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Probing the scalar sector with ZZH. Debajyoti Choudhury, Anindya Datta, Katri Huitu, hep-ph/0302141, to appear in Nucl.Phys.B. outline: Introduction Models: higher representations radion (nonSUSY/SUSY) Conclusions. Introduction. Assume that EWSB due to Higgs mechanism - PowerPoint PPT Presentation
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Oct, 2003 WIN'03, Katri Huitu 1
Probing the scalar sector with ZZH
outline:IntroductionModels:
higher representationsradion (nonSUSY/SUSY)
Conclusions
Debajyoti Choudhury, Anindya Datta, Katri Huitu,
hep-ph/0302141, to appear in Nucl.Phys.B
Oct, 2003 WIN'03, Katri Huitu 2
Introduction • Assume that EWSB due to Higgs mechanism• Light scalars not taking part in the EWSB can
mix with Higgs• In extensions of the Standard Model new scalars
and new representations- spontaneous CP violation, - supersymmetry, - left-right model, - gauge unification,...
• What can a detected set of scalars tell about the model?
• Related works: Burgess et al, IJMP A17(2002) 1841; Ellis et al, PLB 502 (2001) 171; Kane et al PRD 64 (2001) 095013; Ambrosanio et al NPB 624 (2002) 3.
Oct, 2003 WIN'03, Katri Huitu 3
ZZH coupling
• gets contribution from any nonsinglet VEV
• ZZH coupling essential in Higgs production: or gauge boson fusion use to separate between models
02
322 )'( ii
iiZZH HvTZZggL
ZHZff
Lagrangian:
Oct, 2003 WIN'03, Katri Huitu 4
E.g. SU(5) GUT The SM fermions in , 105 and
151055504551010455105 , ,
15455 , , contain neutral scalars
doublets
Y=1 tripletbreaking symmetry SU(5) for need 24
in minimal SU(5) problems with realistic spectrum need more representations
... ...,' ..., 35454570151524455
These contain singlets, triplets (Y=0,1), 4-plets (Y=3/2,1/2), 5-plets (Y=2,1,0)
Oct, 2003 WIN'03, Katri Huitu 5
A strong constraint from the -parameter,
i ii
i iiiii
WZ
W
vT
vTTTr
m
m22
3
223
22
2
2
])1([
cos
experimentally 1. We demand = 1.
i ii
i ii
jj vT
vTcC
223
2432 4
4 max (T3i2 ) C 4 min
(T3i2 )
C 1 BSM Physics
Parametrize the ZZH coupling:
ZZH
gmcL i
W
ZiZZH i
0
cos
Oct, 2003 WIN'03, Katri Huitu 6
fermions of the SM couple to doubletsYt increases with decreasing v1/2:
,2/1v
vyy SMSM
ff
Yt RGE:
42123
2
8
9)
12
17
4
98(
ln2
tt
t
yy
d
dy
223
222 )'( ii iZ vTggm Z mass:
Oct, 2003 WIN'03, Katri Huitu 7
Triplets Added
fine tuning
Triplets (3,0) and (3,1)
1 < C < 4
20
21
21
20
21
12
)02(21
)12(
YY
Y
YY
vv
v
vv
Georgi, Machachek,NPB 262 (1985) 463.
Oct, 2003 WIN'03, Katri Huitu 8
SMff
ffffSMSMff
ffff
v
v
expexp2
2/1
expexp
E.g. in the Georgi – Machachek model, for the fermion widths
ffSMSM
ffGM vv 2
2/1 )/(
Use the measured value and error to constrain the ratio of VEVs
For a 90 % C.L. constraint on the ratio, is 1.64, if exp has 1 limits.
Oct, 2003 WIN'03, Katri Huitu 9
Fiveplets added
(5,0) and (5,1) enhance (5,2) suppresses
(5,0) and (5,2):1 < C < 16
(5,0) and (5,1):1 < C < 12
Oct, 2003 WIN'03, Katri Huitu 10
Radions in RS scenario
5-dim universe, compactify on S1 / Z2
hidden visible
y=0 y=
22||22 dyrdxdxeds cykrc
massless fields: gravitong
rc modulus T(x)
T(x) has zero potential stabilize,
parameters on visible brane scaled by e-krc ,
radion e-k(T-rc), m O(1 TeV)
Randall, Sundrum, PRL 83 (1999) 3370, 4690.
Goldberger, Wise, PRL 83 (1999)4922, PLB475 (2000)275.
Oct, 2003 WIN'03, Katri Huitu 11
Radion couplings:
Stress energy tensor:
)(int SMTL
...)2(2
)(
2)(
22
22
HHHmFFg
g
ZZmWWmffmSMT
haa
a a
aa
ZWf
f
Curvature-Higgs mixing
Giudice, Rattazzi, Wells, NPB 595 (2001) 250;Csaki, Graesser, Kribs, PRD 63 (2001) 065002.
/ ,
, 6
2
1 61
2
1 222
v vH
Hv
HmHmL h
HHgRgxdS visvis )(4 mixing
parameter
Oct, 2003 WIN'03, Katri Huitu 12
Diagonalize
22222
222
36
122tan 6161
,sin6coscos6sin
sincos
mZm
mZZ
ZZM
Rh
hRR
RR
and
,1''
HMRZH
positivity of kinetic terms: ,1/41
12
1/411
12
1 22
6.67.6 :TeV 10
59.075.0 :TeV 1
/
,
v
vH
Oct, 2003 WIN'03, Katri Huitu 13
22
22
21112
1222 611 RZ
MMMMC
Couplings to physical scalars (V=general gauge boson):
' ' 21111222
2
MMHMMVV
v
mL V
Oct, 2003 WIN'03, Katri Huitu 14
unitarity bounds
Han,Kribs,McElrath,PRD 64 (2001)076003
constant C curves
Oct, 2003 WIN'03, Katri Huitu 15
Supersymmetric RS model
We consider
J.A. Casas, J.R. Espinosa, I. Navarro, NPB 620 (2002) 195
Supplement MSSM with a radion T and
dilaton S in the bulk (susy breaking along FS):
To make contact with the superstring theory, the RS model may need to be supersymmetrized.
Extra dimensions may be connected with the supersymmetry breaking method:
Stabilization e.g. AMSB possible.Luty, Sundrum, PRD 62 (2000) 035008
Oct, 2003 WIN'03, Katri Huitu 16
/ ;3 2
2†
tTTM
eP
TT
Lagrangianjiij DDGL
2
1
,2
ji
effij
KG
2
2 *exp ieff
eff
ttK
..|| 212 chHH
i iieff
The warp factor
ZZHvHvgv
LW
HZZ022
0112
2
2
2
cos44311
note: K is model dependent
Oct, 2003 WIN'03, Katri Huitu 17
2Z
tZZ
mZtZL
22
21
2
2/1
2
2
,4
311cos2
vvvvgv
mW
Z
2
2
2
2
22
2
2
3111622
11
8
5
2
11
21
vvvC
Diagonalize H10,H2
0,t sum of the squares of scalar couplings (normalized to SM value):
Coupling to the singlet radion from the trace of stress-energy tensor:
Oct, 2003 WIN'03, Katri Huitu 18
Oct, 2003 WIN'03, Katri Huitu 19
Conclusions
• Sum of the ZZH couplings can be an efficient separator between models
• For scalars in higher representations of SU(2)L, the parameter and perturbativity of the top Yukawa-coupling constrain C
• In higher dimensions, the Higgs-curvature mixing may effect C strongly