Bohdan Grzadkowski University of Warsaw - fuw.edu.plbohdang/Geilo_2014_Grzadkowski.pdf · TYPE II...

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Extending 2HDM by a singlet scalar field - the case for dark matter - Bohdan Grzadkowski University of Warsaw ”From Higgs to Dark Matter 2014”, Geilo, December 15th 2014 Bohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matte

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Extending 2HDM by a singlet scalar field- the case for dark matter -

Bohdan GrzadkowskiUniversity of Warsaw

”From Higgs to Dark Matter 2014”, Geilo, December 15th 2014

Bohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matter -

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Outline:2HDMS ModelMotivationsStrategyResulting Constraints on the parameter spaceDirect DM detection constraintsNew Higgs physics at the LHC?Summary

A. Drozd, B. G., J. F. Gunion and Y. Jiang, ”Extending two-Higgs-doublet models by a singlet scalar field - the Case forDark Matter”, JHEP 1411 (2014) 105, arXiv:1408.2106.

Bohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matter -

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2HDMS model2HDMS - Yukawa Interactions

Type I (only H2 couples to fermions)Type II (H2 couples to up-type fermions, H1 other)

Symmetry: Z2 : H1 → −H1, other scalar fields Z2-evenZ ′

2 : S → −S, other fields Z ′2-even

V =m211H†

1H1 + m222H†

2H2 −[m2

12H†1H2 + h.c.

]+λ1

2

(H†

1H1

)2+λ2

2

(H†

2H2

)2

+ λ3

(H†

1H1

)(H†

2H2

)+ λ4

(H†

1H2

)(H†

2H1

)+

λ5

2

(H†

1H2

)2+ h.c.

+

m20

2S2 +

λS

4!S4 + κ1S2

(H†

1H1

)+ κ2S2

(H†

2H2

)EWSB: Z ′

2 unbroken→ NO VEV FOR S→ NO MIXING WITH H1,2

H1,2 =

(ϕ+

1,2

(v1,2 + ρ1,2 + iη1,2)/√

2

)tanβ ≡ v2

v1, v2

1 + v22 = (246 GeV )2

Bohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matter -

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2HDMS model

Literature

X.-G. He, T. Li, X.-Q. Li, J. Tandean and H.-C. Tsai, Constraints on scalar dark matter from direct experimental searches,Phys. Rev. D 79 (2009) 023521 [arXiv:0811.0658].

B. G. and P. Osland, Tempered two-Higgs-doublet model, Phys. Rev. D 82 (2010) 125026 [arXiv:0910.4068].

M.S. Boucenna and S. Profumo, Direct and indirect singlet scalar dark matter detection in the lepton-specifictwo-Higgs-doublet model, Phys. Rev. D 84 (2011) 055011 [arXiv:1106.3368].

X.-G. He, B. Ren and J. Tandean, Hints of standard model Higgs boson at the LHC and light dark matter searches, Phys.Rev. D 85 (2012) 093019 [arXiv:1112.6364].

Y. Bai, V. Barger, L.L. Everett and G. Shaughnessy, Two-Higgs-doublet-portal dark-matter model: LHC data andFermi-LAT 135 GeV line, Phys. Rev. D 88 (2013) 015008 [arXiv:1212.5604].

X.-G. He and J. Tandean, Low-mass dark-matter hint from CDMS II, Higgs boson at the LHC and darkon models, Phys.Rev. D 88 (2013) 013020 [arXiv:1304.6058].

Y. Cai and T. Li, Singlet dark matter in a type-II two Higgs doublet model, Phys. Rev. D 88 (2013) 115004[arXiv:1308.5346].

L. Wang, A simplified 2HDM with a scalar dark matter and the galactic center gamma-ray excess, arXiv:1406.3598.

C.-Y. Chen, M. Freid and M. Sher, The next-to-minimal two Higgs doublet model, Phys. Rev. D 89 (2014) 075009[arXiv:1312.3949].

Bohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matter -

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Motivations

2HDMSAn attempt to provide both extra CP violation and DM candidate -2HDMS minimal model,2HDM provides an interesting ”low-mass” new physics accessibleat the LHC,To have a chance for MDM < mh/2

Bohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matter -

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Motivations

BR(h→ SS) ∝ λ2x for V (H,S) = · · ·+ λxH†HS2

Bohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matter -

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Strategy

5 mass eigenstates: h,H,A,H±,S

VS =12

m2SS2 + λhvhS2 + λHvHS2 + · · ·

10 parameters in the potential, various basis possible

General Basis:λ1, λ2, λ3, λ4, λ5m2

12, tanβmS, κ1, κ2

Physical Basis:mh,mH ,mA,mH± , sinαm2

12, tanβmS, λh, λH

2 types of Yukawa interactionType I and II Type I Type II

Higgs CV CU CD CU CDh sin(β − α) cosα/ sin β cosα/ sin β cosα/ sin β −sinα/ cos βH cos(β − α) sinα/ sin β sinα/ sin β sinα/ sin β cosα/ cos βA 0 cot β − cot β cot β tan β

Bohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matter -

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StrategyB. Dumont, J. F. Gunion, Y. Jiang and S. Kraml, ”Constraints on and future prospects for Two-Higgs-Doublet Models in light of theLHC Higgs signal”, Phys. Rev. D 90, 035021 (2014), arXiv:1405.3584

theoretical constraints: perturbativity, vacuum stability, perturbativeunitarityexperimental constraints

B/LEP limits H+

S,T,Uheavy Higgs searchesLHC fit at 68% CL

0.5

5

50

1

10

-1 -0.8 -0.6 -0.4 -0.2 0 0.2 0.4 0.6

tan

β

sinα

postLHC8 95%C.L.postLHC8 68%C.L.

postLHC8 68%C.L.-selected

TYPE I

0.5

5

50

1

10

-1 -0.8 -0.6 -0.4 -0.2 0 0.2 0.4

tan

β

sinα

postLHC8 95%C.L.postLHC8 68%C.L.

postLHC8 68%C.L.-selected

TYPE II

Bohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matter -

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Strategy

2HDMTake good 2HDM points

Scalar Singlet parameter scan:

mS ∈ [1 GeV, 1 TeV],λh, λH ∈ [-4π,4π],theoretical constraints: perturbativity, vacuum stability, perturbativeunitarity, EWSB (〈S〉 = 0),BR(h→ SS) < 10%,WMAP/Planck,direct DM detection.

Bohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matter -

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Strategy

Calculation of DM relic abundance Ω:

MicrOmegas by G. Belanger, F. Boudjema, A. Pukhov, A. Semenov, Comput.Phys.Commun. 180 (2009) 747-767, arXiv:0803.2360

ΩWMAP/Planck = 0.1187± 0.0017

Bohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matter -

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Resulting Constraints on the parameter space

# tan β sinα m212 mh mH mA mH±

I-1 1.586 −0.587 +5621 123.71 534.25 645.13 549.25I-2 1.346 −0.663 −2236 126.49 168.01 560.92 556.94

small λh required by BR(h→ SS) < 10%,

substantial λH needed for ΩDM ,

mH can not be too large,

H responsible for DM production!

h just to fit LHC data!

Bohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matter -

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Resulting Constraints on the parameter space

Bohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matter -

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Direct DM detection constraints

Bohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matter -

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Direct DM detection constraints

Bohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matter -

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Direct DM detection constraints

TYPE II - isospin violation

σDM−N =4µ2

ZA

πf 2p

[Z +

fnfp

(A− Z )

]2

BR(h→ SS) ≤ 0.1⇒ λh < 0.015

fnfp

=mn

mp

∑q

[(λhλHξq

h +(

mhmH

)2ξq

H

)f qn

]∑

q

[(λhλHξq

h +(

mhmH

)2ξq

H

)f qp

] −→ mn

mp

∑q ξ

qH f q

n∑q ξ

qH f q

p(S − indep.)

Table: Yukawa couplings of up and down type quarks tolight and heavy Higgs bosons h,H in Type I/II models. TheYukawa Lagrangian is normalised as follows:LYukawa =

mqv ξ

qh qqh +

mqv ξ

qH qqH

Type I Type IIξu

h cosα/ sinβ cosα/ sinβξd

h cosα/ sinβ − sinα/ cosβξu

H sinα/ sinβ sinα/ sinβξd

H sinα/ sinβ cosα/ cosβBohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matter -

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Direct DM detection constraints

TYPE II - isospin violation

σDM−N =4µ2

ZA

πf 2p A2

[ZA

+fnfp

(1− Z

A

)]2

σEXPDM−p ≥ σ

THEODM−p Θ(fn, fp)

Θ(fn, fp) =

[ZA

+fnfp

(1− Z

A

)]2

J. L. Feng, J. Kumar, D. Marfatia and D. Sanford, ”Isospin-Violating Dark Matter”’, Phys. Lett. B 703, 124 (2011) [arXiv:1102.4331]

Bohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matter -

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Direct DM detection constraints

Bohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matter -

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Direct DM detection constraints

tanβ sinα mH mA mH± m212 mS

2.092 -0.41 138 451 399 -12642 3.44; 3.56; 3.953.121 -0.282 187 546 571 8943 4.82; 5.482.192 -0.394 209 488 503 7518 5.401.728 -0.476 177 318 389 9382 5.161.789 -0.461 198 420 430 -6594 4.44; 5.151.488 -0.528 157 553 576 -10094 4.612.375 -0.363 259 260 339 15899 5.83

Table: Summary of the properties of the 2HDM Type II points which make it possible to realize mS < 50 GeV in agreementwith within 99% CL for CDMS II imposing the full set of constraints including the LUX and SuperCDMS bounds and. All massesare given in GeV units.

Bohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matter -

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New Higgs physics at the LHC?

H → SS decay - invisible H!mH ∼ 130− 200 GeV

Bohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matter -

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Conclusions

2HDM is allowed by current collider limits, even in thenon-decoupling regime

2HDMS provides a viable DM candidate and an opportunity forextra CP-violation

LUX requires mS ∼>50 GeV (TYPE I, II) or together withSuperCDMS mS ∼<6 GeV (TYPE II)

CDMS II reqiures |λh| < 0.05, |λH | > 0.1, and implies largeBR(H → SS) (TYPE I, II)

A fit of 2HDMS to LUX, superCDMS and CDMS II is only possiblewithin 99% CL for CDMS II, for TYPE II model,thenms ∼ 3.4− 5.8 GeV. For those points BR(H → SS)∼>90%

Bohdan Grzadkowski University of Warsaw Extending 2HDM by a singlet scalar field - the case for dark matter -