Enlarging Regions of the MSSM Parameter Space for Large $\tan\beta$ via SUSY Decays of the Heavy Higgs Bosons

In the Minimal Supersymmetric Standard Model (MSSM) searches for the heaviest CP-even and CP-odd Higgs $H$, $A$ to tau-lepton pairs severely constrain the parameter region for large values of $\tan\beta$ and light Higgs bosons $H$, $A$. We demonstrate how the experimental constraint can be avoided by new decays to light third-generation sfermions, whose left-right couplings to $H$ can be maximised in regions of large trilinear couplings $A_{b}$, $A_{\tau}$ for sbottoms and staus, or large supersymmetric (SUSY) Higgs mass $\mu$ for stops. Due to the $\tan\beta$-enhancement in the production cross-sections via gluon-fusion and in association with bottom-quark pairs for $H$ and $A$, we find that down-type sfermions, in particular, sbottoms perform a better job in allowing more parameter space than up-type sfermions such as stops, which require much larger values of $\mu$ to compensate for $\tan\beta$. Vacuum stability as well as flavour observables constraints and direct searches for SUSY particles are imposed. We also associate the lightest CP-even Higgs with the observed 125 GeV SM-like Higgs and impose the experimental constraints from the LHC.


Introduction
More than one Higgs doublet is expected in many theories beyond the Standard Model (SM). The most economical and well-studied supersymmetric extension of the SM, the Minimal Supersymmetric Standard Model (MSSM), contains a type-II two Higgs doublet system due to holomorphicity in its electroweak symmetry breaking sector (EWSB). If CP is a good symmetry of the Higgs sector, the scalar Higgs spectrum consists of two CP even Higgs bosons h and H, one CP odd Higgs A and charged Higgs pair H ± ; the lightest CP-even Higgs h is most easily identified with the 125 GeV SM-like Higgs resonance discovered at the LHC. On the other hand, heavier neutral Higgs bosons are being searched for at the LHC via their decay into a pair of tau-leptons and strong constraints are put on the allowed masses as a function of the ratio of the Higgs doublet vacuum expectation values (vev) tan β ≡ H u / H d = v u /v d . In particular, the latest CMS [1] and ATLAS [2] results show that if only decays to SM fermions and gauge bosons are considered, then m H ≈ m A > 500 GeV for tan β 20, ruling out regions of large tan β and moderate m A . These regions however are very appealing since for tan β 1 there is an apparent unification of Yukawa couplings y t ≈ y b ≈ y τ and also a somewhat light Higgs sector has better chances of being probed at the LHC. Furthermore, for tan β 1, the off-diagonal mass mixing between the SM Higgs and the non-standard Higgs 1 is suppressed as sin 2β ∼ 1/ tan β, which is very easy to see in the so-called "Higgs basis" [3]. This conclusion holds even with the inclusion of finite radiative corrections which are important to bring the lighter Higgs mass eigenstate to 125 GeV.
In this work we show that these constrained regions can be consistent with collider searches if there are additional decays for the heavy Higgs bosons which suppress the branching ratios of H and A to tau-leptons, Br(A, H → ττ ). For that purpose we consider the possibility of having additional decays into pairs of sbottoms, stops and staus respectively. This has also been suggested in Ref. [4][5][6] and studied in detail for electroweakinos in Ref. [7,8], where in the latter it was shown that SUSY decays into electroweakinos can be relevant for values of 5 tan β 20. We go beyond these studies by analysing the possible consequences on the destabilisation of the electroweak vacuum and flavour violating contributions, which impose an important constraint on the possible branching ratio to sfermions. We take into account the latest constraints on direct production of these SUSY particles. In particular, we exploit the left-right (LR) coupling of the heavy Higgs bosons to a pair of down-type sfermions which has a term proportional to A f tan β, that allows firstly to overcome the tan β enhancement of the usual dominant bottom-quark contribution to the total decay width and then to even possibly dominate the total decay for a sufficiently large value of the trilinear coupling A f . In the case of stops we find it necessary to consider large values of the Higgs SUSY conserving mass µ in order to overcome the tan β enhancement.
We perform a numerical study and scan the parameter space, calculating the production cross-section for H, A via gluon-fusion and in association with two bottom-quarks with SusHi 1.6.1 [9][10][11][12][13][14][15][16][17][18][19] 2 , and the decays and flavour observables with SARAH 4.11.0 [22][23][24], SPheno 3.3.8 [25,26], and flavio [27]. Finally we study possible stability issues with Vevacious 1.2.02 [28], which tend to constrain the maximum allowed values for A f and µ. We find that indeed it is possible to partially recover some regions of the m A -tan β plane which seem to be disfavoured by current di-tau searches, enlarging the allowed large tan β regions in the MSSM.
The main theoretical considerations are discussed in Sec. 2. Our results for light sbottoms are presented in Sec. 3, for light staus in Sec. 4, and for light stops in Sec. 5. Finally, we conclude in Sec. 6.

Analytical Motivation
We start with the tree-level coupling and decay rate expressions for the heavy Higgs bosons to fermions and sfermions. These expressions are well known and can be found for example in Ref. [29]. We focus on the case of down-type fermions for which the couplings and decay rate take the form, Refs. [20,21] for earlier calculations of QCD corrections to the decays of heavy Higgs bosons to quarks and squarks.
where Φ = H, A, N c is the colour factor, p = 3, 1 for CP-even or odd Higgs bosons, with α the usual Higgs mixing angle that relates the flavour to the mass eigenbasis. In fact, when tan β 1, α → β − π/2 with the lightest Higgs CP-even mass eigenstate SM-like, implying that g Hdd → tan β, so we see that both couplings are enhanced by tan β. We should mention that couplings to up-type quarks on the other hand are suppressed in the same limit by 1/ tan β. From these expressions one can readily calculate Br(H, A → ττ ) when only SM-particle decays are allowed since the total decay width is dominated by decays to bottom-quarks and find that Br(H, A → ττ ) ≈ 0.1, independently of tan β and M Φ . Thus this branching ratio is fixed. The dominant production mechanisms for Φ, as mentioned before, are gluon fusion and production in association with bottom-quarks, with the latter dominating the production for very large values of tan β. Given that g Φdd enters linearly in both production diagrams, we clearly see that there will be a dependence of the form σ H,A × Br(H, A → ττ ) ∝ tan 2 β, where σ H,A represents both production mechanisms, from which we understand how the constraints for large values of tan β come about.
The couplings and decay rates for sfermions take the form, withf i , i = 1, 2 the sfermion mass eigenstates and λf ifj Φ is the well known Kallen lambdafunction which appears in the kinematics of a two-body decay, Notice that contrary to the case of decay to fermions which grows with M Φ , decays to sfermions are suppress by 1/M Φ . The couplings g Φf ifj are combinations of chiral-couplings, The couplings with the same chirality have terms proportional to SM fermions or gauge boson masses and thus are not efficient in enhancing these couplings. Interestingly, the mixed-chirality couplings take the form, which depend on the SUSY breaking trilinear couplings A f and SUSY conserving mass µ. Thus in the large tan β regions we see that there will be terms enhanced by tan β proportional to A d which can be used to increase the couplings to down-type sfermions. In the case of couplings to up-type sfermions, there is only at most a term independent of tan β growing with µ which can be used to increase the coupling 3 . The factor T ijαβ takes into account the chiral mixing in the mass basis and in order to maximise the couplings we should be close to maximal mixing sin θ f ≈ cos θ f ≈ 1/ √ 2, with θ f the mixing angle. We take also into account important loop-level contributions which modify the relation between down-type Yukawas and running masses, where ∆ b is dominated by sbottom-gluino and stop-chargino loop, whereas ∆ τ is dominated by stau-neutralino and sneutrino-chargino loop, and both can be sizeable in the large tan β regime. Given that we want the contribution from the L-R coupling to be maximal in order to enhance the decays into SUSY particles, we must choose the soft breaking masses to be roughly of the same order in particular for the sbottom and stau sectors due to their smaller Yukawa couplings. This implies that we expect mb 2 mb 1 and mτ 2 mτ 1 , which we find in our numerical studies. For stops the story is different given their important loop contribution to the effective Higgs potential which pushes the lightest Higgs mass to 125 GeV. In this case one must choose one of the soft breaking masses (m U 3 or m Q 3 ) to be of the same magnitude as A t 2 TeV, pushing the heavier stop in the few TeV region. However, since we want to have the heavy Higgs bosons decay to stops in the first place, we need the lighter stop to remain light enough to kinematically allow for such decays. Thus in this case the spectrum is more split (mt 1 mt 2 and mt 1 m Φ /2) than for sbottoms and staus and though the mixing is not maximal we can still have stops contributing to the total decay width enough to suppress Br(Φ → ττ ).
Large values of A b , A τ and µ are constrained by colour and electromagnetic charge breaking since they provide cubic terms in the scalar potential that tend to destabilise the neutral electroweak symmetry breaking vacuum [30]. We will see in the next section that this puts strong constraints on the allowed values for A b , A τ and µ. There are flavour violating processes which are enhanced at large tan β, in particular B-meson decays (See e.g. [31]). We will also comment on this in the next sections. We perform a numerical scan for each of the three discussed possibilities.

Light Sbottoms
We describe the parameter space and the codes used in the numerical scan for light sbottom quarks in the next section, before discussing our results in Sec. 3.2.

Numerical Scan
In order to study the feasibility to enlarge regions of large values of tan β currently constrained by H, A → ττ searches, we do a numerical simulation of the productions of H and A via gluon fusion and in association with bottom-quark pairs using SusHi 1.6.1 [9][10][11][12][13][14][15][16][17][18][19], a Fortran code which can calculate these production cross sections in the MSSM. In the case of gluon fusion, it takes into account N LO QCD contributions from the third family of quarks and squarks, N 3 LO corrections due to top-quarks, approximate N N LO corrections due to top squarks and electroweak effects. Very much relevant for large values of tan β for the downtype sector and it particular for the third family Yukawa couplings, it resums higher order tan β-enhanced sbottom contributions. The supersymmetric particle spectrum, as well as cross-sections and decays for SUSY particles, are calculated using SARAH 4.11.0 [22][23][24] and SPheno 3.3.8 [25,26], in particular the SPheno version generated from the MSSM model file in SARAH. We subsequently calculate flavour observables with flavio [27], which takes the Wilson coefficients calculated by FlavorKit [24] as input, and the Higgs production cross sections at the LHC with SusHi 1.6.1 [9][10][11][12][13][14][15][16][17][18][19] for both CP even Higgs bosons using the MMHT 2014 [32] parton distribution functions set via LHAPDF 6.1.6 [33]. Stability of the electroweak vacuum and possible charge/colour breaking minima are investigated using Vevacious 1.2.02 [28], which relies on CosmoTransitions [34] and HOM4PS2 [35]. Due to the lack of SUSY signals so far at the LHC, we decide to consider a natural spectrum, pushing 1 st and 2 ndgeneration sparticles, as well as gluinos and Winos in the multi-TeV range: with vanishing A-terms. For 3 rd -generation sparticles, depending on how we want to suppress the branching ratio Br(H, A → ττ ), we keep either sbottoms, staus or stops light 4 to allow for heavy Higgs SUSY decays to be kinematically accessible. Since |µ|, M 1 M 2 , M 3 , mf 1,2 , the other possible light sparticles in the spectrum are the first three lighter neutralinosχ 0 1 , χ 0 2 ,χ 0 3 and the light charginoχ ± 1 . In the scan with light sbottoms, we fixed and varied the remaining parameters, tan β, µ, B µ , mQ For all points with mb 1 ≥ 300 GeV, which are close to the experimental exclusion limit of the H → ττ searches and for which the decay H →bb * is kinematically accessible, we increased |A b |, both for positive and negative A b , and used a fixed-point iteration to determine the largest possible value, for which the electroweak vacuum is either stable or sufficiently longlived on cosmological scales. Finally, we increased M 1 to enlarge the parameter space by further suppressing the limits from the direct sbottom pair production searches.
We impose that the lightest Higgs particle in the spectrum, which is associated with the scalar resonance discovered at the LHC, satisfies the measurement of the Higgs mass 125 ± 3 GeV taking the theory error into account and the latest signal strengths measurements by ATLAS and CMS at the 2σ level (Tab. 16 in Ref. [36]), in the different relevant channels: bb, W W * , ZZ * , ττ and γγ. We discarded all data points, which have a sbottom quark mass below 300 GeV to satisfy mono-jet searches at 3.2 fb −1 [37] and directly use the latest 13 TeV CMS direct sbottom [38] and stop [39] pair production searches with a luminosity L = 36.1fb −1 by imposing the limit extracted from the provided root files, where we use the QCD squark pair production cross section reported in Ref. [40].
For the main object of our study, the heavy Higgs bosons H, A, we require that both the productions in association with bottom-quarks and via gluon fusion, with subsequent decay into tau pairs, σ bbH × Br(H → ττ ) and σ ggH × Br(H → ττ ), satisfy the bounds from both ATLAS [2] and CMS [1] studies at 13 TeV and 13.3 fb −1 and 12.9 fb −1 , respectively, though due to the large values of tan β we are interested in, the production in association with bottom-quark pairs places stronger constraints.
We make a few comments with respect to flavour observables and constraints. We are able to satisfy all flavour observable constraints (B s → µ + µ − [41], B → τ ν [42], etc) at the 2σ level, except for B → X s γ [42], for which the stop-chargino loop contribution can be significant, whereas the charged Higgs contributions seems to be subdominant. Within the Minimal Flavour violation (MFV) paradigm, a study done in Ref. [31] shows that for A t > 0, µ 800 GeV or M Q 3 1.3 TeV are necessary to satisfy the latest measurements. For A t < 0, constraints are much stronger and always require M Q 3 1.5 TeV. Since we want to have a light enough sbottom for the heavy Higgs bosons to decay, this implies that the only possibility would be to have A t > 0 and µ 800 GeV, which would not affect the main conclusions of this work. However, recall that this is all within the MFV paradigm. Beyond the MFV paradigm, there are new ways to suppress the contribution of the stop-chargino loop, in particular possible additional diagrams involving gluinos and sbottom-strange mixing, which may be able to cancel the chargino-stop contributions [43,44]. Thus we do not impose in our results the constraint from B → X s γ due to the caveats just discussed.

Results
Having taken in consideration all these constraints, we show our results in Figs. 1, 2 and 3. keeping all other parameters fixed, in order to show how we move in the particular planes shown. The big black dots represent the points with A b = 0 and the purple arrow points in the direction of increasing A b . In Fig. 1 on the left, we plot Br(H → ττ ) vs A b . We immediately see from the red and orange points that as A b grows in magnitude, we are able to suppress the Br(H → ττ ) via the additional sbottom decays by factors of order a half or slightly smaller. There are however points which have a large A b but nonetheless a large Br(H → ττ ), which implies that these points do not correspond to maximal mixing between the left and right handed sbottoms. Note as well that we find both metastable and fully stable vacua for |A b | 2 TeV. In the two examples shown in this figure we leave everything fixed except A b and one can see that as A b increases in magnitude one is able to suppress via decays into sbottoms the Br(H → ττ ). However, for the two examples the suppression is not sufficient enough to avoid the LHC constraints from H, A → ττ for one the branches (A b < 0). Comparing the location of most of the red and orange points against the grey points, it is clear that a suppression in Br(H → ττ ) is what allows them to evade the di-tau constraints. There are, however, some stragglers for which Br(H → ττ ) 0.1 and are able however to evade the constraints. These points correspond to large m H such that the constraints from di-taus ameliorate. In Fig. 1 on the right on the other hand, we show the influence of A b on m H . This is clearly seen in the two example black dashed/dotted lines in this figure, where as we move A b keeping all other parameters fixed, we see that m H can either decrease or increase by several GeV's, even ∆m H ∼ 100 GeV. This is coming from the radiative sbottom corrections to the effective Higgs potential, that as we see for large values of tan β can be quite relevant [45]. In the two examples m H increases with increasing A b , but the opposite behaviour, where m H decreases with increasing A b , also occurs for some points in the numerical scan. This last analysis helps us to partially understand Fig. 2. In the figure on the right, we show the main constraining production cross section σ bbH as a function of m H . We see that as m H increases there is a clear reduction in the cross section as expected. Furthermore, we see this explicitly in the two examples represented once again by the dashed black lines.
Here we see the effect of A b shifting m H and reducing or increasing the cross section. On the other hand, on the left of Fig. 2, we show σ bbH × Br(H → ττ ) vs m H . We also display the constraints from the latest ATLAS [2] and CMS [1] A, H → ττ searches at 13 TeV, respectively, represented by the solid and dashed nearly horizontal lines in the figure, showing clearly that the grey points are excluded by these searches. Now we see in the two examples that we have chosen, that the initial points with A b = 0 are right at the border of exclusion and as we vary A b , we either move into the non-excluded area by two effects: a decrease in the production cross section due to a larger m H and a decrease in the Br(H → ττ ) due to di-sbottom decays. Indeed, we see that the line of the two example becomes steeper as we move in the non-excluded area. We can however, also move deeper into the excluded area as depicted by the two examples, by a decrease in m H (which leads to an increase in the production cross section) and an insufficient suppression of the branching ratio Br(H → ττ ).
Finally in Fig. 3, we show tan β vs m H . The grey envelope area of the excluded points indicates the excluded region. We see something very interesting happening. Most of the orange points lie within the grey envelope, implying that without the additional suppression due to the decays into sbottom pairs from the heavy Higgs, they would have been ruled out by the current H, A → ττ searches. The blue points that lie also within the grey envelope have a maximal Br(H → ττ ) ∼ 0.1 as shown in Fig. 1 on the left, but as seen from Fig. 2 on the right, they have a somewhat suppressed production cross section with respect to the grey points. This is most likely due to a suppressed coupling from radiative corrections for these points as shown in Eq. (2.7). This effect has been discussed for decays to stau pairs in Ref. [5]. Focusing on the two example lines, we see that as we change A b , we move horizontally in the plane m H − tan β due to the change in m H as A b varies. In both examples we see that starting from the points with A b = 0 which are represented by the slightly larger black dots, as m H becomes larger we are able to obtain viable points (red points) which are within the grey envelope. On the other hand, to the other side of the big black dot, we move to smaller m H but are further excluded. These two behaviours can be understood by looking how in the two examples m H and Br(H → ττ ) depend on A b as shown in Fig. 1. Although Br(H → ττ ) diminishes for increasing |A b | in both examples, the decrease in Br(H → ττ ) for negative A b is compensated by the increased production cross section for a lighter H. For positive A b , m H increases with increasing A b and thus the production cross section is reduced in addition to the suppression of the branching ratio Br(H → ττ ).

Light Staus
The numerical scan for light staus is very similar to the one for light sbottoms. We discuss any differences to the scan for sbottoms in the next subsection and our results in Sec. 4.2.

Numerical Scan
We decouple winos, squarks, and the first two generations of sleptons and similarly fix the bino mass and the right-handed stop mass to a large enough loop correction to the Higgs mass Initially we keep A τ = 0 fixed and in a second step, we increase |A τ |, and use a fixedpoint iteration to determine the largest possible value with a stable or long-lived electroweak vacuum. Direct stop and sbottom pair production searches are automatically satisfied and we conservatively require mτ ≥ 100 GeV to satisfy the current limits on theτ mass [42] and that the lightest supersymmetric particle is a neutralino. All flavour constraints, and in particular, [42], B → X s γ [42], are satisfied at the 2σ level. Similarly to the scan with light sbottoms, we impose the Higgs signal strength measurements at 2σ as well as the Higgs mass measurement.

Results
The colour coding in Figs. 4 to 6 is the same as for the sbottom case, with the obvious replacements. In Fig. 4 on the left, we see that we can still suppress the Br(H → ττ ) via decays into stau pairs. However, in comparison with the decays into sbottoms, the suppression is less effective which may be related to the number of colour that enters in the sbottom decay case, as well as the larger Yukawa coupling of the bottom-quark with respect to the tau-quark, see Eq. (2.3). Furthermore, the smallest values of Br(H → ττ ) which are stable occur for somewhat small values of A τ , |A τ | ∼ 600 GeV. We have checked that larger values of A τ would lead to stronger suppressions of Br(H → ττ ), however they are excluded by vacuum stability constraints.
In Fig. 4 on the right, contrary to the sbottom case, the dependence of m H on A τ is much milder once again due to the smaller Yukawa and the lack of colour for the stau case. Note that the orange points for which A τ = 0 and which are stable, start at m H 800 GeV. This can be understood by looking at Fig. 5 on the left, where due to our scanning procedure which starts with points that are barely ruled out by the H → ττ searches and considers tan β > 25, the lightest mass m H we can obtain which is barely ruled out is m H ≈ 800 GeV. If we had chosen a lower value of tan β, we could have observed the stau effect for smaller values of m H . Nonetheless, by looking at the two example points and also at the "width" of the orange region, we conclude that the effect of staus is much less significant in allowing a larger parameter region than that of sbottoms. This can also be seen in Fig. 5 on the right.
Finally in Fig. 6, we translate the results to the m H − tan β plane. We see that indeed one can get most of the orange points in the would-be excluded region, delimited by the grey envelope. Again we see that the depth of the orange points in the grey envelope is much thinner compared to the sbottom case of Fig. 3.
There has been an analytical study of the stau case in Ref. [5]. It showed that, at the time, a suppression of up to 20 % of σ bbH × Br(H → ττ ) with respect to the case without SUSY decays was achievable for values of A τ ∼ 1.3 TeV. We find slightly better results in our numerical study, as can been seen in Fig. 5 on the left, where we estimate up to 50 % suppression for σ bbH × Br(H → ττ ) with respect to the case with no SUSY decays. Notice also that values of A τ ∼ 1.3 TeV are on the borderline of metastability, as shown in Fig. 4 on the left and that though an analytical study for the stau case is consistent, a similar one for the sbottom case is not straightforward due to the large dependence of m H on A b .

Light Stops
In the case of stops, given that we want only stops and not sbottoms to be light and that to obtain a mass for the lightest Higgs h of m h ≈ 125 GeV, which implies A t ∼ m Q 3 ∼ 2 TeV, we have in the end that one stop is light (mostly right-handed) while the other stop is much heavier (mostly left-handed). We also consider values of tan β ∈ [25,60]. As mentioned in section 2, the way to increase the branching ratio of H into stops is by increasing the value of µ. However, there are large radiative corrections to the heavy Higgs mass m H which are much stronger than in the case of A b or A τ for the sbottom and stau cases. Thus the scanning procedure of leaving everything fixed except µ is much less efficient and we are only able to retrieve stable points for m H > 2.6 TeV and µ > 2.4 TeV, with very small branching ratio into stops. Vacuum stability is only an issue for the very largest values of µ 4.5 TeV. Performing a random scan we were able to see the effect of stops reducing the Br(H → ττ ) via a Br(H →t 1t * 1 ) 0.4. Their effect seems to start at m H 1 TeV and extend up to m H ≈ 2.2 TeV for values of µ ∈ [1.2, 3.5] TeV. The problem however in this case by performing a random scan is that we loose the guide from the two sets of example points which we showed for the sbottom and stau cases, respectively. Thus we decided to only comment briefly on this possibility in reducing Br(H → ττ ).

Conclusion
Searches for heavy Higgs bosons decaying to a pair of τ leptons severely constrain the parameter space of the MSSM for large tan β. We demonstrate three possible ways how to alleviate the constraints by new decay channels into third-generation sfermion pairs. For large tan β, the coupling of the heavy Higgs to the sbottoms and staus proportional to tan β can be further enhanced by a large value of the trilinear couplings A b and A τ , respectively, while the coupling to stops has a tan β independent part which can be enhanced by the SUSY conserving Higgs mass µ. The maximum size of the trilinear couplings A f and µ, however, is constrained by the stability of the electroweak vacuum.
Our numerical scan shows that light sbottoms have the greatest potential to alleviate the constraints from heavy Higgs searches. After imposing vacuum stability, |A b | can take values up to 2 TeV and leads to a reduction of the branching ratio Br(H → ττ ) by more than a factor two down to Br(H → ττ ) 0.05, which enlarges the available parameter space. Similarly, for light staus we find values of |A τ | ∼ 1.3 TeV with a reduced branching ratio Br(H → ττ ) ∼ 0.07, which allows to slightly enlarge the allowed region of parameter space. Finally, light stops allow very large values of |µ| close to 5 TeV. However, radiative corrections to the heavy Higgs mass m H are large and substantially increase it. It is still possible to observe the effect of a reduced branching ratio Br(H → ττ ) via an increased branching ratio for the decay into light stops Br(H →t 1t * 1 ) 0.4, but a detailed discussion would require to fix the heavy Higgs mass m H as much as possible when increasing |µ|.
Although future searches for heavy Higgs bosons decaying to τ -pairs may tighten the constraints on the MSSM parameter space and eventually exclude the orange points in the figures, our main conclusion, that new decays to light third-generation fermions will alleviate the constraints from heavy Higgs search, holds irrespectively. This scenario can be tested by improving the reach of the searches for light third generation sfermions.