Blind Spots for Direct Detection with Simplified DM Models and the LHC

TL;DR

This paper explores how certain dark matter models with suppressed direct detection signals can still be constrained by collider searches at the LHC, especially through combined analysis of multiple search channels.

Contribution

It demonstrates that interference effects in simplified dark matter models create blind spots for direct detection, which can be constrained by collider data using combined search strategies.

Findings

Collider limits can surpass direct detection in some parameter regions.

Interference effects can suppress direct detection signals.

Combined LHC searches effectively constrain models with blind spots.

Abstract

Using the existing simplified model framework, we build several dark matter models which have suppressed spin-independent scattering cross section. We show that the scattering cross section can vanish due to interference effects with models obtained by simple combinations of simplified models. For weakly interacting massive particle (WIMP) masses $\gtrsim$10 GeV, collider limits are usually much weaker than the direct detection limits coming from LUX or XENON100. However, for our model combinations, LHC analyses are more competitive for some parts of the parameter space. The regions with direct detection blind spots can be strongly constrained from the complementary use of several Large Hadron Collider (LHC) searches like mono-jet, jets + missing transverse energy, heavy vector resonance searches, etc. We evaluate the strongest limits for combinations of scalar + vector, "squark" + vector, and scalar + "squark" mediator, and present the LHC 14 TeV projections.

Figures

Equations

$$\mathcal{L}\supset Z_{\mu }^{\prime }\bar{\chi }{\gamma }^{\mu }(g_{\chi }^V-g_{\chi }^A{\gamma }_5)\chi +\sum _i{Z}_{\mu }^{\prime }{\bar{q}}_i{\gamma }^{\mu }(g_q^V-g_q^A{\gamma }_5)q_i,$$

$$\mathcal{L}\supset -y_{\chi }\bar{\chi }\chi s-{\mu }_{s}s|\Phi {|}^2-{\lambda }_s{s}^2|\Phi {|}^2,$$

$$\mathcal{L}\supset -y_{\chi }\left(h_{\text{SM}}\sin \theta +H\cos \theta \right)\bar{\chi }\chi -\frac{1}{\sqrt{2}}\left(h_{\text{SM}}\cos \theta -H\sin \theta \right)\sum _f{y}_f\bar{f}f,\text{vspace}-6pt$$

$$\mathcal{L}\supset \sum _{i=1,2}{g}_{\tilde{q}}\left({\tilde{u}}_{i,R}^{†}\bar{\chi }{P}_R{u}_i+{\tilde{u}}_{i,L}^{†}\bar{\chi }{P}_L{u}_i+{\tilde{d}}_{i,R}^{†}\bar{\chi }{P}_R{d}_i+{\tilde{d}}_{i,L}^{†}\bar{\chi }{P}_L{d}_i\right)+\text{ h.c.},\text{vspace}-3pt$$

$$y_{\chi }\approx -\left(\frac{8.22\times 10^7{\text{ GeV}}^2}{m_{Z^{\prime }}^2}\right)\frac{g_{\chi }^V{g}_q^V}{\sin 2\theta \left(1-\frac{m_{h_{\text{SM}}}^2}{m_H^2}\right)}.$$

$$y_{\chi }\approx -\left(\frac{2.05\times 10^7{\text{ GeV}}^2}{m_{\tilde{q}}^2-m_{\chi }^2}\right)\frac{g_{\tilde{q}}^2}{\sin 2\theta \left(1-\frac{m_{h_{\text{SM}}}^2}{m_H^2}\right)}.$$

Full text

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41 \doinum10.3390/universe3020041 \pubvolume3

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\TitleBlind Spots for Direct Detection with Simplified DM Models and the LHC \AuthorArghya Choudhury 1,2,∗,†,‡, Kamila Kowalska 3,4,‡, Leszek Roszkowski 1,4,‡ , Enrico Maria Sessolo 3,4,‡ and Andrew J. Williams 4,‡

\corresCorrespondence: a.choudhury@sheffield.ac.uk \firstnoteSpeaker at “Varying Constants and Fundamental Cosmology" – VARCOSMOFUN’16 \secondnoteEmail: a.choudhury@sheffield.ac.uk, kamila.kowalska@tu-dortmund.de, L.Roszkowski@sheffield.ac.uk, enrico.sessolo@ncbj.gov.pl, andrew.williams.2009@live.rhul.ac.uk

1 Introduction

Simplified model spectra (SMS)Goodman and Shepherd (2011); Abdallah et al. (2014); Malik et al. (2015); Abdallah et al. (2015); Abercrombie et al. (2015) have been one of the most popular frameworks for the interpretation of the bounds from mono-photon/mono-jet searches on direct production of dark matter (DM) at the Large Hadron Collider (LHC). In such scenarios, cross section can be parametrized in terms of a few parameters, like the mediator mass or the couplings of the dark matter with the visible sector. Early LHC results were often presented in the effective field theory (EFT) framework, which is a good approximation as long as the mediator masses are well above the collision energy. Various recent studies that analysed the direct detection (DD) and LHC bounds on dark matter have used simplified model scenarios (see, e.g., Abdallah et al. (2014, 2015)) for this reason and found that in general, for weakly interacting massive particle (WIMP) masses above $\sim$5 $\,\mathrm{GeV}$ the limits on spin-independent DM-nucleon cross section ($\sigma^{\rm SI}_{p}$) coming from mono-jet/mono-photon searches are not competitive with the limits from direct detection experiments like LUXAkerib et al. (2014) or XENON100Aprile et al. (2012).

On the other hand, several effects like cascade decays, or cancellations in the couplings, or the interference between different diagrams, which can produce “blind spots” for direct detection searches are not present in the most simple SMS. Thus, the detection issues would be interesting with the models that are halfway between a UV complete model and those SMS. In this work, we combine three popular SMS in pairs. We only consider the simplified model of DM represented by scalar mediators, colored scalar mediators and vector mediators for which the $\sigma^{\rm SI}_{p}$ is significant. In this study we only consider a Dirac fermion dark matter.

In this proceedings, we report on our recent paperChoudhury et al. (2016) in which we dedicated special attention to the direct detection blind spots, which arise from interference between different diagrams in “less simplified” model frameworks (LSMS).

2 The Model Blocks

In this work we present a phenomenological analysis of a three “less simplified” model (LSMS) of DM. These LSMS, to some extent, mimic the properties of more generic UV models.

• •

Model 1. Combining Higgs portal and vector mediators;

• •

Model 2. Combining $t$-channel scalar mediators (charged under color) and Higgs portal;

• •

Model 3. Combining $t$-channel scalar mediators (charged under color) and vector mediators.

For these three models, we always consider a Dirac fermion singlet DM. In the next subsections, we briefly recall the characteristics of the three above-mentioned SMS.111Example of Feynman diagrams for $Z^{\prime}$, Higgs and squark mediators which provide contributions for monojet signature are given in Figure 1.

2.1 Vector Mediator

We consider a leptophobic $Z^{\prime}$ mediator which has negligible mixing with the SM $Z$ boson. To evade the stringent bounds from LHC di-lepton resonance searches, it has been assumed that $Z^{\prime}$ also does not couple to the Standard Model leptons.

The relevant interaction terms for DM phenomenology at collider and direct detection experiments are:

[TABLE]

where $g_{q}^{V}$, $g_{q}^{A}$, $g_{\chi}^{V}$, $g_{\chi}^{A}$ are universal vector quark coupling, universal axial-vector quark coupling, vector and axial-vector couplings to the dark matter respectively. In this study we restrict ourselves to vector boson exchange ($g_{\chi/q}^{A}$ = 0), which contributes $\sigma^{\rm SI}_{p}$. Hence the free parameters become— $m_{\chi},\,m_{Z^{\prime}},\,g_{\chi}^{V}$ and $g_{q}^{V}$; where $m_{\chi}$ is the DM mass and $m_{Z^{\prime}}$ is the $Z^{\prime}$ mediator mass. As the product of $g^{V}_{\chi}$ and $g^{V}_{q}$ only matters for $\sigma^{\rm SI}_{p}$, one may reduce the number of free parameters to 3 by assuming $g^{V}_{\chi}=g^{V}_{q}$.

2.2 Higgs Portal/Scalar Mediator

In this model, it is assumed that the fermion DM singlet ($\chi$) couples to a new singlet real scalar ($s$). The relevant terms for DM phenomenology are:

[TABLE]

where $y_{\chi}$ is the Yukawa coupling between the singlet and the DM. Mixing between the scalar ($s$) and the SM Higgs doublet ($\Phi$) is induced by the mass term— $\mu_{s}$. After electroweak (EW) symmetry breaking, one can diagonalize the mass matrix by a mixing matrix parametrized by a mixing angle $\theta$. Then the relevant interaction terms in the Lagrangian become:

[TABLE]

where $f,\bar{f}$ are SM fermions and $y_{f}$ are the SM Yukawa couplings. The DM couples to quarks via the heavy scalar mediator ($H$), as well as the SM Higgs, $h_{SM}$. Thus, this type of models are characterized by 4 parameters—$m_{\chi},\,m_{H},\,\sin 2\theta,\,y_{\chi}$.

2.3 Scalar $t$-Channel Mediators

Finally, we consider scalar colored mediators which couple the DM directly to the SM quarks. These scalar mediators are exchanged in the $t$-channel for DM production at the LHC. Although our model is not based on SUSY, we adopt the notation $\tilde{q}$ which is used to represent the squarks in the Minimal Supersymmetric Standard Model (MSSM). These new scalars are charged under color and flavor. We also assume that masses and couplings for first two generations are universal and the third generation squarks are beyond the reach of LHC.

The relevant terms for DM phenomenology are:

[TABLE]

where $\tilde{u}_{i,L(R)}$, $\tilde{d}_{i,L(R)}$, $u_{i}$ ($d_{i}$), $P_{L}$ ($P_{R}$) and $g_{\tilde{q}}$ are the $i$th generation left (right) up-type squarks, the $i$th generation left (right) down-type squark, the $i$th generation up (down) quarks, the left (right) chiral projection operators and the coupling strength respectively. The stability of dark matter is assumed to be protected by a discrete symmetry like R-parity. This type of model is characterized by 3 parameters—$m_{\chi},\,m_{\tilde{q}}$ and $g_{\tilde{q}}$, where $m_{\tilde{q}}$ is the universal squark mass and $g_{\tilde{q}}$ is the universal DM-squark coupling.

3 Methodology and Analysis of the Combined Models

Models 1–3 have been implemented using FeynRules Alloul et al. (2014). We have calculated $\sigma^{\rm SI}_{p}$ using $\tt micrOMEGAs\ v.4.1.8$Belanger et al. (2014). For event generation we have used MadGraph5_aMC@NLOAlwall et al. (2014) and PYTHIA8Sjostrand et al. (2008). For Model 2–3, we have generated $\chi\bar{\chi}$ + jets, $\chi\tilde{q}$ + jets associated production, and $\tilde{q}\tilde{q}^{\ast}$ + jets. To obtain the exclusion limits from jets + missing energy and mono jet searches we have used CheckMATEDrees et al. (2014) and our own codes which were previously used in ReferencesKowalska et al. (2015); Chakraborti et al. (2014, 2015). For 14 TeV projections with jets + missing energy and mono-jet analysis we have followed the prescribed cuts given in References ATL (2014a, b). We have also considered the limits on production cross section times branching ratio for $Z^{\prime}\rightarrow q\bar{q}$ and $Z^{\prime}\rightarrow t\bar{t}$ from LHC 8 TeV data with 20.3 ${fb}^{-1}$ Aad et al. (2015a, b, 2016) and the corresponding 14$\,\mathrm{TeV}$ projections with $300\leavevmode\nobreak\ {fb}^{-1}$ATL (2013). We have calculated the partial width of the 125 GeV Higgs to dark matter particles, $\Gamma_{h_{\textrm{SM}}\rightarrow\chi\bar{\chi}}$ , using CalcHEPBelyaev et al. (2013) to compare with the limit fromATL (2015). Considering all these LHC searches, we have compared the upper limits on production cross section times branching ratio or the quantity “upper limits on number of BSM events after all cuts ($N_{BSM}$)” with our models for different values of coupling (e.g., $g_{\chi/q}^{V},\,y_{\chi}$ etc.) to obtain the new limits.

3.1 Model 1: Combining $Z^{\prime}$ and Higgs Portal

In the first LSMS (Model 1) we consider a $Z^{\prime}$ vector boson and an extended scalar sector. Then one can write the relevant terms of Lagrangian as the sum of Equations (1) and (3). With the assumption that $g_{\chi}^{V}=g_{q}^{V}\equiv g_{\chi/q}^{V}$ the free parameters (6) become: $m_{\chi},\,m_{Z^{\prime}},\,m_{H},\,\theta,\,y_{\chi},\,g_{\chi/q}^{V}$.

We assume mixing as maximal as is allowed by the LHC constraints, perturbativity of the couplings, and EW precision observables: $\theta=0.2$. The cross section $\sigma^{\rm SI}_{p}$ depends mildly on the angle, via $\sin 2\theta$. More detailed analytical formulas for $\sigma^{\rm SI}_{p}$ can be found in RefernceChoudhury et al. (2016).

In Figure 2a we present the contours of $\sigma^{\rm SI}_{p}$ in pb in the ($y_{\chi}$, $g_{\chi/q}^{V}$) plane for $m_{\chi}=10\,\,\mathrm{GeV}$, $m_{H}=600\,\,\mathrm{GeV}$ and $m_{Z^{\prime}}=1000\,\,\mathrm{GeV}$. If $y_{\chi}>0$ , $m_{H}\gg m_{h_{\textrm{SM}}}$, and $g_{\chi}^{V}=g_{q}^{V}$, destructive interference does not take place (see Equation (3.3)222The cancellation can only happen in the nonrelativistic limit. The formula for differential WIMP-nucleus scattering cross section is given in Equation (3.2) of Reference Choudhury et al. (2016) and for the relativistic WIMP-quark scattering see Equation 3.4 of Reference Choudhury et al. (2016). of Reference Choudhury et al. (2016)). LUX bounds and XENON-1T projected reach are shown by solid red and dashed red lines. Solid (dashed) purple line presents the upper bound from 8 TeV mono-jet searches (14 TeV projected reach). The green solid vertical line provides the upper limit on the $y_{\chi}$ obtained from a ATLAS/CMS combined analysis of $\Gamma_{h_{\textrm{SM}}\rightarrow\chi\bar{\chi}}$ATL (2015). The limits from $Z^{\prime}\rightarrow q\bar{q}$ and $Z^{\prime}\rightarrow t\bar{t}$ are presented by solid orange line and solid cyan line.

Figure 2 shows that the direct detection limits on coupling ($g_{\chi/q}^{V}$) from LUX data is more severe than the collider limits in general. Only for $m_{\chi}\lesssim 62\,\mathrm{GeV}$, the invisible width of the 125 GeV Higgs boson (green line in Figure 2a,c) is significantly more constraining than the DD bounds. In Figure 2c,d, due to the choice $y_{\chi}<0$  (or if it is positive but $g_{\chi}^{V}=-g_{q}^{V}$), one gets suppressed $\sigma^{\rm SI}_{p}$. This happens due to the destructive interference of the diagrams corresponding to the Higgs portal $Z^{\prime}$ (see Equation (3.3) of ReferenceChoudhury et al. (2016)). The blind spot in the plots Figure 2c,d for for $m_{\chi}=10\,\mathrm{GeV}$ and 100 GeV respectively is a narrow diagonal region, over which the value of $\sigma^{\rm SI}_{p}$ visibly drops below the potential reach of tonne-scale detectors. The condition for the blind spot can be written as:

[TABLE]

Equation (5) shows that the contributions to the amplitude of the diagrams from the Higgs portal and $Z^{\prime}$ are of comparable size for comparable coupling strengths if $m_{Z^{\prime}}$ is at least of the order of a $\,\mathrm{TeV}$ or larger. When Condition (5) is satisfied, Model 1 is beyond the reach of direct detection searches but it can be studied by collider means. For this blind spot region, we show the effect of monojet searches, 125 GeV Higgs partial width measurements and $Z^{\prime}$ resonances searches in the ($m_{Z^{\prime}}$, $g_{\chi/q}^{V}$) plane in Figure 3 for fixed $m_{H}=600\,\mathrm{GeV}$ and two values of DM mass: (a) $m_{\chi}=10\,\mathrm{GeV}$, (b) $m_{\chi}=100\,\mathrm{GeV}$.

The grey regions at the top of Figure 3a are not allowed as $y_{\chi}$ becomes nonperturbative ($y_{\chi}>4\pi$). Color coding in Figure 3a is same as in Figure 2. The bounds from the direct $Z^{\prime}$ resonance searches and the single-jet searches remain almost unchanged over a large range of $m_{\chi}$. In Figure 3, we observe that the limit from $Z^{\prime}\rightarrow t\bar{t}$ searches at 8 TeV (solid orange line), $Z^{\prime}\rightarrow q\bar{q}$ searchesAad et al. (2015b) at 8 TeV (cyan solid line) and future projection of ATLAS mono-jet searches (dashed purple line) are comparable to each other. For resonant searches, 14$\,\mathrm{TeV}$ data (dashed orange line) improved significantly on the 8$\,\mathrm{TeV}$ data for $Z^{\prime}$ masses above 1500$\,\mathrm{GeV}$. In Figure 3b (for fixed $g_{\chi/q}^{V}=0.2$), we show that mono-jet search is always weaker than the direct search for a $Z^{\prime}$.

3.2 Model 2: Combining Higgs Portal and Squarks

Model 2 features some of the properties of SUSY models of DM. In particular the limits are similar to those cases where the neutralino couples to the SM Higgs and additional heavy Higgs bosons. In contrast with MSSM, the DM in our model is a Dirac fermion with free couplings, and the additional scalar is a SM singlet. The relevant terms of Lagrangian for Model 2 is simply the sum of Equations (3) and (4). Hence we have 6 free parameters for Model 2— $m_{\chi},\,m_{\tilde{q}},\,m_{H},\,\theta,\,y_{\chi},\,g_{\tilde{q}}$.

We present our results for Model 2 with fixed values of $m_{\tilde{q}}=1000\,\,\mathrm{GeV}$, $\theta=0.2$, $m_{H}=600\,\,\mathrm{GeV}$ and $m_{\chi}=10\,\,\mathrm{GeV}$ (100 GeV) in Figure 4. Similar to Model 1, cancellations in the amplitude for $\sigma^{\rm SI}_{p}$ do not occur for $y_{\chi}>0$. Hence, we restrict ourselves for the case $y_{\chi}<0$ and one can write the blind spot condition for Model 2 as:

[TABLE]

Figure 4 a,b present the contours of $\sigma^{\rm SI}_{p}$ in the ($y_{\chi}$, $g_{\tilde{q}}$) plane for $m_{\chi}=10\,\,\mathrm{GeV}$ and $m_{\chi}=100\,\,\mathrm{GeV}$ respectively. The color convention in Figure 4 is exactly same as in Figure 2. Additionally, the upper limit from the ATLAS 8 $\,\mathrm{TeV}$ squarks search in jets + missing $E_{T}$Aad et al. (2014) is presented by the solid blue line (see alsoKhachatryan et al. (2015) for the CMS bound). Similar to Model 1, the bound on $|y_{\chi}|$ from the invisible width of the 125 GeV Higgs is much stringent than the DD bounds for $m_{\chi}<62.5\,\mathrm{GeV}$ (see green solid line in Figure 4a). This bound from the invisible width does not applicable to Figure 4b and the blind spot regions which are not in reach of underground DD experiments remain essentially unconstrained for $m_{\chi}\gtrsim 62\,\,\mathrm{GeV}$. The dependence of the bounds on $m_{\tilde{q}}$ and $m_{\chi}$ when Equation (6) holds are presented in great details inChoudhury et al. (2016).

3.3 Model 3: Combining $Z^{\prime}$ and Squarks

We have designed Model 3 to mimic a UV completion characterized by an additional $U(1)_{X}$ symmetry that remains unbroken down to collider energies (see, e.g.,Athanasopoulos et al. (2014)). Among the several possibilities, one way of building a gauge invariant LSMS with the squarks and $Z^{\prime}$ mediated simplified models is the following, which allows the squarks to have the same coupling to the $Z^{\prime}$ as the quarks, and could be seen as an approximation of a full UV theory involving an extended gauge symmetry and a supersymmetric sector (for details see Section 3.3 of ReferenceChoudhury et al. (2016)). Despite being apparently rather involved, the phenomenology of Model 3 is represented by 6 free parameters—$m_{\chi},m_{\tilde{q}},\,m_{Z^{\prime}},\,g_{\chi}^{V},\,g_{q}^{V},\,g_{\tilde{q}}$. With the additional assumption $g_{\chi}^{V}=\pm g_{q}^{V}\equiv g_{\chi/q}^{V}$, this number is further reduced to 5.

We show the $\sigma^{\rm SI}_{p}$ contours in Figure 5a for Model 3 in the ($g_{\chi/q}^{V}$, $g_{\tilde{q}}$) plane for fixed $m_{\tilde{q}}=1000\,\,\mathrm{GeV}$ and $m_{Z^{\prime}}=1000\,\,\mathrm{GeV}$. Color conventions are same as Figure 2 or Figure 4. The case with $m_{\chi}=100\,\,\mathrm{GeV}$ is shown in Figure 5b. It may be noted that the LHC limits barely move by changing the DM mass, but direct detection limits reach their close-to-maximal strength when $m_{\chi}=100\,\,\mathrm{GeV}$. The jets + missing energy and mono-jet searches put comparable constraints on the couplings (blue and purple line). The interplay of LHC limits on the mediators’ mass for blind spot regions are discussed in details in Section 3.3 of ReferenceChoudhury et al. (2016). A complementary use of different detection strategies is needed to constrain a large part of the parameter space which is invisible in direct detection experiments.

4 Summary and Conclusions

In this work we have presented three dark matter models (LSMS) which are simple extensions of simplified DM models and mimic some properties of more realistic models without introducing an excessively large number of parameters. We mainly focussed to the scenarios where the interference between different diagrams produces blind spot for direct detection experiments. These blind spot regions are then further tested with current LHC limits and also with future LHC projections.

In general for $m_{\chi}\geq 10\,\mathrm{GeV}$, the DD bounds on $\sigma^{\rm SI}_{p}$  excludes the coupling constants of WIMP by at least one order of magnitude more strongly than any of the LHC searches considered here. The exceptions are: (i) In models with a Higgs portal (Model 1 and Model 2), for $m_{\chi}\lesssim 1/2\,m_{h_{\textrm{SM}}}$ the parameter space is also strongly constrained by the invisible width of the 125 GeV Higgs boson; (ii) In the parameter space corresponding to suppressed $\sigma^{\rm SI}_{p}$ due to interference effect, i.e., blind spot regions, LHC searches can effectively place strong bounds, especially at the end of Run 2.

We have found the following characteristics for the blind spot regions of Models 1–3:

• •

The Model 1 (combination of Higgs portal and $Z^{\prime}$) is at present not constrained at all by mono-jet searches for the assumption $g_{\chi}^{V}=g_{q}^{V}$. Moreover, under this assumption, the future searches of heavy $Z^{\prime}$ resonances at the LHC will be most effective to probe the blind spot regions.

• •

In Model 2 and Model 3 (involving squark-like mediators), the current limits on the coupling $g_{\tilde{q}}$ from jets + missing energy and mono-jet searches are comparable. However, according to LHC future projectionsATL (2014a, b), the jets + missing energy searches at the 14$\,\mathrm{TeV}$ LHC will outperform the expectations for mono-jet searches in the parameter space with blind spots.

In general we find that, to constrain the DM models at the colliders, it is crucial to use the complementarity of different search strategies. A lot of well motivated DM models, which are not necessarily constrained by DD bounds, demand careful attention at LHC or future colliders. In this work, we have investigated such scenarios in terms of a less-simplified model framework which can be explored at the LHC.

Acknowledgements.

A.C. and L.R. are supported by the Lancaster-Manchester-Sheffield Consortium for Fundamental Physics under STFC Grant No. ST/L000520/1. K.K. is supported in part by the DFG Research Unit FOR 1873 “Quark Flavour Physics and Effective Field Theories”. L.R. and E.M.S. are supported in part by the National Science Council (NCN) research grant No. 2015-18-A-ST2-00748. The work of E.M.S. is supported in part by the Alexander von Humboldt Foundation. The use of the CIS computer cluster at the National Centre for Nuclear Research in Warsaw is gratefully acknowledged.