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Composite Higgs Dynamics on the Lattice

Claudio Pica

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Claudio Pica

Standard Model Higgs

mH = 125.09 ± 0.24 GeV

L = v2

4 TrDµßDµß µ

1+2a H

v +...

°¯iLßR µ

1+c H

v +...

f = p 2

µmf M

1+

, gV = 2

mV2(1+) M1+2

!

J. Ellis and T. You, JHEP 1306 (2013) 103

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Claudio Pica

If EWSB is due to a condensate of strongly-interacting fermions, one would expect, in general, composite scalar particles

To not be excluded by experiments, this scalar states should mimic a SM-like Higgs boson.

This could happen if the composite scalar is a light pseudo-

Goldstone boson of some (higher scale) broken symmetry, e.g:

- approximate scale invariance symmetry (dilaton)

- larger chiral symmetry (composite Goldstone boson Higgs)

Can the Higgs be composite?

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Claudio Pica

Plus

Break EW

UV complete theories available to explore

Natural

Minus

Fermion masses vs FCNC

Electroweak precision data

Light Higgs

Higgs couplings

Technicolor

Higgs is the lightest scalar excitation of the condensate

S. Weinberg & L. Susskind, ‘79

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Claudio Pica

Gauge Group: SU, SO, SP, Exceptional

Matter Representation

# of Flavors per Representation

Parameters

QCD-like IR fixed point No AF

N

f

α

Energy ΛTC

Energy

U

* α

Energy ΛETC

ΛTC

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Claudio Pica

Walking

Energy

U

*

α

Energy ΛETC

ΛTC α

Energy ΛTC

Running IR fixed point

Walking

Holdom, Appelquist, Miranski, Yamawaki, Wijewardhana

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Claudio Pica

SU(N) phase diagram

SU(N)

2 3 4 5 6 7 8

2 4 6 8 10 12 14 16 18

N

n f

Fund

A-Sym

Sym

Adj

Ryttov & Sannino 07 Dietrich & Sannino 07 Sannino & Tuominen 04 Ryttov & Shrock 10

Poppitz & Unsal 9, 10 Pica & Sannino 10

Other groups: SO(n), SP(n), exceptional

Walking region? Large

γ

?

Lattice

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Claudio Pica

Use the Lattice to investigate quantitatively models which can feature the right dynamics:

SU(2) + 2 Dirac Adjoint SU(2)a - MWT

SU(3) + 2 Dirac Symmetric SU(3)s - MWT

SO(4) + 2 Dirac Vector SO(4)v - MWT

SU(3) + 2 Dirac Fund. + Ungauged SU(3)f - pMWT

SU(2) +2 Dirac Fund. + … (U - MWT) SU(2)f - MWT

Minimal (Walking) Models

Only one doublet gauged ➙ small S parameter

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Claudio Pica

TC Higgs is the lightest isospin-0 scalar made of TC-fermions

will contain also a TC-glue component

analogue to QCD lightest scalar:


f0(500) with mass ~ 400-550 MeV


Sannino & Schechter 95 PRD; Harada, Sannino & Schechter 95 PRD, 96PRL;

see also: Pelaez - Confinement X

TC Higgs

H c1QQ¯ + c2QQ¯ QQ¯ + · · ·

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Claudio Pica

Can it be light?

SM radiative corrections shift the TC Higss mass

TC Higgs mass

t

W Z

R. Foadi, M. Frandsen, F. Sannino, Phys.Rev. D 87, 095001

MH2 = (MHTC)2 + 3(4⇡F)2 16⇡2v2

4rt2m2t + 2s

m2W + m2Z 2

+ M2

H (4⇡F)

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Claudio Pica

Can it be light?

Narrow due to kinematics [Similar to f0(980) in QCD]

TC Higgs mass

0.0 0.5 1.0 1.5 2.0

200 400 600 800 1000 1200

k rt M HTC HGeVL

(MHTC)2 ' MH2 + 12 2rt2m2t

R. Foadi, M. Frandsen, F. Sannino, Phys.Rev. D 87, 095001

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Claudio Pica

The leading order interaction of the TC Higgs with EW goldstone bosons can be described by:


with

One can estimate the analogue coupling in QCD






from elastic pi-pi scattering data

TC Higgs couplings?

A. Belyaev, M.S. Brown, R. Foadi, M. Frandsen, PhysRevD.90.035012

LH¶¶ = c

v H @µa@µa

L溺 = cº

fº æ@µºa@µºa

c = 1

6

m (MeV) g ⇡⇡ (GeV) cQCD 457+1413 i(279+117 ) , [35] 3.59+0.110.13 1.0169 ± 0.06 445± 25 i(278+2218) , [35] 3.4 ± 0.5 1.0013 ± 0.17 441+168 i(272+912.5) [36] 3.31+0.350.15 1.0035 ± 0.12 474 ± 6 i(254 ± 4) , [37] 3.58± 0.03 1.0264 ± 0.024

443 ± 2 i(216 ± 4) [38] 2.97± 0.04 1.0479 ± 0.020 452 ± 12 i(260 ± 15) [39] 2.65± 0.01 0.8026 ± 0.053

453 i271 , [40] 3.5 1.0255

TABLE I: Fits to m and g ⇡⇡ extrapolated from the elastic ⇡⇡ scattering(see [35] for a summary of recent results). The last column gives cQCD according to Eq. (17).

of QCD, we expect c ' 1 and, thus, SM-like HWW and HZZ couplings. This need not be the case for walking dynamics, although departures from QCD-like dynamics by no means imply non-standard couplings to massive weak bosons. Finally we note that in TC the HWW and HZZ couplings receive small corrections from tree-level mixing of the electroweak bosons with the TC spin-one resonances5 [26].

B. TC Higgs couplings to f f

The interactions of the TC Higgs or the technipions with two SM fermions are due to four- fermion operators of the form ¯f f0FF0. Here f and f0 are SM flavors, whereas F and F0 are techniflavors, with TC gauge indices contracted to form a TC singlet. At low energy these operators generate vertices such as Hf f¯ and a f f¯ 0. Unlike the coupling to the weak bosons, there are no corresponding quantities in QCD which allow us to estimate the value of these couplings. However, Ward identities guarantee that the couplings of two SM fermions with the EW Goldstone bosons, at zero external momenta, are identical to their SM values. Of course these Ward identities tell us nothing about the Hf f¯ coupling. On the other hand, we have just seen that the interactions of the meson and the pions in QCD are well approximated by a linear sigma model. If this holds in TC as well, then a a f f¯ 0 coupling close to its SM value implies that the TC Higgs couplings to SM flavors are close to their SM values, i.e cf ' 1. In the case of a true techni-dilaton, Ward-identities related to the spontaneously-broken scale symmetry can be used to determine cf [42, 43]. Finally, if SM fermion masses are generated by an ETC sector, we expect

5 Similarly when vector mesons are introduced into the linear sigma model of QCD the fits are altered.

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Claudio Pica

Plus

Higgs is massless

Gauge boson couplings

Minus

Underlying UV complete theory

Higgs mass

Fermion masses/couplings

EW vacuum alignment

Composite Goldstone Higgs

Higgs is a pseudo Goldstone boson

D.B. Kaplan & H. Georgi, ‘84

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Claudio Pica

SU(2)TC with Nf=2 fund

SO(6)/SO(5) chiral symmetry breaking

Common framework for TC and CH

Fundamental 4D underlying theory, 


Spectrum can be obtained via lattice simulations

SU(2) Composite Higgs

G. Cacciapaglia & F. Sannino, JHEP04(2014)111

Appelquist, Sannino, 98, 99 Ryttov, Sannino, 2008

Katz, Nelson Walker, 2005

Gripaios, Pomarol, Riva, Serra, 2009 Galloway, Evans, Luty, Tacchi, 2010

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Claudio Pica

The SU(2) model

L = ° 1

4 Fµ∫a F aµ∫ +U (iµDµ ° m)U + D(i µDµ ° m)D

Q = 0 BB

@

UL DL UeL DeL

1 CC A

L = ° 1

4 Fµ∫a F aµ∫ + iU µDµU + i DµDµD + m

2 QT (°iæ2)C EQ + m 2

°QT (°iæ2)C EQ¢

E = 0 BB

@

0 0 1 0 0 0 0 1

°1 0 0 0 0 °1 0 0

1 CC A

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Claudio Pica

QL = (UL, DL): SU(2)L doublet with zero hypercharge

other two fields: SU(2)L singlets with hypercharge ±1/2

two interesting alignments of the condensate:

1. does not break EW

2. does break EW symmetry

• general superposition:

The model

hQQi /

µ iæ2 0 0 °iæ2

¥ ßB hQQi /= °i E =

µ 0 °i

i 0

¥ ßH

ß0 = cosµ ßB + sinµ ßH

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Claudio Pica

Fundamental 4d underlying dynamics

5 Goldstone bosons

3 eaten by W±,Z

SO(6)~SU(4) ➙ Sp(4)~SO(5)

TC CH

θ ~0

• 1 GB is Higgs-like

• other GB is SM neutral

θ ~ π /2

• GB complex doublet

• SM neutral

• Natural DM candidate

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Claudio Pica

TC-Higgs and PGB Higgs mix

Top reduces TC-Higgs mass

Top contributes to PGB Higgs mass

Generic properties

TC CH

Couplings: for θ near zero:

gW W h1

gW W hSM = 1 +Cµ + O (µ2) gt th1

gt thSM = 1 + Dµ + O (µ2)

• Modified Higgs phenomenology

• a new TeV scalar lighter than 


vectors?

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Claudio Pica

Rescale TC limit:

Spin one resonances

mΩ = mΩTC

sinµ mA = mTCA sinµ fPS sinµ = 246GeV

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Claudio Pica

Lattice results

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Claudio Pica

SU(2) f N f =2

Ref:R. Lewis, C. Pica, F. Sannino, Phys.Rev. D85 (2012) 014504 [arXiv:1109.3513]

A. Hietanen, R. Lewis, C. Pica, F. Sannino, [arXiv:1308.4130 [hep-ph]]

A. Hietanen, R. Lewis, C. Pica, F. Sannino, JHEP 1407 (2014) 116 [arXiv:1404.2794 [hep-lat]]

R. Arthur, A. Hietanen, V. Drach, M. Hansen, C.P., F. Sannino, arXiv:1602.06559 R. Arthur, A. Hietanen, V. Drach, M. Hansen, C.P., F. Sannino, in preparation

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Claudio Pica

Lattice conformal window

SU(N)

2 3 4 5 6 7 8

2 4 6 8 10 12 14 16 18

N

n f

Fund

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Claudio Pica

Scale Setting

0 1 2 3 4 5

0123456

y2 = w02 (m) mPS2 w0a

0 1 2 3 4 5

0123456

y2 = w02 (m) mPS2 w0a

0 1 2 3 4 5

0123456

y2 = w02 (m) mPS2

w0a cut LO cut NNLO

0 1 2 3 4 5

0123456

y2 = w02 (m) mPS2 w0a

0 1 2 3 4 5

0123456

y2 = w02 (m) mPS2 w0a

0 1 2 3 4 5

0123456

y2 = w02 (m) mPS2

w0a cut LO cut NNLO

0 1 2 3 4 5

0123456

y2 = w02 (m) mPS2 w0a

0 1 2 3 4 5

0123456

y2 = w02 (m) mPS2 w0a

0 1 2 3 4 5

0123456

y2 = w02 (m) mPS2

w0a cut LO cut NNLO

0 1 2 3 4 5

0123456

y2 = w02 (m) mPS2 w0a

0 1 2 3 4 5

0123456

y2 = w02 (m) mPS2 w0a

0 1 2 3 4 5

0123456

y2 = w02 (m) mPS2

w0a cut NNLO

β=1.8 β=2.0 β=2.2 β=2.3

0 1 2 3 4 5

0.40.50.60.70.80.91.01.1

y2 = w02 (m) mPS2 w0w0χ

0 1 2 3 4 5

0.40.50.60.70.80.91.01.1

y2 = w02 (m) mPS2 w0w0χ

0 1 2 3 4 5

0.40.50.60.70.80.91.01.1

y2 = w02 (m) mPS2 w0w0χ

0 1 2 3 4 5

0.40.50.60.70.80.91.01.1

y2 = w02 (m) mPS2 w0w0χ

β=1.8 β=2.0 β=2.2 β=2.3

w0(mps2 ) = w0¬ °

1 + Ay2 +B y4 log y2¢ W (t) = t d

d t [t2E(t)], W (w02) ¥ 1

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Claudio Pica

Goldstone bosons

0 5 10 15

0.00.10.20.30.4

( w0χ mPS )2

w 0χ FPS

0 5 10 15

0.00.10.20.30.4

( w0χ mPS )2

w 0χ FPS

0 5 10 15

0.00.10.20.30.4

( w0χ mPS )2

w 0χ FPS

0 5 10 15

0.00.10.20.30.4

( w0χ mPS )2

w 0χ FPS

0 5 10 15

0.00.10.20.30.4

( w0χ mPS )2

w 0χ FPS

0 5 10 15

0.00.10.20.30.4

( w0χ mPS )2

w 0χ FPS

0 5 10 15

0.00.10.20.30.4

( w0χ mPS )2

w 0χ FPS

0 5 10 15

0.00.10.20.30.4

( w0χ mPS )2

w 0χ FPS

β=1.8 β=2.0 β=2.2 β=2.3

0 5 10 15

024681012

( w0χ mPS )2

w 0χ m PS2 mf

0 5 10 15

024681012

( w0χ mPS )2

w 0χ m PS2 mf

0 5 10 15

024681012

( w0χ mPS )2

w 0χ m PS2 mf

0 5 10 15

024681012

( w0χ mPS )2

w 0χ m PS2 mf

0 5 10 15

024681012

( w0χ mPS )2

w 0χ m PS2 mf

0 5 10 15

024681012

( w0χ mPS )2

w 0χ m PS2 mf

0 5 10 15

024681012

( w0χ mPS )2

w 0χ m PS2 mf

0 5 10 15

024681012

( w0χ mPS )2

w 0χ m PS2 mf

β=1.8 β=2.0 β=2.2 β=2.3

mPS2

mf =2B

"

1°aMx˜log m2ps

µ2 +bMx˜+±M a

w0¬ +Mmps2 a w0¬

# fPS =F

"

1°aFx˜log mPS2

µ2 +bFx˜ +±F a

w0¬ +FmPS2 a w0¬

#

w0¬B = 2.88(15)(17)

w0¬F = 0.078(4)(12) ß1/3/F = 4.19(26)

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Claudio Pica

Spin-1 Resonances

0 2 4 6 8

01234

( w0χ mPS )2

w 0χ mV

0 2 4 6 8

01234

( w0χ mPS )2

w 0χ mV

0 2 4 6 8

01234

( w0χ mPS )2

w 0χ mV

0 2 4 6 8

01234

( w0χ mPS )2

w 0χ mV

β=1.8 β=2.0 β=2.2 β=2.3

0 2 4 6 8

01234

( w0χ mPS )2

w 0χ mV

0 2 4 6 8

012345

( w0χ mPS )2

w 0χ mA

0 2 4 6 8

012345

( w0χ mPS )2

w 0χ mA

0 2 4 6 8

012345

( w0χ mPS )2

w 0χ mA

0 2 4 6 8

012345

( w0χ mPS )2

w 0χ mA

0 2 4 6 8

012345

( w0χ mPS )2

w 0χ mA

0 2 4 6 8

012345

( w0χ mPS )2

w 0χ mA

0 2 4 6 8

012345

( w0χ mPS )2

w 0χ mA

0 2 4 6 8

012345

( w0χ mPS )2

w 0χ mA

β=1.8 β=2.0 β=2.2 β=2.3

0 2 4 6 8

012345

( w0χ mPS )2

w 0χ mA

w0¬mX = w0¬m¬X + A(w0¬mPS)2+B(w0¬mPS)4+C a w0

mV / fPS = 13.1(2.2) mA/fPS = 14.5(3.6)

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Claudio Pica

Spin-0 Resonances

0 5 10 15

012345

( w0χ mPS )2

w 0χ mσ

0 5 10 15

012345

( w0χ mPS )2

w 0χ mσ

0 5 10 15

012345

( w0χ mPS )2

w 0χ mσ

0 5 10 15

012345

( w0χ mPS )2

w 0χ mσ

β=2.0 β=2.2

0 5 10 15

012345

( w0χ mPS )2

w 0χ mσ

0 5 10 15

0123456

( w0χ mPS )2

w 0χ ma0

0 5 10 15

0123456

( w0χ mPS )2

w 0χ ma0

0 5 10 15

0123456

( w0χ mPS )2

w 0χ ma0

0 5 10 15

0123456

( w0χ mPS )2

w 0χ ma0

0 5 10 15

0123456

( w0χ mPS )2

w 0χ ma0

0 5 10 15

0123456

( w0χ mPS )2

w 0χ ma0

0 5 10 15

0123456

( w0χ mPS )2

w 0χ ma0

0 5 10 15

0123456

( w0χ mPS )2

w 0χ ma0

β=1.8 β=2.0 β=2.2 β=2.3

0 5 10 15

0123456

( w0χ mPS )2

w 0χ ma0

w0¬mX = w0¬m¬X + A(w0¬mPS)2+B(w0¬mPS)4+C a w0

Preliminar y Preliminar y

ma0/fPS = 16.7(4.9) mæ/fPS = 19.2(10.8)

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Claudio Pica

Spin-0 Resonances

0 5 10 15

0123456

( w0χ mPS )2

w 0χ mη'

0 5 10 15

0123456

( w0χ mPS )2

w 0χ mη'

0 5 10 15

0123456

( w0χ mPS )2

w 0χ mη'

0 5 10 15

0123456

( w0χ mPS )2

w 0χ mη'

β=2.0 β=2.2

0 5 10 15

0123456

( w0χ mPS )2

w 0χ mη'

w0¬mX = w0¬m¬X + A(w0¬mPS)2+B(w0¬mPS)4+C a w0

Preliminar y

m¥0/fPS = 12.8(4.7)

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Claudio Pica

Resonances - Summary

0510152025

m XF PS

QCD Nf = 2

σ : 0(0+ ) η2 : 0(0- ) ρ : 1(1- ) a0 : 1(0+ ) a1 : 1(1+ )

0(0+ )

0(0- ) 1(1- )

1(0+ )

1(1+ )

SU(2) Nf = 2

Preliminar y

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Claudio Pica

Lattice simulations yield first principle results for the NP

dynamics and can provide trustable quantitative results on the spectrum are possible and available

Several interesting models are being investigated, which

include examples of strongly coupled models with light scalars

The study of scalar sector of strongly coupled model is challenging, but seems within reach

SU(2) model viable might be viable as composite goldstone Higgs model, but spin 1 and 0 resonances in the 30-50 TeV region for

Conclusions

Thank you!

sinµ ' 0.1

Figure

TABLE I: Fits to m and g ⇡⇡ extrapolated from the elastic ⇡⇡ scattering(see [35] for a summary of recent results)

Referencias

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