physics 222 ucsd/225b ucsb lecture 15 • extending the

29
Physics 222 UCSD/225b UCSB Lecture 15 • Extending the Higgs Sector => 2 Higgs Doublet Models (2HDM). • I am using the following for today’s lecture: – “Higgs Hunter’s guide” (1990) – TASI 06 lectures by Rainwater

Upload: others

Post on 26-Apr-2022

0 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

Physics 222 UCSD/225b UCSB

Lecture 15

• Extending the Higgs Sector => 2 Higgs Doublet Models (2HDM).• I am using the following for today’s lecture:

– “Higgs Hunter’s guide” (1990)– TASI 06 lectures by Rainwater

Page 2: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

Logic of Today’s Lecture• Reminder of single higgs doublet, i.e. Minimal

Standard Model (SM or MSM).• Overview of constraints for extending the

higgs sector.• Focus on 2 higgs doublet models

– 4 types => discuss 2 of them• Focus on 2HDM type 2, as implemented in

Minimal Supersymmetric Standard Model(MSSM).

Page 3: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

Higgs Field in SM• Standard Model assumes the simplest choice

for the higgs field:– a complex doublet with Y = 1.

• Complex for U(1)• Doublet for SU(2)• Y=1 to make quatum numbers come out right.

!+

! 0"

#$%

&'=

!1+ i!

2

!3+ i!

4

"#$

%&'1

2

The superscript indicate the charge according to:Q = T3 + Y/2

Page 4: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

Higgs Ground State in SM• This particular choice of multiplets is exactly what we

need because it allows us to break both SU(2) andU(1)Y , while at the same time allowing us to choosea ground state that leaves U(1)em unbroken.

• The latter is accomplished by choosing a groundstate that leaves φ+ = 0.

• Use the same higgs field to give mass to fermionsand bosons.

!+

! 0"

#$%

&'=0

v

"#$

%&'1

2

Page 5: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

Extended Higgs Fields• There are in principle many choices one could

make.• The only constraint is that the higgs fields

belongs to some multiplet of SU(2) x U(1).• And unitarity should not be violated at large s.• Apart from that, there are experimental

constraints, the most stringent of which are:

• FCNC are heavily suppressed in nature.

! =M

W

2

MZ

2cos

2"W

# 1

Page 6: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

Comments on ρ=1• Halzen & Martin Exercise 15.4 explores this

further.• Additional discussion can be found in “Higgs

Hunter’s Guide” chapter 4, and referencestherein.

• Bottom line:– There are many ways to satisfy this constraints.– In particular, any model with arbitrary number of

higgs doublets and higgs singlets will satisfy theconstraint.

Page 7: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

Comments on FCNC• Flavor changing neutral currents in quark

sector are heavily suppressed in the SM,proceeding only via “penguin” loops, and other2nd order weak transitions.

• Glashow & Weinberg showed that tree-levelFCNC are forbidden IFF all fermions of agiven electric charge couple one-to-one tohiggs doublets. (see references for details)

=> Multi-higgs doublet models are thus ok aslong as they obey this rule.

Page 8: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

Two higgs Doublet Models• Has been studied theoretically, as well as

limited experimentally, in great detail because:– It’s a minimal extension of the SM higgs sector.– It satisfies both experimental constraints we

mentioned.– It adds new phenomenology by predicting a

charged higgs particle.– It is required in the MSSM, as well as “low energy”

SUSY models in general.

Page 9: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

General 2HDM Potential

!+

! 0"

#$%

&'1

=0

v1

"#$

%&'1

2

!+

! 0"

#$%

&'2

=0

v2ei(

"#$

%&'1

2; tan! =

v2

v1

;

V (!1,!2 ) = "1 !12# v1

2( )2

+ "2 !22# v2

2( )2

+ "3 !12# v1

2( ) + !22# v2

2( )$%

&'

2

+ "4 !12!2

2# !1

*T!2( ) !2*T!1( )$

%&'

+ "5 Re !1*T!2( ) # v1v2 cos($% &'

2

+ "6 Im !1*T!2( ) # v1v2 sin($% &'

2

All λ are real.

From “Higgs Hunter’s guide”.

Page 10: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

A slightly less opaque notation:

I will stick with Higgs Hunter’s guide notation as that’s my primary reference.

Page 11: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

CP violation• In principle, we have the freedom to choose

the two vevs to have an arbitrary phase withregard to each other.

• If on top, λ5 ≠ λ6 then we have CP violation inthe higgs sector.

• In the interest of time, we’re going to ignorethis. See Higgs Hunter’s guide for details.

!+

! 0"

#$%

&'1

=0

v1

"#$

%&'1

2

!+

! 0"

#$%

&'2

=0

v2ei(

"#$

%&'1

2

Page 12: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

Vevs, GF, and mW

• For Standard Model (H&M Exercise 15.2)

• For 2HDM this stays the same, except for:

mW =1

2gv

GF =2

v2

(v1

2+ v

2

2) ! v

2" 246GeV

Page 13: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

Higgs Boson Spectroscopy• One Charged Higgs with mass:

• One CP-odd neutral Higgs with mass:

• And two CP-even higgs that mix.

mH

± = !4(v1

2+ v

2

2)

mA0 = !

6(v1

2+ v

2

2)

M =4v

1

2 !1+ !

3( ) + v22!

54!

3+ !

5( )v1v24!

3+ !

5( )v1v2 4v2

2 !2+ !

3( ) + v12!

5

"

#$%

&'

Page 14: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

Free Parameters in 2HDM

• Four higgs masses• The ratio of vevs:

• and a higgs mixing angle, α, for the neutralCP-even higgs states to mix.

tan! =v2

v1

Page 15: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

Some guiding principles• Charged higgs mass can be very large, to limit loop

contributions to precision data. (Replace a W+ with aH+ wherever you want.)

• A0, CP-odd higgs, doesn’t couple to the Gaugebosons, i.e. no A0WW nor A0ZZ coupling. It’s masscan also be very large.

• Of the remaining neutral CP-even h,H, one must bereasonably low mass to meet the mh constraints fromindirect measurements.

mH ,h

2=1

2M

11+ M

22± (M

11! M

22)2+ 4M

12

2"#

$%

Page 16: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

mH ,h

2=1

2M

11+ M

22± (M

11! M

22)2+ 4M

12

2"#

$%

If M11 >> M22 and M11 >> M12 , then:

mH2 = M11 mh

2 = M22 / 2

M =4v

1

2 !1+ !

3( ) + v22!

54!

3+ !

5( )v1v24!

3+ !

5( )v1v2 4v2

2 !2+ !

3( ) + v12!

5

"

#$%

&'

>>

This is easy to arrange via appropriate choice of λi and without restricting the choice of tanβ = v2 / v1

Page 17: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

Categorizing 2HDM

Options III and IV lead to FCNC and are thus not studied any more in any significant way.

Option I leads to “fermiphobic” higgs, i.e. higgs that only couples to gauge bosons.

MSSM is a special case of Option II.

Page 18: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

Comparing Type I & II

Type I

Type II

Up and down fermions couple the same way in type I models.We can thus eliminate fermion coupling to mh entirely whileat the same time keeping boson coupling maximal. => cos α = 0 while sin(β- α)=1.

Page 19: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

Type-I: Fermiphobic Higgs• Example higgs to di-photon decay:

This is not allowed.

Leave it to you as an exercise to think through what happensto the rest of higgs phenomenology in fermiphobic models.

Page 20: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

Comparing Type I & II

Type I

Type II

Up and down fermions couple differently in type II models.We can thus eliminate down quark coupling to mh entirely whileat the same time keeping boson coupling maximal. => sin α = 0 while sin(β- α)=1.

Page 21: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

BR’s for low mass mh , i.e. below WW threshold. Partial width to bb and tautau are turned off as promised.

mh~110GeV has 50% BR to WW

Page 22: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

SMNo down-quark couplings

Page 23: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

Higgs in MSSM• MSSM is basically a type II 2HDM, but with a

variety of constraints among the parametersdefining the model.

• The details of these are well beyond the scopeof this lecture.

• Instead, we will simply be descriptive, andfocus on the few statements that can be madesimply.

• As reference, we use the TASI06 lectures byRainwater.

Page 24: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

MSSM Higgs• Assuming no CP violation, it is convenient to

look at the masses of the other 3 higgs statesas a function of mA , the mass of the CP-oddhiggs.

• At tree level:

This would imply that mh < mZ for large mA , which is of course already ruled out by experiment.

Loop corrections proportional to mt2 increase mh somewhat.

Page 25: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

The details depend on mixing in the stop sector, and v2 / v1

mh < 140GeV in all cases, and getting close to the limitrequires large v2 / v1 or large masses for all other higgs.

Page 26: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

Conclusions from 2HDM• All the existing standard model constraints can

be met.• There are 3 additional higgs bosons, that all

three of them can be so high in mass that wewon’t find them easily.

• At the same time, both the production anddecay properties of the light higgs can bealtered such as to affect the higgs huntingsignificantly.

Page 27: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

Aside or backup

Page 28: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

SM & WW scattering

Without the higgs, we get M ∝ s / mW2 for large s.

This violates unitarity, as previously discussed.(see H&M 15.6 and homework)

In SM, higgs, and the hWW vertex of a igmw resolve that.(see H&M Exercise 15.5)

Page 29: Physics 222 UCSD/225b UCSB Lecture 15 • Extending the

2HDM & WW scattering

The same cancellation is still satisfied if: (v1

2+ v

2

2) ! v

2

GF now relates to the sum of the squares of the vevs.As a result, the total cross section for higgs associate production is easy to suppress, but difficult to enhance.