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DOI 10.1393/ncc/i2011-10770-8 Colloquia: IFAE 2010

IL NUOVO CIMENTO Vol. 33 C, N. 6 Novembre-Dicembre 2010

Matrix model and β-deformation of

N = 4 Yang-Mills theory(∗)

M. Siccardi

“Sapienza” Universit`a di Roma and INFN, Sezione di Roma - P.le Aldo Moro 2 00185 Rome, Italy

(ricevuto l’ 8 Ottobre 2010; pubblicato online il 2 Febbraio 2011)

Summary. — We present the result of the determination of the effective coupling

constant for the low-energy (abelian) degrees of freedom in the so-called β-deformed N = 4 model, by means of the deep connection between supersymmetric gauge field theories and matrix models.

PACS 11.30.Pb – Supersymmetry.

PACS 11.15.Ex – Spontaneous breaking of gauge symmetries.

In recent years, there has been a renewed interest in a particularN = 1 model, known as the β-deformation of the N = 4 Super Yang-Mills. Since Leigh and Strassler found this model in the nineties [1], various aspects have been studied [2, 3], but only after its gravity dual was found [4], it was extensively investigated in numerous papers [5-7].

This model is obtained by deforming the N = 4 superpotential, enlarging its pa-rameter space, through the introduction of a new coupling constant and a (generically complex) parameter β via the definition

(1) WN =4i)≡ g tr Φ1[Φ2, Φ3]→ WN =4βi)≡ h tr Φ1[Φ2, Φ3]β.

If the scalars have a vanishing vacuum expectation value (vev),ΦI = 0, the theory

is confining and conformally invariant. In the opposite case, for generic values of the deformation parameters, it is possible to identify branches in the moduli space where the gauge group gets spontaneously broken. For the sake of illustration we will concentrate in this paper on particular branches, where only one of the three chiral superfields (which we take to be Φ1) develops a vev,

(2) 1 = diag(ϕ1, ϕ2, . . . , ϕNc).

Although at some special point of the moduli space (corresponding to sets of coinciding ϕa’s) some subgroups of the original U (Nc) gauge group can remain unbroken, at a

(∗) This work is dedicated to Kensuke Yoshida. He was a friend besides being a teacher.

c

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202 M. SICCARDI

generic point, i.e. on what we will be calling the “Coulomb branch” [8], the gauge group will be broken spontaneously to U (1)Nc. In this case, the massless spectrum consists

of Nc “photons”, corresponding to the diagonal elements of the gauge field, and their

gluino superpartners. The two fields combine to form NcAbelian vector supermultiplets

ofN = 1 SUSY. We will denote the corresponding field strength by waα, a = 1, . . . , Nc.

Obviously, there are also Ncmassless chiral multiplets, corresponding to the fluctuations

around the non-vanishing eigenvalues ϕa.

In this situation, although no superpotential can be generated, the kinetic term for the massless fields may receive quantum corrections. The effective low-energy action for the gauge fields is a holomorphic function which must be of the form

(3) Weff

Nc



a,b=1

τabwα,awbα.

The complex Nc×Ncmatrix τabencodes the effective gauge couplings and vacuum angles.

Restricting to the particular branch we considered, τabwill obviously depend only on the

diagonal part of the chiral superfield Φ1, which we shall compactly rewrite as1.

At the classical level, τab is proportional to the identity, τabcl = δabτ0. Standard

non-renormalization theorems guarantee that perturbative quantum effects are limited to one-loop corrections, while non-perturbative instanton-like terms are expected at any order. In other words we will have for τab(1) an expansion of the type

(4) τab(1) = τ0δab+ τab1−loop(1) +



k=1

τab(k)(1) ≡ τ0δab+ ˆτab(1).

The one-loop perturbative correction has already been computed in [8, 9].

In 2002, Dijkgraaf and Vafa [10] conjectured that holomorphic quantities in the low-energy regime are related to the free-low-energy of an auxiliary Matrix Model (MM). Since then, the correspondence has passed various non-trivial tests [11] and it has become a powerful tool in the study of the low-energy limit of a vast class ofN = 1 gauge theories. The Dijkgraaf-Vafa correspondence states that, given anN = 1 model, we must con-sider the superpotential as the action for Hermitian random matrices ˆN× ˆN , ˆΦ, replacing the original chiral superfields. Having built the corresponding partition function,

Z = exp  −Nˆ2 g2 m F  =  d ˆΦ exp  ˆ N gm tr Wtree( ˆΦ)  ,

the correspondence gives the relation that determines the low-energy effective holomor-phic superpotential and the coupling for the massless degrees of freedom, once the large- ˆN limit is considered. In the same limit, the MM enjoys of a ’t Hooft expansion,

(5) − log Z = Nˆ 2 g2 m F = h≥0  gm ˆ N 2h−2 Fh(Si), Si≡ lim ˆ N→∞ gm ˆ Ni ˆ N , such that the leading term is given by the planar contribution.

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MATRIX MODEL AND β-DEFORMATION OFN = 4 YANG-MILLS THEORY 203

For simplicity we shall consider the gauge group breaking U (2)→ U(1)2. Then, the low-energy coupling is simply given by

(6) τˆab= τ  −1 1 1 −1 , τ = 2F m(Si) ∂S1∂S2 = τ1−loop+ τ(1)+ τ(2)+ . . . ,

where the series expansion is naturally introduced by the perturbative expansion of the MM. Stopping at the first order(1) in the MM formulation, the complete expression of

ˆ τ is τ1−loop+ τ(1)+ . . . =− log g 2 1− ϕ2)2 h2(eıβ/2ϕ 1− e−ıβ/2ϕ2)(e−ıβ/2ϕ1− eıβ/2ϕ2) (7) + 8h 4A2sin2β/2 g4Δ4(0)Δ(β)Δ(−β) (−3 + 4 cos β − cos 2β)ϕ61 +2(−5 + 6 cos β − cos 2β)ϕ51ϕ2 +(−13 + 16 cos β − 3 cos 2β)ϕ41ϕ22 +8(−1 + 2 cos β − cos 2β)ϕ31ϕ32 +(−13 + 16 cos β − 3 cos 2β)ϕ21ϕ42 +2(−5 + 6 cos β − cos 2β)ϕ1ϕ52 +(−3 + 4 cos β − cos 2β)ϕ62 + . . . ,

where Δ(x)≡ exp[ıx/2]ϕ1− exp[−ıx/2]ϕ2. As expected, eq. (7) is organized as a power

series expansion in the instanton action, A2 ≡ exp[2πıτ0] ∝ exp[−8π2/g2], so that this

computation —perturbative from the MM point of view— gives non-perturbative informa-tion on the physics on the gauge theory side. In the h2→ g2and β→ 0 limit, tantamount

to recovering the pureN = 4 Super Yang-Mills theory, all corrections vanish, leaving only the overall diagonal contribution, τ0. The result confirms thus the interpretation of the

physics described by the formalism as a spontaneous symmetry breaking phenomenon.

REFERENCES

[1] Leigh R. G. and Strassler M. J., Nucl. Phys. B, 447 (1995) 95. [2] Aharony O., Kol B. and Yankielowicz S., JHEP, 06 (2002) 039. [3] Benini F., JHEP, 12 (2004) 068.

[4] Lunin O. and Maldacena J. M., JHEP, 05 (2005) 033.

[5] Mauri A., Penati S., Santambrogio A. and Zanon D., JHEP, 11 (2005) 024. [6] Rossi G. C., Sokatchev E. and Stanev Ya. S., Nucl. Phys. B, 754 (2006) 329. [7] Kazakov D. I. and Bork L. V., JHEP, 08 (2007) 071.

[8] Dorey N. and Hollowood T. J., JHEP, 06 (2005) 036.

[9] Kuzenko S. M. and Tseytlin A. A., Phys. Rev. D, 72 (2005) 075005.

[10] Dijkgraaf R. and Vafa C., A perturbative window into non-perturbative physics, arXiv preprint hep-th/0208048.

[11] Cachazo F., Douglas M. R., Seiberg N. and Witten E., JHEP, 12 (2002) 071. [12] Rossi G. C., Siccardi M., Stanev Ya. S. and Yoshida K., JHEP, 12 (2009) 043.

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