Screening Stringy Horizons

It has been argued recently that string theory effects qualitatively modify the effective black hole geometry experienced by modes with radial momentum of order $1/\sqrt{\alpha'}$. At tree level, these $\alpha'$-effects can be explicitly worked out in two-dimensional string theory, and have a natural explanation in the T-dual description as coming from the integration of the zero-mode of the linear dilaton, what yields a contribution that affects the scattering phase-shift in a peculiar manner. It has also been argued that the phase-shift modification has its origin in a region of the moduli space that does not belong to the exterior black hole geometry, leading to the conclusion that at high energy the physics of the problem is better described by the dual model. Here, we elaborate on this argument. We consider the contribution of worldsheet instantons in the 2D Euclidean black hole sigma-model and study its influence on the phase-shift at high energy.


Introduction
In the recent paper [1], it has been argued that string theory effects qualitatively modify the effective black hole geometry experienced by modes with radial momentum of order 1/ √ α ′ .
At tree level, these α ′ -effects can be explicitly worked out in two-dimensional string theory, where the black hole background admits an exact worldsheet description in terms of the gauged SL(2, R)/U(1) Wess-Zumino-Witten (WZW) model. In addition, this model is known to have a dual description (in a sense similar to T-duality) that involves a two-dimensional flat tachyonic linear dilaton background, known as Fateev-Zamolodchikov-Zamolodchikov (FZZ) dual [2]. In the FZZ dual model, the α ′ effects studied in [1] have a natural explanation as coming from the integration over the zero-mode of the linear dilaton, what yields a contribution that affects the scattering phase-shift in a peculiar manner. Such contributions and, consequently, the phaseshift modification they produce seem to come from a region of the moduli space that does not belong to the exterior black hole geometry. This led the authors of [1] to conclude that the highenergy physics is better described by the FZZ dual model, rather than by the two-dimensional (2D) black hole σ-model. Here, we elaborate on this argument. We consider worldsheet instanton contributions and study their influence to the phase-shift at high energy. The 2D black hole σ-model contains an operator that controls the worldsheet instanton contributions. This is given by a second screening operator in the worldsheet CFT, and the integration over the zeromode of the linear dilaton, once such screening operator is considered, yields an α ′ -dependent function of the string states momenta. Therefore, it is natural to ask to what extent such α ′dependent function accounts for the high-energy phase-shift discussed in [1]. We will study this in Section 5. Before, in Section 2, we review the 2D Euclidean black hole σ-model. In Section 3, we discuss string scattering amplitudes on the black hole background and the high-energy modification of the phase-shift. In Section 4, we review how such modification is gathered in the FZZ dual theory. In Section 5, we first show how the second screening is associated to worldsheet instantons, and then study their contribution in relation to the stringy phase-shift.

String 2D black hole
String theory admits an interesting exact solution that describes strings propagating on a twodimensional black hole background [3,4]. The metric of the classical Euclidean black hole geometry is given by where θ ∈ [0, 2π) and r ∈ R 0 . On the other hand, the dilaton configuration needed to support this background is given by which tends linearly to infinity when r is large, namely far from the horizon. The metric above describes a semi-infinite cigar-like geometry of R 2 topology. Compact coordinate θ represents the compactified Euclidean time. The horizon of the Lorentzian black hole gets mapped to the tip of the cigar, which is located at r = 0. In the large r region, the Euclidean metric approaches a cylinder of radius L.
The non-linear σ-model that describes 2D string theory propagatig on the background (1)- (2) is given by the gauged Wess-Zumino-Witten (WZW) model for the coset H + 3 /U(1), with H + 3 = SL(2, C)/SU (2). Its Lorentzian version corresponds to the SL(2, R)/U(1) coset [4]. Let us first discuss the σ-model on H + 3 , which in a convenient coordinate system takes the form which involves a scalar field φ and a β-γ commuting ghost system. At large r, one can identify φ ∼ √ kr, and this corresponds to a linear dilaton background. The constant M appearing in (3) can be shown to be related to the two-dimensional black hole mass. Its precise value is not relevant for perturbative physics, as it can be set to 1 by simply rescaling φ. The relevant parameter is actually k = L 2 α ′ , which is the Reynolds number that controls the physics of the problem: It measures the typical strings length, l s = √ α ′ , relative to the curvature radius of the geometry, L. The classical limit thus corresponds to k going to infinity.
Ghost fields β andβ in (3) are not dynamical, and then they can be integrated out. However, it is convenient to keep these fields in the action for practical purposes. One of the reasons for doing this is that it allows for a free field representation of the sl(2, R) k ⊕ sl(2, R) k Kac-Moody symmetry that action (3) exhibits. This free field realization is given by the so-called Wakimoto representation of the sl(2, R) k current algebra, which follows from defining the local currents [5] J + (z) = β(z), together with their complex conjugate counterpart. Considering the free-field propagators both for the scalar field φ and for the β-γ system, the operator product expansion (OPE) of currents (4)-(6) realizes the sl(2, R) k affine Kac-Moody algebra. It can be verified that the interaction term in (3) has a regular OPE with the currents, so it preserves the full sl(2, R) k symmetry.
Through the Sugawara construction, the currents (4)-(6) yield the stress-tensor together with its anti-holomorphic counterpart.
The coset SL(2, R)/U(1) construction can be accomplished by supplementing the SL(2, R) model by adding an extra scalar field X(z) = X L (z) + X R (z) and a fermionic B-C ghost system [6,7,8]. This amounts to improve the stress-tensor (7) with an extra piece, namely 1 and analogously for the anti-holomorphic counterpart. This yields the central charge which consistently tends to 2 in the large k limit.
The BRST charge associated to the U(1) of the coset model is This means that the vertex operators creating physical states of the theory have to have regular 1 Hereafter we omit the diffeomoerphism b-c ghost system contributions.
where j, m andm are isospin variables that label the SL(2, R)×SL(2, R) representations. These variables represent the momenta associated to the radial and Euclidean time coordinates, and the winding number along the latter. More precisely, we have the radial momentum and the right-and left-moving momenta where p θ and ω represent the momentum and the winding number along the θ-direction, respectively. That is to say that the vertices (10) States with p φ ∈ R and m −m ∈ Z correspond to vectors of the continuous series represen- Here, we will be involved with the former.

High-energy scattering
Now, let us discuss string scattering amplitudes on the background (1)-(2). Tree-level string scattering amplitudes are given by the integral of correlation functions of vertex operators on the sphere topology where Vol −1 SL(2,C) is the volume of the conformal Killing group. The subscript M in (14) refers to the fact that expectation value is defined by interacting action (3). More precisely, we can where the worldsheet insertions of three vertices fixed as z 1 =z 1 = 0, z 2 =z 2 = 0, and To perform the functional integral (15) it is convenient to first separate the zero-mode φ 0 of the field φ. That is, consider φ(z,z) = φ 0 +φ(z,z) and then integrate over the dilaton zero-mode φ 0 and fluctuationsφ(z,z) separately. When doing this, one verifies that the integrand in (15) involves a contribution which comes from separating the action (3) in its free part S 0 ≡ S M =0 and the interaction term In (16), quantities with tilde, such asS 0 andS I , are defined by replacing the field φ(z,z) by its fluctuationsφ(z,z), e.g. S 0 =S 0 and S I = e −φ 0 √ 2 k−2S I . Considering the Gauss-Bonnet theorem, which states that the Euler characteristic on the sphere is 1 2π d 2 z √ gR = 2, and using properties of the δ-function, one finds that, after integrating over φ 0 , (16) takes the form where s = N i=1 j i + 1 and where Γ(−s) = R + dη η −1−s e −η . Finally, absorbing a k-dependent factor in the definition of the path integral, one finds with Then, we see that the integration over the dilaton zero-mode is responsible for the prefactor Γ(−s) in (19). This prefactor is crucial for our discussion. This produces poles at configurations , whose residues can be thought of as resonant correlators. The poles s ∈ Z >0 admit a physical interpretation similar to that proposed in Ref. [9] for the analogous poles in Liouville field theory. When integrating over the β-γ system, and because β is a 1-differential, the Riemann-Noch theorem, once combined with (21), yields exactly the same conservation law obtained from the integration over the zero-mode of the field X, namely N i=1 (m i +m i ) = 0. The condition on the total winding number N i=1 (m i −m i ), on the other hand, is more subtle [10,11]. The prefactor Γ(−s) in (19) can be alternatively obtained by virtually integrating over the imaginary part of φ 0 . This produces a δ-function that selects a precise amount of operatorsS I from the series expansion of e −S I . More precisely, the δ-function selects the s th term (−1) s! (S I ) s of the series, with s = N i=1 j i +1. Then, the infrared divergence δ(0) ∼ Γ(0) can be combined with the multiplicity factor (−1)/s! in order to produce the factor Γ(−s) by recalling the formula lim ε→0 Γ(−s + ε)/Γ(ε) = (−1) s /Γ(s + 1) for s ∈ Z ≥0 .

The expression for the two-point function is [8]
The phase-shift δ is defined by the reflection coefficients, given by the two-point function as e iδ ≡ A j j m −m . Since M can be adjusted to absorb the k-dependent functions in the first factor of (22), the only relevant k-dependent piece in the two-point function is given by the prefactor This prefactor is the one responsible for the phase-shift modification at high-energy discussed in [1]. To see this, following [1], one may resort to the Stirling approximation, which states that for large |z| one has Γ(z) ≃ 2π/z (z/e) z (1 + O(1/z)). Applying this to (23), one finds that in the regime p φ ≫ √ k − 2, one finds This gives the high-energy dependence of the phase-shift [1].

The dual theory
The two-dimensional σ-model on the Euclidean 2D black hole geometry is known to be dual to a two-dimensional conformal field theory known as sine-Liouville theory. The latter theory is defined by the action whereX(z,z) ≡ X L (z) − X R (z) is the dual to the bosonic field X(z,z) = X L (z) + X R (z).
Direction X is compact, while ϕ takes values on the real line. That is to say that, unlike the 2D Euclidean black hole σ-model, the model defined by (25) has topology R×S 1 . Thought of as a string σ-model action, sine-Liouville theory (25) represents a flat linear dilaton background in the presence of a non-homogeneous tachyon condensate.

The duality between (3) and (25) has been conjectured by Fateev, Zamolodchikov and
Zamolodchikov (FZZ) in an unpublished work [2], and it has been reviewed and elaborated by Kazakov, Kostov and Kutasov in Ref. [12]. It represents a kind of T-duality. In fact, the supersymmetric version of the FZZ duality actually corresponds to mirror symmetry [13], which relates the N = 2 version of Liouville theory with the Kazama-Susuki SL(2, R)/U(1) model.
In [14], Maldacena explained how the bosonic FZZ duality emerges as a consequence of the supersymmetric extension. More recently, a proof of the FZZ conjectured duality was given by Hikida and Shomerus in Ref. [15]; see also [16].
The interaction term in sine-Liouville action can actually be written as particular cases of (26), namely Correlation functions involving (26) were computed in Ref. [17] using the Coulomb gas approach. The correlators are defined by inserting s + operators of the type λ 2 d 2 z V 1−k/2,k/2,−k/2 and s − operators of the type λ 2 d 2 z V 1−k/2,−k/2,k/2 , satisfying the condition In this theory, the total winding number N i=1 ω i = N i=1 (m i −m i )/k in a given N-point function can be violated up to N − 2 units [2]. The winding number preserving correlation functions correspond to the particular cases s + = s − = ( N i=1 j i + 1)/(k − 2). On the other hand, correlators with N i=1 ω i = 0 correspond to correlators computed with s + − s − = 0, so that the quantity ( N i=1 j i + 1)/(k − 2) in the latter case is not necessarily an integer number. In the case of the two-point function (N = 2) the winding number is preserved, and thus s − = s + .
This implies that one can describe the sine-Liouville 2-point correlation functions by inserting s + + s − operators e − √ k−2 2 ϕ cos( k/2X). It can be shown [12] that, in this case, the integration over the zero-mode of ϕ in the sine-Liouville two-point function yields a factor 2 and, as observed in [1], this factor precisely reproduces the leading piece ∼ p φ log p φ of the phaseshift 3 (24). In addition, is was observed there that the integral over the zero mode of ϕ that in the case of sine-Liouville theory produces the Γ-function (28), receives dominant contributions coming from a region of the moduli space that, in the 2D Euclidean black hole σ-model side, has no representative. This suggests that sine-Liouville description is the approrpiate one to 2 Here, the symbol ≃ means that this has to be understood as valid in the limit p φ >> √ k − 2. 3 Although the coefficient of the term in δ that is linear in p φ differs from that in (24). describe these finite α ′ -effects. To complete the argument, in the next section we will address the following two questions: First, whether (and how) finite α ′ -effects (finite-k effects) can be gathered in the 2D Euclidean black hole σ-model by the integration over φ 0 . Secondly, whether (or to what extent) such α ′ -effects recover the phase-shift (24).

Worldsheet instantons
The conformal field theory defined by the Kac-Moody currents (4)-(6) and the stress-tensor (8) admits another local exactly marginal operator. This is given by Indeed, one can verify that the OPE between (29) and currents (4)-(6) is regular, up to total derivatives. In particular, it yields where h.c. stands for the Hermitian conjugate contribution. Operator (29) commutes with the BRST charge (9), and has dimension 1 with respect to the stress-tensor (8). Then, one can in principle consider operators S II as the screening operator to be used to define the correlation functions. From the two-dimensional conformal field theory point of view, the inclusion of operators (29) is completely natural, as it corresponds to a suitable screening charge in the Coulomb gas representation of 2D CFT correlation functions. However, within the context of the path integral approach, their inclusion is less clear as their interpretation in the worldsheet string σ-model is neither that of a graviton nor of a tachyon condensate. We will argue below that operators (29) are actually associated to a type of worldsheet instantons discussed in Ref. [11].
If one includes both operators (17) and (29) in the correlators, then one finds the following condition for the observables not to vanish where s ands are the amount of operators of the type S I and of the type S II , respectively.
It was proven in [10] that the correlation functions (15) computed with s screening operators of the type (17) and no operators of the type (29) exactly agree with the correlation functions computed by insertings = s/(k − 2) operators of the type (29) and no operators of the type (17) provided the couplings M andM are related bỹ This means that we can write amplitudes (19)-(20) as follows and where the amount of screening operators is given bỹ where the prefactor Γ(−s) in (32), which has an origin completely analogous to the factor Γ(−s) in (19), now exhibits poles at Before discussing this prefactor in relation to the phase-shift, let us discuss condition (35) in relation to the worldsheet instantons. Condition (35) for n = 1, in the case of the N-point function, yields the pole condition which in the convention of [11], which is related to ours through the simple changes of variables j i →ĵ i = j i + 1, and for n = 1 correponds to Interestingly, this is exactly the pole condition that Maldacena and Ooguri conjectured in [11] that would appear in the SL(2, R) WZW N-point correlation functions. One confirms from (37) that such poles actually appear. In [11], these poles were interpreted as worldsheet instantons, corresponding to classical string configurations of momentum j ∼ k that can extend to the large φ region with no cost of energy. These configurations correspond to holomorphic maps γ = γ(z), associated to classical solutions that extend in the φ direction with no potential preventing them from going to φ = ∞. When integrating over auxiliary fields β andβ, one produces an effective potential d 2 z∂γ∂γe √ 2 k−2 φ , which vanishes for configurations with∂γ = 0 (as operators (17) and (29) do). These classical configurations are closely related to the long strings discussed in [18].
Poles (35) with n ≥ 1 also admit an interpretation as worldsheet instantons. In [11], such divergences are discussed for the particular case of the two-point function, namely for and are understood as worldsheet instantons wrapping on S 2 parameterized by the projective plane variables γ,γ.
of (32), which looks pretty much the contribution that yields the stringy phase-shift, cf. (3.3) in [1]. However, a closer look at (39) reveals that there is a factor 2 missing with respect to (24). That is, the factor Γ(−s) that comes from the integration over the dilaton zero-mode once the second screening operator is introduced yields a k-dependent function of the momenta that only accounts for one half of the leading order modification that the phase-shift suffers at high energy. In turn, one concludes, with the authors of [1], that at high energy the physics of the problem is better described by the FZZ dual model, even if the operator that controls the worldsheet instantons are considered in the 2D Euclidean black hole σ-model CFT.
Work partially funded by FNRS-Belgium (convention FRFC PDR T.1025.14 and convention IISN 4.4503.15), by the Communauté Française de Belgique through the ARC program