Higgsino Dark Matter or Not: Role of Disappearing Track Searches at the LHC and Future Colliders

TL;DR

This paper proposes a new disappearing-track search strategy at colliders to detect Higgsino dark matter, especially in scenarios where gauginos are very heavy, complementing non-accelerator experiments.

Contribution

It introduces a novel collider search method using two-hit pixel detector techniques to identify long-lived charged Higgsinos in heavy gaugino scenarios.

Findings

Future 33 TeV colliders can probe almost pure Higgsino dark matter.

Disappearing-track searches with displaced-vertex reconstruction improve background suppression.

Strategy enhances detection prospects for electroweak-charged dark matter candidates.

Abstract

Higgsino in supersymmetric standard models is known to be a promising candidate for dark matter in the Universe. Its phenomenological property is strongly affected by the gaugino fraction in the Higgsino-like state. If this is sizable, in other words, if gaugino masses are less than ${\cal O}(10)$ TeV, we may probe the Higgsino dark matter in future non-accelerator experiments such as dark matter direct searches and measurements of electric dipole moments. On the other hand, if gauginos are much heavier, then it is hard to search for Higgsino in these experiments. In this case, due to a lack of gaugino components, the mass difference between the neutral and charged Higgsinos is uniquely determined by electroweak interactions to be around $350$ MeV, which makes the heavier charged state rather long-lived, with a decay length of about $1$ cm. In this letter, we argue that a charged particle with a flight length of ${\cal O}(1)$ cm can be probed in disappearing-track searches if we require only two hits in the pixel detector. Even in this case, we can reduce background events with the help of the displaced-vertex reconstruction technique. We study the prospects of this search strategy at the LHC and future colliders for the Higgsino dark matter scenario. It is found that an almost pure Higgsino is indeed within the reach of the future $33$ TeV collider experiments. We then discuss that the interplay among collider and non-accelerator experiments plays a crucial role in testing the Higgsino dark matter scenarios. Our strategy for disappearing-track searches can also enlarge the discovery potential of pure wino dark matter as well as other electroweak-charged dark matter candidates.

Figures

Equations

$$\Delta m_{\text{rad}}\simeq \frac{1}{2}{\alpha }_2{m}_Z{\sin }^2{\theta }_w\left(1-\frac{3m_Z}{2\pi m_{{\tilde{\chi }}^{\pm }}}\right),$$

$$\Delta m_0$$

$$\Delta m_{+}$$

$$\Delta m_{\text{tree}}\simeq\frac{v^{2}}{8|\mu|}\Bigl{[}|X|\Delta_{X}+\sin 2\beta\,\text{Re}(Y)\Bigr{]}\,,$$

$$X\equiv {\mu }^{\ast }\left(\frac{g_1^2}{M_1}+\frac{g_2^2}{M_2}\right),Y\equiv {\mu }^{\ast }\left(\frac{g_1^2}{M_1}-\frac{g_2^2}{M_2}\right),$$

$${\sigma }_{\text{SI}}^{(p)}\simeq \frac{4m_{\text{red}}^2{m}_p^2}{\pi v^4{m}_h^4}{F}_{\text{mat}}^2\Delta m_{\text{tree}}^{2}F(X,Y{)}^2,$$

$$F(X,Y)\equiv \frac{|X|{\Delta }_X+\sin 2\beta \text{Re}(X)}{|X|{\Delta }_X+\sin 2\beta \text{Re}(Y)},$$

$$\Delta m_{\text{tree}}\simeq\frac{170~{}\text{MeV}}{F(X,Y)}\left(\frac{m_{p}}{m_{\text{red}}}\right)\biggl{(}\frac{\sigma_{\text{SI}}^{(p)}}{10^{-48}~{}\text{cm}^{2}}\biggr{)}^{\frac{1}{2}}~{}.$$

$$d_e^{h\gamma }$$

$$d_e^{WW}$$

$$f_0(r)=r{\int }_0^1\frac{dx}{r-x(1-x)}\ln \left(\frac{r}{x(1-x)}\right),$$

$$\displaystyle d_{e}\simeq 3\times 10^{-31}\cdot\sin(2\beta)\biggl{(}\frac{1~{}\text{TeV}}{|\mu|}\biggr{)}\biggl{(}\frac{\Delta m_{\text{tree}}}{100~{}\text{MeV}}\biggr{)}F_{\text{ph}}~{}e\text{cm}~{},$$

$$c\tau \simeq 0.7\text{cm}\times {\left[{\left(\frac{\Delta m_{+}}{340\text{MeV}}\right)}^3\sqrt{1-\frac{m_{\pi }^2}{\Delta m_{+}^2}}\right]}^{-1},$$

Full text

††preprint: IPMU 17-0050††preprint: UT-17-11††preprint: KYUSHU-RCAPP-2017-03

I Introduction

The strongest motivation for new physics beyond the Standard Model (SM) is dark matter (DM) in the Universe. Among a variety of DM candidates, weakly-interacting massive particles (WIMPs) offer the most attractive paradigm to explain the observed DM density: $\Omega_{\rm DM}h^{2}\simeq 0.12$ Ade et al. (2016).

Higgsino in a supersymmetric (SUSY) extension of the SM, which is an SU(2)L doublet fermion with hypercharge $1/2$, is a prime example of WIMP DM. The neutral component of Higgsino can mix with the neutral electroweak-inos, bino and wino, and if the dominant portion of the lightest state is Higgsino, then it is called a Higgsino-like state. The amount of the gaugino fractions in a Higgsino-like state strongly affects its phenomenological property. If the masses of SUSY particles other than Higgsino, especially those of the electroweak-inos, are in the multi-TeV region, then the gaugino fraction is quite suppressed and thus the lightest SUSY particle (LSP) can be regarded as an almost pure Higgsino. Such a “split” mass spectrum has various phenomenological and theoretical advantages Wells (2003); *Wells:2004di; Arkani-Hamed and Dimopoulos (2005); *Giudice:2004tc; *ArkaniHamed:2004yi; *ArkaniHamed:2005yv, and thus attracts wide attention Hall and Nomura (2012); *Hall:2012zp; *Nomura:2014asa; Ibe and Yanagida (2012); *Ibe:2012hu; Arvanitaki et al. (2013); Arkani-Hamed et al. (2012); Evans et al. (2013a); *Evans:2013dza; *Evans:2014pxa especially after the discovery of the 125 GeV Higgs boson Aad et al. (2012a); *Chatrchyan:2012ufa; *Aad:2015zhl. The gaugino fraction may be small, but non-accelerator experiments such as DM direct searches and measurements of the electric dipole moments (EDMs) can probe it. As we discuss below, even the gauginos heavier than $\mathcal{O}(10)\,\text{TeV}$ can be probed in future experiments Nagata and Shirai (2015a).

Another motivation for SU(2)L doublet DM is provided by a bottom-up approach. Classifying possible DM candidates in terms of their quantum numbers, we find that an SU(2)L doublet with hypercharge $1/2$ or triplet with hypercharge zero has minimal non-zero electric charge to accommodate electrically neutral DM. Hence, SU(2)L doublet DM is a promising target even though we do not consider SUSY as new physics beyond the SM.

However, SU(2)L doublet fermion DM as it is, which corresponds to completely pure Higgsino DM, has already been excluded by DM direct detection experiments. In this case, the DM is a Dirac fermion, and thus has vector interactions with quarks via the $Z$-boson exchange, which results in a too large DM-nucleon spin-independent (SI) scattering cross section Akerib et al. (2017); *Tan:2016zwf. To avoid this constraint, we need some effects induced at higher energies that generate a mass split between the Dirac DM components, $\Delta m_{0}$, to divide it into two Majorana fermions $\widetilde{\chi}^{0}_{1,2}$, which do not have vector interactions. To assure this, we need $\Delta m_{0}\gtrsim\mathcal{O}(100)\,\text{keV}$ Nagata and Shirai (2015a); otherwise, the inelastic scattering process $\widetilde{\chi}^{0}_{1}N\to\widetilde{\chi}^{0}_{2}N$ ($N$ denotes a nucleon) instead gives a too large scattering cross section. Generically, the interactions that yield $\Delta m_{0}$ should be induced at a scale $\Lambda\lesssim 10^{9}$ GeV to give $\Delta m_{0}\gtrsim\mathcal{O}(100)\,\text{keV}$ Nagata and Shirai (2015a, b). Such effects are actually similar to the contribution of gaugino fractions to the property of the Higgsino DM. Thus, this $\text{SU}(2)_{L}$ DM can also be probed in future non-accelerator experiments if the scale $\Lambda$ is relatively low. Notice that bounds from these experiments give a lower limit on $\Lambda$, while the inelastic-scattering bound gives an upper limit.

We however find that there is a range of $\Lambda$ which is high enough for the SU(2)L doublet fermion DM to be beyond the reach of these experiments but low enough to give $\Delta m_{0}\gtrsim\mathcal{O}(100)\,\text{keV}$ Nagata and Shirai (2015a, b)—correspondingly, we can find appropriately large gaugino masses with which the same situation is realized for Higgsino DM. This situation is completely viable, as the thermal relic abundance of pure Higgsino DM agrees with $\Omega_{\text{DM}}h^{2}\simeq 0.12$ if the Higgsino DM mass $m_{\text{DM}}$ is $\sim 1.1$ TeV Cirelli et al. (2007). A lighter mass region is also promising since there may be non-thermal contribution from high-energy physics, such as late-time decay of gravitinos. Therefore, it is quite important to consider an alternative strategy to probe such almost pure Higgsino DM.

It has been known that almost pure Higgsino is also difficult to probe at hadron colliders Han et al. (2014); Ismail et al. (2016). In this case, not only the neutral states $\widetilde{\chi}^{0}_{1,2}$, but also the charged states $\widetilde{\chi}^{\pm}$ are almost degenerate in mass at tree level. The charged states acquire a slightly heavier mass via the electroweak loop corrections, but still the mass splitting is as small as $\sim 350$ MeV. Due to this small mass splitting, the decay products of $\widetilde{\chi}^{\pm}$ have soft momenta, which makes it hard to detect them. For this reason, the current LHC searches for Higgsinos rely only on mono-jet or mono-$X$ signals, which give poor constraints on Higgsinos due to large SM background (BG). Even a 100 TeV collider can test a small portion of parameter space in the Higgsino DM scenario Low and Wang (2014); *Gori:2014oua; *Arkani-Hamed:2015vfh; *Golling:2016gvc.

However, this small mass splitting may offer a different strategy to probe Higgsinos at colliders. Because of the small mass splitting, the charged Higgsino has rather long lifetime—as it turns out, a mass difference of $\sim 350$ MeV results in a decay length of $\sim 1$ cm. It is therefore interesting to ask whether charged tracks with an ${\cal O}(1)$ cm length can be detected at collider experiments. In this letter, we address this question by taking into account potential improvements in disappearing track searches with fully optimized inner detectors at the LHC and a future 33 TeV collider. Such an improvement may also increase the discovery potential of pure wino DM; thus, we also consider the wino DM case for comparison.

II Higgsino Phenomenology

To begin with, we discuss the mass spectrum of Higgsino components, paying particular attention to the gaugino mass effects on it. The masses of these components split after the electroweak symmetry is broken. These mass splittings are induced by the tree-level mixing with the electroweak-inos, as well as the electroweak radiative corrections. We here assume that the masses of the electroweak-inos are much larger than the TeV scale. At one-loop level, the electroweak-loop contribution to the charged-neutral mass splitting is given by

[TABLE]

where $\alpha_{2}\equiv g_{2}^{2}/4\pi$ with $g_{2}$ the SU(2)L gauge coupling constant, $m_{Z}$ is the $Z$-boson mass, $\theta_{w}$ is the Weinberg angle, and $m_{\widetilde{\chi}^{\pm}}$ is the charged Higgsino mass. We find $\alpha_{2}m_{Z}\sin^{2}\theta_{w}/2\simeq 355$ MeV. After all, the mass difference between the neutral components, $\Delta m_{0}$, and that between the charged component and the Higgsino LSP, $\Delta m_{+}$, are respectively given by

[TABLE]

with

[TABLE]

where $v\simeq 246$ GeV is the Higgs VEV, $\mu$ is the Higgsino mass, $\tan\beta\equiv\langle H_{u}\rangle/\langle H_{d}\rangle$ with $H_{u}$ and $H_{d}$ being the up- and down-type Higgs fields, respectively,

[TABLE]

$\Delta_{X}\equiv\sqrt{1-\sin^{2}\theta_{X}\sin^{2}2\beta}$, $\theta_{X}\equiv\text{arg}(X)$, $M_{1}$ ($M_{2}$) is the bino (wino) mass, and $g_{1}$ is the $\text{U}(1)_{Y}$ gauge coupling. As we discussed above, $\Delta m_{0}\gtrsim\mathcal{O}(100)\,\text{keV}$ is required to suppress the SI inelastic DM-nucleon scattering via the $Z$-boson exchange.

Even in this case, the Higgsino-nucleon SI scattering occurs via the Higgs-boson exchange process induced by the electroweak-ino mixing. The resultant SI scattering cross section with a proton, for instance, is evaluated as

[TABLE]

with

[TABLE]

where $m_{p}$ is the proton mass, $m_{h}\simeq 125$ GeV is the Higgs mass, $m_{\text{red}}\equiv m_{p}m_{\text{DM}}/(m_{p}+m_{\text{DM}})$, $F_{\text{mat}}\equiv\sum_{q=u,d,s}f_{T_{q}}+2f_{T_{G}}/9$, $f_{T_{G}}\equiv 1-\sum_{q=u,d,s}f_{T_{q}}$, and the mass fractions $f_{T_{q}}$ are computed with a QCD lattice simulation as $f_{T_{u}}=0.0149$, $f_{T_{d}}=0.0234$, and $f_{T_{s}}=0.0440$ Abdel-Rehim et al. (2016). In the derivation of Eq. (6), we have dropped the electroweak-loop contribution to the SI scattering cross section, which is found to be negligible for almost pure Higgsino DM Hisano et al. (2015). Using this expression, we find a relation between the SI scattering cross section and the tree-level charged-neutral mass splitting $\Delta m_{\text{tree}}$:

[TABLE]

This equation shows that for a value of $\sigma_{\text{SI}}^{(p)}$ that exceeds the neutrino floor Billard et al. (2014), which lies around $10^{-48}~{}\text{cm}^{2}$ for a DM mass of ${\cal O}(100)$ GeV, the charged-neutral mass splitting is expected to be larger than a few hundred MeV.

In general, the electroweak-ino contribution yields CP violation, which then induces EDMs of the SM particles. Currently, the electron EDM, $d_{e}$, is most stringently restricted: $|d_{e}|<8.7\times 10^{-29}~{}e\text{cm}$ Baron et al. (2014). The Higgsino contribution to the electron EDM is induced by the two-loop Barr–Zee diagrams Barr and Zee (1990); Chang et al. (2005); *Deshpande:2005gi; *Giudice:2005rz and given by the sum $d_{e}=d_{e}^{h\gamma}+d_{e}^{hZ}+d_{e}^{WW}$, where $d_{e}^{h\gamma}$, $d_{e}^{hZ}$, and $d_{e}^{WW}$ are the Higgs-$\gamma$, Higgs-$Z$, and $WW$ loop contributions, respectively. We find Nagata and Shirai (2015a)

[TABLE]

with $f_{0}^{h,W}=f_{0}(|\mu|^{2}/m_{h,W}^{2})$ and

[TABLE]

where $m_{e}$ is the electron mass, $m_{W}$ is the $W$-boson mass, and $e$ is the positron charge. For the electron EDM, $d_{e}^{hZ}$ is always subdominant due to an accidentally small numerical factor Nagata and Shirai (2015a). Using this expression, we can again relate $d_{e}$ with the mass splitting $\Delta m_{\text{tree}}$ as

[TABLE]

where $F_{\text{ph}}$ is the sum of the factors in the parentheses in Eq. (9). By noting that future experiments may probe $d_{e}\sim 10^{-31}~{}e\text{cm}$ Vutha et al. (2010); Hudson et al. (2011), we find that a Higgsino with $\Delta m_{\text{tree}}\gtrsim 100$ MeV can be tested in EDM experiments.

As we have seen above, a Higgsino with $\Delta m_{\text{tree}}>{\cal O}(100)$ MeV can be tested in future non-accelerator experiments. On the other hand, an almost pure Higgsino with $\Delta m_{\text{tree}}$ (much) smaller than $\sim 100$ MeV is beyond the reach of these experiments. It is also challenging to probe such Higgsinos in DM indirect searches, or mono-jet/$X$ searches at the LHC. However, as we mentioned above, in this case we may search for Higgsinos using disappearing tracks at the LHC, since $\widetilde{\chi}^{\pm}$ becomes rather long-lived due to the small mass difference $\Delta m_{+}$. The decay length of $\widetilde{\chi}^{\pm}$ is approximately Chen et al. (1996); *Thomas:1998wy

[TABLE]

where $m_{\pi}$ is the charged pion mass. Hence, we expect that a pure charged Higgsino leaves an ${\cal O}(1)$ cm track in the detector. We will see below that it is indeed possible to detect an ${\cal O}(1)$ cm disappearing track at colliders.

III Disappearing track searches

Disappearing track searches highly rely on the performance of silicon pixel detectors. The CMS detector has three barrel layers of pixel detectors in a magnetic field of 3.8 T at radii of 4.4 cm, 7.3 cm, and 10.2 cm with a pixel size of $100\times 150~{}\mu\text{m}^{2}$ Chatrchyan et al. (2008) 111Recently, the CMS collaboration has replaced the pixel detectors with four layers at radii 2.9 cm, 6.8 cm, 10.9 cm and 16.0 cm Tavolaro (2016).. The ATLAS Pixel detector is located in a magnetic field of 2 T and consists of four barrel layers at radii of 3.3 cm, 5.05 cm, 8.85 cm, and 12.25 cm ATLAS Collaboration (2008). The innermost layer in the ATLAS Pixel detector system called Insertable B-Layer (IBL) Capeans et al. (2010), which was installed before the LHC Run 2 started, has a pixel size of $50\times 250~{}\mu\text{m}^{2}$, while the other layers have a pixel size of $50\times 400~{}\mu\text{m}^{2}$. For concreteness, we mainly consider the ATLAS setup in this section.

The current disappearing track searches by the ATLAS collaboration,222The CMS Run-1 study can be found in Ref. Khachatryan et al. (2015). whose main target is a long-lived charged wino, require four hits in the silicon detectors. Thus, at the LHC Run 1, a target charged particle needs to fly at least 29.9 cm, which corresponds to the location of the innermost layer of the silicon strip detector called SemiConductor Track (SCT), to pass this selection. This Run-1 analysis excludes a pure charged wino with a mass of less than $270$ GeV Aad et al. (2013a). Thanks to the IBL, the required minimum flight length of target particles was shorten (12.25 cm) at the Run 2, giving much better sensitivity to a pure charged wino, which has a decay length of $\sim 6$ cm. The current mass limit on a pure charged wino is $430$ GeV Kaji (2017); *moriond17conf.

A similar strategy may be adopted for charged Higgsino searches. As shown in Eq. (12), an almost pure charged Higgsino has a decay length of $\sim 1$ cm, which suggests us to focus on shorter tracks. To optimize the search strategy for this case, we here require only two hits in the Pixel detector. In addition to these two hits, a reconstructed primary vertex may be utilized to determine the momentum of a disappearing track. Note that the resolution of the position of a primary vertex is ${\cal O}(10)~{}\mu\text{m}$ ATL (2015); *moriond17DV, which is the same order as that of the Pixel detector. Figure 1 illustrates the configuration of the ATLAS inner tracker, where required numbers of hits in the detector are shown by red blobs for the analyses of the ATLAS Run-1&2 and ours. As shown in this figure, our search strategy allows the ATLAS detector to probe a disappearing track with a length of $\gtrsim 5$ cm.

According to the ATLAS Run-2 analysis Kaji (2017); *moriond17conf, there are three classes of BG events in this search: hadrons that scatter with the detector, leptons whose flight direction is bent with Bremsstrahlung, and fake tracks due to mis-identification of hit points. The total number of remaining BG events after the selection cut is expected to be $11.8\pm 3.1$ in the electroweak production channel in the Run-2 study Kaji (2017); *moriond17conf.

As we have reduced the number of hits in the silicon detector, the resolution of the transverse momentum of a disappearing track ($P^{\text{dis}}_{\text{T}}$) may be worse than the current one, $\Delta(1/P_{\text{T}}^{\text{dis}})\sim 10~{}{\rm TeV}^{-1}$. Since $\Delta(1/P_{\text{T}}^{\text{dis}})\propto L^{-2}$ with $L$ the track length, we expect $\Delta(1/P_{\text{T}}^{\text{dis}})\sim 30~{}{\rm TeV}^{-1}$ for our two-hit method. This means that if a disappearing track has $P^{\text{dis}}_{\text{T}}\gtrsim 30$ GeV, its momentum can no longer be measured accurately. This poor momentum resolution may increase the number of BG events significantly.

Meanwhile, these BG events may be reduced with the help of reconstruction of displaced tracks. This technique itself has already been established in the long-lived particle searches with displaced vertices (DVs) Aad et al. (2012b); *Aad:2012zx; *Aad:2015rba with the current reconstruction efficiency of displaced tracks from a radius of 5 cm being about 80% ATLAS (2016). As the hadronic scattering and lepton Bremsstrahlung BG events generally yield a kink signature, these events may be removed efficiently if a DV having a disappearing track and a displaced track is reconstructed. Notice that this requirement scarcely reduces the signal events, since the emitted pion in the charged Higgsino decay is too soft to be reconstructed as a kink signature. The fake-track events may also be resolved with the DV reconstruction, especially those caused by displaced tracks from additional $pp$ interactions, i.e., pile-up events. Moreover, a pixel detector with a reduced pixel size of $25\times 100~{}\mu\text{m}^{2}$ is being developed Lange (2015), which may improve the momentum resolution for a disappearing track in future colliders.

Taking these potential improvements into account, in the following analysis, we use a momentum cut of $P^{\text{dis}}_{\text{T}}>100$ GeV and assume that the number of BG events is not so much increased due to deterioration in the momentum resolution.

IV Result

Now we discuss the prospects of our two-hit method for the long-lived charged Higgsino searches. We use Madgraph5 Alwall et al. (2014), Pythia6 Sjostrand et al. (2006); Sjostrand:2007gs, and Delphes3 de Favereau et al. (2014) for collider simulations and estimate the production cross sections of SUSY particles with Prospino2 Beenakker et al. (1996). We consider the 8 TeV LHC with $20.3$ fb-1* data Aad et al. (2013a), the 13 TeV run with $36.1$ fb*-1* data Kaji (2017); moriond17conf, and the 14-TeV LHC and a future 33 TeV run with an integrated luminosity of $3$ ab-1*. We adopt the same set of kinematic selection criteria as in the Run-1 analysis Aad et al. (2013a), except for the missing energy cut, $E^{\text{miss}}_{\text{T}}>140$ GeV, and the leading-jet transverse momentum cut, $P^{\text{lead}}_{\text{T}}>140$ GeV for the 8 and 13 TeV cases. For the 14 and 33 TeV cases, we require $E_{\text{T}}^{\text{miss}},P^{\text{lead}}_{\text{T}}>400$ GeV and 600 GeV, respectively. As mentioned above, for the selection of disappearing track candidates, we require two hits in the silicon tracker with $P^{\text{dis}}_{\text{T}}>100$ GeV. To estimate the number of BG events for each case, we rescale the observed number of BG events in the ATLAS Run-2 study Kaji (2017); *moriond17conf according to the event rates of the $W+\text{jets}$ and $t\bar{t}$ processes. We find that the expected number of BG events is $\sim 10$ for these cases.

In Fig. 2, we show the expected limits from the 8 TeV, 13 TeV, 14 TeV, and 33 TeV searches in the yellow dot-dashed line, the blue dashed line, the green dashed band, and the red bands, respectively. For the 33 TeV run, we assume that the second layer of a pixel detector is located at a radius of 5 and 3 cm for the upper and lower bands, respectively. The upper (lower) line of each band corresponds to ten (zero) BG events. The systematic error in BG expectation is assumed to be $10~{}\%$. In addition, we show the decay lengths of Higgsino with $\Delta m_{\text{tree}}=0$, 75, and 150 MeV in black dotted lines from top to bottom. The vertical blue stripe at $\sim 1.1$ TeV indicates the favored mass value for pure Higgsino DM in terms of thermal relic abundance Cirelli et al. (2007). This figure shows that the Run-2 data already have a sensitivity to pure Higgsino. The reach of the high-luminosity LHC is expected to be 500–600 GeV. Moreover, a future 33 TeV $pp$ collider may probe pure Higgsino with a mass of $\gtrsim 1$ TeV, with which we can test the pure Higgsino DM scenario.

Our two-hit search strategy can also extend the reach of charged wino searches. To see this, we perform a similar analysis for the wino LSP and show the results in Fig. 3. The colors and types of the lines and stripes are the same as in Fig. 2. The 8 TeV and 13 TeV limits in this figure are taken from Refs. Aad et al. (2013a); Kaji (2017); *moriond17conf. It is found that the reach of the high-luminosity LHC for a pure wino can exceed 1 TeV. A future 33 TeV collider may probe a pure wino with a mass of $\gtrsim 2.5$ TeV, where (the most of) the observed DM density is explained by the thermal relic abundance of the wino LSP Hisano et al. (2007).

Finally, we note in passing that our two-hit search may probe Higgsino and wino up to 1.7 TeV and 4 TeV or even larger, respectively, at a 100 TeV collider with an integrated luminosity of 3 ab*-1*.

V Conclusion and discussion

In this letter, we have discussed the testability of the Higgsino DM scenario. We have seen that a wide region of parameter space for the Higgsino DM scenario can be probed in future non-accelerator experiments. However, if the electroweak-inos are so heavy that the tree-level charged-neutral Higgsino mass difference is less than ${\cal O}(100)$ MeV, Higgsinos may escape from these non-accelerator searches. To probe such cases, in this paper, we propose a new collider search strategy for almost pure Higgsinos based on the first two layers of the Pixel detector, which is sensitive to ${\cal O}(1)$ cm disappearing tracks. We have found that using this two-hit search method we can probe 1 TeV pure Higgsino, whose thermal relic abundance agrees with $\Omega_{\text{DM}}h^{2}\simeq 0.12$, at a 33 TeV collider. As a consequence, the non-accelerator experiments and the disappearing track searches play a complementary role in probing Higgsinos, and thus the interplay among these experiments is of great importance to test the Higgsino DM scenario experimentally.

This method can also improve the disappearing track searches for long-lived charged winos. In fact, since pure charged winos have relatively long decay length, $\sim 6$ cm, we expect a number of signal events with the two-hit search strategy. In this case, we may even require two disappearing tracks, which can reduce the SM BG significantly. We also note that this two-hit strategy is useful for the search of other electroweak-charged DM candidates. A detailed study of these searches, as well as the reduction of BG by means of DVs, will be discussed elsewhere Fukuda et al. .

As we have seen, our proposal for the detection of disappearing tracks extends the LHC reach of the Higgsino and wino DM searches significantly. Nonetheless, the mass values favored by thermal relic are beyond the LHC reach, and thus we need a new hadron collider to cover the entire region for the DM scenario. It is worth emphasizing that to maximize the potential of such a collider, not only an increase in the beam energy and luminosity, but also an improvement in the tracker system is of crucial importance, which should be considered seriously when we discuss proposals for future colliders.

Note Added: During the completion of this paper, a related study Mahbubani et al. (2017) was submitted to arXiv where pure Higgsino searches based on disappearing tracks at the LHC and a future 100 TeV collider were discussed on the assumption that a charged track with a length of 10 cm is detectable. We also noticed that the ATLAS collaboration started to study a possibility of using a two-hit strategy to search for long-lived charged winos Kaji et al. (2017).

Acknowledgements.

We are grateful to M. Saito for helpful correspondence. The work of H.O. was supported by JSPS KAKENHI Grant Number 15K17653. The work of S.S. was supported by World Premier International Research Center Initiative (WPI), MEXT, Japan. The work of H.F. is supported in part by a Research Fellowship for Young Scientists from the Japan Society for the Promotion of Science (JSPS).