
Apply the supplied complex beta integral with , , and . Its numerator arguments become , , , while its denominator arguments become , , . Thus the four-point amplitude is the Virasoro–Shapiro amplitude
where is momentum-independent. The integral converges initially when , , and ; the displayed answer elsewhere is its analytic continuation.
The gamma function has simple poles at nonpositive integers and no zeros. At generic fixed , the amplitude therefore has simple -channel poles at , , with the same towers in and by crossing symmetry. They describe exchange of the closed string tachyon, massless states, and the infinitely many massive levels. The reciprocal denominator factors can give zeros at negative values ; special kinematics can also make an exchange residue vanish.
To see the structure of a generic residue, set , , , so . At , the Gamma function recurrence reduces the remaining factors to a constant times . The Virasoro–Shapiro amplitude pole residue is thus a polynomial of degree in the other channel invariant, consistent with exchange up to spin . Crossed numerator poles must not simply be multiplied: near and , , and the zero of cancels the putative double pole. The leading singular part is proportional to
The tree amplitude is meromorphic, with no loop threshold branch cuts; its channel singularities express factorization and string dual resonance.
Take an oriented closed string in flat, critical bosonic string theory, with and a mostly-plus target Minkowski metric. After continuation of the worldsheet to Euclidean signature, the Polyakov path integral sums over embeddings and worldsheet metrics, divided by worldsheet diffeomorphisms and Weyl transformations. In a flat target its kinetic action is
Target-time continuation or analytic continuation of external momenta defines the Lorentzian scattering amplitude; a naive real Euclidean Gaussian for timelike would not be convergent.
An external tachyon is represented by the tachyon vertex operator , with conformal weights . The physical integrated vertex has , so . Schematically its tree amplitude is
The Faddeev-Popov determinant from conformal gauge is represented by the worldsheet ghost fields. At tree level the worldsheet is a Riemann sphere, whose unpunctured complex structure has no moduli. Its residual conformal automorphisms are the Möbius transformations, . Fix three insertion points, accompanying their unintegrated vertices by the required ghost factors. The remaining complex insertion positions are integrated over the sphere; equivalently one integrates all positions and divides by the residual conformal group.
The embedding fields are free, with
Their zero-mode integral gives momentum conservation, and their nonzero-mode Gaussian integral gives the Koba-Nielsen factor
This explains the sphere tachyon position integral without needing its evaluation. For four tachyons the resulting Virasoro–Shapiro amplitude displays the exchanged string spectrum directly.
Use all-incoming external momenta and introduce alongside the two printed dimensionless Mandelstam variables. Since and , one obtains . The physical center-of-mass energy squared in the channel is . The channel measures the analogous crossed momentum transfer, with sign determined by the mostly-plus convention. Rewriting the Gamma factors in a symmetric form gives
The Gamma function poles imply, at generic fixed values of the other invariant,
The denominator Gamma factors can remove residues at special intersecting channel kinematics; the statement concerns a generic single-channel limit. An -channel pole occurs when the intermediate momentum satisfies the mass-shell condition for a closed-string state:
The pole at exchanges the ground-state tachyon, the pole at exchanges massless states, and the positive integer poles exchange the infinite massive tower. The -channel interpretation is the crossed version. Factorization means that each residue is a sum of products of couplings to intermediate physical states that couple to the chosen external particles. It need not expose every representation at that mass.
For example, the Gamma function recurrence and Gamma function residue at a nonpositive integer give the dimensionless Virasoro–Shapiro amplitude pole residue
The residue polynomial has degree , consistent with maximum spin in the exchanged level. The amplitude also has the corresponding -channel poles by crossing symmetry.
The massless fields can be treated as target backgrounds rather than separate asymptotic insertions. Write the target metric as , introduce a Kalb–Ramond field , and a dilaton . In conventional Euclidean signs their string nonlinear sigma model action is
Here is the antisymmetric tensor density. The three backgrounds correspond to the graviton, antisymmetric tensor and scalar states at closed-string level one. Expanding the vacuum functional in , then Fourier expanding the backgrounds, produces exactly their integrated string vertex operators. Its functional derivatives therefore generate the amplitudes with massless external strings. The connected vacuum functional organizes connected amplitudes; the spacetime effective action organizes the corresponding vertices after treating massless propagation consistently.
At momenta small compared with , massive string propagators can be expanded in powers of momenta over their masses. The analytic part of the amplitudes consequently determines local higher-derivative interactions, ordered by powers of . Massless exchange poles are retained through propagation of the massless fields, rather than expanded into local contact terms. Up to field redefinitions, the leading massless-sector action in the string-frame metric is
The terms denoted contain additional derivatives, including curvature-squared terms in the bosonic theory. The expansion concerns the massless sector around the perturbative bosonic background; the tachyon instability remains and is not cured by omitting its field from this displayed action. Thus this is a formal perturbative effective description, not a claim of a stable bosonic vacuum.
Finally split the dilaton into a constant and its variation, . By the Gauss-Bonnet theorem, its dilaton Euler-characteristic weighting on a connected closed oriented surface follows from
Define the string coupling by . A genus- path integral is weighted by
The sphere carries , the torus carries , and each extra handle adds . At higher genus one integrates over complex-structure moduli as well as insertion points, with the associated antighost insertions supplying the correct moduli measure. With canonically normalized external vertices an -point genus- amplitude scales as .
Summing connected worldsheets of every genus of a surface yields the string-loop effective action expansion
Each coefficient has its own low-energy expansion. The two parameters have different roles: resolves finite string size through higher derivatives, while counts additional string loops.
Use a genus-zero Polyakov path integral, target signature and all four momenta incoming. Define the Mandelstam variables by , , . The string mass-shell condition is and momentum conservation is , so
The reduced amplitude omits the overall momentum-conservation Dirac delta distribution and any conventional overall scattering-matrix phase. Interpret each tachyon vertex operator as normal ordered; self-contractions must not be included.
The free-boson worldsheet propagator is . Wick theorem then evaluates the normal-ordered exponential correlator as the Koba-Nielsen factor
The worldsheet zero mode supplies momentum conservation. Four vertices give and the sphere contributes through the string genus expansion, leaving .
The sphere's residual Möbius transformations fix three insertion points. In sphere gauge fixing for four string vertices, take . The worldsheet ghost fields, equivalently the Faddeev-Popov determinant for this residual group, supply . At finite , this determinant grows as , while the matter correlator decays as by momentum conservation and the tachyon mass shell; their product has a finite limit. Equivalently the weight- matter operator at infinity is normalized with , while the ghost pair uses the inverse factor. After stripping the fixed-position normalization, only
remains. Here choose the standard complex-coordinate measure . With instead, the reduced normalization must acquire a factor two to give the same requested amplitude. Absolute vertex/sphere normalization is a convention; this choice fixes it consistently with the displayed prefactor.
Set , , . Then and the integrand is . To evaluate the complex beta integral first work where . This ensures convergence near , and infinity. Set and . Schwinger parameterization gives
Completing the square, the Gaussian integral is . Change variables to and ; their Jacobian determinant is . Integrating gives . The remaining integral is the ordinary beta function . Thus
Restoring and substituting the Mandelstam variables proves the Virasoro–Shapiro amplitude:
For physical scattering the original position integral generally fails to converge. The formula defines the amplitude by analytic continuation from the convergence domain, with the desired scattering boundary value at real poles; the convergent integral should not be claimed valid for every physical momentum.
The gamma function is a meromorphic function, with simple poles at nonpositive integers and no zeros, while its reciprocal is an entire function. Consequently it is a meromorphic function of the independent invariants and a crossing-symmetric scattering amplitude: permuting leaves it unchanged. Its generic channel poles are
and the same tower in and . They represent the exchanged bosonic string mass spectrum: the tachyon, massless states including the graviton, and an infinite sequence of massive closed-string levels. There are no threshold branch cuts at this tree order.
A precise check of factorization is the Virasoro–Shapiro amplitude pole residue. Near , set in the nonsingular factor. The gamma function recurrence gives
Combining this with shows
The residue is a degree- polynomial in , consistent with exchange up to spin and scattering-amplitude factorization. At exceptional kinematics reciprocal Gamma zeros can remove apparent poles. In particular, when both and approach nonpositive integers, the zero from cancels the putative double pole, leaving channel simple-pole terms. Thus one must not count products of numerator poles without using .