# Likelihood analysis of supersymmetric SU(5) GUTs

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## Abstract

We perform a likelihood analysis of the constraints from accelerator experiments and astrophysical observations on supersymmetric (SUSY) models with SU(5) boundary conditions on soft SUSY-breaking parameters at the GUT scale. The parameter space of the models studied has seven parameters: a universal gaugino mass \(m_{1/2}\), distinct masses for the scalar partners of matter fermions in five- and ten-dimensional representations of SU(5), \(m_5\) and \(m_{10}\), and for the \(\mathbf {5}\) and \({\bar{\mathbf{5}}}\) Higgs representations \(m_{H_u}\) and \(m_{H_d}\), a universal trilinear soft SUSY-breaking parameter \(A_0\), and the ratio of Higgs vevs \(\tan \beta \). In addition to previous constraints from direct sparticle searches, low-energy and flavour observables, we incorporate constraints based on preliminary results from 13 TeV LHC searches for jets + Open image in new window events and long-lived particles, as well as the latest PandaX-II and LUX searches for direct Dark Matter detection. In addition to previously identified mechanisms for bringing the supersymmetric relic density into the range allowed by cosmology, we identify a novel \({\tilde{u}_R}/{\tilde{c}_R} - \tilde{\chi }^{0}_{1}\) coannihilation mechanism that appears in the supersymmetric SU(5) GUT model and discuss the role of \({{\tilde{\nu }}_\tau }\) coannihilation. We find complementarity between the prospects for direct Dark Matter detection and SUSY searches at the LHC.

## 1 Introduction

In the absence so far of any experimental indications of supersymmetry (SUSY) [1, 2, 3, 4, 5, 6, 7, 8, 9], nor any clear theoretical guidance how SUSY may be broken, the building of models and the exploration of phenomenological constraints on them [10, 11, 12, 13, 14, 15, 16, 17] have adopted a range of assumptions. One point of view has been to consider the simple parametrization of soft SUSY breaking in which the gaugino and scalar masses, as well as the trilinear soft SUSY-breaking parameters, are all constrained to be universal at the SUSY GUT scale (the CMSSM [10, 11, 12, 13, 18, 19, 20, 21, 22, 23, 24, 25, 26, 27, 28, 29, 30, 31, 32, 33, 34, 35, 36, 37, 38, 39, 40, 41, 42, 43, 44, 45]). An alternative point of view has been to discard all universality assumptions, and treat the soft SUSY-breaking parameters as all independent phenomenological quantities (the pMSSM [15, 46, 47, 48, 49, 50, 51, 52, 53, 54, 55, 56, 57, 58, 59, 60, 61, 62, 63, 64]), imposing diagonal mass matrices and the minimal flavour violation (MFV) criterion. Intermediate between these extremes, models with one or two non-universal soft SUSY-breaking contributions to Higgs masses (the NUHM1 [10, 11, 12, 13, 65, 66, 67, 68, 69] and NUHM2 [14, 67, 68, 69, 70, 71]) have also been considered.

It is interesting to explore also models that are less simplified than the CMSSM, but not as agnostic as the pMSSM, in that they incorporate a limited number of simplifying assumptions. GUTs motivate the assumption that the gaugino masses are universal, and constraints on flavour-changing neutral interactions suggest that the soft SUSY-breaking masses for scalars with identical quantum numbers are also universal. However, there is no compelling phenomenological reason why the soft SUSY-breaking masses for scalars with different quantum numbers should be universal.

Specific GUTs may also provide some guidance in this respect. For example, in an SO(10) GUT the scalar masses of all particles in a given generation belonging to a single \(\mathbf {16}\) representation of SO(10) would be universal, as would those for the \(\mathbf {5}\) and \({\bar{\mathbf{5}}}\) SU(5) Higgs representations that belong to a single \(\mathbf {10}\) of SO(10) and break electroweak symmetry, as in the NUHM1. In contrast, the SU(5) framework is less restrictive, allowing different masses for scalars in \({\bar{\mathbf{5}}}\) and \(\mathbf {10}\) representations [72], and also for the \(\mathbf {5}\) and \({\bar{\mathbf{5}}}\) Higgs representations. Thus it is a 1-parameter extension of the NUHM2. In this paper we explore the theoretical, phenomenological, experimental and cosmological constraints on this SU(5)-based SUSY GUT model.

This relaxation of universality is relevant for the evaluation of several different constraints from both the LHC and elsewhere. For example, the most powerful LHC constraints on the CMSSM, NUHM1 and NUHM2 are those from the classic Open image in new window searches [1, 2, 3, 6, 7, 8]. These constrain principally the right-handed squarks, whose decays are dominated by the \({\tilde{q}_R} \rightarrow q \,\tilde{\chi }^{0}_{1}\) channel that maximizes the Open image in new window signature. On the other hand, the decay chains of left-handed squarks are more complicated, typically involving the \(\tilde{\chi }^{\pm }_{1}\), resulting in a dilution of the Open image in new window signature and more importance for final states including leptons. In a SUSY SU(5) GUT, the left-handed squarks and the right-handed up-type squarks appear in \(\mathbf {10}\) representations whereas the right-handed down-type squarks appear in \({\bar{\mathbf{5}}}\) representations, with independent soft SUSY-breaking masses. Hence the impacts of the LHC Open image in new window and other constraints need to be re-evaluated.

The possible difference between the soft SUSY-breaking contributions to the masses of the squarks appearing in a \(\mathbf {10}\) of SU(5), i.e., up-type squarks and left-handed down-type squarks, and those appearing in a \({\bar{\mathbf{5}}}\) of SU(5), i.e., right-handed down-type squarks, offers a new avenue for compressing the stop spectrum. Also, as we shall see, with \(m_5 \ne m_{10}\) there is the possibility that \(m_{{\tilde{u}_R}, {\tilde{c}_R}}\) are much smaller than the other squark masses, leading to another type of compressed spectrum.^{1}

In principle, the constraints from flavour observables may also act differently when \(m_5 \ne m_{10}\). For example, the soft SUSY-breaking masses of the left- and right-handed charge +2/3 quarks are independent, and flavour observables such as BR(\(b \rightarrow s \gamma \)) and \(\mathrm{BR}(B_s \rightarrow \mu ^+\mu ^-)\) depend on both of them, in general.

Another experimental constraint whose interpretation may be affected by the non-universality of scalar masses is \((g-2)_\mu \). A priori, a SUSY explanation of the discrepancy between the Standard Model (SM) prediction and the experimental measurement of \((g-2)_\mu \) requires relatively light smuons, either right- and/or left-handed, which are in \(\mathbf {10}\) and \({\bar{\mathbf{5}}}\) representations, respectively. It is interesting to investigate to what extent the tension between a SUSY interpretation of \((g-2)_\mu \) and the LHC constraints on squarks that is present in more constrained SUSY models could be alleviated by the extra degree of freedom afforded by the \({\bar{\mathbf{5}}}\)–\(\mathbf {10}\) disconnect in SU(5).

Finally, we recall that in large parts of the regions of the CMSSM, NUHM1 and NUHM2 parameter spaces favoured at the 68% CL the relic \(\tilde{\chi }^{0}_{1}\) density is brought into the range allowed by Planck [74] and other data via coannihilation with the stau and other sleptons [75, 76, 77, 78, 79, 80, 81, 82]. In an SU(5) GUT, the left- and right-handed sleptons are in different representations, \({\bar{\mathbf{5}}}\) and \(\mathbf {10}\), respectively. Hence they have different masses, in general, providing more flexibility in the realization of coannihilation. Specifically, as mentioned above, the freedom to have \(m_5 \ne m_{10}\) allows the possibility that the right-handed up- and charm-flavour squarks, \({\tilde{u}_R}\) and \({\tilde{c}_R}\), are much lighter than the other squarks, opening up the novel possibility of \({\tilde{u}_R}/{\tilde{c}_R} - \tilde{\chi }^{0}_{1}\) coannihilation, as we discuss below.

Our analysis of the available experimental constraints largely follows those in our previous studies of other variants of the MSSM [10, 11, 12, 13, 14, 15, 16, 17], the main new feature being that we incorporate the constraints based on the preliminary results from LHC searches for jets \(+\) Open image in new window events with \({\sim } 13\)/fb of data at 13 TeV [9]. For this purpose, we recast available results for simplified models with the mass hierarchies \(m_{\tilde{g}}\gg m_{\tilde{q}}\) and vice versa. We also include the preliminary constraints from LHC searches in 13-TeV data for the heavy MSSM Higgs bosons and long-lived charged particles, and incorporate in combination the recent PandaX [83] and LUX [84] data.

The SUSY SU(5) GUT model we study is set up in Sect. 2, and our implementations of constraints and analysis procedure are summarized in Sect. 3. Section 4 describes how we characterize different Dark Matter (DM) mechanisms, including the novel \({\tilde{u}_R}/{\tilde{c}_R} - \tilde{\chi }^{0}_{1}\) coannihilation mechanism, \({{\tilde{\nu }}_\tau }\) coannihilation and a hybrid possibility. Section 5 contains our results in several model parameter planes, and Sect. 6 describes various one-dimensional likelihood functions including those for several sparticle masses, \((g-2)_\mu \) and various other observables. Higgs boson branching ratios (BRs) are presented in Sect. 7, followed by a comparison of the SU(5) with the NUHM2 results in Sect. 8. The possibility of a long-lived \({\tilde{\tau }}_1\) is discussed in Sect. 9, and the prospects for direct DM detection are discussed in Sect. 10. Finally, Sect. 11 presents a summary and some conclusions.

## 2 Supersymmetric SU(5) GUT model

We assume a universal, SU(5)-invariant gaugino mass parameter \(m_{1/2}\), which is input at the GUT scale, as are the other SUSY-breaking parameters listed below.

*t*quark (and possibly the

*b*quark and the \(\tau \) lepton) that may play an important role in generating electroweak symmetry breaking. In our discussion of flavour constraints, we assume the MFV scenario in which generation mixing is described by the Cabibbo–Kobayashi–Maskawa (CKM) model. This is motivated by phenomenological constraints on low-energy flavour-changing neutral interactions, as is our assumption that the soft SUSY-breaking scalar masses for the different \(\mathbf {10}_i\) and \({\bar{\mathbf{5}}}_i\) representations are universal in generation space, and are denoted by \(m_{10}\) and \(m_{5}\), respectively. In contrast to the CMSSM, NUHM1 and NUHM2, we allow \(m_5 \ne m_{10}\). We assume a universal soft trilinear SUSY-breaking parameter \(A_0\).

We assume the existence of two Higgs doublets \(H_u\) and \(H_d\) in \(\mathbf {5}\) and \({\bar{\mathbf{5}}}\) representations that break electroweak symmetry and give masses to the charge \(+\)2/3 and charge −1/3 and −1 matter fields, respectively. It is well known that this assumption gives a (reasonably) successful relation between the masses of the *b* quark and the \(\tau \) lepton [85, 86, 87], but not for the lighter charge −1/3 quarks and charged leptons. We assume that whatever physics resolves this issue is irrelevant for our analysis, as would be the case, for instance, if corrections to the naive SU(5) mass relations were generated by higher-dimensional superpotential terms [88]. In the absence of any phenomenological constraints, we allow the soft SUSY-breaking contributions to the \(H_u\) and \(H_d\) masses, \(m_{H_u}\) and \(m_{H_d}\), to be different from each other, as in the NUHM2, as well as from \(m_5\) and \(m_{10}\). As in the CMSSM, NUHM1 and NUHM2, we allow the ratio of Higgs vacuum expectation values, \(\tan \beta \), to be a free parameter.

In addition to these electroweak Higgs representations, we require one or more Higgs representations to break the SU(5) GUT symmetry. The minimal possibility is a single \(\mathbf {24}\) representation \(\Sigma \), but we do not commit ourselves to this minimal scenario. It is well known that this scenario has problems with rapid proton decay^{2} and GUT threshold effects on gauge coupling unification. We assume that these issues are resolved by the appearance of additional fields at or around the GUT scale that are otherwise irrelevant for TeV-scale phenomenology. The effective low-energy Higgsino mixing coupling \(\mu \) is a combination of an input bilinear \(H_u H_d\) coupling and possible trilinear and higher-order couplings to GUT-scale Higgs multiplets such as \(H_u \Sigma H_d\). We assume that these combine to yield \(\mu = {\mathcal O}(1) \,\, \mathrm {TeV}\) and positive, without entering into the possibility of some dynamical mechanism, and commenting below only briefly on the case \(\mu < 0\).

## 3 Implementations of constraints and analysis procedure

Our treatments in this paper of many of the relevant constraints follow very closely the implementations in our previous analyses of other supersymmetric models [10, 11, 12, 13, 14, 15, 16]. For the convenience of the reader, we summarise the constraints in Table 1. In the following subsections we review our implementations, highlighting new constraints and instances where we implement constraints differently from our previous work.

### 3.1 Electroweak and flavour constraints

We treat as Gaussian constraints all electroweak precision observables, all *B*-physics and *K*-physics observables except for \(\mathrm{BR}(B_{s, d} \rightarrow \mu ^{+}\mu ^{-})\). The \(\chi ^2\) contribution from \(\mathrm{BR}(B_{s, d} \rightarrow \mu ^{+}\mu ^{-})\), combined here in the quantity \(R_{\mu \mu }\) [13], is calculated using a combination of the CMS [89] and LHCb [90] results described in [91] with the more recent result from ATLAS [92]. We extract the corresponding \(\chi ^2\) contribution in Table 1 by applying to the two-dimensional likelihood provided by the combination of these experiments the minimal flavour violation (MFV) assumption that applies in the SU(5) model. We calculate the elements of the CKM matrix using only experimental observables that are not included in our set of flavour constraints.

Observable | Source | Constraint |
---|---|---|

Th./Ex. | ||

\(\rightarrow \quad \mathbf {m_t}\) [GeV] | [93] | \(\mathbf {173.34\pm 0.76}\) |

\(\Delta \alpha _\mathrm{had}^{(5)}(M_Z)\) | [94] | \(0.02771 \pm 0.00011\) |

\(M_Z\) [GeV] | \(91.1875\pm 0.0021\) | |

\( \Gamma _{Z}\) [GeV] | \(2.4952\pm 0.0023\pm 0.001_\mathrm{SUSY}\) | |

\(\sigma _\mathrm{had}^{0}\) [nb] | \(41.540\pm 0.037\) | |

\(R_l\) | \(20.767\pm 0.025\) | |

\( A_\mathrm{FB}(\ell )\) | \(0.01714\pm 0.00095\) | |

\( A_{\ell }(P_\tau )\) | 0.1465 ± 0.0032 | |

\( R_\mathrm{b}\) | 0.21629 ± 0.00066 | |

\( R_\mathrm{c}\) | 0.1721 ± 0.0030 | |

\( A_\mathrm{FB}({b})\) | 0.0992 ± 0.0016 | |

\( A_\mathrm{FB}({c})\) | 0.0707 ± 0.0035 | |

\( A_{b}\) | 0.923 ± 0.020 | |

\( A_{c}\) | 0.670 ± 0.027 | |

\({A_\mathrm{LR}^{e}}\) | 0.1513 ± 0.0021 | |

\( \sin ^2 \theta _\mathrm{w}^{\ell }(Q_\mathrm{fb})\) | 0.2324 ± 0.0012 | |

\(M_W\) [GeV] | \(80.385 \pm 0.015\pm 0.010_\mathrm{SUSY}\) | |

\( a_{\mu }^\mathrm{EXP} - a_{\mu }^\mathrm{SM}\) | \((30.2 \pm 8.8 \pm 2.0_\mathrm{SUSY})\times 10^{-10}\) | |

\(\rightarrow \quad \mathbf {M_h}\) [GeV] | \(\mathbf {125.09} \pm \mathbf{0.24} \pm \mathbf{1.5}_\mathrm{SUSY}\) | |

\(\rightarrow \quad \mathbf{BR}_{b \rightarrow s \gamma }^\mathrm{EXP/SM}\) | \(\mathbf {1.021} \pm \mathbf {0.066}_\mathrm{EXP} \pm \mathbf {0.070}_\mathrm{TH,SM} \pm \mathbf {0.050}_\mathrm{TH,SUSY}\) | |

\(\rightarrow \quad {\mathbf {R}}_{\mu \mu }\) | | |

\(\rightarrow \quad \) | \(\mathbf {1.02} \pm \mathbf{0.19}_\mathrm{EXP} \pm \mathbf{0.13}_\mathrm{SM}\) | |

\(\rightarrow \quad \mathbf {BR}_{B \rightarrow X_s \ell \ell }^\mathrm{EXP/SM}\) | \(\mathbf {0.99} \pm \mathbf{0.29}_\mathrm{EXP} \pm \mathbf{0.06}_\mathrm{SM}\) | |

\(\rightarrow \quad \mathbf {BR}_{K \rightarrow \mu \nu }^\mathrm{EXP/SM}\) | \(\mathbf {0.9998} \pm \mathbf{0.0017}_\mathrm{EXP} \pm \mathbf{0.0090}_\mathrm{TH}\) | |

\(\rightarrow \quad \mathbf {BR}_{K \rightarrow \pi \nu {\bar{\nu }}}^\mathrm{EXP/SM}\) | \(\mathbf {2.2} \pm \mathbf{1.39}_\mathrm{EXP} \pm \mathbf{0.20}_\mathrm{TH}\) | |

\(\rightarrow \quad \mathbf {\Delta M}_{B_s}^\mathrm{EXP/SM}\) | \(\mathbf {1.016} \pm \mathbf{0.074}_\mathrm{SM}\) | |

\(\rightarrow \quad {\frac{\mathbf {\Delta M}_{B_s}^\mathrm{EXP/SM}}{\Delta \mathbf{M}_{B_{d}}}^\mathrm{EXP/SM}}\) | \(\mathbf {0.84} \pm \mathbf{0.12}_\mathrm{SM}\) | |

\(\rightarrow \quad \mathbf {\Delta \epsilon }_K^\mathrm{EXP/SM}\) | \(\mathbf {1.14} \pm \mathbf{0.10}_\mathrm{EXP+TH}\) | |

\(\rightarrow \quad \mathbf {\Omega _{CDM} h^2}\) | \(\mathbf {0.1186} \pm \mathbf{0.0020}_\mathrm{EXP} \pm \mathbf {0.0024}_\mathrm{TH}\) | |

\(\rightarrow \mathbf {\sigma ^\mathrm{SI}_p}\) | \((\mathbf{m}_{{\tilde{\chi }}_\mathbf{1}^\mathbf{0}}, {\sigma ^\mathrm{SI}_\mathbf{p}})\) | |

\(\rightarrow \quad \) | [130] | |

\(\rightarrow \quad {\tilde{\mathbf{q}}} \rightarrow \mathbf{q} \tilde{\chi }^\mathbf{0}_\mathbf{1} , {\tilde{\mathbf{g}}} \rightarrow f {\bar{f}} \tilde{\chi }^\mathbf{0}_\mathbf{1} \) | [9] | \(\mathbf {\sigma } \cdot \mathrm{BR}\) |

\(\rightarrow \mathbf {H/A \rightarrow \tau ^+ \tau ^-}\) | |

### 3.2 Higgs constraints

We use the combination of ATLAS and CMS measurements of the mass of the Higgs boson: \(M_h= 125.09 \pm 0.24 \,\, \mathrm {GeV}\) [116]. We employ the FeynHiggs 2.11.2 code [109, 110, 111, 112, 113, 114, 115] to evaluate the constraint this imposes on the parameter space, assuming a one-\(\sigma \) theoretical uncertainty of \(1.5 \,\, \mathrm {GeV}\).^{3}

The \(\chi ^2\) contributions of 85 Higgs search channels from the LHC and the Tevatron are evaluated using HiggsSignals, see [136, 137], where a complete list of references can be found. The \(\chi ^2\) contributions from the limits from searches for the heavy neutral MSSM Higgs bosons in the \(H/A \rightarrow \tau ^+\tau ^-\) channels are evaluated using the code HiggsBounds [133, 138, 139, 140], which incorporates the results of CMS searches [132, 133] with \({\sim } 25~\mathrm{fb}^{-1}\) of 8 TeV data. The contributions from the two possible production modes, \(gg \rightarrow H/A\) and \(b \bar{b} \rightarrow H/A\), are combined in a consistent manner, depending on the MSSM parameters. The results from HiggsBounds have been compared with the published CMS analysis, and are in very good agreement [133]. The corresponding \(\chi ^2\) contribution is labelled “2D likelihood” in Table 1. For the corresponding constraint with 13 fb\(^{-1}\) of 13 TeV data, we implement an approximate treatment of the \(\chi ^2\) contribution using the preliminary result of ATLAS [134], as we describe in more detail below. Limits from other Higgs boson searches are not relevant for the investigation in this paper and are therefore not included.

### 3.3 LHC Open image in new window constraints at 13 TeV

ATLAS and CMS have recently announced preliminary results from Open image in new window searches with \({\sim } 13\)/fb of data at 13 TeV, using simplified models for gluino and squark pair production [5, 9]. These searches assume \(m_{\tilde{g}}\ll m_{\tilde{q}}\) and \(m_{\tilde{q}}\ll m_{\tilde{g}}\), respectively, and 100% BRs for the decays \({\tilde{g}}\rightarrow f {\bar{f}} \tilde{\chi }^{0}_{1}\) (\(f = q, b, t\)) and \(\tilde{q}\rightarrow q \tilde{\chi }^{0}_{1}\), respectively, which maximize the possible corresponding Open image in new window signatures. Neither of these assumptions is valid in the SUSY SU(5) GUT model: as we will see in more detail later, the \(m_{\tilde{g}}\) and \(m_{\tilde{q}}\) masses are quite similar in much of the favoured region of parameter space,^{4} and in general other decay modes dilute the Open image in new window signature, although larger-multiplicity final states may compensate through an increase in transverse energy \(H_T\) [141]. These other decay modes populate other search channels including leptons, which we do not consider in this paper as they were of limited importance in our previous analyses of the CMSSM, NUHM1 and NUHM2, having impact only for relatively large squark masses and small \(m_{1/2}\).

*smaller*than in the corresponding simplified model by a factor \({>} 2\) due to the destructive interference between the

*s*-channel gluon exchange diagram and the

*t*-channel squark exchange diagram in \(q \bar{q} \rightarrow {\tilde{g}}{\tilde{g}}\), thus weakening the LHC constraints as discussed below. On the other hand, the \(\tilde{q}\tilde{q}+ \tilde{q}\bar{\tilde{q}}\) cross section (right panel) is generally

*a factor*\(\gtrsim 10\)

*larger*than in the simplified model, except in the \({\tilde{u}_R}/{\tilde{c}_R} - \tilde{\chi }^{0}_{1}\) coannihilation strip at small \(m_{\tilde{u}_R}, m_{\tilde{c}_R}, m_{\tilde{\chi }^{0}_{1}} \sim 500 \,\, \mathrm {GeV}\) and \(m_{1/2} \sim 2500 \,\, \mathrm {GeV}\), to which we return later. The enhancement of the squark cross section is due to the fact that in the squark-neutralino simplified model there is no production mode with total baryon number \(B = 2/3\), \(qq \rightarrow \tilde{q} \tilde{q}\), because gluinos are assumed to be absent. On the other hand, in our model \(m_{\tilde{g}}\sim \min (m_{\tilde{q}})\), and \(qq \rightarrow \tilde{q} \tilde{q}\) (with

*t*-channel \({\tilde{g}}\) exchange) becomes the dominant squark production mode in the large \(m_{\tilde{q}}\) region, due to the valence quark-parton dominance in the proton in the large

*x*regime.

In addition, within the 95% CL region in Fig. 2 we have indicated the dominant (\({>} 50\)%) \({\tilde{g}}\) decays found in our analysis. We note that many model points do not have any decay mode with BR \({>} 50\)% within the 95% CL region and that, for those that do, the dominant decays are two-body \({\tilde{g}}\rightarrow \tilde{q}{\bar{q}}\) modes that were not considered in [9]. Because of this and the fact that the \({\tilde{g}}{\tilde{g}}\) cross section is always smaller than in the gluino simplified model by a factor \(> 2\) (see the left panel of Fig. 1), the LHC 13-TeV Open image in new window constraint from the gluino simplified model has only negligible impact. Our LHC 13-TeV Open image in new window constraint on the gluino mass actually comes indirectly from the squark mass constraint estimated using the squark simplified model discussed below, since the squark and gluino masses are related via renormalization group evolution in the SU(5) model. The left panel in Fig. 2 was obtained before implementing the LHC 13-TeV Open image in new window 95% confidence limit on gluino and squark pair production, while in the right panel this constraint is included. We note that the simplified-model exclusion in this analysis extended to \(m_{\tilde{g}}\lesssim 1650 \,\, \mathrm {GeV}\), below the gluino mass at the pre-LHC 13 TeV best-fit point, and barely reaching the 68% CL contour (solid red line).

Because the \({\tilde{q}_R} \rightarrow q \, \tilde{\chi }^{0}_{1}\) decays are important, and also because the \(\tilde{q}\tilde{q}+ \tilde{q}\bar{\tilde{q}}\) cross section in our sample is much larger than that found at large \(m_{\tilde{q}}\) for \(\tilde{q}\bar{\tilde{q}}\) in the simplified model with \(m_{\tilde{q}}\ll m_{\tilde{g}}\), as seen in the right panel of Fig. 1, we have implemented a recast of this search in our global analysis,^{5} and the comparison between the left panels (without this contribution) and the right panels (with this contribution) in Fig. 3 shows the importance of this constraint.

The aforementioned CMS analysis [9] also looks at three simplified gluino models assuming 100% BR for \(\tilde{g} \rightarrow f \bar{f} {\tilde{\chi }}_1^0\) with \(f = q, b, t\), respectively, and provides corresponding cross-section upper limit maps as a function of \(m_{\tilde{g}}\) and \(m_{{\tilde{\chi }}_1^0}\). We implement these constraints by defining Open image in new window by analogy with Eq. (2).

We also consider the \(pp \rightarrow \tilde{q} \tilde{g}\) process, treating it as follows. This process is only relevant when \(m_{\tilde{q}}\sim m_{\tilde{g}}\). In this regime, if \(m_{\tilde{q}}> m_{\tilde{g}}\) (\(m_{\tilde{g}}> m_{\tilde{q}}\)), \(\tilde{q}\) (\(\tilde{g}\)) tends to decay into \(\tilde{g}\) (\(\tilde{q}\)), radiating soft jets. If these soft jets are ignored, we are left with the \({\tilde{g}}{\tilde{g}}\) (\(\tilde{q}\tilde{q}\)) system. In this approximation, the impact of \(pp \rightarrow \tilde{q} \tilde{g}\) can therefore be estimated by adding an extra contribution \(\sigma _{\tilde{q} \tilde{g}} BR_{\tilde{q} \rightarrow q \tilde{g}}\) (\(\sigma _{\tilde{q} \tilde{g}} BR_{\tilde{g} \rightarrow q \tilde{q}}\)) to \(\sigma _{{\tilde{g}}{\tilde{g}}}\) (\(\sigma _{\tilde{q}\tilde{q}} + \sigma _{\tilde{q}\bar{\tilde{q}}}\)). In general, SUSY searches are designed to look for high \(p_T\) objects, and one loses a small amount of sensitivity by ignoring soft jets. We therefore believe that our implementation of the \(pp \rightarrow \tilde{q} \tilde{g}\) process is conservative.

Finally, we estimate the total \(\chi ^2\) penalty from the LHC 13-TeV Open image in new window constraint to be Open image in new window .^{6}

### 3.4 Constraints on long-lived charged particles

We also include in our analysis LHC constraints from searches for heavy long-lived charged particles (HLCP) that are, in general, relevant to coannihilation regions where the mass difference between the lightest SUSY particle (LSP) and the next-to-lightest SUSY particle (NLSP) may be small and the NLSP may therefore be long-lived. As we discuss below, important roles are played in our analysis by \({\tilde{\tau }}_1\), \(\tilde{\chi }^{\pm }_{1}\) and \(\tilde{u}_R/\tilde{c}_R\) coannihilation, but only in the \({\tilde{\tau }}_1\) case is the NLSP - LSP mass difference small enough to offer the possibility of a long-lived charged particle. We implement in our global analysis the preliminary CMS 13-TeV result [130] using tracking and time-of-flight measurements, based on the recipe and the efficiency map as a function of the pseudo-rapidity and velocity of the HLCP given in [131]. We use Pythia 8 [143] and Atom [144, 145, 146, 147, 148] to generate and analyse the events, and assume that the efficiencies for detecting slow-moving \({\tilde{\tau }}_1\)s are similar at 8 and 13 TeV.^{7} The efficiency contains a lifetime-dependent factor \(\propto \mathrm{exp}(- d m/ p \tau )\), where *d* is a distance \(d \simeq 10\) m that depends on the pseudorapidity, and *m*, *p* and \(\tau \) are the mass, momentum and lifetime of the long-lived particle. This factor drops rapidly for particles with lifetimes \({\lesssim } 10\) ps, corresponding to \(m_{{\tilde{\tau }}_1} - m_{\tilde{\chi }^{0}_{1}} \gtrsim 1.6 \,\, \mathrm {GeV}\).

### 3.5 Constraints on heavy neutral Higgs bosons from Run II

^{8}: \(\chi ^2({H/A \rightarrow \tau ^+ \tau ^-}) = \max ( \chi ^2({ggF}), \chi ^2({bb{\phi }}) )\).

Ranges of the SUSY SU(5) GUT parameters sampled, together with the numbers of segments into which each range was divided, and the corresponding total number of sample boxes. The mass parameters are expressed in TeV units

Parameter | Range | Number of segments |
---|---|---|

\(m_{1/2}\) | (0, 4) | 2 |

\(m_{5}\) | (−2.6, 8) | 2 |

\(m_{10}\) | (−1.3, 4) | 3 |

\(m_{H_u}\) | (−7, 7) | 3 |

\(m_{H_d}\) | (−7, 7) | 3 |

\(A_0\) | (−8, 8) | 1 |

\(\tan {\beta }\) | (2, 68) | 1 |

Total number of boxes | 108 |

### 3.6 Other constraints

The most important other constraint update is that on spin-independent DM scattering. We incorporate in our global fit the recent result published by the PandaX-II experiment [83], which we combine with the new result from the LUX Collaboration [84], as discussed in more detail in Sect. 8.

For the electroweak observables we use FeynWZ [97, 98], and for the flavour constraints we use SuFla [122, 123]. For the Higgs observables, we use FeynHiggs 2.11.2 [109, 110, 111, 112, 113, 114, 115] (including the updates discussed in Sect. 3.2), HiggsBounds 4.3.1 [133, 138, 139, 140] and HiggsSignals 1.4.0 [136, 137]. We calculate the sparticle spectrum using SoftSusy 3.3.10 [151] and sparticle decays using SDECAY 1.3b [152] and StauDecay 0.1 [82]. The DM density and scattering rate are calculated using micrOMEGAs 3.2 [128] and SSARD [129], respectively. Finally, we use SLHALib 2.2 [153, 154] to interface the different codes.

### 3.7 Sampling procedure

As discussed in the previous Section, the SUSY SU(5) GUT model we study has seven parameters: \(m_{1/2}\), \(m_5\), \(m_{10}\), \(m_{H_u}\), \(m_{H_d}\), \(A_0\) and \(\tan {\beta }\). The ranges of these parameters that we scan in our analysis are listed in Table 2. The quoted negative values actually correspond to negative values of \(m^2_5, m^2_{10}, m^2_{H_u}\) and \(m^2_{H_d}\): for convenience, we use the notation \(\mathrm{sign}(m^2) \times \sqrt{|m^2|} \rightarrow m\). The negative values of \(m_5\) and \(m_{10}\) that are included in the scans may be compatible with early-Universe cosmology [155], and yield acceptable tachyon-free spectra. In the portions of the scans with negative values of \(m_{H_u}\) and \(m_{H_d}\), although the effect of the top quark Yukawa coupling in the renormalization group equations is important, it may not be the mechanism responsible for generating electroweak symmetry breaking, since \(m_{H_u}\) and \(m_{H_d}\) are negative already at the input scale.

We sample this parameter space using MultiNest v2.18 [156, 157, 158], dividing the seven-dimensional parameter space into 108 boxes, as also described in Table 2. This has two advantages: it enables us to run MasterCode on many nodes in parallel, and it enables us to probe more efficiently for local features in the likelihood function. For each box, we choose a prior such that 80% of the sample has a flat distribution within the nominal range, while 20% of the sample is in normally distributed tails outside the box. Our resultant total sample overlaps smoothly between boxes, avoiding any spurious features at the box boundaries. The total number of points in our sample is \({\sim } 125 \times 10^6\), of which \({\sim } 8 \times 10^6\) have \(\Delta \chi ^2 < 10\).

## 4 Dark matter mechanisms

*R*-parity, may be brought into the narrow range allowed by the Planck satellite and other measurements [74] via a combination of different mechanisms. It was emphasized previously [16] in studies of the CMSSM, NUHM1 and NUHM2 that simple annihilations of pairs of LSPs into conventional particles would not have been sufficient to bring the relic \(\tilde{\chi }^{0}_{1}\) density down into the Planck range for values of \(m_{\tilde{\chi }^{0}_{1}}\) compatible with the LHC search limits and other constraints on these models. Instead, there has to be some extra mechanism for suppressing the LSP density. Examples include enhanced, rapid annihilation through direct-channel resonances such as

*Z*,

*h*,

*H*/

*A*. Another possibility is coannihilation with some other, almost-degenerate sparticle species [18, 159, 160, 161, 162]: candidates for the coannihilating species identified in previous studies include the \({\tilde{\tau }}_1, {\tilde{\mu }}, {\tilde{e}}, {{\tilde{\nu }}}, {\tilde{t}_1}\) and \(\tilde{\chi }^{\pm }_{1}\).

^{9}:

*H*/

*A*funnel mechanisms may be relevant simultaneously:

## 5 Results

### 5.1 Parameter planes

We display in Fig. 4 features of the global \(\chi ^2\) function for the SUSY SU(5) GUT model in the \((m_5, m_{1/2})\) plane (left panel) and the \((m_{10}, m_{1/2})\) plane (right panel), profiled over the other model parameters.^{10} Here and in subsequent parameter planes, the best-fit point is shown as a green star, the 68% CL regions are surrounded by red contours, and the 95% CL regions are surrounded by blue contours (as mentioned above, we use the \(\Delta \chi ^2 = 2.30\) and \(\Delta \chi ^2 = 5.99\) contours as proxies for the boundaries of the 68 and 95% CL regions in the fit). The regions inside the 95% CL contours are shaded according to the dominant DM mechanisms discussed in the previous section, see the criteria (4, 6, 7). In the (relatively limited) unshaded regions there is no single dominant DM mechanism.

As we see in Fig. 4, the best-fit point is at relatively small values of \(m_5, m_{10}\) and \(m_{1/2}\), close to the lower limit on \(m_{1/2}\), whereas the 68% CL region extends to much larger values of \(m_5, m_{10}\) and \(m_{1/2}\). The values of the model parameters at the best-fit point are listed in Table 3.^{11} The upper row of numbers are the results from the current fit including the latest LHC 13-TeV and PandaX-II/LUX constraints, and the numbers in parentheses in the bottom row were obtained using instead the previous LHC 8-TeV and XENON100 constraints, but the same implementations of the other constraints. The most significant effect of the new LHC data has been to increase the best-fit value of \(m_{1/2}\) by \({\sim } 160 \,\, \mathrm {GeV}\): the changes in the other fit parameters are not significant, in view of the uncertainties. As we discuss in more detail later, the favoured fit regions are driven by the \((g-2)_\mu \) constraint towards the boundary of the region excluded by the Open image in new window constraint. Away from this boundary, the global \(\chi ^2\) function is quite flat.

*H*/

*A*poles is dominant. We also see darker shaded hybrid regions where \({\tilde{\tau }}_1\) and

*H*/

*A*annihilation are important simultaneously. At larger values of \(m_{1/2} \gtrsim 3000 \,\, \mathrm {GeV}\), in the green shaded regions, the dominant DM mechanism is \(\tilde{\chi }^{\pm }_{1} - \tilde{\chi }^{0}_{1}\) coannihilation. There is also a band in the \((m_{10}, m_{1/2})\) plane with \(m_{10} \gtrsim 1500 \,\, \mathrm {GeV}\) and \(m_{1/2} \sim 1000 \,\, \mathrm {GeV}\), allowed at the 95% CL, where \({{\tilde{\nu }}_\tau }^\mathrm{NLSP}\) coannihilation is important.

Parameters of the best-fit point in the SUSY SU(5) GUT model, with mass parameters given in GeV units. The numbers in parentheses in the bottom row are for a fit that does not include the LHC 13-GeV constraints and the recent PandaX-II and LUX constraints on DM scattering. Note that we use the same convention for the sign of \(A_0\) as in [10, 11, 12, 13, 14, 15, 16], which is opposite to the convention used in, e.g., SoftSUSY, and that we use the notation \(\mathrm{sign}(m^2) \times \sqrt{|m^2|} \rightarrow m\) for \(m_5, m_{10}, m_{H_u}\) and \(m_{H_d}\)

\(m_{1/2}\) | \(m_5\) | \(m_{10}\) | \(m_{H_u}\) | \(m_{H_d}\) | \(A_0\) | \(\tan {\beta }\) |
---|---|---|---|---|---|---|

1050 | −220 | 380 | −5210 | −4870 | −5680 | 12 |

(890) | (−80) | (310) | (−4080) | (−4420) | (5020) | (11) |

*Q*the renormalization scale and \(Q_0\) some reference scale,

*S*sums over the generations. The \({\tilde{u}_R}/{\tilde{c}_R} - \tilde{\chi }^{0}_{1}\) coannihilation mechanism becomes important in a region of the SUSY SU(5) GUT parameter space where \(m_5^2\) is very large and positive (\({\sim } 27\) TeV\(^2\)), \(m_{10}^2\) is small and negative (\({\sim } -1.4\) TeV\(^2\)), \(m_{H_u}^2\) is very large and negative (\({\sim } -23\) TeV\(^2\)), and \(m_{H_d}^2\) is very large and positive (\({\sim } 50\) TeV\(^2\)). In this region, therefore, \(X_t\) is very large and negative (\({\sim } -35\) TeV\(^2\)), \(X_b\) and \(X_\tau \) are suppressed because of small Yukawa couplings (\(\tan {\beta }\) is not large in this region), and

*S*is also very large and negative (\({\sim } -73\) TeV\(^2\)), since \(m_{H_u}^2 - m_{H_d}^2\) is large and negative and \(\mathrm{Tr} (m^2_q - m^2_l - 2 m^2_{u^c} + m^2_{d^c} + m^2_{e^c} )\) vanishes at the GUT scale. Inspection shows that the \(X_t\) terms in (8) and (9) drive the stop and sbottom masses upwards, and the

*S*terms in (8) and (10) drive the left-handed squark and right-handed slectron masses upwards. On the other hand, the

*S*term in (9) drives the right-handed squark masses downwards. Since there are no counteracting

*X*terms for the \({\tilde{u}_R}\) and \({\tilde{c}_R}\), these have lower masses than the other sfermions, opening the way to a \({\tilde{u}_R}/{\tilde{c}_R} - \tilde{\chi }^{0}_{1}\) coannihilation region.

^{12}

As discussed in more detail later, we used the Atom [144, 145, 146, 147, 148] simulation code for a dedicated verification that points in this region escape all the relevant LHC constraints. These points avoid exclusion by the LHC constraints through a combination of a strong mass degeneracy, \(m_{{\tilde{u}_R}/{\tilde{c}_R}} - m_{\tilde{\chi }^{0}_{1}} \lesssim 50 \,\, \mathrm {GeV}\), leading to strong suppression of the standard Open image in new window signature, and the reduction of the production rate compared to the simplified model that assumes mass degeneracy of all eight light flavour squarks (see Fig. 1). These effects are clearly visible in Fig. 18 of [4].

Figure 5 displays the corresponding information in the \((m_5, m_{10})\) plane of the SUSY SU(5) GUT model. As already reported in Table 3, here we see directly that the best-fit point has very small (and slightly negative) \(m_5\), and that \(m_{10}\) is somewhat larger, exploiting the possibility that \(m_5 \ne m_{10}\), which is offered in this model. We also see again that the 68% CL region extends to values of \(m_5\) and \(m_{10}\) beyond the \({\tilde{\tau }}_1\) coannihilation region. We also note that in most of the rest of this plane \(\tilde{\chi }^{\pm }_{1} - \tilde{\chi }^{0}_{1}\) coannihilation is dominant, with only scattered regions where rapid *H* / *A* annihilation is important, even in combination with \({\tilde{\tau }}_1\) coannihilation.

^{13}The best-fit point has \(\tan {\beta }= 13\), as also reported in Table 3.

The pink \({\tilde{\tau }}_1- \tilde{\chi }^{0}_{1}\) coannihilation region is very prominent in the \((\tan {\beta }, m_{1/2})\) projection shown in the upper panel of Fig. 6, as is the blue rapid *H* / *A* annihilation region and the purple \({\tilde{\tau }}_1- \tilde{\chi }^{0}_{1}\) coannihilation + *H* / *A* funnel hybrid region at large \(\tan {\beta }\) and \(m_{1/2}\). While the *H* / *A* funnel appears in the CMSSM only when \(\tan \beta \gtrsim 45\) for \(\mu > 0\) [18, 19, 20, 21, 22], in the SU(5) SUSY GUT model, it is found at significantly lower \(\tan \beta \), due to the separation of \(m_{H_u}\) and \(m_{H_d}\) from \(m_{5}\) and \(m_{10}\), effectively making \(m_A\) (and \(\mu \)) free parameters as in the NUHM2. There is also a region in the \((\tan {\beta }, m_{1/2})\) plane with \(\tan {\beta }\lesssim 10\) and \(m_{1/2} \sim 1000 \,\, \mathrm {GeV}\) where \({\tilde{\nu }_\tau }^\mathrm{NLSP}\) coannihilation is important.

The \({\tilde{\tau }}_1- \tilde{\chi }^{0}_{1}\) coannihilation region and the purple \({\tilde{\tau }}_1- \tilde{\chi }^{0}_{1}\) coannihilation \(+\) *H* / *A* funnel hybrid region are prominent for \(|m_5| \lesssim 3000 \,\, \mathrm {GeV}\) in the \((\tan {\beta }, m_5)\) and \((\tan {\beta }, m_{10})\) planes shown in the lower part of Fig. 6, with \(\tilde{\chi }^{\pm }_{1} - \tilde{\chi }^{0}_{1}\) coannihilation dominant at smaller values of \(\tan {\beta }\), in particular. The \({\tilde{u}_R}/{\tilde{c}_R} - \tilde{\chi }^{0}_{1}\) coannihilation region appears in a small island for \(\tan {\beta }\sim 8\) and \(m_{10} \sim -1200 \,\, \mathrm {GeV}\) in the \((\tan {\beta }, m_{10})\) plane shown in the lower right panel of Fig. 6.

As is well known, the calculation of \(M_h\) in the MSSM is particularly sensitive to the value of the trilinear soft SUSY-breaking parameter \(A_0\) as well as the stop squark masses. The latter depend in the SUSY SU(5) GUT model on \(m_{10}\) and \(m_{1/2}\), but are insensitive to \(m_5\).

^{14}We observe the same behaviour in the right panel of Fig. 9, where the one-dimensional likelihood profile for \(M_A\) is shown. Indeed, the lightest pseudoscalar mass allowed at \(\Delta \chi ^2 = 4\) is \({\sim }920\) GeV. The best-fit point in the global fit has \((M_A, \tan {\beta }) \simeq (1600 \,\, \mathrm {GeV}, 13)\): this is considerably beyond the present and projected LHC reach, though poorly determined.

## 6 One-dimensional likelihood functions

We now discuss the one-dimensional \(\Delta \chi ^2\) functions for various observable quantities.

Figure 10 displays those for \(m_{\tilde{g}}\) (top left), \(m_{\tilde{q}_L}\) (top right), \(m_{\tilde{d}_R}\) (centre left), \(m_{\tilde{u}_R}\) (centre right), \(m_{\tilde{t}_1}\) (bottom left) and \(m_{{\tilde{\tau }}_1}\) (bottom right). The solid blue line in each panel corresponds to the current analysis of the supersymmetric SU(5) model including LHC Run 2 data at 13 TeV, the dashed blue line shows the result of an SU(5) fit in which the LHC 13-TeV results are not included, and the solid grey line corresponds to ‘fake’ NUHM2-like results obtained by selecting a subset of the SU(5) sample with \(m_5/m_{10} \in [0.9, 1.1]\), which we discuss in more detail later.^{15}

Concerning future \(e^+e^-\) colliders, one can see that the best-fit masses of the lightest neutralino and stau are \(\sim 500 \,\, \mathrm {GeV}\), and some other 68% CL ranges go down to \(500 \,\, \mathrm {GeV}\), offering the possibility of pair production at a collider with \(\sqrt{s} \sim 1 \,\, \mathrm {TeV}\), as envisaged for the final stage of the ILC [172, 173]. Going to higher centre-of-mass energies, e.g., \(\sqrt{s} \lesssim 3 \,\, \mathrm {TeV}\) [173, 174] as anticipated for CLIC, significant fractions of the 68% CL ranges of electroweak sparticle masses can be covered.

As already noted, a novel feature of the SUSY SU(5) GUT model with (\(m_5 \ne m_{10}\)) is that the \({\tilde{u}_R}\) and \({\tilde{c}_R}\) may be much lighter than the other squarks. This leads to the possibility of a \({\tilde{u}_R}/{\tilde{c}_R} - \tilde{\chi }^{0}_{1}\) coannihilation strip where \(m_{\tilde{u}_R}\) and \(m_{\tilde{c}_R} \sim 500 \,\, \mathrm {GeV}\), which is visible as a second local minimum of \(\chi ^2\) with \(\Delta \chi ^2 > 4\) in the centre right panel of Fig. 10.

We have checked specifically whether this strip is allowed by the available LHC constraints. To this end, we verified using the Atom simulation code that points along this strip are consistent with the published constraints from the LHC 8-TeV data. We have also checked that this strip is consistent with the preliminary simplified-model search for \(\tilde{q}\tilde{q}+ \tilde{q}\bar{\tilde{q}}\) at 13 TeV reported by CMS. The left panel of Fig. 13 displays as a solid/dashed blue line the one-dimensional \(\chi ^2\) function for \(m_{\tilde{u}_R} - m_{\tilde{\chi }^{0}_{1}}\) including/omitting the 13-TeV data (the corresponding lines for \(m_{\tilde{c}_R} - m_{\tilde{\chi }^{0}_{1}}\) are very similar), and the right panel of Fig. 13 shows the region of the \((m_{\tilde{u}_R}, m_{\tilde{\chi }^{0}_{1}})\) plane where \(\Delta \chi ^2 < {5.99}\), i.e., allowed at the 95% CL. We find that \(\sigma (\tilde{q}\tilde{q}+ \tilde{q}\bar{\tilde{q}}) < 0.1\) pb in this region, whereas the cross-section upper limit as given in [9] is \({\gtrsim } 1\) pb. We conclude that this simplified-model search does not affect the likelihood in this \({\tilde{u}_R}/{\tilde{c}_R} - \tilde{\chi }^{0}_{1}\) coannihilation strip region. However, it will be explored further by future LHC data with increased luminosity.

Particle masses at the best-fit point in the SUSY SU(5) GUT model (in GeV units)

\({{\tilde{\tau }}_1}\) | \({{\tilde{\tau }}_2}\) | \({\tilde{e}_L}\) | \({\tilde{e}_R}\) | \({{\tilde{\nu }}_\tau }\) | \({\tilde{q}_L}\) | \({\tilde{t}_1}\) | \({\tilde{t}_2}\) |
---|---|---|---|---|---|---|---|

470 | 660 | 630 | 678 | 570 | 2130 | 1840 | 2180 |

\({\tilde{b}_1}\) | \({\tilde{b}_2}\) | \({\tilde{u}_R}\) | \({\tilde{d}_R}\) | \({\tilde{g}}\) | \(M_{H,A}\) | \(m_{\tilde{\chi }^{0}_{1}}\) | \(m_{\tilde{\chi }^{0}_{2},\tilde{\chi }^{\pm }_{1}}\) |

1940 | 2090 | 2000 | 1980 | 2310 | 1620 | 460 | 860 |

*Z*peak, which are present in the SM and the SUSY SU(5) GUT model is unable to mitigate.

The principal \(\chi ^2\) contributions of observables at the best-fit point in the SUSY SU(5) GUT model, together with the total \(\chi ^2\) function

\(A_\mathrm{LR}^{e}\) | \(A_b\) | \(A_\mathrm{FB}(\ell )\) | \(A_\mathrm{FB}(b)\) | \(A_\mathrm{FB}(c)\) | \(A_{l}(P_\tau )\) | |

3.40 | 0.35 | 0.78 | 6.79 | 0.82 | 0.08 | |

\(R_b\) | BR(\(b \rightarrow s \gamma \)) | BR(\(B_u \rightarrow \tau \nu _\tau \)) | \(\Omega _{\tilde{\chi }^{0}_{1}} h^2\) | \(\sigma ^\mathrm{SI}_p\) | \(\mathrm{BR}(B_{s, d} \rightarrow \mu ^{+}\mu ^{-})\) | |

0.26 | 0.00 | 0.18 | 0.00 | 0.00 | 2.09 | |

\(\sin ^2\theta _{\mathrm {eff}}\) | \(M_W\) | \(R_l\) | \(R(K \rightarrow l \nu )\) | \((g-2)_\mu \) | \(M_h\) | |

0.60 | 0.07 | 1.04 | 0.0 | 8.28 | 0.01 | |

\(\sigma _\mathrm{had}^0\) | \({\frac{\Delta M_{B_s}}{\Delta M_{B_d}}}\) | \(\epsilon _K\) | \(H/A \rightarrow \tau ^+ \tau ^-\) | HiggsSignals | Total | |

2.54 | 1.78 | 1.94 | 0.00 | 67.95 | 0.3 | 100.34 |

In order to compare the quality of the SU(5) fit to the results of previous MasterCode analyses of competing models [15], we follow the prescription used there of subtracting from the total \(\chi ^2\) given in Table 5 and Fig. 15, namely 100.34, the \(\chi ^2\) contributions originating from HiggsSignals [136, 137], which dominate the global \(\chi ^2\) function and would bias the analysis. Fig. 15 lists 36 separate contributions to the total \(\chi ^2\) function. The first three (\(m_t, M_Z\), and \(\Delta \alpha _\mathrm{had}^{(5)} (M_Z)\)) are treated as nuisance parameters and the two LHC MET constraints at 8 and 13 TeV are applied as a single constraint. Omitting the HiggsSignals constraints in our determination of the number of degrees of freedom leaves 30 constraints, with seven parameters for the SU(5) model and hence 23 degrees of freedom.The \(\chi ^2\) contributions from the relevant constraints sum to 32.39, corresponding to a \(\chi ^2\) probability of 9%. This can be compared with the \(\chi ^2\) probability values of 11, 12, 11 and 31% found in [15] for the CMSSM, NUHM1, NUHM2 and pMSSM10, respectively, using LHC Run 1 constraints. However, as in [15], we stress that these \(\chi ^2\) probabilities are only approximate since, for example, they neglect correlations between the observables. A more complete treatment using toys, as done in the last reference of [37, 38, 39, 40, 41, 42, 43, 44, 45], is beyond the scope of this work.

There are a couple of important corollaries to this observation, one concerning \(m_{\tilde{t}_1}\). It is sensitive to \(A_0\) as well as the soft SUSY-breaking contributions to the \({\tilde{t}_L}\) and \({\tilde{t}_R}\) mass parameters (which are both given by \(m_{10}\) in the SUSY SU(5) GUT model). Since \(A_0\) is relatively poorly determined, the \(\chi ^2\) minimum for \(m_{\tilde{t}_1}\) is relatively shallow, as seen in the lower left panel of Fig. 10.

The second observation concerns the sign of \(\mu \). All our analysis has been for \(\mu > 0\), which is the sign capable of mitigating the discrepancy between the experimental value of \((g-2)_\mu \) and the SM prediction. For \(\mu < 0\), the large-mass plateau would have a similar height as in Fig. 14, but the \(\chi ^2\) function would rise monotonically at low values of \(m_5\), \(m_{10}\) and \(m_{1/2}\), instead of featuring a dip. Thus, the \(\mu < 0\) possibility would be disfavoured by \(\Delta \chi ^2 \gtrsim 2\), and the global minimum would lie at large masses and be ill defined.

^{16}

## 7 Higgs branching ratios

We present in Fig. 19 the one-dimensional likelihood functions for the ratios of supersymmetric SU(5) and SM predictions for the BRs of \(h \rightarrow \gamma \gamma \) (left panel), \(h \rightarrow Z Z^*\) (middle panel)^{17} and \(h \rightarrow gg\) decays (right panel). We see that in each case the preferred region in the fit corresponds to a prediction in the SU(5) model that deviates from the SM case by at most a few %, whereas the present experimental uncertainties in the different coupling modifiers squared (employing some theory assumptions) are typically \(\mathcal{O}(30)\)% [179], and a precision of \({\mathcal O}(5-10\%)\) (with the same theory assumptions) can be reached by the end of the LHC programme. On the other hand, future \(e^+e^-\) colliders such as the ILC, CLIC or FCC-ee anticipate a precision at the percent level for couplings to fermions and at the permille level for couplings to massive gauge bosons [173, 180]. This offers the possiblity that deviations from the SM in the SUSY SU(5) GUT model can be measured in the future.

## 8 Comparison with previous results

Figure 20 compares the one-dimensional \(\chi ^2\) likelihood functions for \(m_{\tilde{g}}\) (upper left), \(m_{\tilde{q}_R}\) (upper right), \(m_{\tilde{t}_1}\) (lower left) and \(m_{{\tilde{\tau }}_1}\) (lower right) found in the SU(5) model including LHC 13-TeV constraints (solid blue lines) with the restricted fake NUHM2 sample (solid grey lines) and, for comparison, results from our previous NUHM2 analysis that used only the LHC 7- and 8-TeV constraints (dashed grey lines) [14]. We see here and in Fig. 10 that the restricted ‘fake’ NUHM2 sample exhibits, in general, best-fit masses that are similar to those found in the full SU(5) sample. The most noticeable differences are that lower masses are disfavoured in the restricted sample relative those in the full SU(5) model, indicating that the latter has some limited ability to relax the NUHM2 lower bounds on sparticle masses, e.g., at the 95% CL. The previous NUHM2 analysis [14] also yielded similar best-fit masses but, as could be expected, gave 95% CL lower limits on sparticle masses that were further relaxed. Similar features can also be observed in Figs. 16, 17, 18 and 19, where we have also included the ‘fake’ NUHM2 subsample.

Restricting further our SU(5) to mimic the NUHM1, let alone the CMSSM, is not useful because of the increased sampling uncertainties in such restricted samples. However, we showed in [14] that our NUHM2 LHC 7- and 8-TeV results for the exhibited sparticle masses were broadly similar to those for the NUHM1 and the CMSSM [13], and we expect the impacts of the LHC 13-TeV data on these models to be comparable to that in the NUHM2.

Finally, we ask whether or not there is a significant improvement in the SU(5) fit compared to that in the NUHM2 subsample, thanks to the additional parameter (\(m_5\) and \(m_{10}\) replacing \(m_0\)). The NUHM2 subsample has a total \(\chi ^2 = 100.8\), which is reduced to 32.8 when we remove the contributions from HiggsSignals, as discussed earlier. It should be noted that the NUHM2 subsample is statistically significantly smaller than that of the SU(5) sample. The quoted NUHM2 \(\chi ^2\) represents only an upper bound on the \(\chi ^2\) of the best-fit point that would be found in a more complete sample of the NUHM2. Since the NUHM2 model has one less parameter than the SU(5) model, it has 24 degrees of freedom, and its \(\chi ^2\) probability is 11%. According to the Wilks test [181], the probability that the data are represented better by the SU(5) model than by the NUHM2 subsample is 50%, while the *F* test [182] yields a 40% probability. Therefore we conclude that there is no evidence that the extra parameter of SU(5) provides a significant improvement.

## 9 The possibility of a long-lived \({\varvec{{\tilde{\tau }}_1}}\)

The upper right plot of Fig. 21 compares the \(\tilde{\tau }_{1}\) lifetime with its mass. The plane is characterized by a strip with \(800 \,\, \mathrm {GeV}\lesssim {{\tilde{\tau }}_1} \lesssim 1200 \,\, \mathrm {GeV}\) allowed at the 68% CL, while the 95% CL region is significantly wider, ranging from \(m_{{\tilde{\tau }}_1} \sim 500 \,\, \mathrm {GeV}\) to \(m_{{\tilde{\tau }}_1} \sim 2000 \,\, \mathrm {GeV}\).

The lower panels of Fig. 21 display the regions of the \((m_5, m_{1/2})\) (left) and \((m_{10}, m_{1/2})\) (right) planes in the SUSY SU(5) GUT model where the lowest-\(\chi ^2\) points have \(10^{-10} \, \mathrm{s}< \tau _{{\tilde{\tau }}_1} < 10^3 \, \mathrm{s}\). The colour-coding indicates the lifetimes of these points, as indicated in the legends. The contours for \(\Delta \chi ^2 < 2.30 (5.99)\) relative to the best-fit point in our sample are shown as solid red and blue lines, respectively. One can see that larger lifetimes occur all over the displayed parameter space, with a slight preference for larger \(m_5\) or \(m_{10}\) values.

## 10 Direct dark matter detection

Figure 22 displays our results for the SUSY SU(5) GUT model in the \((m_{\tilde{\chi }^{0}_{1}}, \sigma ^\mathrm{SI}_p)\) plane. The combined PandaX-II/LUX constraint (black line) establishes a 95% CL that reaches \(\sigma ^\mathrm{SI}_p\) \(\simeq 2 \times 10^{-46}\) cm\(^2\) for \(m_{\tilde{\chi }^{0}_{1}} = 50 \,\, \mathrm {GeV}\) and \({\simeq } 10^{-45}\) cm\(^2\) for \(m_{\tilde{\chi }^{0}_{1}} = 500 \,\, \mathrm {GeV}\), providing the upper boundary of the 95% CL region in the \((m_{\tilde{\chi }^{0}_{1}}, \sigma ^\mathrm{SI}_p)\) plane seen in Fig. 22. We see that there are regions favoured at the 68% CL that lie relatively close to this boundary, whereas the main 68% CL region and the best-fit point have smaller values of \(\sigma ^\mathrm{SI}_p\). We also note that the *H* / *A* funnel and \(\tilde{\chi }^{\pm }_{1} - \tilde{\chi }^{0}_{1}\) DM mechanisms favour values of \(\sigma ^\mathrm{SI}_p\) that are relatively close to the PandaX-II/LUX boundary, whereas the \({{\tilde{\tau }}_1} - \tilde{\chi }^{0}_{1}\) mechanism and its hybridization with the *H* / *A* funnel favour smaller values of \(\sigma ^\mathrm{SI}_p\). The upcoming XENON1T [193] experiment will be able to probe the whole \(\tilde{\chi }^{\pm }_{1}\) coannihilation region and a substantial part of the *H* / *A* funnel region.

We also display in Fig. 22 the projected 95% exclusion sensitivity of the future LUX-Zeplin (LZ) and XENONnT experiments (solid purple and dashed blue lines respectively) [193, 194], and the astrophysical neutrino ‘floor’ (dashed orange line) [195, 196], below which astrophysical neutrino backgrounds dominate (yellow region). We see that much of the \({{\tilde{\tau }}_1} - \tilde{\chi }^{0}_{1}\) coannihilation region and the region of its hybridization with the *H* / *A* funnel lie below the projected sensitivities of the LZ and XENONnT experiments, and substantial portions of them also lie below the neutrino ‘floor’. On the bright side, however, we recall that the \({{\tilde{\tau }}_1} - \tilde{\chi }^{0}_{1}\) region, in particular, lies at relatively small values of \(m_5, m_{10}\) and \(m_{1/2}\), offering greater prospects for detection at the LHC than, e.g., the \(\tilde{\chi }^{\pm }_{1} - \tilde{\chi }^{0}_{1}\) region, so there is complementarity in the prospects of the LHC and direct DM experiments for probing the SUSY SU(5) GUT model, as was noted previously for other SUSY models [16].

## 11 Summary and conclusions

We have explored in this paper the experimental, phenomenological, astrophysical and cosmological constraints on the minimal SUSY SU(5) GUT model. In this scenario the GUT-scale universal soft SUSY-breaking scalar mass \(m_0\) is replaced by independent masses for the \(\mathbf {10}\) and \({\bar{\mathbf{5}}}\) sfermions. This flexibility introduces some features that are novel compared to the GUT-universal CMSSM, NUHM1 and NUHM2.

In general we observe that many best-fit values of the coloured particles are within the reach of the HL-LHC, but that the preferred regions clearly extend beyond the reach of the final stage of the LHC. On the other hand, the best-fit masses of some electroweakly interacting particles are \({\sim } 500 \,\, \mathrm {GeV}\), offering the possibility of pair production at a collider with \(\sqrt{s} \sim 1 \,\, \mathrm {TeV}\), as envisaged for the final stage of the ILC. Going to higher centre-of-mass energies, \(\sqrt{s} \lesssim 3 \,\, \mathrm {TeV}\) as anticipated for CLIC, significant fractions of the 68% CL ranges of electroweak sparticle masses can be covered.

One novelty is the appearance of a \({\tilde{u}_R}/{\tilde{c}_R} - \tilde{\chi }^{0}_{1}\) coannihilation region that appears where \(m_5^2\) is large and positive, \(m_{10}^2\) is small and negative, and \(m_{H_u}^2\) and \(m_{H_d}^2\) are large and negative. On the other hand, we find that \({\tilde{t}_1} - \tilde{\chi }^{0}_{1}\) coannihilation is not important in the SUSY SU(5) GUT model, nor are the focus-point region and rapid \(\tilde{\chi }^{0}_{1} \tilde{\chi }^{0}_{1}\) annihilation via direct-channel *h* and *Z* poles. We have checked that the \({\tilde{u}_R}/{\tilde{c}_R} - \tilde{\chi }^{0}_{1}\) coannihilation region is not yet excluded by searches for Open image in new window events at the LHC, because the production rate is reduced compared to the case where all eight squarks are mass degenerate and the small \({\tilde{u}_R}/{\tilde{c}_R} - \tilde{\chi }^{0}_{1}\) mass difference suppresses this signature. However, this region may be accessible with future LHC runs.

We have also highlighted the possibility that a \({{\tilde{\nu }}_\tau }\) NLSP might have an important coannihilation role. Another novelty is the composition of the \({{\tilde{\tau }}_1}\) NLSP in a significant region of the model parameter space. In the GUT-universal CMSSM, NUHM1 and NUHM2 models, the universality of \(m_0\) and the greater renormalization for SU(2) doublets impose a substantial mass difference between the \({{\tilde{\tau }}_2}\) and the \({{\tilde{\tau }}_1}\), with the latter being predominantly a \({{\tilde{\tau }}_R}\). However, in the SUSY SU(5) GUT model with \(m_5 \ne m_{10}\), the \({\tilde{\tau }_R}\) and \({{\tilde{\tau }}_L}\) may have similar masses, and the off-diagonal entries in the \({{\tilde{\tau }}}\) mass matrix may cause large mixing and repulsion between the \({{\tilde{\tau }}_1}\) and \({{\tilde{\tau }}_2}\) masses.

On the other hand, one experimental signature that is shared by the SUSY SU(5) GUT model and GUT-universal models is the possible appearance of a long-lived (metastable) \({{\tilde{\tau }}_1}\). This is a feature of a significant fraction (but not all) of the \({\tilde{\tau }_1} -\tilde{\chi }^{0}_{1}\) coannihilation region.

The prospects for direct DM detection are mixed: they are relatively good in the \(\tilde{\chi }^{\pm }_{1} - \tilde{\chi }^{0}_{1}\) coannihilation region, but less promising in the rapid *H* / *A* annihilation and hybrid regions, though potentially detectable in the planned LUX-Zeplin experiment. On the other hand, the \({{\tilde{\tau }}_1} -\tilde{\chi }^{0}_{1}\) coannihilation region probably lies beyond the reach of this experiment, as does part of the hybrid region. Indeed, portions of these regions lie below the neutrino ‘floor’. On the other hand, substantial parts of these regions are accessible to LHC searches for long-lived particles and Open image in new window .

## Footnotes

- 1.
This possibility has also been noted in a supersymmetric SO(10) GUT framework [73].

- 2.
We note that this problem becomes less severe for supersymmetry-breaking scales beyond a TeV [69].

- 3.
We use a modified version of FeynHiggs 2.11.2 that includes two-loop QCD corrections in the evaluation of the \({\overline{\mathrm {DR}}}\) running top mass and an improved evalution of the top mass in the \({\overline{\mathrm {DR}}}\)-on-shell conversion for the scalar tops.

- 4.
An exception is provided by the \({\tilde{u}_R}\) and \({\tilde{c}_R}\), which may be much lighter than the gluino and other squarks in some regions of parameter space. We will discuss this possibility in detail below.

- 5.
The \(\tilde{u}_R/\tilde{c}_R- \tilde{\chi }^{0}_{1}\) coannihilation strip visible in the upper panels of Fig. 3 at \(m_{\tilde{u}_R} \simeq m_{\tilde{\chi }^{0}_{1}} \sim 500 \,\, \mathrm {GeV}\) is the subject of a later dedicated discussion.

- 6.
One could be concerned that summing up the \(\chi ^2\) contributions from different simplified-model limits would overestimate the exclusion limit, since these signal regions are not necessarily independent. This would be indeed the case if the same event sample were confronted with multiple overlapping signal regions. In our case, however, the signal sample is divided into statistically independent sub-samples, corresponding to the simplified-model topologies \(\tilde{g} \rightarrow b \bar{b} {\tilde{\chi }}_1^0, \rightarrow t \bar{t} {\tilde{\chi }}_1^0\), etc., and these sub-samples are confronted with the corresponding simplified-model limits only once. In such a case the Open image in new window estimate (2) provides a conservative limit when there is no significant excess in the data.

- 7.
- 8.
A more conservative approach would be to choose the strongest search channel based on the expected sensitivity rather than that observed. However, the expected limit shown in [134] is similar to that observed, so we do not expect that this approach would lead to a significant change.

- 9.
- 10.
- 11.
The SLHA files for the best-fit point and other supplementary material can be found in [17].

- 12.
An SLHA file corresponding to the \({\tilde{u}_R}/{\tilde{c}_R} - \tilde{\chi }^{0}_{1}\) coannihilation region can be found in [17].

- 13.
The RGE evolution of the Yukawa couplings blows up for \(\tan \beta \gtrsim 60\).

- 14.
We note, however, that this constraint might weaken with a larger parameter sample.

- 15.
The \(\Delta \chi ^2\) functions for the NUHM2 subsample are calculated relative to its minimum \(\chi ^2\), which is \({\sim } 0.4\) higher than the minimum \(\chi ^2\) for the full SU(5) sample.

- 16.
For conditions to have a long-lived \(\tilde{\chi }^{\pm }_{1}\) with a bino-like LSP: see, e.g., [178].

- 17.
The likelihood function for \(h \rightarrow W W^*\) is very similar to that for \(h \rightarrow Z Z^*\), because of custodial symmetry.

## Notes

### Acknowledgements

The work of M.B., V.C., M.L. and D.M.-S. is supported by the European Research Council via Grant BSMFLEET 639068. The work of R.C. is supported in part by the National Science Foundation under Grant No. PHY-1151640 at the University of Illinois Chicago, and in part by Fermilab, operated by Fermi Research Alliance, LLC under Contract No. De-AC02-07CH11359 with the United States Department of Energy. This work of M.J.D. is supported in part by the Australian Research Council. The work of J.E. is supported in part by STFC (UK) via the research Grant ST/L000326/1, and the work of H.F. is also supported in part by STFC (UK). The work of S.H. is supported in part by CICYT (Grant FPA 2013-40715-P) and also by the Spanish MICINN Consolider-Ingenio 2010 Program under Grant MultiDark CSD2009-00064. The work of K.A.O. is supported in part by DOE Grant de-sc0011842 at the University of Minnesota. The work of K.S. is partially supported by the National Science Centre, Poland, under research Grants DEC-2014/15/B/ST2/02157 and DEC-2015/18/M/ST2/00054. The work of G.W. is supported in part by the Collaborative Research Center SFB676 of the DFG, “Particles, Strings and the early Universe”, and in part by the European Commission through the “HiggsTools” Initial Training Network PITN-GA-2012-316704.

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