Search for the Higgs portal to a singlet fermionic dark matter at the LHC

Search for the Higgs portal to a singlet fermionic dark matter at the LHC

Seungwon Baek, P. Ko, Wan-Il Park
School of Physics, KIAS,
85 Hoegiro Dongdaemun-gu, Seoul 130-722, Korea
sbaek1560@gmail.com pko@kias.re.kr wipark@kias.re.kr
Abstract

We consider a simple extension of the standard model with a singlet fermionic dark matter. Its thermal relic density can be easily accommodated by a real singlet scalar messenger that mixes with the standard model Higgs boson. The model can change significantly the Higgs signals at the LHC via sizable invisible decays of two Higgs-like scalar bosons. After imposing the constraints from the electroweak precision tests, colliders and dark matter search experiments, one concludes that two or one or none of the two Higgs bosons, depending on the mass relations among two scalar bosons and the dark matter fermion and their couplings. In particular, if a standard model Higgs-like scalar boson is discovered around 120–125 GeV region at the LHC, it would be almost impossible to find the second Higgs-like boson since it is mostly a singlet scalar, whether it is heavier or lighter. This model can be further tested by direct dark matter search experiments.

1 Introduction

The Standard Model (SM) of particle physics has been very successful for describing many phenomena observed at various experiments, except for neutrino oscillation, nonbaryonic cold dark matter (DM) and baryon number asymmetry of the universe, as well as some theoretical shortcomings such as hierarchy problem, strong CP problem, etc. At present, the only part of the SM which experiments could not unveil is the Higgs sector, namely electroweak symmetry breaking (EWSB) sector. The absence of signal at LEP experiment puts a lower bound on the mass of the SM Higgs particle at about  Barate:2003sz . However, the most recent results from ATLAS and CMS at the LHC have excluded the SM Higgs boson in the mass range of GeV at CL  ATLAS . Hence, the only remaining window for the light Higgs mass is . This is consistent with the electroweak precision test (EWPT) which strongly favors the light SM Higgs boson.

When we consider Higgs physics, it is very important to notice that dark matter can easily modify Higgs phenomenology. For example, in the real singlet scalar DM model with symmetry, this happens through the invisible Higgs decay into a pair of DM’s: where is a real singlet scalar dark matter. In this model lagrangian, the stability of the real singlet scalar is guaranteed by an ad hoc symmetry . There are a number of works in this direction Silveira:1985rk ; hep-ph/0702143 ; hep-ph/0011335 (see Refs.  Kanemura:2010sh ; Mambrini:2011ik ; Raidal:2011xk ; He:2011de ; Ma:2011kc ; Gupta:2011gd for recent discussions). One can consider a complex scalar cold dark matter (CDM), for which one has qualitatively similar results arXiv:0811.0393 .

One can also consider singlet dark matter with higher spins: singlet fermion or singlet vector boson dark matter. There are some works in this direction, sometimes under the name of Higgs-portal dark matter KYLee:2008 ; Kanemura:2010sh ; Kanemura:2011vm ; Lindner:2011it ; arXiv:1110.4405 ; Kanemura:2011mw ; Lebedev:2011iq , many of which work in the effective lagrangian approaches with the SM particles and the singlet dark matters. For the case of a singlet fermionic dark matter, Ref. KYLee:2008 employed a renormalizable lagrangian similar to our present work. But overall phenomenology of the scalar sector such as the EWPT was not discussed. In this paper, we will make more emphasis on the EWPT, the Higgs phenomenology at the LHC and the interplay between the DM sector and two Higgs-like scalar bosons, which makes the first attempt to consider all the relevant phenomenological aspects related with the singlet fermion dark matter and the Higgs bosons.

If we consider a singlet fermion CDM scenario at a renormalizable lagrangian level, there appears an additional singlet scalar which plays a role of messenger between the SM sector and the DM . In this scenario, there will be at least two scalars and , the mixtures of the SM Higgs boson and the singlet scalar (see Refs. Profumo:2007 ; Barger:2007 for recent discussions on the singlet scalar extension of the SM). Since the scalar boson spectrum is qualitatively different from the singlet scalar DM scenario where there is only one SM Higgs boson, it is important to analyze the singlet fermion CDM scenario in a more quantitative way, and understand the generic signatures at the LHC and at other DM search experiments. It is also important to notice that the effective lagrangian approach with the SM Higgs boson can miss some important features of dark matter models such as our model with two Higgs-like scalar bosons. For example, we will observe that there is a generic cancellation of the Higgs boson contributions in the direct detection cross section between the DM and a nucleon, which can not be seen in the effective lagrangian approach.

In the singlet fermion DM model with a real singlet scalar messenger, the Higgs phenomenology can be modified in some different reasons:

  • Mixing between and makes the physical Higgs bosons and have reduced couplings with the SM fermions and the SM weak gauge bosons.

  • can decay into a pair of CDM’s if kinematically allowed.

  • can contribute to the decay width of the heavier scalar boson , if kinematically allowed.

  • The first two dilution factors make the production and the detection of two Higgs bosons more difficult than the SM Higgs boson case. There is an ample parameter space where one of the scalar bosons or both can not be discovered at the LHC even at 10 fb (see Fig. 10).

  • Presence of two scalars and relaxes the strong constraint from the direct detection cross section, whereas the couplings of can be still large and the can be substantial. This makes an important difference from the real singlet scalar CDM with , in which the direct detection cross section puts a strong constraint on the .

  • Even if no SM Higgs boson is found at the LHC in the end, it does not necessarily imply that the perturbative unitarity of scattering amplitude is broken, or there should be new strongly interacting EWSB sector. Our scenario with and can describe such a situation, and would be perfectly fine.

These features are also qualitatively true in other hidden sector DM models, regardless of strongly or weakly interacting hidden sector Hur:2007uz ; arXiv:1103.2571 ; ko_talks ; Englert:2011yb . In case the hidden sector gauge interaction is a confining gauge theory like QCD, there will appear Nambu-Goldstone (NG) bosons at low energy, which could be the CDM. And new composite scalar bosons (similar to meson in QCD) in the hidden sector can mix with the SM Higgs boson or a real singlet messenger scalar . The number of neutral scalar bosons will depend on the number of hidden sector quark flavors, and becomes model dependent. One crucial difference of this type of scenario from the multi-Higgs doublet models is that there will be only neutral scalar bosons, and not any charged scalar bosons.

Finally, in a class of models where the dark matter sector and the SM sector carry a new gauge symmetry in common, one could have similar phenomena. If the new gauge boson gets its mass from spontaneous symmetry breaking due to a new scalar field , there will be a generic mixing between this new scalar field and the SM Higgs field, via interaction term and nonzero VEV’s of and . For example, two of the present authors studied the gauged extension of the SM and explained the PAMELA excess, without any conflict with many constraints from the low energy experiments, colliders and astrophysical observations baek_ko .

All these models have a similar consequences for the Higgs phenomenology, namely more than one Higgs-like neutral scalar bosons with substantial invisible branching ratios, and improves the fit to the electroweak precision data. It would not be easy to distinguish one model from another using the experimental data, and it is beyond the scope of this paper to attempt such a study here.

In this paper, we study the singlet fermion dark matter model to see if it can explain the recent LHC data while fulfilling other observational and cosmological requirements, and if Higgs particle(s) can be discovered from the future data-accumulation at the LHC, keeping in mind that there could be other models which might have similar observational consequences. Our model is one of the simplest extension of the SM with a singlet fermion dark matter and thus could serve as a good starting point for phenomenological analysis and the analysis strategy can be applied to other models for more general study.

This paper is organized as follows. In Sec. 2, we define the singlet fermion CDM model with two Higgs-like scalar bosons. In Sec. 3, we calculate the decay rates for , and discuss the relevant constraints from colliders, electroweak precision tests and dark matter phenomenology. In Sec. 4, the phenomenology of two Higgs scalar bosons is discussed for three different cases: , GeV, and , assuming the mass of one Higgs boson is 120 GeV, and discuss the detectability of two Higgs boson at the LHC. Finally the results and their implications are summarized in Sec. 5.

2 The model

We consider an extension of the SM, adding a singlet Dirac dark matter111We get similar results for a Majorana dark matter case. and a singlet scalar . The singlet fermion DM is assumed to live in the hidden sector, and communicates with the SM sector via the scalar . Then, the model lagrangian has 3 pieces, the hidden sector and Higgs portal terms in addition to the SM lagrangian:

(1)

where

(2)

with

(3)

The model without the singlet fermion DM, namely the SM plus an additional singlet scalar field has been studied in detail in  Profumo:2007 ; Barger:2007 . Note that a real scalar singlet dark matter model can be obtained if we remove the fermionic DM and impose symmetry: .

The Higgs potential has three parts: the SM, the hidden sector and the portal parts

(4)

where can be read from (2), (3) and

(5)

In general the Higgs potential develops nontrivial vacuum expectation values, and , and we can expand and as

(6)

where and are the Goldstone bosons and and are physical scalar fields after and develops nonzero VEV’s. Assuming all the Higgs sector parameters are real, that is, there is no CP violation in the Higgs sector, we obtain

(7)

from the tadpole conditions. The quartic couplings can be traded for the Higgs mass parameters

(8)

Now the Higgs mass matrix can be diagonalized by introducing mixing angle so that

(9)

The mass eigenstates with masses and are expressed in terms of the SM Higgs and the singlet as

(10)

We take

(11)

as free parameters for the Higgs sector. We have two additional free parameters, the DM mass and its coupling to the singlet scalar :

(12)

Therefore, we have introduced 9 more new parameters in total, compared with the SM lagrangian. These new parameters are constrained by various theoretical, experimental and observational data: perturbative unitarity of gauge boson scattering amplitudes, EWPT, collider searches for Higgs boson(s), DM relic density, DM direct detection experiments, etc.

3 Constraints

In this section we consider the following constraints on the model parameters:

Note that the first three constraints are independent of the dark matter sector, and they apply to the SM plus a singlet scalar model without dark matter as well.

3.1 Perturbative unitarity of gauge boson scattering amplitudes

The perturbative unitarity of scattering amplitudes for longitudinal weak gauge bosons in our model requires bwlee ; Englert:2011yb ,

(13)

This is a rather weak constraint compared with other constraints that will be described subsequently, and thus does not play an important role.

3.2 LEP bound

The LEP data severely constrains the ratio of Higgs-- coupling strength to that of the SM,  Barate:2003sz . For example, as shown in Fig. 10(a) in Ref. Barate:2003sz , if is less than 90 GeV, the should be less than .

The signal strength or “the reduction factor” in the event number of a specific final state SM particles, , in the Higgs boson decays is defined as

(14)

where and are the production cross section of , and the branching ratio of respectively, while and are the corresponding quantities of the SM Higgs with mass . Then we find

(15)

where . The denotes the total decay width of the SM Higgs boson with mass and the is that of (the invisible decay modes of ’s). Note that the signal strength is reduced by in the production cross section due to the mixing between and , as shown in (15), even if the invisible mode () or the Higgs-splitting mode () is kinematically forbidden in the Higgs decay. In other words, a reduced signal of the Higgs boson at the LHC would be a generic signature of the mixing of the SM Higgs boson with extra singlet scalar boson(s).

For the numerical analysis, we take the SM-like Higgs mass to be 120 GeV as a benchmark value, for which the SM Higgs decays dominantly into , and we obtain

(16)

This can be compared with the hidden sector decay width

(17)

For , GeV and GeV, we get GeV which is much larger than (16). This may impose serious problems in searching for Higgs at the LHC as will be discussed below.

For , the Higgs splitting mode will open, which would generate very peculiar signals at colliders such as , hence could be a target at future collider experiments.

3.3 The oblique parameters:

The extended Higgs sector gives extra contribution to the gauge boson self-energy diagrams, as the SM Higgs boson does. This can affect the EWPT leading to the constraints on the oblique parameters, and , by the Higgs sector 222If the Higgs masses are not much larger than electroweak scale, and parameters should be also taken into account. However, their contributions are smaller than those of , and parameters and makes no much difference. Hence we ignore the effects on and in our argument.. Since the newly added singlet scalar is electrically neutral, do not change from the SM predictions, and we only need to calculate and boson self-energy diagrams, .

It is straight-forward to get ,

(18)

The functions and are defined in the Appendix. For the reference Higgs mass we fix GeV. The above expressions show that there is a symmetry in the and parameters in the simultaneous exchange of and such that

(19)
Figure 1: Left (Right) panel: Exclusion plot in plane with several choices of . The colored region for the given value of the Higgs mass is excluded by EWPT. (Note that by definition and only the region satisfying this relation is meaningful.)

In order to obtain constraints on the parameters and from parameters, in Fig. 1 we show an exclusion plot in plane by the EWPT at 95% CL  Barger:2007 ; Baak:2011ze . The colored region for the given value is excluded in the left (right) panel. We can see that can be much heavier than   only when the is dominated by the SM component (i.e. ) (see the left panel). The possibility is also allowed. In this case can be lighter than only when is SM-like (i.e. ) (see the right panel.)

Fig. 2 shows that the EWPT constraint on our model is generically much less severe than on the SM. Since is very small, we assume for this plot. The ellipses are (68, 90, 95) % CL contours Baak:2011ze . The thick black curve shows the SM prediction with the Higgs boson mass in the region GeV. The red, green dots correspond to , respectively. The dots are for from above for each color. The SM always predicts a negative for the Higgs mass larger than GeV. However, can be either positive or negative in our model. The positive can fit to the EWPT data better.

Figure 2: parameters in our model. The ellipses are (68, 90, 95) % CL contours. The thick black curve shows the SM prediction with the Higgs boson mass in the region GeV. The red, green dots correspond to , respectively. The dots are for from above for each color.

3.4 Dark matter relic density

The present relic density of cold dark matter,  Jarosik:2010iu , is related with the thermally averaged annihilation cross section at freeze-out roughly by

(20)

In this paper, we restrict ourselves to the case of , for which the DM pair annihilation into in the -channel becomes dominant. We can approximate the annihilation cross section

(21)

The typical value is many orders of magnitude smaller than needed in (20). However, a huge enhancement is possible near the resonance region, as can be seen in Fig. 3. The figure shows the present dark matter relic density as a function of for , , (maximal mixing) and . In the figure, the double-dip is due to two -channel resonances near (). We adapted the micrOMEGAs package  Belanger:2008sj to our model for numerical calculation.

Figure 3: Dark matter thermal relic density () as a function of for  GeV,  GeV, and .

3.5 Direct detection

For the CDM in the mass range

(22)

there is a strong upper bound on the spin-independent (SI) dark matter-proton scattering cross section from various direct detection experiments  Aprile:2011hi :

(23)

The spin-independent (SI) elastic scattering cross section for a Dirac fermion dark matter to scatter off a proton target is given by

(24)

where is the reduced mass , and is given by

(25)

The couplings ’s describe the effective SI four fermion interactions of the quarks and the dark matter, and are given by

(26)

The parameter ’s are defined by the following matrix elements

for , and . The numerical values of the hadronic matrix elements we used are Belanger:2008sj

(27)

Note that recent study of these parameters in the lattice QCD yields somewhat lower values Bali:2011rs . In case we adopt these new numbers, the constraints from the direct detection experiments will become milder.

After all, for the case , we find

(28)

A remark is in order here. One might think that the strong constraint on the SI cross section from DM direct detection experiments exclude a possibility of the SM Higgs decay mode into a pair of DM, since the DM couplings to the Higgs boson is constrained by the direct detection experiments. However this is not true in general. For the case of vector [17] and scalar [6] Higgs portal DM, the invisible branching ratios can be as large as 80% and 60%, respectively, even without the singlet scalar messenger . In our model, there are two Higgs-like scalar bosons, mixtures of and . Then, as can be seen in (26), there would be a destructive interference between and contributions to the scattering amplitude due to orthogonality of the Higgs mixing matrix, which is a very generic aspect in case there are extra singlet scalar bosons that can mix with the SM Higgs boson. Hence, for regions , a cancellation occurs in and even the large , regions are only weakly constrained. This feature is shown in Fig. 4, where we show a region in the plane that is excluded by the upper bound of (pb). We also note that and are not strongly correlated near the Higgs resonance where the relic density can be explained. This helps to evade the strong bound on while accommodating the correct CDM density in the universe. As we’ll see below, this opens up a very interesting parameter space for Higgs boson search at the LHC, making one or two of the Higgs-like scalar bosons can decay into a pair of DM’s with a substantial invisible branching ratio(s).

Figure 4: Region in the plane that is excluded by (pb). For this plot, we fixed , . The values used are shown in the plot. As becomes closer to , the constraint gets weaker, as explained in the text.

4 Implications for the Higgs search at the LHC

In this section, we investigate the allowed parameter space, taking into account of all the constraints discussed in the previous section, and see if it is possible to discover the Higgs(es) at the LHC. We study the following three benchmark scenarios classified according to the Higgs mass relations:

  • Scenario 1 (S1):  GeV

  • Scenario 2 (S2):  GeV

  • Scenario 3 (S3):  GeV

4.1 S1:  GeV

Figure 5: Contour plot in plane. We fixed ,  GeV, and  GeV. The red line represents . The sky blue region is excluded by (pb) obtained by XENON100. The region above the dashed blue line is ruled out by EWPT at 95% CL. The solid (dashed) black (brown) lines show reduction factors for : 0.1, 0.3, 0.5, 0.7, 0.9 (0.2, 0.4, 0.6, 0.8) from above (below).

In this case, it turns out that the DM direct detection constraint is very strong as we can expect from Fig. 4, and only small is allowed for the mixing angle . This can also be seen in Fig. 5 where we show a contour plot in plane. We fixed , GeV, and for this plot. The blue region is excluded by the non-observation of DM at direct detection experiments. The region bounded by the red curve satisfies , and the equality holds on the boundary. The solid black (dashed brown) lines show reduction factors for (): 0.1, 0.3, 0.5, 0.7, 0.9 (0.8, 0.6, 0.4, 0.2) from above. Since the heavier Higgs is quite heavy with GeV, the contributions to parameters become large for large as can be seen in Figs. 1 and 2. The region above the dashed blue line is ruled out by EWPT at 95% CL. We can see that invisible Higgs decay BR can be sizable, reducing signal strength significantly for  GeV. Considering all these constraints, we find only the lower blank region is allowed and we get , . As a consequence, the possibility of detecting at the LHC would be closed unless one can achieve a substantial increase in the integrated luminosity. However, if the Higgs cascade decay channel is kinematically allowed, it is still possible to detect via exotic Higgs decay channels via , which clearly deserves more detailed study at the LHC. In this region the allowed DM direct detection cross section is just below the current experimental sensitivity and the current or near-future direct detection experiments can probe this scenario.

In fact, these features remain the same even if the CDM is very heavy so that both Higgs bosons cannot decay into a pair of CDM’s. For example, one can achieve thermal relic density with GeV, GeV, and . For such a heavy DM, the constraint from the direct detection is rather weak, and one can have rather large . Such a heavy CDM can accommodate the PAMELA excess if it decays via higher dimensional operators. Also, the vacuum stability condition should be modified from the SM case, since there are additional contributions from scalar boson and the fermionic DM . These two contributions will compete and can change the stability bound curve. It would remain to be seen if the Higgs boson with mass around 120 GeV might be still consistent with no new physics up to Planck scale or not. These issues are somewhat outside the main subjects of this work, and will be addressed in more detail in a separate publication work .

4.2 S2:

Figure 6: Contour plot in plane. We fixed ,  GeV,  GeV. Others are the same with Fig. 5. Note that the direct detection bound and the EWPT do not constrain this scenario for this choice of parameters.
Figure 7: Contour plot in plane for the case S1 and S2 with (pb) as the upper-bound from direct detection experiments. The orange shaded regions are excluded by the constraint from EWPT. The borders correspond to from right. The reddish shaded regions are excluded by the upper-bound of dark matter-nucleon cross section. The borders correspond to from above. The green lines are from above for . The blue lines are for from above.

In the S2, the direct detection cross section is drastically suppressed due to the destructive interference between and . The suppression factor is proportional to . As we noticed above the cancellation does not necessarily mean too small annihilation cross section for the relic density, or a small branching ratio for invisible Higgs decays. This is especially true near the -channel resonance region. This feature can be clearly seen in Fig. 6 where there is no constraint from the DM direct detection results (namely, no blue box compared with Fig. 5) and the relic density can be still explained. For this plot we fixed which is quite large and makes the invisible decays quite effective once kinematically allowed. For the Higgs boson masses, we chose  GeV,  GeV. For Higgs invisible decays are closed and a simple sum rule holds between the two reduction factors as can be seen from (15) (see the discussion in Sec. 4.4 and Fig. 10):

(29)

This is because the Higgs invisible and splitting decay modes are kinematically closed and the event reduction occurs only at the Higgs boson productions. If and is nearly maximal, both and are close to . So both Higgs bosons can be observed at the LHC by the standard Higgs search method. This would be a clear signal for S2 as well as the existence of additional singlet scalar.

Again from Fig. 7, it is clear that if becomes close to , wide ranges of and are allowed. If , for example, the constraint from direct detection becomes almost irrelevant due to the destructive interference between ’s contributions (see Eq. (15)). The constraint from the EWPT is also irrelevant. In this case, both of and can be close to 0.5 if the mixing is nearly maximal, but it happens only for implying that invisible decay branching ratios for the two Higgs bosons are negligible. This would be another case where we can see both Higgses.

4.3 S3:  GeV

Figure 8: Contour plot in plane for the case S3 with ,  GeV,  GeV. The purple region is excluded by the LEP Higgs search bound  GeV. Others are the same with Fig. 5. Note that the direct detection bound and the EWPT do not constrain this scenario for this choice of parameters.
Figure 9: Contour plot in plane for the case S3 with (pb) as the upper-bound from direct detection experiments. The borders of color-shaded regions correspond to from right (below) for purple (reddish) regions. The purple shaded regions excluded by the constraint on from LEP data. The borders correspond to from right. The reddish shaded regions are excluded by the upper-bound of dark matter-nucleon cross section. The blue lines are from left for .

In this case, for , the constraints from , and oblique parameters of EWPT become irrelevant as shown in the right panel of Fig. 1. The most stringent constraint comes from the LEP Higgs search bound. In Fig. 8, we show the case of ,  GeV, and  GeV with the LEP excluded region shown in purple which corresponds to . The current constraint from the DM direct detection experiments is satisfied for the parameter set chosen for the plot. We see that can take any value from 0 to 1. If and the invisible decay of is closed, only is allowed. That is, if is observed with we can conclude that the reduction of the signal strength is due to the Higgs decay to the hidden sector dark matter. In Fig. 9, we can find the dependence of on due to the constraint from direct detection. For example, if only is allowed.

4.4 The LHC reach

In this subsection we concentrate on the parameter space that can be probed at the LHC in near future. For this purpose we show scattered plots in plane in Fig. 10. We take the Higgs masses as benchmark points for each scenario as follows:

  • S1: GeV, GeV,

  • S2: GeV, GeV,

  • S3: GeV, GeV.

We scanned the remaining parameters in the range

(30)

All the points in the plots satisfy

  • the unitarity condition (13),

  • the LEP Higgs mass bound Barate:2003sz ,

  • the EWPT fits at 95% CL Barger:2007 ; Baak:2011ze ,

  • the direct search bound of DM by XENON100, pb,

  • the relic density of DM, .

We can divide the into two regions:

(31)

where the former region can be probed in near future direct search experiments. The relic density is also divided into two regions:

(32)

where the former is the WMAP 3 allowed region. The different colors and sizes of the points represent different regions of and as table 1.

big red small orange
big blue small green
Table 1: Color Schemes for and

The region that the LHC can probe at 3 level with 5 (10) fb luminosity is represented by solid (dashed) line CMS-TDR ; ATLAS-TDR . The S1 scenario can be tested fully at the LHC with 10 fb by observing . In the case of S2 the LHC may see both Higgs bosons with the standard search strategy. However, there are still some points which the LHC has difficulty to find two Higgs bosons. These are the points near the origin () where the invisible decays becomes dominant. In S3 the region with small can not be probed with the standard decay channels. However, once is open, this region can also be tested at the LHC.

Figure 10: Scatter plot in plane for the scenario S1, S2 and S3 (from above). The region that the LHC can probe at 3 level with 5 (10) fb luminosity is represented by solid (dashed) line. The points represent 4 different cases: , (big red), , (big blue), , (small orange), and , (small green). (See the text for more detail).

4.5 The implications of the recent LHC reports on our model

Recently the ATLAS ATLAS_Dec13 and the CMS CMS_Dec13 at the LHC reported that the allowed SM Higgs mass range is further constrained to be  GeV (ATLAS) and  GeV (CMS) and they also saw a hint with the mass in the range  GeV. The analysis in our paper with a Higgs mass 120 GeV does not change much by changing it to 125 GeV. In our model the Higgs with mass  GeV can be either or . Assuming to be discovered with 3 significance, we can see that the possible Higgs signal at the LHC should be () for the scenario S1 (S3). In these models the remaining Higgs lies beyond the reach of the LHC. For the scenario S2, the LHC may have seen either or . The other Higgs may or may not be probed at the LHC with more luminosity. In summary, if we consider the recent results for the SM Higgs boson at the LHC as a real singal for the Higgs bosons around 125 GeV Higgs boson with in our model, the other Higgs boson can be either light or heavy, and it would be very difficult to discover it at the LHC 333Similar discussions were presented in Refs.  Kadastik:2011aa ; Djouadi:2011aa after the ATLAS and the CMS reported the new results on the SM Higgs boson..

5 Conclusions

In this paper we considered a simple extension of the SM where the fermionic DM in the hidden sector can interact with the SM sector through Higgs portal. A new singlet scalar has been introduced as a messenger between the hidden sector and the SM sector. It mixes with the SM Higgs boson and behaves like a second Higgs boson. This opens up a new possibility that the Higgs search program can be quite non-standard.

Considering the constraints mainly from the LEP Higgs search bound, electroweak precision observables, thermal dark matter density and dark matter direct detection experiments, we investigated the possible Higgs search scenarios in three categories:

  • Scenario 1 (S1): The light Higgs boson has mass and the heavier one is much heavier than .

  • Scenario 2 (S2): The two Higgs bosons are almost degenerate in mass: . We assume .

  • Scenario 3 (S3): The heavy Higgs boson has mass .

For S1, the constraints from EWPT and DM direct search data severely restrict the discovery likelihood of the heavier Higgs. The mixing angle in this case is pushed to small value causing significant signal reduction for the discovery (see the top plot in Fig. 10). However, is possible while is still not so small. Hence can be discovered even if it has a sizable invisible branching ratio. Most of the points in the top plot of Fig. 10 are also sensitive to near-future DM direct search experiements. Especially, the lighter Higgs may behave like the SM Higgs boson if , and then can be discovered at the LHC. On the other hand, the heavier Higgs is very difficult to observe at the LHC, since for . It would be important to measure as precisely as possible, and see if it deviates from the SM value or not in order to test our model. However, because of theoretical and experimental uncertainties, it would be a difficult job, especially for GeV. If one could improve the sensitivity on from below , one might be able to find out the heavier Higgs boson at the LHC with higher luminosity.

On the other hand, for S2, the constraints from the EWPT become weak. Interestingly the constraint from direct detection experiments is drastically alleviated due to a strong cancellation in the . As the result, there is an ample room to discover one or both of the Higgs particles with the standard Higgs search method at the LHC, if the invisible decays of is kinematically closed and the relation holds. There is also possibility that both Higgs bosons may not be seen at the LHC, if invisible decay modes become significant and (see the middle plot in Fig. 10). In this particular case, both Higgs bosons would not be discovered at the LHC, and also no new particles appear below TeV. This would seem to be in conflict with the theorem by Lee, Quigg and Thacker bwlee . However in our model, it is possible that we observe no particles including Higgs bosons and other new resonances at the electroweak scale, without violating the unitarity of the longitudinal weak gauge boson scattering amplitudes.

In the case S3, the most stringent constraint is from LEP Higgs mass bound for the lighter Higgs. As a consequence, it is difficult to detect while can be seen at the LHC (see the bottom plot in Fig. 10). The DM direct detection experiment may also see a signal.

In summary, in the fermionic DM model with Higgs portal, it is easy to explain the DM relic density while satisfying the DM direct detection bounds from the cancellation. Two Higgs-like bosons can decay into dark matter pair, thereby the signals for the Higgs bosons being reduced significantly. We have a big chance of discovering one or both of Higgs particles at the LHC in the near future if two Higgs bosons have hierarchical mass spectra. On the other hand, we may find no Higgs bosons or new resonances if and . Even if we find no Higgs boson at the LHC, it would not imply that perturbative unitarity in the longitudinal weak gauge bosons is violated, since our model is renormalizable and respects unitarity, still having a possibility of no visible effects at the LHC at all. It would remain to be seen which route is realized in the nature.

Acknowlegements

We are greatful to Suyong Choi, Dong Hee Kim and Soo Bong Kim for useful discussions. This work of PK was supported in part by the National Research Foundation (NRF) through Korea Neutrino Research Center (KNRC) at Seoul National University.

Appendix A The loop functions for the and parameters

The loop functions for the and parameters are listed below:

References

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