ebook img

Electroweak Symmetry Breaking from SUSY Breaking with Bosonic See-Saw Mechanism PDF

0.12 MB·English
Save to my drive
Quick download
Download
Most books are stored in the elastic cloud where traffic is expensive. For this reason, we have a limit on daily download.

Preview Electroweak Symmetry Breaking from SUSY Breaking with Bosonic See-Saw Mechanism

Electroweak Symmetry Breaking from SUSY Breaking with Bosonic See-Saw Mechanism Hyung Do Kim ∗ School of Physics, Seoul National University, Seoul 151-747, Korea We introduce the idea of bosonic see-saw mechanism in analogy with the see-saw mechanism. Bosonic see-saw is a new symmetry breaking mechanism and we apply it to explain electroweak symmetry breaking as an inevitable consequence of supersymmetry breaking. The breaking of electroweak symmetry occurs at tree level once supersymmetry is broken. Absence of color/charge breaking in this model is related to doublet-triplet splitting in grand unified theory. An extension of MSSM with a weak triplet shows very interesting results especially when µ=0. It provides the mostnaturalunderstandingofwhywehaveonlyelectroweaksymmetrybreakingratherthanhaving 5 color/charge breaking. In the limit µ = 0, the model predicts very light chargino mass, 104 GeV 0 while Higgs is heavy,130 GeV. 0 2 n The standard model(SM) has a beautiful structure of the electroweak symmetry breaking is a surprising can- a explaining all the matters and forces except gravity in cellation of µ2 (500 GeV)2 and the Higgs soft scalar 0 J terms of quark/lepton(s) and gauge interactions. All masssquaredm∼2Hu [6]. Ifµwereslightlylarger,wewould the quarks and leptons are massless as long as elec- never have the electroweak symmetry breaking. And if 1 troweak symmetry is unbroken, and they can get mass µ were slightly smaller, the Higgs would develop its vac- 1 from Yukawa interactions only after electroweak sym- uum expectation value (VEV) exponentially larger than v metry breaking. Within the framework of the standard the weak scale. Thus it is desirable to consider models 9 model, Higgs potential can be arbitrary and we choose in which the weak scale electroweak symmetry breaking 5 the sign of the coefficient of quadratic (quartic) term to can be explained for a broad range of parameters. 0 be negative (positive) such that the Higgs potential has In this paper we first introduce a simple idea called 1 0 a desired mexican hat shape. It would not be easy to ’bosonic see-saw mechanism’. We apply ’bosonic see- 5 understand why the quadratic term has a negative sign saw mechanism’ to explain the electroweak symmetry 0 while the quartic term is positive within the standard breaking. When down type Higgs couples to the extra / h model. vector-like pair of Higgs, we can soften the little hierar- p chy problem. Finally we consider a model in which the - The SM is just regarded as a low energy effective the- electroweaksymmetryiscloselytieduptothesupersym- p e ory of some extended one and gauge hierarchy problem metry h suggests a modification of the standard model at TeV Let us briefly discuss the conventional see-saw mech- v: scale. Supersymmetry(SUSY) [1, 2] is one of the most anism explaining the lightness of neutrino masses [7, 8]. Xi promising candates for it. In supersymmetric extensions For ν, the left-handed neutrino which is an SU(2)L dou- of the standard model, we can get a better understand- blet, and N a singlet, the possible interactions are r ing of the electroweak symmetry breaking. First of all, a the Higgs potential is no longer arbitrary and should = MNN +l HLN +h.c., (1) ν ν L − be a sum of supersymmetric F/D terms and soft super- symmetry breaking terms. The quartic term is calcu- where H = (H+,H0) is the Higgs doublet and L = lated from gauge couplings and is positive definite. The (ν,l−). After the electroweak symmetry breaking, it be- quadratic term (soft terms) is a sum of supersymmetric comes mass term (µ term) and soft supersymmetry breaking ν 1 0 m ν terms which are calculable in certain mediation mecha- Mν(cid:18)N (cid:19) = 2(cid:18)mD MD (cid:19)(cid:18)N (cid:19), (2) nism of supersymmetry breaking. In the minimal super- symmetricstandardmodel(MSSM)withgaugemediated where m = l H0 . The lightest neutrino mass for D ν SUSY breaking [3, 4, 5], a radiative correction by large h i m M is then D top Yukawa coupling gives negative Higgs mass squared. ≪ If µ were zero, the above picture might have been beau- m2 m = D. (3) tifulandcouldbeconsideredasapossibleexplanationof ν − M the electroweaksymmetry breaking. However,in reality, Note the sign of the lighter eigenvalue. As the deter- minant of the matrix is negative definite (-m2 ) and the D heavieroneisnearlyM,thelightereigenvalueisnegative ∗[email protected] definite. TheresultisvalidaslongasmD M. Wecan ≪ 2 make the mass term to be positive definite by the field From now on, we focus on the application of bosonic redefinition of neutrinos. Therefore, this observation is see-saw mechanism to the electroweak symmetry break- not important for neutrinos (fermions) but it will turn ing. As we have two Higgs fields H and H in MSSM, u d out to be very important for later consideration. there are three possibilites. First, H couples to heavy u Bosonicsee-sawmechanismworksforbosonsinsteadof Higgs. Second, H couples to it. Finally, both of them d fermions(neutrinos). Althoughthemechanismworksfor couple to it. When there is no radiative correction, the any scalar fields (superfields), here we take Higgs as an first option looks the most natural. However, we know example for a clear illustration. Supersymmetric exten- thattopYukawagiveslargeradiativecorrectionsandthe sion of the standard model requires two Higgs chiral su- secondoptionisthebest. Ifbothofthemcoupletoheavy perfieldsH andH . Supposethereisanadditionalmas- Higgs and X, we can not make them light and the third u d sive pair H′ and H′, the electroweak doublets with the option does not work. Thus we consider only the second u d oppositehypercharge. LetX = +F θ2beasuperfield possibility in this paper. X ··· representing supersymmetry breaking F = F = 0. As H′ andH′ couple to X directly, they are the mes- h Xi 6 u d For the superpotential sengersof SUSY breakingand M is the messenger scale. We can calculate soft terms mediated by gauge inter- W = l1XHu′Hd+MHu′Hd′, (4) actions. We also assume that there is a pair of color triplet Higgs fields which complete the messenger fields the scalar mass squared matrix for H ,H′∗ is d u into SU(5) multiplets. The soft terms from gauge medi- ation are positive definite [9]. 0 l∗F∗ ˆ2 = 1 . (5) M (cid:18)l1F |M|2 (cid:19) m2 = 2c α 2Λ2. (8) Φ i 4π When √F M, the lightest scalar mass squared be- Xi (cid:16) (cid:17) ≪ comes negative definite, where Λ = l2F/M and ci is the quadratic Casimir of 2 i-th gauge g|roup. N|ote that l1 10−2l2 is required to m2Hd = −(cid:12)(cid:12)lM1F(cid:12)(cid:12) . ohnavlyedΛiff∼ere1n0ceTweVithwthhieleusmu2HaldM∼S∼S1M00isGtehVe.trTeielllenvoewlctohne- (cid:12) (cid:12) Whenever F = 0, the mass sq(cid:12)uare(cid:12)d is negative and we tributionfrombosonicsee-sawwhichisnegativedefinite. 6 The most interesting consequence comes with the ad- endupwithsymmetrybreaking. Therefore,attreelevel, dtion of the electroweak triplet Σ. Let us explain why weobtaintheelectroweaksymmetrybreakingasaconse- we need Σ and how it brings an interesting result. quence ofsupersymmetry breaking. We cando the same InMSSM,thenicemechanismofradiativeelectroweak thing to H instead of H . Note that the sign here is u d symmetry breaking is spoiled by large µ term. Large µ physical as the matrix is for scalar mass squared. It is term in MSSM is due to the fact that we have not seen called ’bosonic see-saw mechanism’ as it is opposed to Higgs yet. In MSSM, the quartic couplings are given usual see-saw mechanism which works for the fermions. by gauge couplings and Higgs mass is predicted to be The bosonic see-saw mechanism shows a similarity to light. m2 > 114 GeV requires a large radiative correc- the (fermionic) see-saw mechanism. H tion and it is possible only with heavy stop. If stop is There are heavy states. (heavy Higgs v.s. N) heavy, radiative corrections are too large and the elec- • troweaksymmetrybreakingbecomeslargeunlesslargeµ Thereareinteractionsbetweenheavyandmassless term cancels it. The lightness of Higgs mass in MSSM • states. (Hu′ and Hd v.s. ν and N) is mainly due to the small quartic terms from gauge in- teractions and it can be relaxed if there are additional Off-diagonal elements are generated if fields get • VEVs. (X F =0 v.s. H H0 =0) quartic couplings in the theory in addition to the usual X →h i6 →h i6 D-term. Thus we consider the modification of MSSM to The crucial difference is the negative sign of bosonic give the addtional quartic terms. see-saw mechanism which can not be eliminated by The most transparent application of the bosonic see- rephasing scalar fields. In general, X = 0 and we can saw mechanism comes out if µ = 0. However, the limit redefinefieldsandcouplingssuchthahtXi˜6=X X does µ=0 in MSSM poses several problems [10]. not have a scalar VEV ( X˜ =0). Then we ob−thainimore h i Peccei-Quinn(PQ) symmetry and R symmetry general superpotential, • As Higgs fields carry PQ and R charge and the W = l1XHu′Hd+l2XHu′Hd′ +MHu′Hd′. (6) symmetryisexactinthelimitµ=0,oncetheyget VEVs, there appears a massless Goldstone boson Now Yukawa couplings are which is in confict with experiments. W = l H Quc+l H Qdc+l′H′Quc. (7) Electroweak symmetry breaking u u d d u u • 3 If Hu gets a VEV from negative m2Hu, Hd gets its where α = 4gπ2 is the SU(2) gauge coupling and αf = VEV through Bµ term. Therefore,if µ=0 (Bµ= f2 are similarly defined Yukawa couplings for f = 0n)o,ttgheetdtohweinr-mtyapseseqsu.arks and charged leptons can l41π,l2,lΣ1,lΣ2,lt. We assume lt′ ≪1 and neglects its con- tribution. Other Yukawa couplings are also neglected as Chargino mass they are small. The effects are summarized as follows. • If µ = 0, higgsino can get their mass only by the H : Softscalarmasssquaredisnegativeatthetree d electroweak symmetry breaking and the lightest • level from the bosonic see-saw mechanism. There charginomassisalwayslighterthanMW whichcan are threshold corrections from gauge and Yukawa not be compatible with the current bound on the interactionsandthesignisopposite. IfYukawaand lightest chargino mass, 104 GeV. gauge couplings are of similar size, the threshold These problems can be solved if extra fields are intro- correctionsatthe messengerscalecancelwitheach duced. InNMSSM,anextrasingletreplacesµterm. The other. Therefore,negativemasssquaredatthetree singlet gets a VEV and it generates µ term effectively. level dominates. Thentheelectroweaksymmetrybreakingisafinetuning H : Threshold corrections at the messenger scale just as in MSSM. An alternative way is to introduce an • u are positive for both gauge and Yukawa contribu- extra weak triplet Σ with no hypercharge. tions. Wehaveslightlylargerm2 comparedtothe Letusconsiderthemostinterestinglimitµ=0(µ-less Hu MSSM with gauge mediation. We should also con- SSM). We can forbid µ term by a discrete symmetry, so sider negativ one loop correction from messenger called’Uparity’,whichisaZ2 subgroupofPeccei-Quinn scale to the weak scale 3 m2log M. symmetry. Under the U parity, −4π2 t˜ mt˜ (H ,uc,Σ) (H ,uc,Σ). Σ : Threshold corrections are positive for gauge u → − u • andYukawacontributions. Thuswegetm2 heavier Σ ThemostgeneralsuperpotentialconsistentwiththeU than other soft scalar masses which is necessary to parity is [11] suppress the VEV of Σ compared to H and H . u d W = M2ΣtrΣ2+lΣ1HuΣHd+lΣ2HuΣHd′. (9) • Third generation Q,uc (→ stop) Threshold correction from Yukawa mediation is These terms are enough to break PQ and R symmetry. negative. We get lighter stop mass compared to Atthe sametime charginomasscanbeheavierthanM Z the MSSM which makes the negative contribution as we have new sources for it. to m2 smaller than usual. Soft supersymmetry breaking terms are Hu Vsoft = m2Hu|Hu|2+m2Hd|Hd|2+m2ΣtrΣ†Σ Tfrohmemcohsatrcghinaollenmgainssgpbhoeunnodmceonmolboigniecdalctoontshtreaipnrteccoismioens +AlΣ1HuΣHd+BMΣtrΣ2+h.c.. (10) data. The charginomass is obtainedfrom Yukawa inter- The neutral componentof Σ gets a VEV once Hu and actions (A : Higgsino-Wino-Higgs and B : Higgsino-ψΣ- H get VEVs [11], Higgs) in the µ-less theory [15]. A is the gauge coupling d vΣ = m2Σ+MΣ2 +lΣ1BMΣ2ΣMvΣ2 + 12lΣ12v2. (11) daabnialdel BSTUi(s(T2a)<nsey0wm.6mY)ureektsratywr.iacTtcshoeluΣpb1loi(nulgΣn1dlΣ<o1n0th.t6ha)te[v1pi5roe]l.caiFtseioosrncluΣvsa1tro∼i-- 1, we obtain the lightest chargino mass to be 104 GeV vΣ < 9 GeV is obtained if mΣ is larger than the elec- whichistheboundfromLEPII.Thecharginomassesare troweak scale. Letus go backto the calculationofsoftterms. As our (104,119,252) GeV for lΣ1 = 1,(M2,MΣ) = (120,150) GeV. Note thatif we allownonzeroµ, we cansatisfy the messengerfieldshavedirectcouplingswithmatter/Higgs fields, there are additional contributions. The Yukawa chargino mass bound with a smaller lΣ1. More precise calculationofT isneededaswedealwithlightspectrum mediated ones are calculated using the formalism of an- (charginos are near 100 GeV). For the neutralinos, the alytic continuation into superspace [12, 13, 14], lower mass bound 40 GeV is easily satisfied. ∆m2 = 3α2Σ2 + αΣ2αl2 Λ2 The Higgs mass can be calculated if all the parame- Hu (cid:20) 4π2 4π2 (cid:21) ters are chosen. As we have a new quartic couplings for ∆m2 = αΣ1αΣ2 Λ2 the Higgs from W =l1HuΣHd, the lightest scalar Higgs Hd h− 2π2 i massis heavierthanthe oneinthe MSSMandisaround ∆m2 = αtαΣ2 Λ2 120 to 130 GeV before considering the one loop correc- Q,uc h− 8π2 i tion. Therefore, in this model we do not need to tune ∆m2 = 3αtαΣ2 + 3α2Σ2 + αΣ2αl2 5ααΣ2 Λ2, the parameters to raise up the Higgs mass beyond the Σ (cid:20) 4π2 4π2 4π2 − 4π2 (cid:21) currentbound114GeV.Thebosonicsee-sawmechanism 4 gives m2 <0 at the messenger scale and m2 is driven tons get their masses. The mechanismworksnicely even Hd Hu to be negative by RG running to the weak scale. Both if µ = 0 though we need additional weak triplet. The m2 and m2 are negative at the weak scale and the chargino remains light (near 104 GeV) when µ = 0 and Hu Hd minimum is at around tanβ = vu (1). Unlike in it is robust against radiative corrections. Higgs is heavy vd ∼ O the MSSM, the potential is not bound from below for (about130GeVbeforeconsideringradiativecorrections) m2Hu < 0, m2Hd < 0 as the new quartic coupling l1 pre- but the full spectrum of Higgs can be obtained only af- vents them from running away along D-flat direction. terconsideringtheradiativecorrectionsandweleavethe In this paper we proposeda new mechanismto under- detailed calculation of it for future work. The bosonic standtheelectroweaksymmetrybreaking. AsH couples see-saw mechanism can be applied differently in other d directlytothemessengerofsupersymmetrybreaking,the problems. soft scalar mass squared is negative by the bosonic see- saw mechanism when supersymmetry is broken. The This work is supported by the ABRL Grant No. R14- soft scalar mass squared of H is driven to be nega- 2003-012-01001-0,the BK21 program of Ministry of Ed- u tive and the symmetry breaking minimum is at around ucation, Korea. tanβ = vu (1). There is a new SU(2) triplet Σ vd ∼ O L whichcouplestoH andH . Thelightestcharginomass u d is predicted to be light due to the absence of supersym- metricmassµandliesjustabovethecurrentmassbound [1] H. P. Nilles, Phys.Rept. 110, 1 (1984). 104 GeV. The lightest Higgs mass is heavy as we have [2] H.E.HaberandG.L.Kane,Phys.Rept.117,75(1985). a new quartic coupling. All the soft parameters appear [3] M.DineandA.E.Nelson,Phys.Rev.D48,1277(1993) fromgaugemediationandnewYukawa(Higgs)mediation [arXiv:hep-ph/9303230]. and they are calculable. Gauge mediation gives positive [4] M.Dine,A.E.NelsonandY.Shirman,Phys.Rev.D51, definite soft scalar masses which guarantees the absence 1362 (1995) [arXiv:hep-ph/9408384]. of color/charge breaking minima. Yukawa(Higgs) medi- [5] M. Dine, A. E. Nelson, Y. Nir and Y. Shirman, Phys. ation gives negative contributions to H and the third Rev. D 53, 2658 (1996) [arXiv:hep-ph/9507378]. d generationQanduc (stop)andpositivecontributions to [6] S. Chang, C. Kilic and R. Mahbubani, arXiv:hep-ph/0405267. H and Σ. The contributions of Yukawa(Higgs) medi- u [7] M.Gell-Mann,P.RamondandR.Slansky,Print-80-0576 ation softens the little hierarchy problem of MSSM. As (CERN) Higgs can be heavy, the fine tuning problem is no longer [8] T. Yanagida, In Proceedings of the Workshop on the severe. Baryon Number of the Universe and Unified Theories, Thesetupconsideredherenaturallyarisefromthefive Tsukuba, Japan, 13-14 Feb 1979 dimensional geometric setup [16]. The orbifold GUT [9] G. F. Giudice and R. Rattazzi, Phys. Rept. 322, 419 (1999) [arXiv:hep-ph/9801271]. fixes the location of gauge and Higgs fields to be in [10] J.E.KimandH.P.Nilles,Phys.Lett.B138,150(1984). the bulk and the distant brane is a source of supersym- [11] J. R. Espinosa and M. Quiros, Nucl. Phys. B 384, 113 metry breaking. In this case Higgs is very special and (1992). can feel the supersymmetry breaking directly. The mas- [12] G. F. Giudice and R. Rattazzi, Nucl. Phys. B 511, 25 sive vector-like fields introduced here is just the massive (1998) [arXiv:hep-ph/9706540]. Kalaza-Klein towers of bulk Higgs fields. Gaugino me- [13] N. Arkani-Hamed, G. F. Giudice, M. A. Luty diation can be considered at the same time as there is and R. Rattazzi, Phys. Rev. D 58, 115005 (1998) [arXiv:hep-ph/9803290]. nosymmetrypreventingthecouplingsofsupersymmetry [14] Z. Chacko and E. Ponton, Phys. Rev. D 66, 095004 breaking fields with gauge sector. In the orbifold GUT, (2002) [arXiv:hep-ph/0112190]. the doublet-triplet splitting of Higgs fields is explained [15] A. E. Nelson, N. Rius, V. Sanz and M. Unsal, JHEP by the boundary condition (or orbifold projection) and 0208, 039 (2002) [arXiv:hep-ph/0206102]. thesetupgiveninthispapernaturallyarisesfromhigher [16] H. D. Kim and S. Raby, JHEP 0301, 056 (2003) dimensions. Moreprecisely,onlyH shouldbebulkfields [arXiv:hep-ph/0212348]. d asin [17]. The setuphas beenstudiedto understandthe [17] H. D. Kim, J. E. Kim and H. M. Lee, Eur. Phys. J. C 24, 159 (2002) [arXiv:hep-ph/0112094]. top/bottom mass hierarchy without large tanβ in [17]. [18] N. Arkani-Hamed and M. Schmaltz, Phys. Rev. D 61, Furthermore, the smallness of l1 compared to l2 can be 033005 (2000) [arXiv:hep-ph/9903417]. explainedbythezeromodelocalizationofHd[18,19,20]. [19] R. Kitano and T. j. Li, Phys. Rev. D 67, 116004 (2003) We proposeda new idea called’bosonic see-sawmech- [arXiv:hep-ph/0302073]. anism’. Once supersymmetry is broken, at same time it [20] H. D. Kim, S. Raby and L. Schradin, gives the VEV to the Higgs fields, i.e., quarks and lep- arXiv:hep-ph/0411328.

See more

The list of books you might like

Most books are stored in the elastic cloud where traffic is expensive. For this reason, we have a limit on daily download.