B anomalies and dark matter: a complex connection

  • D. G. Cerdeño
  • A. Cheek
  • P. Martín-Ramiro
  • J. M. MorenoEmail author
Open Access
Regular Article - Theoretical Physics


We study an extension of the Standard Model that addresses the hints of lepton flavour universality violation observed in \(B\rightarrow K^{(*)} l^+l^-\) decays at LHCb, while providing a viable candidate for dark matter. The model incorporates two new scalar fields and a Majorana fermion that induce one-loop contributions to B meson decays. We show that agreement with observational data requires the new couplings to be complex and that the Majorana fermion can reproduce the observed dark matter relic density. This combination of cosmological and flavour constraints sets an upper limit on the dark matter and mediator masses. We have studied LHC dijet and dilepton searches, finding that they rule out large regions of parameter space by setting lower bounds on the dark matter and mediator masses. In particular, dilepton bounds are much more constraining in a future high-luminosity phase. Finally, we have computed the scattering cross section of dark matter off nuclei and compared it to the sensitivity of current and future direct detection experiments, showing that parts of the parameter space could be accessible in the future to multi-ton experiments. Future collider and direct DM searches complement each other to probe large areas of the parameter space of this model.

1 Introduction

LHCb has reported anomalies in the measured decay rates of the B meson, which have been interpreted as hints of lepton flavour universality violation [1, 2]. The SM predicts equal rates for the processes \(B\rightarrow K^{(*)} \mu ^+\mu ^-\) and \(B\rightarrow K^{(*)} e^+e^-\), and it is customary to study the ratios of these branching ratios, defined as R(K) and \(R(K^*)\), since the dependencies on hadronic matrix elements (and associated uncertainties) cancel out [3]. The measurements of these hadronically clean observables deviate consistently (although perhaps with not enough statistical significance) from the SM prediction \(R(K^{(*)})=1\) [4]. These hints are complemented by measurements of other observables that are more sensitive to hadronic physics. In particular, the differential branching fractions [1, 2, 5] and angular observables [6, 7, 8, 9, 10, 11, 12, 13] associated to the processes \(B\rightarrow \phi \mu ^+\mu ^-\) and \(B\rightarrow K^{(*)} \mu ^+\mu ^-\) also deviate from the SM predictions. Interestingly, all the apparent anomalies involve the transition \(b \rightarrow s\mu ^{+}\mu ^{-}\).

In order to account for these experimental results, one can modify the SM effective Hamiltonian, which involves penguin and box diagrams, by including one-loop contributions from new exotic particles. A full classification of the various particle combinations, considering different gauge representations, was presented in Refs. [14, 15]. Among the different models, some featured neutral scalar or fermions that, if stable, could play the role of dark matter (DM).1 The first possibility was investigated in Ref. [41], where it was found that the large new couplings required to reproduce the correct DM relic abundance induce sizeable 1-loop contributions to DM-nucleon scattering, leading to very strong limits from direct detection experiments. In addition, as reported by [42], the Higgs portal coupling typically dominates over other new physics effects. The second possibility was addressed in Ref. [43], where the fermionic dark matter field was accompanied by one additional scalar and one additional coloured fermion.

In this work, we consider a modification of the model of Ref. [43]. Namely, we will also assume a fermionic dark matter particle, but with two extra scalar fields, one of which has a colour charge. On top of this, we include the latest SM theoretical prediction for the mass difference in \(B_{s}-\)mixing [44], which differs from the experimental observation by \(1.8\,\sigma \). In order to reduce this tension and provide an explanation for the B anomalies, complex couplings are needed, leading to new CP-violation sources, a scenario that has not been studied in the context of one-loop models so far. We explore the parameter space of this model, taking into account all the flavour observables, DM constraints, and LHC collider signatures.

This paper is organised as follows. In Sect. 2, we introduce the details of the particle physics model, address the constraints from the observed DM relic abundance and \(B_{s}-\)mixing and discuss the implications on the model’s parameter space. In Sect. 3, we investigate the possibility of observing this scenario at the LHC, for which we take into account dijet and dimuon searches. We also include a projection of the potential reach of the High Luminosity phase of the LHC. Finally, in Sect. 4, we compute the DM-nucleus scattering cross section and study current constraints and the future reach of direct DM detection experiments. The conclusions are presented in Sect. 5.

2 The model

In this article, we consider a model in which the DM particle is a Majorana fermion, \(\chi \), with two extra scalar fields, \(\phi _q\) and \(\phi _l\), which couple to left-handed quarks and leptons, respectively.2 The interactions between the new particles and the SM are described by the Lagrangian,
$$\begin{aligned} \mathcal {L}_{\text {int}}^{\text {NP}} = \lambda _{Q_i}\bar{Q}_{i}\phi _{q}P_{R}\chi + \lambda _{L_i}\bar{L}_{i}\phi _{l}P_{R}\chi + \mathrm {h.c.}, \end{aligned}$$
where \(Q_i\) and \(L_i\) denote the SM left-handed quark and lepton doublets of each generation, and \(\lambda _{Q_i}\) and \(\lambda _{L_i}\) are the corresponding new couplings. The quantum numbers for the new fields are summarised in Table 1. We impose a \({\mathcal {Z}}_2\) parity under which the SM fields are invariant, and which guarantees the stability of the DM candidate, as long as \(m_{\phi _{q,l}} > m_{\chi }\). Upon rotation from the electroweak to the quark mass eigenbasis, the couplings \(\lambda _{Q_i}\) are rotated in flavour space. Assuming that the electroweak and mass eigenbasis are aligned for the leptons and down-type quarks, the couplings to the up-type quarks are generated by the CKM rotation as follows:
$$\begin{aligned} \lambda _{Q_i}\bar{Q}_{i} \rightarrow \lambda _{Q_j}(\bar{u}_{L,i}V_{ij}, \bar{d}_{L,j}). \end{aligned}$$
From now on, we will denote the couplings in the mass eigenbasis with the corresponding quark or lepton label. These couplings are, in general, complex.
Table 1

Quantum numbers of the new fields. We also indicate the charges under \({\mathcal {Z}}_2\)





\({\mathcal {Z}}_2\)

\(\phi _{q}\)



1 / 6


\(\phi _{l}\)





\(\chi \)





Fig. 1

One-loop diagram contribution from the new particles to the \(b \rightarrow s\mu ^{+}\mu ^{-}\) transitions

This model induces new physics contribution to flavour observables at the one loop level. In particular, a new box diagram appears for the \(b \rightarrow s\mu ^{+}\mu ^{-}\) transition, as shown in Fig. 1. These effects can be described using an effective field theory approach, thus parameterising the new contributions as corrections to the corresponding Wilson coefficients of the effective Hamiltonian,
$$\begin{aligned} \mathcal {H}_{\text {eff}}^{\mu ^{+}\mu ^{-}}= & {} -\frac{4G_{F}}{\sqrt{2}}V_{tb}V_{ts}^{*}(C_{9}\mathcal {O}_{9} + C_{9}^{\prime }\mathcal {O}_{9}^{\prime } \nonumber \\&+\, C_{10}\mathcal {O}_{10} + C_{10}^{\prime }\mathcal {O}_{10}^{\prime }) + \text {h.c.}, \end{aligned}$$
where the effective operators \(\mathcal {O}_{9}\), \(\mathcal {O}_{9}^{\prime }\), \(\mathcal {O}_{10}\), \(\mathcal {O}_{10}^{\prime }\) are defined as:
$$\begin{aligned} \mathcal {O}_{9}= & {} \frac{\alpha _{\text {em}}}{4\pi }(\bar{s}\gamma ^{\mu }P_{L}b)(\bar{\mu }\gamma _{\mu }\mu ), \end{aligned}$$
$$\begin{aligned} \mathcal {O}_{9}^{\prime }= & {} \frac{\alpha _{\text {em}}}{4\pi }(\bar{s}\gamma ^{\mu }P_{R}b)(\bar{\mu }\gamma _{\mu }\mu ), \end{aligned}$$
$$\begin{aligned} \mathcal {O}_{10}= & {} \frac{\alpha _{\text {em}}}{4\pi }(\bar{s}\gamma ^{\mu }P_{L}b)(\bar{\mu }\gamma _{\mu } \gamma _{5}\mu ), \end{aligned}$$
$$\begin{aligned} \mathcal {O}_{10}^{\prime }= & {} \frac{\alpha _{\text {em}}}{4\pi }(\bar{s}\gamma ^{\mu } P_{R}b)(\bar{\mu }\gamma _{\mu }\gamma _{5}\mu ). \end{aligned}$$
The Wilson coefficients \(C_{9}\), \(C_{9}^{\prime }\), \(C_{10}\), \(C_{10}^{\prime }\) contain both the SM and new physics (NP) contributions,
$$\begin{aligned} C_{9}= & {} C_{9}^{\text {SM}} + C_{9}^{\text {NP}},\nonumber \\ C_{10}= & {} C_{10}^{\text {SM}} + C_{10}^{\text {NP}}, \end{aligned}$$
with the primed coefficients defined in an equivalent way.

Global fits [20, 45, 46, 47, 48, 49, 50, 51, 52, 53] have been used to determine the new physics contribution to the Wilson coefficients in order to reproduce the observed experimental results. These fits favour \(C_{9}^{\text {NP}} = -C_{10}^{\text {NP}}\), and suggest that no new physics is required for operators involving electrons or tau leptons. Motivated by these results, we assume negligible couplings to the first quark generation (i.e., \(\lambda _{Q_1} = 0\)) and to the first and third lepton generations (i.e., \(\lambda _{e}=\lambda _{\tau }=0\)). This provides an explanation for the \(R_{K^{(*)}}\) anomalies, while relaxing the bounds from other searches.

Therefore, in total, we are left with six free parameters in this model, namely the masses of the three new particles (\(m_{\chi }\), \(m_{\phi _{l}}\), \(m_{\phi _{q}}\)), and the couplings to \(b-\)type quarks, \(s-\)type quarks, and leptons (\(\lambda _b\), \(\lambda _s\), \(\lambda _{\mu }\)).

It should be noted that the couplings \(\lambda _{1}|\phi _{l}|^{2}|H|^{2}\) and \(\lambda _{2}|\phi _{q}|^{2}|H|^{2}\) are allowed by gauge symmetry in the Lagrangian of Eq. (2.1). However, they only lead to an overall shift to the masses of \(\phi _{l}\) and \(\phi _{q}\) after electroweak symmetry breaking since the couplings to the Higgs play no phenomenological role in the relevant range of \(\phi _{l,q}\) masses. Likewise, the terms \(\lambda _{3}|\phi _{l}H|^{2}\) and \(\lambda _{4}|\phi _{q}H|^{2}\) are also allowed by gauge symmetry. They typically induce a small split in the masses of the neutral and charged components of the doublets \(\phi _{l}\) and \(\phi _{q}\) in the range of \(\phi _{l,q}\) masses that survive the collider constraints. Finally, a term of the form \((\phi _{l}H)^{2}\) can lead to large contributions to neutrino masses at one loop, which forces the corresponding coupling to be extremely small [43]. We will neglect these couplings in the following.

As mentioned in the Introduction, similar models have been discussed in the literature, featuring either scalar DM [41, 54, 55, 56] or fermionic DM [43]. Our model differs from that of Ref. [43] in that we have two extra scalar fields which couple to the lepton or quark sectors.

2.1 Dark matter relic abundance

In order for \(\chi \) to be a viable DM candidate, it must reproduce the observed relic abundance, which can be inferred from Planck satellite data to be \(\Omega h^2=0.1199\pm 0.0022\) [57]. The pair-annihilation proceeds through the two \(t-\)channel diagrams with \(\phi _q\) and \(\phi _l\), shown in Fig. 2.
Fig. 2

Tree-level contributions to the DM pair annihilation

The stringent flavour constraints force the couplings to quarks to be much smaller than the couplings to leptons (muons and neutrinos), and the combination of flavour and collider bounds impose \(m_{\phi _{q}} > m_{\phi _{l}}\), with coloured scalars generally above 1 TeV. Therefore DM annihilation into a \(\mu ^-\mu ^+\) or \(\nu _\mu {\bar{\nu }}_{\mu }\) pair is the dominant channel. The thermally-averaged annihilation cross section, \(\langle \sigma v\rangle \), can be expressed as a plane wave expansion in terms of the dimensionless parameter \(x=m_{\chi }/T\). For the case of a Majorana fermion, the zero-velocity term is helicity suppressed, and the leading contribution comes from the linear term in 1 / x [58],
$$\begin{aligned} \langle \sigma v\rangle = 2 \frac{|\lambda _{\mu }|^{4}m_{\chi }^{2}\left( m_{\phi _{l}}^{4} + m_{\chi }^{4}\right) }{16\pi \left( m_{\phi _{l}}^{2} + m_{\chi }^{2}\right) ^{4}} \, \frac{1}{x}\ , \end{aligned}$$
where we have neglected the muon and the neutrino masses. In order to reproduce the correct relic abundance, we can now impose \(\langle \sigma v\rangle = 2.2\times 10^{-26}~\hbox {cm}^3~\hbox {s}^{-1}\) (where \(x\sim 20\) at freeze-out).

We will use this relation to fix \(m_{\phi _{l}}\) as a function of the other parameters, thus effectively reducing by one the number of free parameters. Furthermore, due to the suppression of the velocity-independent term for \(\langle \sigma v\rangle \), indirect detection bounds are not expected to constrain our model.

2.2 \(B_{s}-\)mixing and other flavour constraints

This model introduces new couplings to the s and b quarks (and to the rest of the quarks by rotation of the CKM matrix). We must therefore incorporate constraints from B meson physics.

The most relevant bounds are those that involve \(b \rightarrow s\mu ^{+}\mu ^{-}\) transitions. The new physics contribution to the Wilson coefficient comes from box and photon-penguin diagrams [14, 15], \(C_{9}^\mathrm{NP}=C_{9}^{\text {box}}+C_{9}^{\gamma }\), with3
$$\begin{aligned} C_{9}^{\text {box}}= & {} \frac{\sqrt{2}}{128\pi \alpha _{\text {em}}G_{F}m^{2}_{\psi }} \frac{\lambda _{s}\lambda _{b}^{*}}{V_{tb}V_{ts}^{*}} |\lambda _{\mu }|^{2} \left( F(x_{q},x_{l}) \right. \nonumber \\&\left. +\, 2G(x_{q},x_{l}) \right) ,\nonumber \\ C_{9}^{\gamma }= & {} \frac{\sqrt{2}}{8G_{F}m^{2}_{\psi }} \frac{\lambda _{s}\lambda _{b}^{*}}{V_{tb}V_{ts}^{*}} F_{9}(x_{q}), \end{aligned}$$
where we have defined the dimensionless variables \(x_{q} = m_{\phi _{q}}^{2} / m_{\chi }^{2}\) and \(x_{l} = m_{\phi _{l}}^{2} / m_{\chi }^{2}\), and the loop functions are:
$$\begin{aligned} F(x,y)= & {} \frac{1}{(1-x)(1-y)} + \frac{x^{2}\log x}{(1-x)^{2}(x-y)}\nonumber \\&+\, \frac{y^{2}\log y}{(1-y)^{2}(y-x)},\nonumber \\ G(x,y)= & {} \frac{1}{(1-x)(1-y)} + \frac{x\log x}{(1-x)^{2}(x-y)}\nonumber \\&+\,\frac{y\log y}{(1-y)^{2}(y-x)},\nonumber \\ F_{9}(x)= & {} \frac{-2x^{3} + 9x^{2} - 18x + 6\log x + 11}{36(x-1)^{4}}. \end{aligned}$$
The term \(G(x_{q},x_{l})\) vanishes if \(\chi \) is a Dirac particle.

In order to constrain the Wilson coefficients we use the first global fit that takes into account the possibility that \(C_{9}\) and \(C_{10}\) are complex [59]. This is a natural scenario that arises when new CP-violation sources are introduced, and has not been studied in detail in the literature so far.

Likewise, the new physics contribution to \(B_{s}-\)mixing can be parameterised in terms of an effective Hamiltonian,
$$\begin{aligned} \mathcal {H}_{\text {eff}}^{b\bar{s}} = C_{B\bar{B}}^{\text {NP}} \, (\bar{s}_{\alpha }\gamma ^{\mu }P_{L}b_{\alpha })(\bar{s}_{\beta }\gamma _{\mu }P_{L}b_{\beta }), \end{aligned}$$
where \(\alpha \) and \(\beta \) are colour indices. The new physics contribution to the Wilson coefficient is given by
$$\begin{aligned} C_{B\bar{B}}^{\text {NP}} = \frac{1}{128\pi ^{2}m^{2}_{\psi }} (\lambda _{s}\lambda _{b}^{*})^{2} \left( F(x_{q},x_{q}) + 2G(x_{q},x_{q}) \right) , \end{aligned}$$
where the loop functions F and G were already defined in Eq. (2.11).
In order to quantify the allowed magnitude of the Wilson coefficient \(C_{B\bar{B}}^{\text {NP}}\), we follow the steps of [44] and introduce a complex parameter \(\Delta \) in the following way:
$$\begin{aligned} \frac{M_{12}^{\text {SM}} + M_{12}^{\text {NP}}}{M_{12}^{\text {SM}}} \equiv |\Delta |e^{i\phi _{\Delta }}, \end{aligned}$$
where \(M_{12}^{\text {SM}}\) and \(M_{12}^{\text {NP}}\) describe the SM and new physics contributions to \(B_{s}-\)mixing, and their values are given by the corresponding box diagrams. The complex phase, \(\phi _{\Delta }\), quantifies the CP-violating effects introduced by the imaginary parts of the new couplings. We find:
$$\begin{aligned} |\Delta |= & {} \frac{\Delta M_{s}^{\text {exp}}}{\Delta M_{s}^{\text {SM}}} = \left| 1+\frac{C_{B\bar{B}}^{\text {NP}}}{C_{B\bar{B}}^{\text {SM}}} \right| ,\nonumber \\ \phi _{\Delta }= & {} \text {Arg} \left( 1+\frac{C_{B\bar{B}}^{\text {NP}}}{C_{B\bar{B}}^{\text {SM}}} \right) , \end{aligned}$$
where \(\Delta M_{s}\) is the mass difference of the mass eigenstates of the \(B_s\) meson.
The parameter \(|\Delta |\) can be constrained using the most precise experimental measurement of \(\Delta M_{s}\)[60] and the last update on its theoretical prediction [44], which show a \(1.8 \sigma \) difference,
$$\begin{aligned} \Delta M_{s}^{\text {exp}}= & {} (17.757 \pm 0.021) \, \text {ps}^{-1},\nonumber \\ \Delta M_{s}^{\text {SM}}= & {} (20.01 \pm 1.25) \, \text {ps}^{-1}. \end{aligned}$$
The dominant uncertainties in the calculation of \(\Delta M_{s}^{\text {SM}}\) come from lattice predictions for the non-perturbative bag parameter, \(\mathcal {B}\), and decay constant, \(f_{B_{s}}\), and to a lesser extent from the uncertainty in the values of CKM elements. Both of these errors have been considerably reduced since the last theory update for the mass difference [61]. The last average given by the lattice community [62] gives significantly more precise values for \(\mathcal {B}\) and \(f_{B_{s}}\).
From these values, one can infer \(|\Delta | = 0.887 \pm 0.055\), and using the data provided in Ref. [44] we obtain \(C_{B\bar{B}}^{\text {SM}} = 4.897 \times 10^{-5} \; {\mathrm {TeV}}^{-2} \,\). Using Eq. (2.15) we find that the Wilson coefficient has to satisfy
$$\begin{aligned} \sqrt{\left( 1 + \frac{\text {Re}\, C_{B\bar{B}}^{\text {NP}}}{C_{B\bar{B}}^{\text {SM}}} \right) ^{2} + \left( \frac{\text {Im}\, C_{B\bar{B}}^{\text {NP}}}{C_{B\bar{B}}^{\text {SM}}} \right) ^{2}} \in \, [0.777, 0.998] \quad (2\sigma ). \end{aligned}$$
CP-violating effects are further constrained by the CP asymmetry of the golden mode \(B_{s} \rightarrow J/\psi \, \phi \) [60],
$$\begin{aligned} A_{\text {CP}}^{\text {mix}}(B_{s} \rightarrow J/\psi \phi ) = \sin (\phi _{\Delta } - 2\beta _{s}) \, = -\,0.021 \pm 0.031, \end{aligned}$$
where \(\beta _{s} = 0.01852 \pm 0.00032\) [63], and penguin contributions are neglected. Using Eq. (2.15), this can be interpreted as an additional constraint on the real and imaginary parts of \(C_{B\bar{B}}^{\text {NP}}\) (and in turn, on the real and imaginary parts of the couplings \(\lambda _{s}\lambda _{b}^{*}\)).
Fig. 3

The dark (light) green area is the \(1\sigma \) (\(2\sigma \)) allowed region by \(b \rightarrow s \mu ^+ \mu ^- \) observables in the \(({\text {Re}}(\lambda _s \lambda _b^*), {\text {Im}}(\lambda _s \lambda _b^*) )\) plane. Dark (light) blue regions correspond to \(1\sigma \; (2\sigma )\) \(B_s-\) mixing allowed regions. We take \(\lambda _\mu = \sqrt{4\pi } \) and \(m_{\phi _q} = 1.5 \, {\mathrm {TeV}}\) (top row), \(2.5 \, {\mathrm {TeV}}\) (bottom row). The specific values of \(m_\chi \), \(m_{\phi _l}\) are given in the plot and \(m_{\phi _l}\) is fixed to reproduce the measured DM relic abundance

In Fig. 3, the effect of all of these constraints on the real and imaginary parts of the couplings \(\lambda _{s}\lambda _{b}^{*}\) for several benchmark points is shown. Regions that are allowed by \(b \rightarrow s\mu ^{+}\mu ^{-}\) observables and \(B_{s}-\)mixing (given by Eqs. (2.17) and (2.18)) are shaded in green and blue, respectively. For illustrative purposes, the figure shows the constraints for multiple values of DM and mediator masses, while keeping \(\lambda _\mu =\sqrt{4\pi }\) fixed. We remind the reader that the mass of \(m_{\phi _{l}}\) is fixed so as to reproduce the correct relic density using Eq. (2.9).

As we can observe, in order to simultaneously satisfy both types of constraints, complex couplings are needed (\(\text {Im}(\lambda _{s}\lambda _{b}^{*})\ne 0\)). Also, as the mass of the dark matter particle and the mediators increase, both areas are more difficult to reconcile. In practise, this leads to an upper bound on the masses of the exotic new particles. The precise limit depends on the choice of couplings, which we will discuss in Sect. 3.

Finally, the new physics couplings to the up-type quarks are generated via CKM rotation,
$$\begin{aligned} \lambda _{u}= & {} V_{us}\lambda _{s} + V_{ub}\lambda _{b}, \nonumber \\ \lambda _{c}= & {} V_{cs}\lambda _{s} + V_{cb}\lambda _{b}. \end{aligned}$$
These couplings generate a new physics contribution to \(D^{0}-\)mixing, and the Wilson coefficient \(C_{D\bar{D}}^{\text {NP}}\) is obtained replacing \(\lambda _{s}\) and \(\lambda _{b}^{*}\) in Eq. (2.13) by \(\lambda _{u}\) and \(\lambda _{c}^{*}\), respectively.
In contrast to \(B_{s}-\)mixing, there is no precise theory determination for the mass difference in the \(D^{0}\) system. Therefore, in order to constrain the new physics contribution to \(C_{D\bar{D}}\) we use the measured value of the mass difference in \(D^{0}-\)mixing. The experimental bound on the mixing diagram is given by [64]
$$\begin{aligned} |M_{12}|_{D\bar{D}}^{\text {exp}} \in [0.6, 7.5] \times 10^{-3} \, \text {ps}^{-1} \quad (2\sigma ), \end{aligned}$$
whereas the new physics contribution to \(D^{0}-\)mixing is described by
$$\begin{aligned} |M_{12}|_{D\bar{D}} = \frac{|C_{D\bar{D}}|}{2M_{D^{0}}}\langle {D^{0}}| \mathcal {O} |{\bar{D}^{0}}\rangle , \end{aligned}$$
where \(\mathcal {O}\) is a combination of operators containing all possible SM and new physics contributions to \(D^{0}-\)mixing. Using the last results from [65] we get the following bound on the Wilson coefficient:
$$\begin{aligned} |C_{D\bar{D}}^{\text {exp}}| \le 5.695 \times 10^{-8} \; {\mathrm {TeV}}^{-2} \quad (2\sigma ). \end{aligned}$$
Although this model induces new physics contributions to other flavour observables (such as \(b \rightarrow s\gamma \), \(b \rightarrow s\nu \bar{\nu }\) and effective \(Z\mu ^{+}\mu ^{-}\) and \(Zq_{i}q_{j}\) couplings), their size is very small and does not produce significant deviations from current experimental searches.

2.3 Benchmark scenarios

All the new physics contributions to the observables described above depend on five independent parameters: the three masses of the new particles, \(m_{\chi }\), \(m_{\phi _{q}}\) and \(m_{\phi _{l}}\), the product of the couplings \(\lambda _{s}\lambda _{b}^{*}\) and the absolute value of the coupling \(|\lambda _{\mu }|\).
Fig. 4

Diagrams for the pair production of the coloured scalar mediator, \(\phi _q\), leading to Open image in new window signatures in the final state. Diagrams (a1)–(a4) are generated by purely QCD interactions, and diagrams (b), (c1)–(c4) are generated by DM t-channel exchange

The three masses only enter the Wilson coefficients through the factor \(m_{\chi }^{-2}\) and the dimensionless loop functions. In addition, all the Wilson coefficients are proportional to \(\lambda _{s}\lambda _{b}^{*}\) or \(|\lambda _{\mu }|^{2}\) or both. In order to constrain our model, we consider two scenarios by fixing the value of \(|\lambda _{\mu }|\). Then we scan over the mass parameters \(m_{\chi }\) and \(m_{\phi _{q}}\), with \(m_{\phi _{l}}\) fixed by the requirement of reproducing the correct relic abundance, and check all the flavour observables described in Sect. 2.2. In this way, for any combination of masses and a fixed value of \(|\lambda _{\mu }|\) we get a set of allowed values for \(\lambda _{s}\lambda _{b}^{*}\). We consider two hierarchies between \(|\lambda _{s}|\) and \(|\lambda _{b}|\) that lead to different constraints from \(D^{0}-\)mixing, and, ensuring that \(\text {Im}(\lambda _s\lambda _b^*)\ne 0\), we define the following benchmark scenarios:
  1. (A1)

    \(|\lambda _{\mu }| = 2\), with \(\lambda _{b} = \lambda _{s}^*\);

  2. (A2)

    \(|\lambda _{\mu }| = 2\), with \(\lambda _{b} = 4\lambda _{s}^*\);

  3. (B1)

    \(|\lambda _{\mu }| = \sqrt{4\pi }\), with \(\lambda _{b} = \lambda _{s}^*\);

  4. (B2)

    \(|\lambda _{\mu }| = \sqrt{4\pi }\), with \(\lambda _{b} = 4\lambda _{s}^*\),

where \(|\lambda _{\mu }| = \sqrt{4\pi }\) is the perturbative limit. After establishing a hierarchy between \(|\lambda _{s}|\) and \(|\lambda _{b}|\), we calculate their maximum and minimum allowed values from the corresponding maximum and minimum allowed values of \(\lambda _{s}\lambda _{b}^{*}\). Scenarios with \(|\lambda _{s}| > |\lambda _{b}|\) are excluded by \(D^{0}-\)mixing constraints. Likewise, as we will see in Sect. 3, smaller values of \(\lambda _\mu \) are constrained by LHC bounds.

3 LHC constraints and prospects for high-luminosity

In this section, we study the experimental signatures that this model would produce at the LHC. DM search strategies in both ATLAS and CMS involve analysing final states containing jets and leptons produced in association with a DM particle, identified from missing transverse energy. In this model, direct production of the coloured and leptonic scalar doublets \(\phi _q\) and \(\phi _l\), respectively, typically leads to such final states.

Let us first consider production processes that involve the coloured scalar, \(\phi _q\). In this case, our model could lead to visible signals in final states with both Open image in new window signatures. When the new physics coupling \(\lambda _q\) is smaller than the strong interaction coupling, \(\alpha _{\text {QCD}}\), pure QCD processes constitute the main contribution to the cross section [66]. In this model, this implies that QCD diagrams dominate over those with new physics couplings. As a consequence, monojet searches for this model are less effective than dijet searches and we will concentrate on the latter. The Open image in new window processes are shown in Fig. 4, where diagrams (a) correspond to the QCD contributions, and diagrams (b) and (c) involve new physics couplings. The main production channel is the pair production of the coloured scalar particles, that subsequently decays into a DM particle and a quark,In addition, the scalar doublet \(\phi _q\) has the same quantum numbers as squarks in supersymmetric (SUSY) models. Therefore, the kinematics in its production and decay in diagrams (a) of Fig. 4 mimic those of squarks in SUSY models with decoupled gluinos. As a consequence, limits from ATLAS and CMS squark searches can be used to constrain the model.
One can also consider the pair production of the leptonic scalar, \(\phi _l\). In this case, the production process is mediated by W or Z bosons and involves the electroweak coupling, as shown in Fig. 5. The decays of \(\phi _l\) lead to clean final states with one or two leptons and missing energy. Although flavour constraints require \(\lambda _\mu \gg \lambda _q\), the cross section of this process is smaller than the production of the coloured mediator for similar mediator masses. However, since \(m_{\phi _l}\) is fixed for every value of \(m_{\chi }\) to reproduce the correct relic abundance, there are regions of the parameter space where both searches are complementary. We will here consider the processwhere the dimuon channel leads to the strongest constraints. As in the previous case, we can exploit the analogy between \(\phi _l\) and sleptons to use the limits from slepton searches to constrain this model.
Fig. 5

Diagrams for the pair production of the leptonic scalar mediator, \(\phi _l\), leading to Open image in new window signatures in the final state

3.1 Simulation details

We have implemented this model in Feynrules 2.3[67]. The calculation of the matrix elements and the event generation is done using MadGraph5_aMC@NLO 2.6.3[68]. Production and decay of the new particles are considered independently using the narrow width approximation, as implemented in MadSpin[69], which further accounts for spin correlations in decay chains.4 We then use Pythia 8.235[70] to shower the parton-level events and we pass the output to CheckMATE 2.0.26 [71], which compares the expected signal with supersymmetric searches at the LHC and derives an exclusion limit. As we have explained above, we can apply squark and slepton searches to constrain the coloured and leptonic mediator, respectively.

In order to describe initial and final state radiation and reproduce the correct jet structure precisely, we consider leading order (LO) production with parton shower matching and multijet merging when needed. The LO multijet merging techniques describe how parton shower emissions can be combined with full matrix element calculations to achieve a better accuracy in the description of the radiation spectrum. Using this technique, every jet is classified according to its \(p_T\) and then compared to a hardness scale \(Q_{\text {cut}}\). In this way, emissions above the hardness scale \(Q_{\text {cut}}\) are described at LO accuracy using the corresponding matrix element calculation for an extra hard, wide-angle QCD emission in the final state, while emissions below this scale are defined as soft or collinear jets and the all-orders resummation description from the parton shower is preserved. Note that even though \(\mathcal {O}(\alpha _s)\) corrections are included using this procedure, the calculation remains formally \(\text {LO}+\text {LL}\) accurate after parton shower due to missing virtual corrections.

After hadronization, the showered events and the production cross sections are passed to CheckMATE. Each model point is tested against all the implemented experimental analyses to determine the optimal signal region. For this signal region, CheckMATE compares the simulated signal with the actual experimental observation and determines whether the model point is excluded at the \(90\%\) confidence level.

3.2 Results

Constraints from LHC searches for the four benchmark points defined in Sect. 2.3 are presented in Fig. 6 on the \((m_{\chi },\,m_{\phi _{q}})\) plane, for all the points that satisfy the flavour constraints of Sect. 2.2 and that reproduce the correct DM relic abundance. This figure shows the complementarity between the experimental limits obtained from the Open image in new window and Open image in new window searches. The experimental results used in our analysis are summarised in Table 2. The colour code represents the average value of the coupling \(|\lambda _b|\) in the region allowed by flavour constraints, defined as \(|\lambda _b|_\mathrm{mean} = (|\lambda _b|_\mathrm{max} + |\lambda _b|_\mathrm{min}) / 2\), where \(|\lambda _b|_\mathrm{max}\) and \(|\lambda _b|_\mathrm{min}\) are the maximum and minimum allowed values respectively. The variation of our results when choosing either the minimum or maximum value for \(|\lambda _b|\) has been checked and is insignificant.
Fig. 6

LHC limits from the Open image in new window (green) and Open image in new window (blue) searches. On the left (right), results for the scenario with \(|\lambda _\mu | = 2\) (\(|\lambda _\mu | = \sqrt{4\pi }\)) are presented. The figures in the upper panel correspond to \(\lambda _b = \lambda _s^*\), while the bottom panel shows limits for \(\lambda _b = 4\lambda _s^*\). The colour code represents the average value of the coupling \(|\lambda _b|\) in the region allowed by flavour constraints, as defined in the text. Solid lines represent the current exclusion limits, whereas dashed ones correspond to the projected reach of the LHC High luminosity phase

Table 2

List of experimental searches sensitive to our model, where l denotes electron and muon. The third column describes the final state targeted by the analysis and the last column displays the total integrated luminosity



Final state

\(\mathcal {L}\) [\(\hbox {fb}^{-1}\)]

13 TeV

1710.11412 [72]

Open image in new window


ATLAS-CONF-2017-039 [73]

Open image in new window


14 TeV

atlas_phys_pub_013_011 [74]

Open image in new window


atlas_phys_2014_010_hl_3l [75]

Open image in new window


Regarding the Open image in new window search, the limits in every scenario show that for the lightest DM mass, coloured mediators with masses below \(\sim \)1 TeV are excluded. Even though heavier DM produces larger amounts of missing energy in final states, the cross section decreases rapidly with the \(m_{\chi }\), leading to similar exclusion limits. It is interesting to note that exclusion limits are slightly stronger for the scenarios with \(|\lambda _{b,t}| > |\lambda _{s,c}|\), where mediators with masses below \(\sim \)1.1 TeV are excluded. The reason for this is that final states with either top or bottom quarks are more sensitive than final states with light jets to some experimental searches, which are specifically designed to target topologies with top and bottom quarks signatures. The most stringent experimental search involves final states with at least two (\(b \bar{b}\) production) or four (\(t \bar{t}\) production) jets or exactly two leptons and missing energy [72]. In particular, the most sensitive signal region is optimised to detect events featuring a DM particle produced in association with a \(t \bar{t}\) pair, which decays fully hadronically.

Regarding the Open image in new window search, the limits show that models with dark matter masses below approximately \( 30 \; {\mathrm {GeV}}\) are ruled out for \(|\lambda _\mu | = 2\), with the exclusion limit going down to \(\sim 13 \; {\mathrm {GeV}}\) for \(|\lambda _\mu | = \sqrt{4\pi }\). This corresponds to mediator masses below \(360 \; {\mathrm {GeV}}\) for \(|\lambda _\mu | = 2\) and \(410 \; {\mathrm {GeV}}\) for \(|\lambda _\mu | = \sqrt{4\pi }\). The Open image in new window cross section mainly depends on \(m_{\phi _l}\), so the limits on \(m_\chi \) can be understood through its relation with \(m_{\phi _l}\) given by the DM relic condition (2.9) for a particular value of \(\lambda _\mu \). The most stringent search involves final states with \(2l + 0 j\), 2l and at least 2 jets, or 3l and missing energy [73]. In particular, the most sensitive signal region is characterised by \(2l + 0j\) and a dilepton invariant mass \(m_{ll} > 300 \; {\mathrm {GeV}}\), and it is optimised to target slepton pair production.

The most remarkable result is that LHC limits completely exclude the scenario with \(|\lambda _\mu | = 2\) and \(\lambda _b = \lambda _s^*\), as well as a sizeable region of the scenario with \(\lambda _b = 4\lambda _s^*\) for the same \(|\lambda _\mu |\). These constraints become weaker for larger values of \(|\lambda _\mu |\) and, for the scenarios with \(|\lambda _\mu | = \sqrt{4\pi }\), most of the parameter space is allowed. It is crucial to note that the limits coming from final states with jets and leptons are complementary to each other. While the former exclude regions of the parameter space with large \(m_\chi \) and small \(m_{\phi _q}\), the latter rule out models with very heavy mediator masses \(m_{\phi _q}\) and light dark matter. Importantly, these limits are also complementary to the ones coming from direct detection, where dark matter masses below \(12 \; {\mathrm {GeV}}\) lie below the neutrino floor. Therefore, it is fundamental to consider both approaches to explore the model.

It is worth mentioning that the small couplings required by flavour constraints lead to decay widths slightly below the QCD scale for \(m_{\phi _{q}}\lesssim 370 \; {\mathrm {GeV}}\). Strictly speaking, this means that the computation of the decay width cannot be handled perturbatively and that the new particle \(\phi _q\) may hadronize into bound states with SM quarks, analogous to R-hadrons [76], before decaying. However, the typical width involved is \(\Gamma _{\phi _q} \sim \mathcal {O}(10^{-2})-\mathcal {O}(10^{-3}) \; {\mathrm {GeV}}\), which means lifetimes of the order \(\tau \sim 10^{-22} \; \text {s}\), so any potential bound state would decay promptly in the detector. This region of the parameter space is excluded by ATLAS and CMS R-hadron searches [77, 78].

We have also studied the limits that could be obtained with \(3000 \; \text {fb}^{-1}\) of 14 TeV data once the LHC High Luminosity phase [79] is completed. As we can observe in the plots, the main gain would come from the leptonic channels, which would allow to test a considerable amount of the model’s parameter space. In particular, scenarios with \(|\lambda _\mu | < 2\) would be completely excluded. The experimental searches giving the strongest exclusion limits target the same final states and are shown in the low panel of Table 2.

4 Direct DM detection prospects

Finally, in this section we discuss whether our model is expected to produce an observable response in direct detection experiments. We have calculated this response, by matching the model parameters to effective DM-nucleon interaction terms,
$$\begin{aligned} {\mathcal {L}}_{\text {int}}=\sum _{N} \sum _i c_i^{N}\mathcal {O}_i \overline{\chi } \chi \overline{N} N\ , \end{aligned}$$
where N is the corresponding nucleon, and \(\mathcal {O}_i\) is the set of non-relativistic operators [80, 81]. The values for the coefficients \(c_i^N\) can be derived as the non-relativistic limit of the original interaction Lagrangian, and the differential rate can be computed using the corresponding nuclear form factors from Refs. [81, 82], and for a given choice of the DM halo properties. We have adopted the so-called standard halo model [83] with local DM density \(\rho _{\chi }=0.4\ \text {GeV/cm}^3\), a central velocity of \(v_0=220\ \text {km s}^{-1}\), and a escape speed of \(v_{\text {esc}}=544\ \text {km s}^{-1}\) to calculate the number of expected recoils in a specific experiment.
The leading tree-level DM-quark interactions are given by scalar (\(\overline{\chi }\chi \overline{\psi }\psi \)) and vector (\(\overline{\chi }\gamma ^{\mu }\chi \overline{\psi }\gamma _{\mu }\psi \)) type interactions. The latter is the leading contribution to \(\mathcal {O}_1\) for Dirac DM [84], but it vanishes in the case of Majorana DM. For scalar type interactions Majorana DM does not in general vanish, but with our models chiral structure, it does. With sub-dominant couplings to the first generation of quarks, and given that \(m_{\phi _{q}}>m_{\phi _{l}}\), one-loop contributions to the DM-nucleon scattering cross sections will generally be larger than the tree level process. The loop contributions for a generic fermionic DM that involve the exchange of a photon can be classified as electric and magnetic dipoles (\(\overline{\chi }i\sigma ^{\mu \nu }\gamma ^5\chi F_{\mu \nu }\) and \(\overline{\chi }\sigma ^{\mu \nu }\chi F_{\mu \nu }\), respectively), anapole (\(\overline{\chi }\gamma ^{\mu }\gamma ^5\chi \partial ^{\nu }F_{\mu \nu }\)), and charge radius (\(\overline{\chi }\gamma ^{\mu }\chi \partial ^{\nu }F_{\mu \nu }\)). However, in the particular case of Majorana DM considered in this work, the magnetic dipole and charge radius effective couplings are forbidden by charge conjugation symmetry. Thus, the dominant one-loop interaction is the anapole moment [85]. When taking the non-relativistic limit, the anapole moment gives contributions to the \(\mathcal {O}_8\) and \(\mathcal {O}_9\) operators [86, 87], which are velocity and momentum dependent. In terms of the fundamental parameters of the model, the corresponding couplings read
$$\begin{aligned} c_8= & {} 2 e \mathcal {A} Q_N,\nonumber \\ c_9= & {} - e \mathcal {A} g_N, \end{aligned}$$
where e is the electron charge, \(Q_N\) is the nucleon charge, and \(g_N\) are the nucleon g-factors (\(g_p=5.59\) and \(g_n=3.83\)). The effective coupling to the anapole interaction term, \(\mathcal {A}\), reads [88]
$$\begin{aligned} \mathcal {A}= & {} -\frac{e\,|\lambda _\mu |^2}{96\pi ^2m_{\chi }^2} \left[ \frac{3}{2} \log \frac{\mu }{\epsilon } - \frac{1+3\mu -3\epsilon }{\sqrt{(\mu -1-\epsilon )^2-4\epsilon }}\right. \nonumber \\&\left. {{\,\mathrm{arctanh}\,}}{\left( \frac{\sqrt{(\mu -1-\epsilon )^2-4\epsilon }}{\mu -1+\epsilon }\right) } \right] \ , \end{aligned}$$
with \(\mu \equiv m_{\phi _{l}}^{2}/m_{\chi }^2\) and \(\epsilon \equiv m_l^2/m_{\chi }^2\). The nuclear responses to the \(\mathcal {O}_8\) and \(\mathcal {O}_9\) operators are markedly weaker than that of \(\mathcal {O}_1\), which implies that, in general, the scattering cross section is very small and beyond current experimental limits. Furthermore, because our DM particle interacts with the quark sector, it is not a priori clear that the spin-independent \(\mathcal {O}_1\) and spin-dependent \(\mathcal {O}_4\) arising from the so-called twist-2 operator [89, 90, 91] and the axial vector operator respectively are still negligible.
Fig. 7

Theoretical predictions for the anapole coupling, \(\mathcal {A}\), as a function of the DM mass, \(m_{\chi }\) for the four benchmark points: A1 (red points), A2 (green), B1 (orange), and B2 (blue). For comparison, we show the current exclusion line by Xenon1T [92] and the predicted reach of LZ [94, 95] and DarkSide-20k [96]. The shaded area represents the neutrino floor. The plot on the right-hand side incorporates LHC constraints, explained in more detail in Sect. 3

Fig. 8

The same as in Fig. 7, but for the spin-independent coupling, \(c_1\), that originates from the twist-2 coupling

Given the range of DM masses that we consider in this study, the main constraint is due to Xenon1T results [92], which we simulate using the prescription outlined in appendix A of Ref. [93], achieving good agreement. As we can see in Fig. 7, the theoretical predictions for this model are beyond the reach of current experimental searches. We also show the reach of future direct detection experiments. The LZ detector, will employ 5.6 tons of liquid xenon with 1000 days exposure as outlined in [94, 95]. The DarkSide-20k experiment [96], is an argon detector which will employ 20 tons of fiducial mass for a duration of 10 years. We have assumed that the DarkSide collaboration will be able to achieve a threshold energy of 5 keV, a reasonable assumption considering the results from DarkSide-50 [97]. For reference we have also calculated the neutrino floor for anapole interactions in the \((\mathcal {A},\, m_{\chi })\) plane. We have used the prescription described in Ref. [98] and the expected neutrino fluxes from Refs. [99, 100, 101, 102, 103, 104]. It is clear that our model favourably lays in a region of parameter space that would be probed by a generation of experiments with multi-ton targets, that can probe near or even slightly beyond the neutrino floor. Spectral analysis with the neutrino background compounded with annual modulation data, could provide complete discrimination between model and the anapole moment which is both velocity and momentum dependent.

For completeness, we have also calculated the effect on the total scattering cross section from aforementioned twist-2 operator and spin-dependent interaction. The former contribute to the spin-independent scattering cross section (operator \(\mathcal{{O}}_1\)) and can be sizeable if the new coupling to quarks is large or the colour mediator is very light. We have explicitly checked that once LHC constraints are included in the parameter space of the model, these terms are always subdominant to the anapole term discussed above.5 We represent in Fig. 8 the theoretical predictions for \(c_1\) as a function of the DM mass from this contribution. For the spin-dependent interaction, we found that the predicted rate for our sampled parameter space is always sub-dominant.

Had we chosen to work with a Dirac fermion, the dipole and charge radius contributions should have been added. As it has been pointed out in Ref. [84], the fairly large coupling to muons that is required to explain the flavour anomalies leads to effective DM couplings that are orders of magnitude higher than those coming from the tree level contribution, the most important being the charge-radius interaction. This we have checked, and in fact above \(m_{\chi }\sim 10\) GeV, all our parameter points are excluded by Xenon1T. Below \(m_{\chi }\sim 10\), the model is excluded by both LHC constraints and indirect detection bounds. Unlike in the Majorana case, the s-wave contribution to the thermal cross section \(\langle \sigma v\rangle \) is no longer helicity suppressed and hence excluded [105].

Our results suggest that future multi-ton direct detection experiments, such as DarkSide [96], would be able to probe this model in the mass range \(m_{\chi }\sim \) 10–60 GeV. It is very interesting to point out that many of the points in this DM mass range feature very heavy \(\phi _q\) and therefore would be beyond the reach of collider searches. In a sense, future direct DM detection and the LHC complement each other to probe a large part of the model’s parameter space.

5 Conclusions

In this article, we have studied a particle physics model that addresses the hints of lepton flavour universality violation observed by LHCb in \(b \rightarrow s\mu ^{+}\mu ^{-}\) transitions, and that provides a solution to the dark matter problem. The scenario that we have analysed incorporates two new scalar fields and a Majorana fermion that provide one-loop contributions to B meson decays.

The Majorana fermion is stable and can reproduce the observed DM relic abundance. We have studied the effect of new physics in flavour observables, for which \(B_{s}-\)mixing and \(b \rightarrow s\mu ^{+}\mu ^{-}\) processes provide the most important constraints. In order to find an explanation for the B anomalies and to reduce the \(1.8\,\sigma \) tension between the predicted and measured mass difference in \(B_{s}-\)mixing, complex couplings are needed. We have used results from the first global fit that takes into account this possibility. The combination of flavour bounds and constraints on the DM relic abundance leads to upper limits on the masses of the exotic states, and in general points towards a rather light DM candidate (with a mass \(m_{\chi }\lesssim 200\) GeV).

We have studied the signatures that this model would produce at the LHC. The dominant processes are the pair production of the coloured and leptonic scalars. For the former, the strongest exclusion limits are given by Open image in new window searches. For the latter, the final states are very clean, containing 1 or 2 leptons and missing energy. Both searches are complementary and exclude different regions of the parameter space, setting lower bounds on DM and mediator masses. The high-luminosity phase improves bounds coming from both searches, with dilepton being the most pronounced. The collider constraints are weakened when the \(\lambda _{\mu }\) parameter is pushed towards the perturbative limit.

Finally, we have investigated how DM direct detection experiments constrain this model. Given the range of DM masses that we consider in this study, the main constraint is due to Xenon1T results. The small new couplings required by flavour constraints means that one-loop contributions to the DM-nucleon scattering cross section are generally larger than the tree level process. In particular, the dominant loop induced interaction is the anapole moment. We have shown that this model is not excluded by current data and could be probed by the next generation of experiments with multi-ton targets in the mass range \(m_{\chi }\sim \) 10–60 GeV.


  1. 1.

    An alternative to this one-loop solution is to consider \( Z^\prime \) [16, 17] or leptoquark [18, 19] tree-level contributions, see e.g., Ref. [20] and references therein. The DM problem has been addressed in the framework of these constructions [21], see e.g., Refs. [22, 23, 24, 25, 26, 27, 28, 29, 30, 31, 32, 33, 34, 35, 36] for the \(Z^\prime \), and Refs. [37, 38, 39, 40] for the leptoquark models.

  2. 2.

    As we will comment in Sect. 4, the alternative construction with Dirac DM is ruled out mainly by experimental results from direct DM detection.

  3. 3.

    We have neglected the Z-penguin contribution to \(C_{9}^{\text {NP}}\), since it is suppressed by \((m_{b}/m_{Z})^{2}\) and is subdominant compared to the photon exchange.

  4. 4.

    The narrow width approximation is not valid in benchmark points B1 and B2, for which we have taken interference effects into account.

  5. 5.

    Note that box diagrams containing a W boson give an additional contribution, which is further suppressed by CKM factors and electroweak couplings and can thus be safely neglected.



We would like to thank Alejandro Ibarra for useful discussions. DC and AC are grateful for the support from the Science and Technology Facilities Council (STFC). DC acknowledges the partial support of the Centro de Excelencia Severo Ochoa Program through the IFT-UAM/CSIC Associate programme. PMR and JMM acknowledge support from the Spanish Research Agency (Agencia Estatal de Investigación) through the contract FPA2016-78022-P and IFT Centro de Excelencia Severo Ochoa under Grant SEV-2016-0597.


  1. 1.
    LHCb Collaboration, R. Aaij et al., Differential branching fractions and isospin asymmetries of \(B \rightarrow K^{(*)} \mu ^+ \mu ^-\) decays. JHEP 06, 133 (2014). arXiv:1403.8044
  2. 2.
    LHCb Collaboration, R. Aaij et al., Angular analysis and differential branching fraction of the decay \(B^0_s\rightarrow \phi \mu ^+\mu ^-\). JHEP 09, 179 (2015). arXiv:1506.08777
  3. 3.
    G. Hiller, F. Kruger, More model-independent analysis of \(b \rightarrow s\) processes. Phys. Rev. D 69, 074020 (2004). arXiv:hep-ph/0310219 ADSGoogle Scholar
  4. 4.
    M. Bordone, G. Isidori, A. Pattori, On the Standard Model predictions for \(R_K\) and \(R_{K^*}\). Eur. Phys. J. C 76, 440 (2016). arXiv:1605.07633 ADSGoogle Scholar
  5. 5.
    Belle Collaboration, J.T. Wei et al., Measurement of the differential branching fraction and forward–backword asymmetry for \(B \rightarrow K^{(*)}\ell ^+\ell ^-\). Phys. Rev. Lett. 103, 171801 (2009). arXiv:0904.0770
  6. 6.
    CMS Collaboration, V. Khachatryan et al., Angular analysis of the decay \(B^0 \rightarrow K^{*0} \mu ^+ \mu ^-\) from pp collisions at \(\sqrt{s} = 8\) TeV. Phys. Lett. B 753, 424–448 (2016). arXiv:1507.08126
  7. 7.
    Belle Collaboration, A. Abdesselam et al., Angular analysis of \(B^0 \rightarrow K^\ast (892)^0 \ell ^+ \ell ^-\), in Proceedings, LHCSki 2016—A First Discussion of 13 TeV Results, Obergurgl, Austria, April 10–15, 2016 (2016). arXiv:1604.04042
  8. 8.
    BaBar Collaboration, J.P. Lees et al., Measurement of angular asymmetries in the decays \(B \rightarrow K^{*+-}\). Phys. Rev. D 93, 052015 (2016). arXiv:1508.07960
  9. 9.
    CMS Collaboration, A.M. Sirunyan et al., Measurement of angular parameters from the decay \({\rm B}^0 \rightarrow {\rm K}^{*0} \mu ^+ \mu ^-\) in proton–proton collisions at \(\sqrt{s} = \) 8 TeV. Phys. Lett. B 781, 517–541 (2018). arXiv:1710.02846
  10. 10.
    ATLAS Collaboration, M. Aaboud et al., Angular analysis of \(B^0_d \rightarrow K^{*}\mu ^+\mu ^-\) decays in \(pp\) collisions at \(\sqrt{s}= 8\) TeV with the ATLAS detector. JHEP 10, 047 (2018). arXiv:1805.04000
  11. 11.
    Belle Collaboration, S. Wehle et al., Lepton-flavor-dependent angular analysis of \(B\rightarrow K^\ast \ell ^+\ell ^-\). Phys. Rev. Lett. 118, 111801 (2017). arXiv:1612.05014
  12. 12.
    CDF Collaboration, T. Aaltonen et al., Measurements of the angular distributions in the decays \(B \rightarrow K^{(*)} \mu ^+ \mu ^-\) at CDF. Phys. Rev. Lett. 108, 081807 (2012). arXiv:1108.0695
  13. 13.
    LHCb Collaboration, R. Aaij et al., Angular analysis of the \(B^{0} \rightarrow K^{*0} \mu ^{+} \mu ^{-}\) decay using 3 fb\(^{-1}\) of integrated luminosity. JHEP 02, 104 (2016). arXiv:1512.04442
  14. 14.
    B. Gripaios, M. Nardecchia, S.A. Renner, Linear flavour violation and anomalies in B physics. JHEP 06, 083 (2016). arXiv:1509.05020 ADSCrossRefGoogle Scholar
  15. 15.
    P. Arnan, L. Hofer, F. Mescia, A. Crivellin, Loop effects of heavy new scalars and fermions in \(b\rightarrow s\mu ^+\mu ^-\). JHEP 04, 043 (2017). arXiv:1608.07832 ADSGoogle Scholar
  16. 16.
    A.J. Buras, J. Girrbach, Left-handed \(Z^{\prime }\) and \(Z\) FCNC quark couplings facing new \(b \rightarrow s \mu ^+ \mu ^-\) data. JHEP 12, 009 (2013). arXiv:1309.2466 ADSGoogle Scholar
  17. 17.
    R. Gauld, F. Goertz, U. Haisch, An explicit \(Z^{\prime }\)-boson explanation of the \(B \rightarrow K^* \mu ^+ \mu ^-\) anomaly. JHEP 01, 069 (2014). arXiv:1310.1082 ADSGoogle Scholar
  18. 18.
    M. Bauer, M. Neubert, Minimal leptoquark explanation for the R\(_{D^{(*)}}\), R\(_K\), and \((g-2)_g\) anomalies. Phys. Rev. Lett. 116, 141802 (2016). arXiv:1511.01900 ADSGoogle Scholar
  19. 19.
    A. Angelescu, D. Becirevic, D.A. Faroughy, O. Sumensari, Closing the window on single leptoquark solutions to the \(B\)-physics anomalies. JHEP 10, 183 (2018). arXiv:1808.08179 ADSGoogle Scholar
  20. 20.
    B. Capdevila, A. Crivellin, S. Descotes-Genon, J. Matias, J. Virto, Patterns of new physics in \(b\rightarrow s\ell ^+\ell ^-\) transitions in the light of recent data. JHEP 01, 093 (2018). arXiv:1704.05340 ADSGoogle Scholar
  21. 21.
    A. Vicente, Anomalies in \(b \rightarrow s\) transitions and dark matter. Adv. High Energy Phys. 2018, 3905848 (2018). arXiv:1803.04703 Google Scholar
  22. 22.
    D. Aristizabal Sierra, F. Staub, A. Vicente, Shedding light on the \(b\rightarrow s\) anomalies with a dark sector. Phys. Rev. D 92, 015001 (2015). arXiv:1503.06077 ADSGoogle Scholar
  23. 23.
    G. Bélanger, C. Delaunay, S. Westhoff, A dark matter relic from muon anomalies. Phys. Rev. D 92, 055021 (2015). arXiv:1507.06660 ADSCrossRefGoogle Scholar
  24. 24.
    W. Altmannshofer, S. Gori, S. Profumo, F.S. Queiroz, Explaining dark matter and B decay anomalies with an \(L_\mu - L_\tau \) model. JHEP 12, 106 (2016). arXiv:1609.04026 ADSGoogle Scholar
  25. 25.
    A. Celis, W.-Z. Feng, M. Vollmann, Dirac dark matter and \(b \rightarrow s \ell ^+ \ell ^-\) with \(\rm U(1)\) gauge symmetry. Phys. Rev. D 95, 035018 (2017). arXiv:1608.03894 ADSGoogle Scholar
  26. 26.
    J.M. Cline, J.M. Cornell, D. London, R. Watanabe, Hidden sector explanation of \(B\)-decay and cosmic ray anomalies. Phys. Rev. D 95, 095015 (2017). arXiv:1702.00395 ADSGoogle Scholar
  27. 27.
    P. Ko, T. Nomura, H. Okada, Explaining \(B\rightarrow K^{(*)}\ell ^+ \ell ^-\) anomaly by radiatively induced coupling in \(U(1)_{\mu -\tau }\) gauge symmetry. Phys. Rev. D 95, 111701 (2017). arXiv:1702.02699 ADSGoogle Scholar
  28. 28.
    J. Ellis, M. Fairbairn, P. Tunney, Anomaly-free models for flavour anomalies. Eur. Phys. J. C 78, 238 (2018). arXiv:1705.03447 ADSCrossRefGoogle Scholar
  29. 29.
    S. Baek, Dark matter contribution to \(b\rightarrow s \mu ^+ \mu ^-\) anomaly in local \(U(1)_{L_\mu -L_\tau }\) model. Phys. Lett. B 781, 376–382 (2018). arXiv:1707.04573 ADSGoogle Scholar
  30. 30.
    K. Fuyuto, H.-L. Li, J.-H. Yu, Implications of hidden gauged \(U(1)\) model for \(B\) anomalies. Phys. Rev. D 97, 115003 (2018). arXiv:1712.06736 ADSGoogle Scholar
  31. 31.
    P. Cox, C. Han, T.T. Yanagida, Right-handed neutrino dark matter in a U(1) extension of the standard model. JCAP 1801, 029 (2018). arXiv:1710.01585 ADSCrossRefGoogle Scholar
  32. 32.
    A. Falkowski, S.F. King, E. Perdomo, M. Pierre, Flavourful \(Z^{\prime }\) portal for vector-like neutrino dark matter and \(R_{K^{(*)}}\). JHEP 08, 061 (2018). arXiv:1803.04430 ADSGoogle Scholar
  33. 33.
    L. Darmé, K. Kowalska, L. Roszkowski, E.M. Sessolo, Flavor anomalies and dark matter in SUSY with an extra U(1). JHEP 10, 052 (2018). arXiv:1806.06036 ADSCrossRefGoogle Scholar
  34. 34.
    S. Singirala, S. Sahoo, R. Mohanta, Exploring dark matter, neutrino mass and \(R_{K^{(*)},\phi }\) anomalies in \(L_{\mu }-L_{\tau }\) model. arXiv:1809.03213
  35. 35.
    S. Baek, C. Yu, Dark matter for \(b\rightarrow s \mu ^+ \mu ^-\) anomaly in a gauged \(U(1)_X\) model. JHEP 11, 054 (2018). arXiv:1806.05967 ADSGoogle Scholar
  36. 36.
    A. Kamada, M. Yamada, T.T. Yanagida, Self-interacting dark matter with a vector mediator: kinetic mixing with U(1)\(_{(B-L)_3}\) gauge boson. arXiv:1811.02567
  37. 37.
    C. Hati, G. Kumar, J. Orloff, A.M. Teixeira, Reconciling \(B\)-meson decay anomalies with neutrino masses, dark matter and constraints from flavour violation. JHEP 11, 011 (2018). arXiv:1806.10146 ADSGoogle Scholar
  38. 38.
    S.-M. Choi, Y.-J. Kang, H.M. Lee, T.-G. Ro, Lepto-quark portal dark matter. JHEP 10, 104 (2018). arXiv:1807.06547 ADSCrossRefGoogle Scholar
  39. 39.
    J.M. Cline, \(B\) decay anomalies and dark matter from vectorlike confinement. Phys. Rev. D 97, 015013 (2018). arXiv:1710.02140 ADSGoogle Scholar
  40. 40.
    I. de Medeiros Varzielas, O. Fischer, Non-Abelian family symmetries as portals to dark matter. JHEP 01, 160 (2016). arXiv:1512.00869 ADSCrossRefGoogle Scholar
  41. 41.
    J. Kawamura, S. Okawa, Y. Omura, Interplay between the b\(\rightarrow s\ell \ell \) anomalies and dark matter physics. Phys. Rev. D 96, 075041 (2017). arXiv:1706.04344 ADSGoogle Scholar
  42. 42.
    B. Bhattacharya, D. London, J.M. Cline, A. Datta, G. Dupuis, Quark-flavored scalar dark matter. Phys. Rev. D 92, 115012 (2015). arXiv:1509.04271 ADSCrossRefGoogle Scholar
  43. 43.
    J.M. Cline, J.M. Cornell, \(R({K^{(*)}})\) from dark matter exchange. Phys. Lett. B 782, 232–237 (2018). arXiv:1711.10770 ADSGoogle Scholar
  44. 44.
    L. Di Luzio, M. Kirk, A. Lenz, Updated \(B_s\)-mixing constraints on new physics models for \(b\rightarrow s\ell ^+\ell ^-\) anomalies. Phys. Rev. D 97, 095035 (2018). arXiv:1712.06572 ADSGoogle Scholar
  45. 45.
    S. Descotes-Genon, L. Hofer, J. Matias, J. Virto, Global analysis of \(b\rightarrow s\ell \ell \) anomalies. JHEP 06, 092 (2016). arXiv:1510.04239 ADSGoogle Scholar
  46. 46.
    T. Hurth, F. Mahmoudi, S. Neshatpour, On the anomalies in the latest LHCb data. Nucl. Phys. B 909, 737–777 (2016). arXiv:1603.00865 ADSCrossRefGoogle Scholar
  47. 47.
    W. Altmannshofer, P. Stangl, D.M. Straub, Interpreting hints for lepton flavor universality violation. Phys. Rev. D 96, 055008 (2017). arXiv:1704.05435 ADSCrossRefGoogle Scholar
  48. 48.
    G. D’Amico, M. Nardecchia, P. Panci, F. Sannino, A. Strumia, R. Torre et al., Flavour anomalies after the \(R_{K^*}\) measurement. JHEP 09, 010 (2017). arXiv:1704.05438 ADSGoogle Scholar
  49. 49.
    G. Hiller, I. Nisandzic, \(R_K\) and \(R_{K^{\ast }}\) beyond the standard model. Phys. Rev. D 96, 035003 (2017). arXiv:1704.05444 ADSGoogle Scholar
  50. 50.
    L.-S. Geng, B. Grinstein, S. Jäger, J. Martin Camalich, X.-L. Ren, R.-X. Shi, Towards the discovery of new physics with lepton-universality ratios of \(b\rightarrow s\ell \ell \) decays. Phys. Rev. D 96, 093006 (2017). arXiv:1704.05446 ADSGoogle Scholar
  51. 51.
    M. Ciuchini, A.M. Coutinho, M. Fedele, E. Franco, A. Paul, L. Silvestrini et al., On flavourful Easter eggs for New Physics hunger and Lepton Flavour Universality violation. Eur. Phys. J. C 77, 688 (2017). arXiv:1704.05447 CrossRefGoogle Scholar
  52. 52.
    A.K. Alok, B. Bhattacharya, A. Datta, D. Kumar, J. Kumar, D. London, New physics in \(b \rightarrow s \mu ^+ \mu ^-\) after the measurement of \(R_{K^*}\). Phys. Rev. D 96, 095009 (2017). arXiv:1704.07397 Google Scholar
  53. 53.
    T. Hurth, F. Mahmoudi, D. Martinez Santos, S. Neshatpour, Lepton nonuniversality in exclusive \(b{\rightarrow }s{\ell }{\ell }\) decays. Phys. Rev. D 96, 095034 (2017). arXiv:1705.06274 ADSGoogle Scholar
  54. 54.
    C.-W. Chiang, H. Okada, A simple model for explaining muon-related anomalies and dark matter. arXiv:1711.07365
  55. 55.
    B. Barman, D. Borah, L. Mukherjee, S. Nandi, Correlating the anomalous results in \(b \rightarrow s\) decays with inert Higgs doublet dark matter and muon \((g-2)\). arXiv:1808.06639
  56. 56.
    B. Grinstein, S. Pokorski, G.G. Ross, Lepton non-universality in \(B\) decays and fermion mass structure. JHEP 12, 079 (2018). arXiv:1809.01766 ADSGoogle Scholar
  57. 57.
    Planck Collaboration, P.A.R. Ade et al., Planck 2015 results. XIII. Cosmological parameters. Astron. Astrophys. 594, A13 (2016). arXiv:1502.01589
  58. 58.
    S. Chang, R. Edezhath, J. Hutchinson, M. Luty, Leptophilic effective WIMPs. Phys. Rev. D 90, 015011 (2014). arXiv:1402.7358 ADSCrossRefGoogle Scholar
  59. 59.
    A.K. Alok, B. Bhattacharya, D. Kumar, J. Kumar, D. London, S.U. Sankar, New physics in \(b \rightarrow s \mu ^+ \mu ^-\): distinguishing models through CP-violating effects. Phys. Rev. D 96, 015034 (2017). arXiv:1703.09247 ADSGoogle Scholar
  60. 60.
    HFLAV Collaboration, Y. Amhis et al., Averages of \(b\)-hadron, \(c\)-hadron, and \(\tau \)-lepton properties as of summer 2016. Eur. Phys. J. C C77, 895 (2017). arXiv:1612.07233
  61. 61.
    M. Artuso, G. Borissov, A. Lenz, CP violation in the \(B_s^0\) system. Rev. Mod. Phys. 88, 045002 (2016). arXiv:1511.09466 ADSGoogle Scholar
  62. 62.
    S. Aoki et al., Review of lattice results concerning low-energy particle physics. Eur. Phys. J. C 77, 112 (2017). arXiv:1607.00299 ADSCrossRefGoogle Scholar
  63. 63.
    CKMfitter Group Collaboration, J. Charles, A. Hocker, H. Lacker, S. Laplace, F.R. Le Diberder, J. Malcles et al., CP violation and the CKM matrix: assessing the impact of the asymmetric \(B\) factories. Eur. Phys. J. C 41, 1–131 (2005). arXiv:hep-ph/0406184 ADSCrossRefGoogle Scholar
  64. 64.
    UTfit Collaboration, M. Bona, Neutral charm mixing results from the Utfit collaboration. PoS CKM2016, 143 (2017)Google Scholar
  65. 65.
    A. Bazavov et al., Short-distance matrix elements for \(D^0\)-meson mixing for \(N_f=2+1\) lattice QCD. Phys. Rev. D 97, 034513 (2018). arXiv:1706.04622 ADSGoogle Scholar
  66. 66.
    H. An, L.-T. Wang, H. Zhang, Dark matter with \(t\)-channel mediator: a simple step beyond contact interaction. Phys. Rev. D 89, 115014 (2014). arXiv:1308.0592 ADSGoogle Scholar
  67. 67.
    A. Alloul, N.D. Christensen, C. Degrande, C. Duhr, B. Fuks, FeynRules 2.0—a complete toolbox for tree-level phenomenology. Comput. Phys. Commun. 185, 2250–2300 (2014). arXiv:1310.1921 ADSCrossRefGoogle Scholar
  68. 68.
    J. Alwall, R. Frederix, S. Frixione, V. Hirschi, F. Maltoni, O. Mattelaer et al., The automated computation of tree-level and next-to-leading order differential cross sections, and their matching to parton shower simulations. JHEP 07, 079 (2014). arXiv:1405.0301 ADSzbMATHCrossRefGoogle Scholar
  69. 69.
    P. Artoisenet, R. Frederix, O. Mattelaer, R. Rietkerk, Automatic spin-entangled decays of heavy resonances in Monte Carlo simulations. JHEP 03, 015 (2013). arXiv:1212.3460 ADSCrossRefGoogle Scholar
  70. 70.
    T. Sjöstrand, S. Ask, J.R. Christiansen, R. Corke, N. Desai, P. Ilten et al., An Introduction to PYTHIA 8.2. Comput. Phys. Commun. 191, 159–177 (2015). arXiv:1410.3012 ADSzbMATHCrossRefGoogle Scholar
  71. 71.
    D. Dercks, N. Desai, J.S. Kim, K. Rolbiecki, J. Tattersall, T. Weber, CheckMATE 2: from the model to the limit. Comput. Phys. Commun. 221, 383–418 (2017). arXiv:1611.09856 ADSCrossRefGoogle Scholar
  72. 72.
    ATLAS Collaboration, M. Aaboud et al., Search for dark matter produced in association with bottom or top quarks in \(\sqrt{s}=13\) TeV pp collisions with the ATLAS detector. Eur. Phys. J. C 78, 18 (2018). arXiv:1710.11412
  73. 73.
    ATLAS Collaboration, Search for electroweak production of supersymmetric particles in the two and three lepton final state at \(\sqrt{s}=13\,TeV\) with the ATLAS detector, ATLAS-CONF-2017-039 (2017)Google Scholar
  74. 74.
    Prospects for benchmark supersymmetry searches at the high luminosity LHC with the ATLAS Detector, Tech. Rep. ATL-PHYS-PUB-2013-011. CERN, Geneva (2013)Google Scholar
  75. 75.
    Search for supersymmetry at the high luminosity LHC with the ATLAS experiment, Tech. Rep. ATL-PHYS-PUB-2014-010. CERN, Geneva (2014)Google Scholar
  76. 76.
    G.R. Farrar, P. Fayet, Phenomenology of the production, decay, and detection of new hadronic states associated with supersymmetry. Phys. Lett. B 76, 575–579 (1978)ADSCrossRefGoogle Scholar
  77. 77.
    ATLAS Collaboration, G. Aad et al., Search for long-lived stopped R-hadrons decaying out-of-time with pp collisions using the ATLAS detector. Phys. Rev. D 88, 112003 (2013). arXiv:1310.6584
  78. 78.
    CMS Collaboration, Search for stopped long-lived particles produced in pp collisions at \(\sqrt{s}=13~{\rm TeV}\). CMS-PAS-EXO-16-004 (2017)Google Scholar
  79. 79.
    G. Apollinari, O. Bruning, T. Nakamoto, L. Rossi, High luminosity large hadron collider HL-LHC, CERN Yellow Report, 1–19 (2015). arXiv:1705.08830
  80. 80.
    J. Fan, M. Reece, L.-T. Wang, Non-relativistic effective theory of dark matter direct detection. JCAP 1011, 042 (2010). arXiv:1008.1591 ADSCrossRefGoogle Scholar
  81. 81.
    A.L. Fitzpatrick, W. Haxton, E. Katz, N. Lubbers, Y. Xu, The effective field theory of dark matter direct detection. JCAP 1302, 004 (2013). arXiv:1203.3542 ADSCrossRefGoogle Scholar
  82. 82.
    N. Anand, A.L. Fitzpatrick, W.C. Haxton, Weakly interacting massive particle-nucleus elastic scattering response. Phys. Rev. C 89, 065501 (2014). arXiv:1308.6288 ADSCrossRefGoogle Scholar
  83. 83.
    A.K. Drukier, K. Freese, D.N. Spergel, Detecting cold dark matter candidates. Phys. Rev. D 33, 3495–3508 (1986)ADSCrossRefGoogle Scholar
  84. 84.
    A. Ibarra, S. Wild, Dirac dark matter with a charged mediator: a comprehensive one-loop analysis of the direct detection phenomenology. JCAP 1505, 047 (2015). arXiv:1503.03382 ADSCrossRefGoogle Scholar
  85. 85.
    C.M. Ho, R.J. Scherrer, Anapole dark matter. Phys. Lett. B 722, 341–346 (2013). arXiv:1211.0503 ADSMathSciNetCrossRefGoogle Scholar
  86. 86.
    M.I. Gresham, K.M. Zurek, Effect of nuclear response functions in dark matter direct detection. Phys. Rev. D 89, 123521 (2014). arXiv:1401.3739 ADSCrossRefGoogle Scholar
  87. 87.
    E. Del Nobile, Complete Lorentz-to-Galileo dictionary for direct dark matter detection. Phys. Rev. D 98, 123003 (2018). arXiv:1806.01291 ADSCrossRefGoogle Scholar
  88. 88.
    J. Kopp, L. Michaels, J. Smirnov, Loopy constraints on leptophilic dark matter and internal bremsstrahlung. JCAP 1404, 022 (2014). arXiv:1401.6457 ADSCrossRefGoogle Scholar
  89. 89.
    J. Hisano, K. Ishiwata, N. Nagata, Gluon contribution to the dark matter direct detection. Phys. Rev. D 82, 115007 (2010). arXiv:1007.2601 ADSCrossRefGoogle Scholar
  90. 90.
    J. Hisano, R. Nagai, N. Nagata, Effective theories for dark matter nucleon scattering. JHEP 05, 037 (2015). arXiv:1502.02244 ADSMathSciNetzbMATHCrossRefGoogle Scholar
  91. 91.
    T. Jubb, Dark matter : no place for WIMPs. PhD thesis, IPPP, Durham University (2017)Google Scholar
  92. 92.
    XENON Collaboration, E. Aprile et al., Dark matter search results from a one ton-year exposure of XENON1T. Phys. Rev. Lett. 121, 111302 (2018). arXiv:1805.12562
  93. 93.
    B.J. Kavanagh, P. Panci, R. Ziegler, Faint light from dark matter: classifying and constraining dark matter-photon effective operators. arXiv:1810.00033
  94. 94.
    LZ collaboration, D.S. Akerib et al., LUX-ZEPLIN (LZ) Conceptual Design Report. arXiv:1509.02910
  95. 95.
    B.J. Mount et al., LUX-ZEPLIN (LZ) Technical Design Report. arXiv:1703.09144
  96. 96.
    C.E. Aalseth et al., DarkSide-20k: a 20 tonne two-phase LAr TPC for direct dark matter detection at LNGS. Eur. Phys. J. Plus 133, 131 (2018). arXiv:1707.08145 CrossRefGoogle Scholar
  97. 97.
    DarkSide Collaboration, P. Agnes et al., Low-mass dark matter search with the DarkSide-50 Experiment. Phys. Rev. Lett. 121, 081307 (2018). arXiv:1802.06994
  98. 98.
    J. Billard, L. Strigari, E. Figueroa-Feliciano, Implication of neutrino backgrounds on the reach of next generation dark matter direct detection experiments. Phys. Rev. D 89, 023524 (2014). arXiv:1307.5458 ADSCrossRefGoogle Scholar
  99. 99.
    T.K. Gaisser, M. Honda, Flux of atmospheric neutrinos. Annu. Rev. Nucl. Part. Sci. 52, 153–199 (2002). arXiv:hep-ph/0203272 ADSCrossRefGoogle Scholar
  100. 100.
    G. Battistoni, A. Ferrari, T. Montaruli, P.R. Sala, The atmospheric neutrino flux below 100-MeV: the FLUKA results. Astropart. Phys. 23, 526–534 (2005)ADSCrossRefGoogle Scholar
  101. 101.
    S. Horiuchi, J.F. Beacom, E. Dwek, The diffuse supernova neutrino background is detectable in super-kamiokande. Phys. Rev. D 79, 083013 (2009). arXiv:0812.3157 ADSCrossRefGoogle Scholar
  102. 102.
    A.M. Serenelli, W.C. Haxton, C. Pena-Garay, Solar models with accretion. I. Application to the solar abundance problem. Astrophys. J. 743, 24 (2011). arXiv:1104.1639 ADSCrossRefGoogle Scholar
  103. 103.
    Y. Huang, V. Chubakov, F. Mantovani, R.L. Rudnick, W.F. McDonough, A reference Earth model for the heat producing elements and associated geoneutrino flux. arXiv:1301.0365
  104. 104.
    G.B. Gelmini, V. Takhistov, S.J. Witte, Casting a wide signal net with future direct dark matter detection experiments. JCAP 1807, 009 (2018). arXiv:1804.01638 ADSCrossRefGoogle Scholar
  105. 105.
    R.K. Leane, T.R. Slatyer, J.F. Beacom, K.C.Y. Ng, GeV-scale thermal WIMPs: not even slightly ruled out. Phys. Rev. D 98, 023016 (2018). arXiv:1805.10305 ADSCrossRefGoogle Scholar

Copyright information

© The Author(s) 2019

Open AccessThis article is distributed under the terms of the Creative Commons Attribution 4.0 International License (, which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.

Funded by SCOAP3

Authors and Affiliations

  1. 1.Department of Physics, Institute for Particle Physics PhenomenologyDurham UniversityDurhamUK
  2. 2.Instituto de Física Teórica, IFT-UAM/CSICUniversidad Autónoma de MadridMadridSpain

Personalised recommendations