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J. Phys. A: Math. Theor. 42 No 44 (6 November 2009) 442003 (5pp)
doi:10.1088/1751-8113/42/44/442003

FAST TRACK COMMUNICATION

Konishi at strong coupling from ABE

Adam Rej and Fabian Spill

Blackett Laboratory, Imperial College, London SW7 2AZ, UK

E-mail: adam.rej@imperial.ac.uk and fabian.spill@imperial.ac.uk

Received 31 August 2009
Published 8 October 2009

Abstract. In this communication, we derive analytically the scaling dimension of the Konishi operator in the planar \mathcal {N}=4 gauge theory at strong coupling from the asymptotic Bethe equations. The first two leading terms agree with the recent string computation and numerical analysis of TBA equations. At the third order we find a spurious logarithm of the coupling constant, which should be absent in the anomalous dimension of any finite operator of the planar \mathcal {N}=4 SYM theory. Showing the cancellation of this term would provide an important test at strong coupling of the recently proposed sets of TBA equations for the planar AdS/CFT correspondence.

PACS numbers: 11.25.Tq, 02.30.Ik

1. Introduction and summary

The planar \mathcal {N}=4 gauge theory exhibits a very remarkable property absent in most gauge theories. Namely, the dilatation operator is believed to be asymptotically integrable. In the groundbreaking paper [1], the one-loop integrability of the dilatation operator in certain subsectors of the gauge side of the AdS/CFT correspondence was discovered. Later on [2], the complete one-loop dilatation operator was found and the corresponding one-loop Bethe equations were written down [3]. After many non-trivial stepsNote1, the form of the all-loop asymptotic Bethe equations (ABE) was conjectured [4] up to the so-called dressing factor [5], which only contributes starting from the four-loop order. Subsequently, relying on the crossing equation proposed in [6] and assuming certain transcendentality properties, it was possible to uniquely fix this factor [7]. In this way, the asymptotic spectrum of the planar \mathcal {N}=4 SYM theory has been completely determined. The asympoticity of these equations means that for a generic operator with L constituent fields the corresponding anomalous dimension can be calculated correctly up to the \mathcal {O}(g^{2L}) order.

Beyond this order the asymptotic Bethe equations are not valid, as it was shown in [8]. Asymptotic integrability was established by disregarding the contribution of a certain class of Feynman diagrams while studying the structure of mixing of the operators. These diagrams are commonly referred to as wrapping diagrams, the reason being their topological properties [9]. In the spin chain picture, these diagrams correspond to the interactions wrapping around the spin chain. Since the interaction between two nearest neighbours provides a factor of g2, the first of the wrapping diagrams may appear at the order \mathcal {O}(g^{2 L}) , where L is the length of the spin chain. For twist-two (length-two) operators supersymmetry delays the wrapping interactions to the four-loop order.

In the seminal paper of [10] it was proposed to evaluate the first Lüscher corrections, previously studied for the AdS5 × S5 sigma model and single excitation in [11], to calculate the leading wrapping corrections to the shortest unprotected operator in the \mathfrak {sl}(2) sector, i.e. the Konishi operator. The result remarkably coincides with very complicated field theory computations [12, 13].

As for other integrable sigma models, the full solution of the spectral problem is believed to be given in terms of a set of TBA equations. Recently, there has been a lot of progress in this direction [14–18], and ultimately the Y-system [19] and the TBA equations for the ground state [21–22] have been formulated. The authors of [21] have also proposed the TBA equations for excited states in the \mathfrak {sl}(2) sector. They were used in [23] to numerically calculate the spectral curve for the Konishi operator up to relatively large values of the coupling constant λ ≊ 700. The resulting strong coupling expansion takes the following form:

Equation (1)

with aTBA  =  0.0044 and bTBA  =  1.0095. On the other hand, the computations on the string theory side performed in [24] suggest a different value of the subleading coefficient b^{{\rm string}}=\frac{1}{2} . Please note that the leading coefficient 2 has already been suggested in [25].

In this communication, assuming g=\frac{\sqrt{\lambda }}{4\pi } \gg 1 , we determine \Delta _\mathcal {K}(\lambda ) to the order \mathcal {O}\big (\frac{1}{\lambda ^{\frac{1}{4}}} \big) using the asymptotic Bethe ansatz with the BHL/BES dressing factor [7, 27]. We find

Equation (2)

with a^{{\rm ABA}}=0, b^{{\rm ABA}}=\frac{3}{4}+\frac{U}{4\pi }-\frac{\log \left(1+\pi ^2\right)}{2 }+\log (2)+\frac{\cot ^{-1}(\pi )}{\pi }\simeq 0.270\,086 . Please refer to the next section for the definition of U. Interestingly, the result obtained from the asymptotic Bethe ansatz violates the analytic structure of the strong coupling expansion advocated in [24]. The first two coefficients of the expansion seem to be in agreement with the results of [23, 24] suggesting that the finite size corrections are delayed also for the large values of the coupling constant. It should be stressed that for short operators at strong coupling, infinite number of Lüscher corrections are expected to start contributing at the same order, in contradistinction to the weak coupling case. Their first manifestation should be the cancellation of the logarithmic term and a finite contribution bwrapping  =  bbABA. It would be an important test of the \mathfrak {sl}(2) TBA equations [21] to prove analytically that this is indeed the case, especially due to the fact that logarithms are often difficult to distinguish numerically.

2. Strong coupling solution of the asymptotic Bethe equations

In what follows, we will use the \mathfrak {su}(2) asymptotic Bethe equations, although the descendants of the Konishi operator may be found in other simple sectors of the theory. The corresponding state of the \mathfrak {su}(2) spin chain has length L  =  4 and two excitations M  =  2. It can be easily checked that this is the only state with these quantum numbers obeying the momentum constraint. One thus expects that the corresponding solution may also be found from the \mathfrak {su}(2) Bethe equations at large values of λ, without the necessity to continue from weak to strong coupling.

For \sqrt{\lambda }\gg 4\pi it is convenient to use the momentum representation of the Bethe equations. The equations for the Konishi operator are given by

Equation (3)

with the momenta of the individual magnons being p1  =  p  =  –p2. We would like to emphasize once again that by definition this equation is not valid at strong coupling for a finite value of the length, and thus not for L  =  4! Despite this fact, we will attempt to solve it in order to estimate the order of the finite size corrections. The corresponding scaling dimension may be found from [26]

Equation (4)

The large λ expansion of the dressing factor θ(p1, p2) has been proposed in [27]:

Equation (5)

Equation (6)

Here, qr denote the rescaled higher charges and the coefficients c(n)r,s are given by

Equation (7)

It was argued in [7] that the strong-coupling expansion of the dressing phase may be obtained, upon resummation, from the one proposed at weak coupling. At the leading order equation (3) is dominated by the AFS dressing phase [5]:

Equation (8)

and can be consistently solved by assuming p=\frac{p_0}{\lambda ^{1/4}}+ \cdots

Equation (9)

For the Konishi operator we choose m  =  1. Please refer to [5] for further discussion of different values of m. In the same way, one can proceed to the next order and determine the next coefficient in the momentum expansion:

Equation (10)

Here, again only the AFS part of the dressing factor contributes. Interestingly, upon substituting in (4) and expanding in large λ, the canonical dimension is cancelled by the anomalous dimension part, i.e.

Equation (11)

This curious mechanism has been already observed for the \mathfrak {su}(1|1) Bethe equations in [28] and is intrinsic to the properties of the AFS dressing phase. At the next order, however, one finds that all θn(p1, p2), n ≥ 0, contribute. In particular, expanding θ1(p, – p) to the leading order in λ, one finds

Equation (12)

The appearance of the logarithm of the coupling constant enforces to seek the solution to (3) in the form

Equation (13)

All higher θn(p, – p), n ≥ 2, depend only on the first term of the above expansion. By expanding the first few of them, we have found that the leading contribution can be cast in the following form:

Equation (14)

Clearly, their overall contribution ∑n = 22i θn(p, – p) is divergent. This sum, however, may be performed by means of the Borel summation. Indeed, since

Equation (15)

and using the integral representation of the gamma function we find

Equation (16)

with U  =  –0.982 309 890 318 86 .... Alternatively, one can use the integral representation of the zeta function, or directly its series representation. All these regularizations lead again to (16). We have also used the DHM integral representation [29] to numerically calculate the strong coupling expansion of the dressing phase and found agreement with the analytic expressions proposed in this communication. Combining all the terms together, it is straightforward to determine the coefficients p2 and p2l in (13). Upon substituting (13) in (4) and expanding, one finds (2).

Acknowledgments

The authors would like to thank Lisa Freyhult, Sergey Frolov, Nikolay Gromov, Tomasz Łukowski, Matthias Staudacher and Arkady Tseytlin for discussions. Adam Rej is grateful to STFC for support. Fabian Spill would like to thank the Deutsche Telekom Stiftung for a PhD fellowship.

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Notes

Note1
 Please see [4] for further references.

  1. Konishi at strong coupling from ABE

    Adam Rej and Fabian Spill 2009 J. Phys. A: Math. Theor. 42 442003

  2. Appendix II: Langmuir's papers

    R N Franklin 2009 Plasma Sources Sci. Technol. 18 010402

  3. Relativistic echo dynamics and the stability of a beam of Landau electrons

    E Sadurní and T H Seligman 2008 J. Phys. A: Math. Theor. 41 102002

  4. Implications of the very High Energy Gamma-Ray Detection of the Quasar 3C279

    M. Böttcher et al. 2009 ApJ 703 1168

  5. Magnetic ordering in the XY pyrochlore antiferromagnet Er2Ti2O7: a spherical neutron polarimetry study

    A Poole et al 2007 J. Phys.: Condens. Matter 19 452201

  6. A Possible Period for the K-Band Brightening Episodes of GX 17+2

    Jillian Bornak et al 2009 ApJ 701 L110

  7. Evolution of Dark Matter Phase-Space Density Distributions in Equal-Mass Halo Mergers

    Ileana M. Vass et al. 2009 ApJ 698 1813

  8. How Massive are Massive Compact Galaxies?

    Adam Muzzin et al 2009 ApJ 706 L188

  9. Global Galactic Dynamo Driven by Cosmic Rays and Exploding Magnetized Stars

    Michał Hanasz et al 2009 ApJ 706 L155

  10. Single-photon generation and detection

    G S Buller and R J Collins 2010 Meas. Sci. Technol. 21 012002



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