h125 & Natural Alignment
in the Z3 NMSSM
Nausheen R. Shah
University of Michigan
Aug 7, 2015
In Collaboration with:
M. Carena, H. Haber, I. Low & C. Wagner
arXiv:1508.xxxxx
Nausheen R. Shah -- DPF 2015
Higgs Discovery!
ATLAS + CMS: mh ~ 125 GeV
• What does the observed Higgs tell us about BSM physics?
• Implications for extended Higgs Sector?
• Higgs Couplings?
Aug 7, 2015
2
Nausheen R. Shah -- DPF 2015
Still large uncertainties in couplings…
Aug 7, 2015
CMS-PAS-HIG-14-009ATLAS-CONF-2014-009
but approximately consistent with SM.
3
Nausheen R. Shah -- DPF 2015
Projected Higgs Precision
Aug 7, 2015
4
Nausheen R. Shah -- DPF 2015
NATURAL ALIGNMENT IN THE Z3 NMSSM
Aug 7, 2015
5
Nausheen R. Shah -- DPF 2015
Z3 NMSSM
• 2 Doublets (Hu, Hd) + Singlet (S)
• Singlet couples only to the Higgs Sector.
• Singlet acquires vev: μ = λ vs
• 3 CP-Even Higgses:
• Mixing between all three (Hu, Hd and S).
• 2 CP-Odd Higgses:
• Mixtures of “MSSM” mA and singlet.
• Charged Higgs
• Singlet-like CP-even and odd masses anti-correlated.• Singlino mass: 2 κ μ/λ
Aug 7, 2015
6
Nausheen R. Shah -- FNAL LPC
• Interaction basis: (Hu, Hd, S)
• Hu: Couples only to up-type fermions
• Hd: Couples only to down-type fermions
• S: Only couples to Higgs
June 3, 2015
7
<Hu> = vu
<Hd> = vd
tβ = vu/vd
<S> =μ/λ
CP-Even Higgs Bases
Nausheen R. Shah -- FNAL LPC
• Interaction basis: (Hu, Hd, S)
• Hu: Couples only to up-type fermions
• Hd: Couples only to down-type fermions
• S: Only couples to Higgs
• “Extended” Higgs basis: (HNSM, HSM, S)
• HNSM: (down, up, V) = (yd tβ, yu/ tβ, 0)
• HSM: (down, up, V) = (yd, yu, ghVV)
June 3, 2015 7
<Hu> = vu
<Hd> = vd
tβ = vu/vd
<S> =μ/λ
<HNSM> = 0<HSM> = v
CP-Even Higgs Bases
Nausheen R. Shah -- FNAL LPC
• Interaction basis: (Hu, Hd, S)
• Hu: Couples only to up-type fermions
• Hd: Couples only to down-type fermions
• S: Only couples to Higgs
• “Extended” Higgs basis: (HNSM, HSM, S)
• HNSM: (down, up, V) = (yd tβ, yu/ tβ, 0)
• HSM: (down, up, V) = (yd, yu, ghVV)
• Mass basis: (H3, H2, H1)
• Hi = κiNSM HNSM + κi
SM HSM + κiS S
June 3, 2015
7
<Hu> = vu
<Hd> = vd
tβ = vu/vd
<S> =μ/λ
<HNSM> = 0<HSM> = v
CP-Even Higgs Bases
Nausheen R. Shah -- FNAL LPC
• Interaction basis: (Hu, Hd, S)
• Hu: Couples only to up-type fermions
• Hd: Couples only to down-type fermions
• S: Only couples to Higgs
• “Extended” Higgs basis: (HNSM, HSM, S)
• HNSM: (down, up, V) = (yd tβ, yu/ tβ, 0)
• HSM: (down, up, V) = (yd, yu, ghVV)
• Mass basis: (H3, H2, H1) (H, h125, hS)
• Hi = κiNSM HNSM + κi
SM HSM + κiS S
June 3, 2015
7
<Hu> = vu
<Hd> = vd
tβ = vu/vd
<S> =μ/λ
<HNSM> = 0<HSM> = v
CP-Even Higgs Bases
Nausheen R. Shah -- DPF 2015
“Extended” Higgs Basis
• Tree-level mass matrix in the (HNSM, HSM, S) basis:
Aug 7, 2015
8
• Alignment: Mixing between HNSM-SM=0 & SM-S =0 • Alignment conditions, (+ stop corrections to always obtain h125):
NSM-SM mixing cancels for
Nausheen R. Shah -- DPF 2015125 GeV Higgs Naturally!
Well Known• 125 GeV Higgs• Tree-level contribution to
Higgs mass from λ.• λ ~ 0.65-0.7
• Low tan β• Light Stops
Aug 7, 2015
9
M. Carena, H. Haber, I. Low, N.R.S., C. Wagner, ’15 (preliminary)
Alignment (No-Mixing):
Nausheen R. Shah -- DPF 2015
SM-Like Higgs Naturally!
• Perturbative up to GUT scale.• λmax ~ 0.7, κmax ~ λ/2
Not so well known:• Leads to excellent Alignment
(very little mixing with Heavy Higgs) in the mA- tan β plane.
Aug 7, 2015
10
M. Carena, I. Low, N.R.S, C. Wagner, ‘13
M. Carena, H. Haber, I. Low, N.R.S., C. Wagner, ’15(preliminary)
Nausheen R. Shah -- DPF 2015 Aug 7, 2015
11
Singlet Alignment
h125 ~ HSM
LIGHT SPECTRUMSinglino: 2 κ μ/λ ~ < μ
CP-even/odd singlet massesanti-correlated
Nausheen R. Shah -- DPF 2015
Misalignment
• NMSSMTools + HiggsBounds/Signals• Allowed “misalignment”
Aug 7, 2015
12
. tan β =2
. tan β =2.5
. tan β =3
__
M. Carena, H. Haber, I. Low, N.R.S., C. Wagner, ’15(preliminary)
Nausheen R. Shah -- DPF 2015
Singlet Spectra
Density of scan not relevant
Aug 7, 2015
13
. tan β =2 . tan β =2.5 . tan β =3M. Carena, H. Haber, I. Low, N.R.S., C. Wagner, ’15
(preliminary)
singlet always less than mH/2
Nausheen R. Shah -- DPF 2015
MSSM-like A and H decays into tt
• Decay BR depends on tan β
Aug 7, 2015
14
. tan β =2 . tan β =2.5 . tan β =3
M. Carena, H. Haber, I. Low, N.R.S., C. Wagner, ’15(preliminary)
MSSM-like mH MSSM-like mA
Nausheen R. Shah -- DPF 2015
MSSM-like H BR
• Apart from tt, significant decays into H2+H1 and neutralino/charginos
Aug 7, 2015
15
M. Carena, H. Haber, I. Low, N.R.S., C. Wagner, ’15(preliminary)
Coupling to h125 pair suppressed
due to alignment.
. tan β =2 . tan β =2.5 . tan β =3
Nausheen R. Shah -- DPF 2015
MSSM-like A BR
• Into singlet-like H1/H2-Z and inos
Aug 7, 2015
16
M. Carena, H. Haber, I. Low, N.R.S., C. Wagner, ’15(preliminary)
h125 decay suppresseddue to alignment
. tan β =2
. tan β =2.5
. tan β =3
Nausheen R. Shah -- DPF 2015
Singlet-like HS BR
• Singlet mainly decays to bb and WW
Aug 7, 2015
17
M. Carena, H. Haber, I. Low, N.R.S., C. Wagner, ’15(preliminary)
h125 h125
Nausheen R. Shah -- DPF 2015
Now & FutureAug 7, 2015
18
XS factor ~ 4 at 14 TeV compared to 8 TeV M. Carena, H. Haber, I. Low, N.R.S., C. Wagner, ’15(preliminary)
CMS PAS HIG-15-001
CMS 1505.03831 HVV/SM ~10%8 TeV
Nausheen R. Shah -- DPF 2015
Now & FutureAug 7, 2015
19
XS factor ~ 4 at 14 TeV compared to 8 TeV M. Carena, H. Haber, I. Low, N.R.S., C. Wagner, ’15(preliminary)
CMS PAS HIG-15-001
CMS 1505.03831 HVV/SM ~10%8 TeV
Nausheen R. Shah -- DPF 2015
Conclusions and Outlook
• Z3 NMSSM Higgs sector at low tan β.
• Naturally obtain 125 GeV Higgs (light stops).
• Leads to alignment with the non-SM like Higgs.
• Perturbativity and the requirement of alignment with the singlet
• naturally light singlets (both CP-even and odd) and singlino + higgsinos (charged and neutral).
• Due to large BR of non-SM Higgs into singlet like states + inos, very interesting LHC phenomenology.
Aug 7, 2015
20
Nausheen R. Shah -- DPF 2015
BACKUP SLIDES
24Aug 7, 2015
Nausheen R. Shah -- DPF 2015
ALIGNMENTSM-Like Higgs in 2HDM
Aug 7, 2015
25
CP-Even: H1, H2
CP-Odd: ACharged Higgs: H+-
Nausheen R. Shah -- DPF 2015
Higgs Basis
• HSM has completely SM-like couplings.
• Mixing between HSM and HNSM ,“cos (β-α)”, gives non-SM behavior of observed h125.
Aug 7, 2015
26
If sin α = - cos βor equivalentlycos (β-α) = 0
SM-like HIGGS!!
ALIGNMENT
Nausheen R. Shah -- FNAL LPC
Contamination allowed in h125 ??
• How much “non-standardness” is allowed by h125 measurements??
• κNSM HNSM + κSM HSM + κS S
• Singlet: Only couples to Higgs
• Ratios to SM:
• ghgg= (κSM + κNSM/tβ)
• ghdd = (κSM - κNSM tβ)
• ghVV = κSM
• Significant κS OK
• Large κNSM from sign change of ghdd
June 3, 2015
27
h125
Nausheen R. Shah -- FNAL LPC
Heavy H to VV ?
• CMS 1505.03831
June 3, 2015
28
Nausheen R. Shah -- FNAL LPC
Direct Searches for heavy resonances?
• Strong constraints on SM-like Higgs decay to VV ~12-6% SM value for masses 160-500 GeV.
• What does this imply for SM and NSM components of extra Higgs??• 160 GeV < mhS < 350 GeV
• BR(WW+ZZ) ~1• gF production XS impacted.
• With κh125NSM ~ 0
• κhSSM ~ κh125
S
• κh125S smaller than allowed by h125
measurements!
June 3, 2015
29
~ κh125S
Nausheen R. Shah -- DPF 2015
Higgsinos/Singlinos
• Interesting relationship between masses of Heavy Higgs and the higgsinos and singlinos.
• The Singlino mass is given by 2 κ vs which in terms of μ, (μ = λ vs) is 2 κ μ/λ
• Since κ ~ < λ/2, (perturbative upto GUT scale)• Singlino mass ~ < Higgsino mass• Can be much lighter.
• In our region of interest only first term dominant.
Aug 7, 2015
30
Aug 7, 2015 Nausheen R. Shah -- DPF 2015 31
Nausheen R. Shah -- DPF 2015 Aug 7, 2015
32
Nausheen R. Shah -- DPF 2015 Aug 7, 2015
33
Nausheen R. Shah -- DPF 2015 Aug 7, 2015
34
M. Carena, I. Low, N.R.S, C. Wagner, ‘13
Nausheen R. Shah -- DPF 2015
CP-Odd Mass Matrix
• In the (“MSSM mA”, Singlet) basis:
Aug 7, 2015
35
Nausheen R. Shah -- DPF 2015
MisalignmentAug 7, 2015
36
. tan β =2 . tan β =2.5 . tan β =3
__
Nausheen R. Shah -- DPF 2015
Fine-Tuning (No-mixing in stops)
• Larger tan β => Heavier Stops => Larger Fine Tuning
Aug 7, 2015
37
Nausheen R. Shah -- DPF 2015
Higgs Spectra
• CP-even vs. Odd
Aug 7, 2015
38
Nausheen R. Shah -- DPF 2015
H3 BR
• H1 H1 /H2 H2
Aug 7, 2015
39
Nausheen R. Shah -- DPF 2015
BR H3
• tt + a Z
Aug 7, 2015
40
Nausheen R. Shah -- DPF 2015
A2 BR
• A1 H1 / A1 H2
Aug 7, 2015
41
Nausheen R. Shah -- DPF 2015
A2 BR
• tt + chargino/neutralinos
Aug 7, 2015
42
Nausheen R. Shah -- DPF 2015
RGEAug 7, 2015
43
Nausheen R. Shah -- DPF 2015
Phenomenological Consequences
1. The gluon fusion production cross section of the would be heavy MSSM states (A and H) is enhanced due to the top Yukawa contributions at low tan β, and can be of the order of a few pb.
2. The non-standard Higgs bosons may have relevant decays into the lighter singlet like Higgs bosons as well as into the light electroweakinos.
3. The decay of non-standard Higgs bosons into taus and bottoms will be suppressed due to the small values of tan β and the presence of additional decays.
Aug 7, 2015
44
Top Related