39
Higgs Physics Shaouly Bar-Shalom 1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel ([email protected] .il) EFT-Naturalness: an effective field theory analysis of Higgs naturalness EPS-HEP2015, Vienna, July 22-29

Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel ([email protected])

Embed Size (px)

Citation preview

Page 1: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom1

arXiv/1405.2924 [PRD 2015]

SBS (Technion), A. Soni (BNL) & J. Wudka (UCR)

Shaouly Bar-ShalomTechnion, Israel

([email protected])

EFT-Naturalness: an effective field theory analysis

of Higgs naturalness EPS-HEP2015, Vienna, July 22-29

Page 2: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom2

outline

• Naturalness …

• “EFT naturalness”: a complete parameterization of all higher dimensional effective operators (@ any dim.!) that can potentially “soften” the 2 behavior of mh

2 look for naturalness conditions in the heavy underlying theory

• Constraints, signals of EFT naturalness & concluding remarks

Page 3: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom3

NaturalnessThe “master equation”:

t

driving force behind search for NP

Page 4: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom4

NaturalnessThe “master equation”:

t

driving force behind search for NP

The hierarchy/naturalness problem:

GeVSMmtreemmassphysicalm hhh 126)()()( 222 GeVSMmtreemmassphysicalm hhh 126)()()( 222 GeVSMmtreemmassphysicalm hhh 126)()()( 222 GeVSMmtreemmassphysicalm hhh 126)()()( 222 GeVSMmtreemmassphysicalm hhh 126)()()( 222 GeVSMmtreemmassphysicalm hhh 126)()()( 222

Page 5: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

New Physics

Shaouly Bar-Shalom5

NP particle masses are lighter than

SM is not a complete description of the heavy physics below ; there being other particles yet to be discovered

with masses below

The parameters of the theory are such that there are cancellations between the SM and NP contributions to mh (symmetries/accidental) … e.g., SUSY, little Higgs/composite models …

All NP particle masses are heavier than

= the scale of the effective action

use EFT techniques

Higgs Physics

Page 6: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom6

Underlying setup:

E

new heavy physics

SM +

(SM fields and symmetries …)

Below M:

M ~ O(10 TeV)

Page 7: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom7

Underlying setup:

E

new heavy physics

SM +

(SM fields and symmetries …)

EFT naturalness: conditions among fi for theory to be natural at < M

= the scale of the effective action (Wilsonian-like)

Below M:

M ~ O(10 TeV)

Page 8: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom8

Ask: what are the “EFT naturalness” conditions?

the conditions for the physics above that can soften naturalness in the Higgs sector

The EFT-naturalness conditions are most likely due to a higher symmetry of the underlying physics …

EFT Naturalness :

Page 9: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom9

The “roadmap” to EFT naturalness: a taste of the problem …

Page 10: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom10

The “roadmap” to EFT naturalness: a taste of the problem …

2.816

)(22

2

2

2

eff

hh

h

h Fmm

m

10%

1%

naturalA theory, F(eff), for which h~1 is natural

while one with

h~10(100) suffers from fine-tuning of

10%(1%)

Page 11: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom11

Integrating out the heavy fields (M); generates an infinite series of vertices suppressed by inverse powers of (< M)

The EFT 1-loopv contribution to the Higgs mass:

Page 12: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom12

Integrating out the heavy fields (M); generates an infinite series of vertices suppressed by inverse powers of (< M)

EFT naturalness: what eff. interactions can tame the little hierarchy problem?

The EFT contribution to the Higgs mass:

Page 13: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom13

We need the set of operators which give

the leading contribution to

To Calculate

Page 14: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom14

EFT:

Its a mess in general – underlying physics not known, too many operators …

needs some guiding principles !

set the “rules of the game” …

Page 15: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom15

EFT framework:

“light fields” [@ E M] = SM fields

Gauge-symmetry [@ E M] = SM: SU(3)xSU(2)xU(1) (useful for classifying the higher dim operators)

Underlying NP (heavy) is weakly coupled, renormalizable, obeys gauge-invariance & preserves symmetries of the known dynamics (SM) (useful for classifying the higher dim operators)

Assume: physics at E M is described by

Page 16: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom16

“light fields” [@ E M] = SM fields

Gauge-symmetry [@ E M] = SM: SU(3)xSU(2)xU(1) (useful for classifying the higher dim operators)

Underlying NP (heavy) is weakly coupled, renormalizable, obeys gauge-invariance & preserves symmetries of the known dynamics (SM) (useful for classifying the higher dim operators)

Many operators can be constructed under these conditions, O(50)BUT: only very few can balance the SM’s 1-loop quadratic terms !

Assume: physics at E M is described by

EFT framework:

Page 17: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom17

EFT corrections to Higgs mass

Page 18: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom18

EFT corrections to Higgs mass

From heavy scalar exchanges: singlets or triplets

From heavy vector exchanges: singlets or triplets

From heavy fermion exchanges: singlets, doublets or triplets

Page 19: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom19

EFT corrections to Higgs mass

Page 20: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom20

EFT corrections to Higgs mass

Page 21: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom21

EFT naturalness upshot:

),,( Mff ihh ),,1( Mff inatural

2.816

)(22

2

2

2

eff

hh

h

h Fmm

m

Provides the necessary conditions in the underlying theory(i.e., in terms of the coefficients of the higher dim. operators)

for the theory to be natural (or to have a certain degree of fine-tuning)

Page 22: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom22

Less ignorance

More insight regarding the heavy new physics for naturalness

explicitly calculating the higher-dim coefficients…

Page 23: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom23

Less ignorance: examples of interactions of the new heavy particles that can address naturalness

heavy fermions = singlets, doublets & triplets:

heavy scalars = singlets & triplets:

heavy vectors X = singlets & triplets:

Page 24: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom24

Less ignorance: examples of interactions of the new heavy particles that can address naturalness

Integrate out heavy fields (,X,) & allowing for the more general case of different scales

heavy fermions = singlets, doublets & triplets:

heavy scalars = singlets & triplets:

heavy vectors X = singlets & triplets:

Page 25: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom25

Matching the effective theory @

Page 26: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom26 F(eff) > 0 !

Matching the effective theory @

Page 27: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom27

Assume that the heavy masses are clustered around a value M:

expected values:

e.g., u ~ 3M and/or a triplet heavy vector-like (colored) quark with y ~ 1

EFT naturalness conditions – a simple example:

Page 28: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom28

EFT naturalness conditions – a simple example:

find the values of () for which EFT corrections to mh can “soften” naturalness in the Higgs sector at a certain for some value of M of the NP threshold …

Page 29: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom29

Regions in the plane which corresponds to h=1 (natural) and h=10 (10% fine-tuning) for an EFT-naturalness scale 3 < < 10 TeV & < M <

3

find the values of () for which EFT corrections to mh can “soften” naturalness in the Higgs sector at a certain for some value of M of the NP threshold …

EFT naturalness conditions – a simple example:

Page 30: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom30

Regions in the plane which corresponds to h=1 (natural) and h=10 (10% fine-tuning) for an EFT-naturalness scale 3 < < 10 TeV & < M <

3

Example: extensions of the SM with a typical mass scale of M ~ 7 TeV and with ~ 9 & ~ 5

will yield an effective action which is natural up to ~ 5 TeV (an order of magnitude improvement over the pure SM …)

EFT naturalness conditions – a simple example:

Page 31: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom31

EFT naturalness operators can cause 2 types of effects:

• A shift to the -parameter

• A shift of the Higgs couplings to SM fermions & gauge-bosons

M(scalar triplet,vectors) > ~ 10 TeV

no useful limit…

Constraints from current data

Page 32: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom32

Expected signals of EFT-Naturalness

Modified vertices involving Higgs, gauge-bosons and fermions from the EFT-naturalness higher-dim operators

Tail of new physics responsible for EFT-naturalness can be searched for in multi-boson associated production of the form:

VV nh+m V+X (n,m=0,1,2, …)

e.g., pp Wh+X, Zh+X

Page 33: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom33

Summary• There is a UV completion to the SM which is natural up to some scale !

• What do we know about the underlying NP?

Page 34: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom34

Summary• There is a UV completion to the SM which is natural up to some scale !

• What do we know about the underlying NP?

• Our EFT-naturalness analysis:

• provides insight about this theory: relations among parameters of the UV theory (for naturalness)

• signals expected in multi-boson scattering processes, e.g., pp Wh+X, Zh+X

Page 35: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom35

Summary• There is a UV completion to the SM which is natural up to some scale !

• What do we know about the underlying NP?

• Our EFT-naturalness analysis:

• provides insight about this theory: relations among parameters of the UV theory (for naturalness)

• signals expected in multi-boson scattering processes, e.g., pp Wh+X, Zh+X

• Naturalness in the UV is not that complicated: need new singlet(s) or triplet(s) bosons or else singlet, doublet or triplet fermion(s)

Page 36: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom36

THANK YOU!

Page 37: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom37

backups

Page 38: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom38

vectors loopscalars loop

fermions loop

Loop calculations

Page 39: Higgs PhysicsShaouly Bar-Shalom1 arXiv/1405.2924 [PRD 2015] SBS (Technion), A. Soni (BNL) & J. Wudka (UCR) Shaouly Bar-Shalom Technion, Israel (shaouly@physics.technion.ac.il)

Higgs PhysicsShaouly Bar-Shalom44

Signals of potential heavy natural NP

• Higgs+jet/lepton production via off-shell heavy fermion ``decay”

• * h ( = quark or lepton)

• deviations in Higgs pair production

• VV hh (s-channel exchange of heavy bosons)

• qq,ee hh (t-channel exchange of heavy fermions)

V

V

2D