2hdms for “4g”: from high intensity to high energy to the cosmos

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2HDMs for “4G”: From high intensity to high energy to the cosmos Amarjit Soni HET, BNL ([email protected] ) SCALARS 2011, Warsaw SCALARS'11; WARSAW A.SONI 1

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2HDMs for “4G”: From high intensity to high energy to the cosmos. Amarjit Soni HET, BNL ( [email protected] ) SCALARS 2011, Warsaw. Motivation [1]. Seen 3; why not 4? Enhanced prospects for DEWSB [ Holdom (‘86); Bardeen et al (’90); Hung & Isidori (‘97); Hung & Xiong (‘11)]………… - PowerPoint PPT Presentation

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Page 1: 2HDMs for “4G”: From high intensity to high energy to the cosmos

SCALARS'11; WARSAW A.SONI 1

2HDMs for “4G”: From high intensity to high energy to the cosmos

Amarjit SoniHET, BNL

([email protected])

SCALARS 2011, Warsaw

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Motivation [1]

• Seen 3; why not 4?

• Enhanced prospects for DEWSB• [Holdom(‘86); Bardeen et al (’90); Hung &

Isidori(‘97); Hung & Xiong(‘11)]…………

• Enhanced prospects for baryogenesis[Jarlskog & Stora(’88); Branco et al(‘98); Hou(‘08)]

SCALARS'11; WARSAW A.SONI 2

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Motivation [II]NFC: built in…..a very serious problem for almost all BSMs

• Cannot be just simple SM4: DM link? [See e.g. Volovik(‘03); Lee, Liu & AS (‘11)]

• Readily accounts for B-CP-anomalies [A.S et al (’08; ’10); Buras et al (‘10)]

• Accounts also for AFB(tt) [Davoudiasl,McElmurry & A S]

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May be the best reason

• My license plate: udcstbgz (since ‘89 NY)

• Used to be OSCILL8 (before ‘89 in CA)

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“SM4”: a revisit

• potential of B-physics forSM4 studied extensively with George Hou~86-88

• Inspired by classic works on “SSB w/o fundamental scalars” by Cornwall and Norton [‘73], studied with Norton and students Carpenter & Siegemund-Broka, role of heavy quarks in DEWSB in [87-90]

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CAN NOT BE JUST SM4

• Neutrino4 must be very heavy [LEP, Fermilab]• D0,CDF mt’, mb’ > 350GeV [bounds in SM4]• 4G fermions very likely play important role

IN DEWSB -> likely a strongly coupled 4G• Generic 2HDMmodels [see Bar-Shalom,

Nandi and A. S ‘11] suggest significant differences in search strategies from SM4

and constraints of oblique parameters

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HINTS of CKM breaking

Based on Enrico Lunghi+AS0707.0212; 0803.4340; 0903.5059;0912.0002

1010.6069

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Delta K pi

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Important to Examine only DeltaF=2 observables:Leave out Vub sin 2 β = 0.87+-.09{Lunghi+AS,hep-ph/08034340}

( became possible only due significantly reduced error in BK)

Gamiz et al;Becirevic;

Tantalo.

Antonio et al(RBC-UKQCD)

0702042

2.1-2.7 σ- deviation from the directly measured values of sin 2 β requires careful follow-up SCALARS'11; WARSAW A.SONI 10

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Predict sin2β & fB

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Mawhinney, plenary LAT’11

HUGE STRIDES IN LATTICE

CALCULATION OF BK!

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In a nutshell

• Bulk of NP effects is in Bd,Bs mixing & in sin2β {CONFIRMS our 2008 findings}

• Bulk of NP NOT in B->τν, or in εK [Presence of subdominant effects therein certainly possible]

• Many, many checks for robustness of the conclusions

• VERY DIFFICULT to RECONCILE RESULTS with CKM-SM

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Overall perspective• Sin 2 β from “penguin” dominated modes (ΦKS ,ηKS, …..) tends to be even smaller than from “gold-plated” mode• ΔACP (K π) = ACP (K+ π0) - ACP (K+ π -) is nowhere near zero (~14.4%) and rather difficult to

understand. . Also CDF, D0: S(ψΦ) & LHCb mild indication….unsettled . D0, dimuon asymmetry exptal analysis extremely difficult ->

NEEDS confirmationImplications of our analysis is that such nonSM effects

requiring the presence of NP with a new CP-odd phase should persist

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Taking the anomalies seriously

• The most interesting theoretical framework to address these is in fact warped extra dimension……Fermion geography/localization

provides a unique construct to simultaneously address EW-planck and flavor hierachies ..Agashe,Perez & AS’04; Buras et al ‘08; Neubert et al’08• 4G is the simplest way to address these• The two may well be linked via duality

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4G & BCP-anomalies

A.S. et al ‘10; Nandi & A.S’10;Buras et al’10; Hou & Ma’10

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A. S et al 0807.1971; 1002.0595 {Note constraints from S,T, b -> s gamma,K-> pi nu nu ….are all included} C ALSO A.Buras et al 1002.2126

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Predicted range of S(psiKs) in SM4 (with mt’=400 GeV) is (shown in red) comparedwith the experimentally measured value via the psi Ks mode (1 sigma error) and

with the SM (1 sigma)

SM4 seems to predict sin2 beta around 0.70 with an error of about 0.06;S. Nandi and A.S, 1011.6091

World Average

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Recent D0 result is vertical axis and combined D0, CDF each For SM4 error on Delta_Gamma_s is increased

by a factor of two resulting in ~50% increase in a_sl^s

S.Nandi and A.S,1011.6091

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Br(Bs->µµ): a very clean processIMPORTANT Correlation with S(psi phi)

SM4 may increase or decreaseBr by ~ O(3)

LHC EPS’11 <9.0X10-9

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Detection of 4G [SM4] quarks[Atwood, Gupta, AS’11]

• An important feature: To a rather good approximation, pair production is

near threshold . Using this feature showed robust signals:1) Single lepton2) Opposite sign leptons3) Same sign dileptonsAll 3 viable

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Search for 4th generation at hadron colliders

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An important caveat:

• B-CP anomalies only need a heavy top-like quark, possessing akin to charged weak interactions: the underlying theory need not be simple SM4

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4G2HDM:LEET for DEWSB[Bar-Shalom,Nandi, A.S ‘11]

• 2 Higgs doublet model for the 4th ; 2nd doublet with v2/v1 >> 1 couples only to 4th gen

• FCNC only among 3rd and 4th gen• Significant modifications to t’, b’ decays• t’->t h, b h+ very large BR, similarly for b’• Requires modification to search strategies• Can account for tt FB asymmetry

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Phenomenology of type-I 4G2HDM

• FCNC effects only in t’ t & b’ b transitions e.g.,

• Enhanced ht’t Yukawa interaction

b->s , Z-> bb, oblique corrections …….etc See

Bar-Shalom, Nandi, AS,arXiv:1105.6095

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t’ decay pattern

t’ decays:

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b’ decay pattern

b’ decays:

Bar-Shalom

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Top pair FB asymmetry from strongly coupled 4G quarks

• [Davoudiasl, McElmurry and AS arXiv:1108.1173]• CDF has been reporting ~2 sigma deviation from SM

in the integrated asymm. And in the high invariant top pair mass about 3.5 sigma deviation from SM:

• 0.158 +- 0.075 vs 0.058+-0.009• For high (>450 GeV), 0.475+-0.114 vs 0.088+-0.013• NEW (EPS’11) D0 finds similar integrated

asymmetery (a bit more significant than CDF); in the high mass region they see some increase but not so pronounced

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We consider a simple toy 4G model with [FC] scalars

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Baryogenesis

• For SM3, there is unique CP invariance [Jarlskog ‘87]

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In 4G models

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DM possibilities in 4G models

• Lee,Liu, AS arXiv: 1105.3490• Link heaviness of 4 with new abelian gauge

interaction: B – 4 L4 distinguishing it from SM3 neutrinos • Just a heavy 4 in SM4 is NOT a viable

DMcandidate …conflicts with direct detection bounds[CDMS & XENON} both for Dirac (spin independent) or Majorana (spin dependent) cases [XENON 10]

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New B-xiL gauge symmetry for 4G

• [its similar to earlier 3G studies: Ma arXiv:9709.474; Lee & Ma, 1001.0768]

• Relevant effective new interaction is:

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Summary & Outlook• 4G extensions of SM3 should be seriously considered• It is highly unlikely to be just SM4• Heavier 4G quarks can trigger DEWSB and consequently can be a

simpler solution to hierarchy problem w/o the need for multitude of new parameters

• It facilitates significantly baryogenesis over SM3• Unlike almost all BSM models, 4G extension need not cause flavor

or CP problem• Simple solution to B-CP anomalies• AFB (tt) may be a hint of a strongly coupled 4G• Experimental searches for t’ -> t h, b’->t h+- should be given a high

priority [in addition to conventional modes]

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XTRAS

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