PHYSICAL REVIEW D 72, 055003 (2005)

Chiral fermions and quadratic divergences Xavier Calmet, Paul H. Frampton, and Ryan M. Rohm University of North Carolina, Chapel Hill, North Carolina 27599-3255, USA (Received 17 December 2004; published 6 September 2005) We present an alternative to the standard model with unitary gauge group UNp and chiral fermions in bifundamentals. Although the construction allows scalars in adjoints and bifundamentals, only models without adjoint scalars have strikingly, without supersymmetry, absence of one-loop quadratic divergence in the scalar propagator. Decisive support for these ideas could arise from new experimental results anticipated at the LHC proton collider. DOI: 10.1103/PhysRevD.72.055003

PACS numbers: 12.60.Cn, 11.10.Gh, 11.25.Wx

I. INTRODUCTION Exciting experimental results from LHC are soon expected, for the first time in an energy region well above the weak scale. Two examples of theories for this important new energy regime are the old idea of low-scale supersymmetry, for which no evidence has yet emerged, or the more recently suggested alternative of conformality in which the standard model is part of a conformally invariant theory. Both extend the well-established standard model [1], although the higher-loop corrections are better understood in the supersymmetric case and, as we shall see, there is an unresolved paradox about U1 factors in the conformality case. It is the conformality approach which is further developed in this article, and for which the new experimental data will shortly be decisive. One of the principal motivations for extending the standard model of particle phenomenology, over the last three decades and more, has been the concern about naturalness of the light Higgs scalar mass (e.g. [2]). One expects new physics to appear well above the weak scale, for example, at the Planck scale for gravity, at a grand unified theory (GUT) scale for grand unification or at a right-handed neutrino mass scale for the seesaw mechanism [3] of neutrino mass. In any such case the appearance of quadratic divergences in the Higgs scalar propagator of the standard model would suggest a heavy Higgs scalar mass thus necessitating fine-tuning and unnaturalness. The main result of the present article is that the conditions for cancellation of one-loop quadratic divergences and for the presence of chiral fermions are the same. There are several popular approaches to this naturalness question; here we shall discuss a less popular but seemingly equally valid approach. The popular ideas are (i) that the scalar is a bound state of two fermions in a technicolor theory [4], though no fully convincing model exists; (ii) that there is an extra symmetry, supersymmetry [5], which protects the light Higgs mass once it is introduced by hand; (iii) that there are large extra dimensions [6] near the weak scale which avoid the need of a much higher physics scale; (iv) that among the 10100 vacua of string theory the smallness 100 GeV of the Higgs mass is

1550-7998= 2005=72(5)=055003(4)$23.00

correlated to the smaller scale 1 meV of cosmic dark energy [7]. An alternative approach is to use nonsupersymmetric gauge theories derived from the most highly supersymmetric N  4 gauge theories. Such nonsupersymmetric N  0 gauge theories can be systematically constructed [8–11] from N  4 ones by using suitable orbifolding. The resulting theories are not coupled to gravity; we here assume this vanishing-gravity limit to be a sufficiently accurate approximation to the physics of any foreseeable collider experiment, which would be sensitive only to nongravitational interactions. Some intriguing correlations of the bifundamental representations to the standard model, as well as a new explanation of charge quantization, are given in [9]. Models can be constructed with four-dimensional conformal invariance at high energies; for the models we consider here, the renormalization group -functions vanish for all SUN gauge groups. However, other desirable properties require UN gauge groups so there is still a subtlety of decoupling U1 factors (discussed later). For example, in [10] there is a Z7 model which contains all the states of the standard model and in [11] there is a Z12 model allowing grand unification at a scale 4 TeV. In the sequence of Zp models as we shall see the first with chiral fermions is Z4 but the Z7 and Z12 examples also fall into the class we shall investigate. We shall then discuss the quadratic divergence of the scalar propagator at one loop. II. CLASSIFICATION OF ABELIAN QUIVER GAUGE THEORIES We consider the compactification of the type-IIB superstring on the orbifold AdS5  S5 = where  is an Abelian group   Zp of order p with elements exp2iA=p, 0  A  p  1. The resultant quiver gauge theory has N residual supersymmetries with N  2, 1, 0 depending on the details of the embedding of  in the SU4 group which is the isotropy of the S5 . This embedding is specified by the four integers Am ; 1  m  4 with

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© 2005 The American Physical Society

XAVIER CALMET, PAUL H. FRAMPTON, AND RYAN M. ROHM

m Am  0modp

(1)

which characterize the transformation of the components of the defining representation of SU4. We are here interested in the nonsupersymmetric case N  0 which occurs if and only if all four Am are nonvanishing. The gauge group is UNp . The fermions are all in the bifundamental representations jp  m4 m1 j1 Nj ; N jAm 

PHYSICAL REVIEW D 72, 055003 (2005)

The converse also holds: If all ai  0 then there are chiral fermions. This follows since by assumption A1  A2 , A1  A3 , A1  A4 . Therefore reality of the fundamental representation would require A1 A1 hence, since A1  0, p is even and A1 p2 ; but then the other Am cannot combine to give only vectorlike fermions. It follows that: In an N  0 quiver gauge theory, chiral fermions are possible if and only if all scalars are in bifundamental representations. For the lowest few orders of the group , the members of the infinite class of N  0 Abelian quiver gauge theories are tabulated below:

(2) III. QUADRATIC DIVERGENCES

which are manifestly nonsupersymmetric because no fermions are in adjoint representations of the gauge group. Scalars appear in representations ip  i3 i1 j1 Nj ; N j ai 

(3)

in which the six integers (ai , ai ) characterize the transformation of the antisymmetric second-rank tensor representation of SU4. The ai are given by a1  A2  A3 , a2  A3  A1 , a3  A1  A2 . It is possible for one or more of the ai to vanish in which case the corresponding scalar representation in the summation in Eq. (3) is to be interpreted as an adjoint representation of one particular UNj . One may therefore have zero, two, four, or all six of the scalar representations, in Eq. (3), in such adjoints. It is one purpose of the present article to investigate how the renormalization properties and occurrence of quadratic divergences depend on the distribution of scalars into bifundamental and adjoint representations. Note that there is one model with all scalars in adjoints for each even value of p (see Model Nos. 1, 3, 12). For general even p the embedding is Am  p2 ; p2 ; p2 ; p2 . This series is the complete list of N  0 Abelian quivers with all scalars in adjoints. To be of more phenomenolgical interest the model should contain chiral fermions. This requires that the embedding be complex: Am 6  Am (mod p). It will now be shown that for the presence of chiral fermions all scalars must be in bifundamentals. The proof of this assertion follows by assuming the contrary, that there is at least one adjoint arising from, say, a1  0. Therefore A3  A2 (mod p). But then it follows from Eq. (1) that A1  A4 (mod p). The fundamental representation of SU4 is thus real and fermions are nonchiral.1 1

The Lagrangian for the nonsupersymmetric Zp theory can be written in a convenient notation which accommodates simultaneously both adjoint and bifundamental scalars as

This is almost obvious but for a complete justification, see [12].

TABLE I. The table continues to infinity but we stop at p  7. Model No. p 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30

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2 3 4 4 4 4 5 5 5 5 5 6 6 6 6 6 6 6 6 7 7 7 7 7 7 7 7 7 7 7

Am

ai

(1111) (1122) (2222) (1133) (1223) (1111) (1144) (2233) (1234) (1112) (2224) (3333) (2244) (1155) (1245) (2334) (1113) (2235) (1122) (1166) (3344) (1256) (1346) (1355) (1114) (1222) (2444) (1123) (1355) (1445)

(000) (001) (000) (002) (011) (222) (002) (001) (012) (222) (111) (000) (002) (002) (013) (011) (222) (112) (233) (002) (001) (013) (023) (113) (222) (333) (111) (233) (113) (122)

Scalar Scalar Chiral Contains bifunds. adjoints fermions? SM fields? 0 2 0 2 4 6 2 2 4 6 6 0 2 2 4 4 6 6 6 2 2 4 4 6 6 6 6 6 6 6

6 4 6 4 2 0 4 4 2 0 0 6 4 4 2 2 0 0 0 4 4 0 2 0 0 0 0 0 0 0

No No No No No Yes No No No Yes Yes No No No No No Yes Yes Yes No No No No No Yes Yes Yes Yes Yes Yes

No No No No No No No No No No No No No No No No No No No No No No No No No No No Yes Yes Yes

CHIRAL FERMIONS AND QUADRATIC DIVERGENCES

PHYSICAL REVIEW D 72, 055003 (2005)

1 ab aby ba  ba ba  ba  ab L   F;r;r F;r;r  i ab rA4 ;r  D r;rA4  2D rai ;r D r;rai  irAm ;r  D r;rAm 4 yca ybc ca  ab PL bc  ab  2ig  r;rAi rAi ;rAi A4 rAi A4 ;r  r;rAi PL rAi ;rA4 rA4 ;r p ca bc ca  ab PL bc  ab  2igijk  r;rAi rAi ;rAi Aj rAk A4 ;r  r;rAi PL rAi ;rAi Ak A4 rAj ;r ybc yab yda ycd bc cd da  g2 ab r;rai rai ;r  r;rai rai ;r r;raj raj ;r  r;raj raj ;r  ycd yda ycd yda bc ab bc  4g2 ab r;rai rai ;rai aj rai aj ;raj raj ;r  r;rai rai ;rai aj rai aj ;rai rai ;r ;

where ;   0, 1, 2, 3 are Lorentz indices; a; b; c; d  1 to N are UNp group labels; r  1 to p labels the node of the quiver diagram (when the two node subscripts are equal it is an adjoint plus singlet and the two superscripts are in the same UN: when the two node subscripts are unequal it is a bifundamental and the two superscript labels transform under different UN groups); ai i  f1; 2; 3g label the first three of the 6 of SU4; Am m  f1; 2; 3; 4g  Ai ; A4  label the 4 of SU4. By definition A4 denotes an arbitrarily chosen fermion () associated with the gauge boson, similarly to the notation in the N  1 supersymP metric case. Recall that m4 A m1 m  0 (mod p). As we showed in the previous section, the infinite sequence of nonsupersymmetric Zp models can have scalars

(4)

in adjoints (corresponding to ai  0) and bifundamentals (ai  0). Denoting by x the number of the three ai which are nonzero, the models with x  3 have only bifundamental scalars, those with x  0 have only adjoints, while x  1, 2 models contain both types of scalar representations. As we have seen, to contain the phenomenologically desirable chiral fermions, it is necessary and sufficient that x  3. Let us first consider the quadratic divergence question in the mother N  4 theory. The N  4 Lagrangian is like Eq. (4) but since there is only one node all those subscripts become unnecessary so the form is simply

1 ab ba ba ba bc yca bc ca  ab   ab  ab L   F F  i ab  D ba  2D aby i D i  im  D m  2ig i PL  i;r  i PL i  4 p  ab PL bc yca    ab PL bc ca  g2 ab ybc  yab bc cd yda  ycd da   2igijk  i i j j i i i i j j j j k k bc ycd yda bc ycd yda  4g2 ab  ab i j i j i j j i :

(5)

All N  4 scalars are in adjoints and the scalar propagator has one-loop quadratic divergences coming potentially from three scalar self-energy diagrams: (a) the gauge loop (one quartic vertex); (b) the fermion loop (two trilinear vertices); and (c) the scalar loop (one quartic vertex). For N  4 the respective contributions of (a, b, c) are computable from Eq. (5) as proportional to g2 N1; 4; 3 which cancel exactly. The N  0 results for the scalar self-energies (a, b, c) are computable from the Lagrangian of Eq. (4). Fortunately, the calculation was already done in [13]. The result is amazing. The quadratic divergences cancel if and only if x  3, exactly the same ‘‘if and only if’’ as to have chiral fermions. It is pleasing that one can independently confirm the results of [13] directly from the interactions in Eq. (4). To give just one explicit example, in the contributions to diagram (c) from the last term in Eq. (4), the 1=N corrections arise from a contraction of  with y when all the four color superscripts are distinct and there is consequently no sum over color in the loop. For this case, examination of the node subscripts then confirms proportionality to the Kronecker delta, 0;ai . If and only if all ai 

0, all the other terms in Eq. (4) do not lead to 1=N corrections to the N  4. Some comments on the literature are necessary. In the 1999 paper of Csaki, Skiba, and Terning [14] it was claimed that there are always 1=N corrections to spoil cancellation for finite N and that N 1028 is necessary. This was because of a technical error that the orbifolded gauge group is not SUNp but UNp and bifundamentals carry U1 charges. A paper by Fuchs [15] in 2000, which has been largely ignored, corrected this point. The conclusion is that the chiral Z7 , Z12 models of [10,11] which contain the standard model are free of one-loop quadratic divergences in the scalar propagator. Nevertheless the overall conformal invariance would not be respected by U1 factors which would have nonzero positive beta functions. Clearly these factors must somehow be decoupled. This mysterious decoupling of U1’s from AdS/CFT which would not be conformally invariant has been commented upon in [16,17]. A better understanding of these U1’s may be necessary to achieve the hope of a fully four-dimensionally conformally invariant extension of the standard model. There is the paradoxical require-

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PHYSICAL REVIEW D 72, 055003 (2005)

ment that the U1 gauge factors must be present in the UV to cancel quadratic divergences but must decouple in the IR to preserve four-dimensional conformal invariance at lower energy. Quadratic corrections at higher than oneloop order merit further study. Eventually gravity, at the Planck scale, will inevitably break conformal invariance because Newton’s constant is dimensionful. A realistic hope is that there is a substantial window of energy scales where conformal invariance is an excellent approximation between, say, 4 TeV [11] for at least a few orders of magnitude in energy even towards a scale approaching the seesaw scale 1010 GeV. It is difficult to foresee how large the conformality window is. Finally it is interesting to note that the present models seem to have all the ingredients of the so-called little Higgs models [18], which were proposed later than [8], with the quiver diagram here interpreted as the theory space there. As there, the one-order-of-magnitude ratio of the Higgs mass to the conformality scale is provided by a one-loop suppression factor. This conformality idea, that an augmented standard model possess an energy window of conformal invariance

starting just above the weak interaction scale, requires the existence of new undiscovered particles accessible to the LHC: gauge bosons which fill out the unitary gauge group UNp which contains the established SU3  SU2  U1; chiral fermions in bifundamental representations of UNp ; and, as shown in the present article, complex scalars also in bifundamentals of UNp . The new experimental results should be able to distinguish these definite predictions coming from the assumption of fourdimensional conformal invariance.

[1] S. L. Glashow, Nucl. Phys. 22, 579 (1961); S. Weinberg, Phys. Rev. Lett. 19, 1264 (1967); A. Salam, in Proceedings of the 8th Nobel Symposium, Stockholm, 1968, edited by N. Svartholm (Almquist and Wiksells, Stockholm, 1968), p. 367; S. L. Glashow, J. Iliopoulos, and L. Maiani, Phys. Rev. D 2, 1285 (1970). [2] G. ’t Hooft, Cargese Summer Inst. Report No. QCD161:S77:1979, 1979, p. 135; L. Susskind, Phys. Rev. D 20, 2619 (1979); I. Jack and D. R. T. Jones, Phys. Lett. B 234, 321 (1990). [3] P. Minkowski, Phys. Lett. B 67, 421 (1977); T. Yanagida, in Proceedings of the Workshop on the Unified Theory and the Baryon Number in the Universe, edited by O. Sawada and A. Sugamoto (KEK, Tsukuba, 1979), p. 95; S. L. Glashow, in Quarks and Leptons, edited by M. Levy et al. (Plenum, New York, 1980), p. 707; M. Gell-Mann, P. Ramond, and R. Slansky, in Supergravity, edited by P. Van Nieuwenhuizen and D. Freedman (North-Holland, Amsterdam, 1979), p. 315; R. N. Mohapatra and G. Senjanovic, Phys. Rev. Lett. 44, 912 (1980). [4] S. Weinberg, Phys. Rev. D 13, 974 (1976); 19, 1277 (1979); L. Susskind, Phys. Rev. D 20, 2619 ( 1979); E. Farhi and L. Susskind, Phys. Rep. 74, 277 (1981). [5] J. Wess and B. Zumino, Nucl. Phys. B70, 39 (1974); H. P. Nilles, Phys. Rep. 110, 1 (1984); H. E. Haber and G. L. Kane, Phys. Rep. 117, 75 (1985). [6] I. Antoniadis, Phys. Lett. B 246, 377 (1990); N. ArkaniHamed, S. Dimopoulos, and G. R. Dvali, Phys. Lett. B

429, 263 (1998); I. Antoniadis, N. Arkani-Hamed, S. Dimopoulos, and G. R. Dvali, Phys. Lett. B 436, 257 (1998). W. Lerche, D. Lust, and A. N. Schellekens, Nucl. Phys. B287, 477 (1987); R. Bousso and J. Polchinski, J. High Energy Phys. 06 (2000) 006. P. H. Frampton, Phys. Rev. D 60, 085004 (1999). P. H. Frampton and C. Vafa, hep-th/9903226. P. H. Frampton, Phys. Rev. D 60, 121901 (1999); see also 60, 085004 (1999). P. H. Frampton, Mod. Phys. Lett. A 18, 1377 (2003); see also: P. H. Frampton, R. M. Rohm, and T. Takahashi, Phys. Lett. B 570, 67 (2003). P. H. Frampton and T. W. Kephart, Int. J. Mod. Phys. A 19, 593 (2004). P. Brax, A. Falkowski, Z. Lalak, and S. Pokorski, Phys. Lett. B 538, 426 (2002). C. Csaki, W. Skiba, and J. Terning, Phys. Rev. D 61, 025019 (2000). In this paper, the orbifolded gauge group was assumed to be SUNp rather than UNp and hence bifundamentals which do have U1 charges were incorrectly incorporated. E. Fuchs, J. High Energy Phys. 10 (2000) 028. E. Witten, Adv. Theor. Math. Phys. 2, 253 (1998). J. Polchinski, Int. J. Mod. Phys. A 16, 707 (2001). N. Arkani-Hamed, A. G. Cohen, T. Gregoire, E. Katz, A. E. Nelson, and J. G. Wacker, J. High Energy Phys. 08 (2002) 021.

ACKNOWLEDGMENTS One of us (P. H. F.) thanks D. R. T. Jones for discussions. This work was supported in part by the U.S. Department of Energy under Grant No. DE-FG02-97ER-41036. Note added—The models discussed here do have triangle anomalies of the U11 2 U12 type; cancellation of such anomalies and the relation to conformal invariance is currently under investigation.

[7]

[8] [9] [10] [11]

[12] [13] [14]

[15] [16] [17] [18]

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Chiral fermions and quadratic divergences

ig ijk ab r;r Ai. PL bc r Ai;r Ai Aj ca. rяAkяA4;r я ab r;r Ai. PL bc r Ai;r Ai Ak A4 ca. rяAj;r я g2 ab r;r ai .... the Baryon Number in the Universe, edited by O. Sawada.

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