News
The pMSSM10 prior to LHC RUN II [Apr 13, 2015]
We present a frequentist analysis of the parameter space of the pMSSM10, in which the following 10 soft SUSYbreaking parameters are specified independently at the mean scalar top mass scale Msusy = Sqrt[M_stop1 M_stop2]: the gaugino masses M_{1,2,3}, the 1stand 2ndgeneration squark masses M_squ1 = M_squ2, the thirdgeneration squark mass M_squ3, a common slepton mass M_slep and a common trilinear mixing parameter A, the Higgs mixing parameter mu, the pseudoscalar Higgs mass M_A and tan beta. We use the MultiNest sampling algorithm with 1.2 x 10^9 points to sample the pMSSM10 parameter space. A dedicated study shows that the sensitivities to stronglyinteracting SUSY masses of ATLAS and CMS searches for jets, leptons + MET signals depend only weakly on many of the other pMSSM10 parameters. With the aid of the Atom and Scorpion codes, we also implement the LHC searches for EWinteracting sparticles and light stops, so as to confront the pMSSM10 parameter space with all relevant SUSY searches. In addition, our analysis includes Higgs mass and rate measurements using the HiggsSignals code, SUSY Higgs exclusion bounds, the measurements Bphysics observables, EW precision observables, the CDM density and searches for spinindependent DM scattering. We show that the pMSSM10 is able to provide a SUSY interpretation of (g2)_mu, unlike the CMSSM, NUHM1 and NUHM2. As a result, we find (omitting Higgs rates) that the minimum chi^2/dof = 20.5/18 in the pMSSM10, corresponding to a chi^2 probability of 30.8 %, to be compared with chi^2/dof = 32.8/24 (31.1/23) (30.3/22) in the CMSSM (NUHM1) (NUHM2). We display 1dimensional likelihood functions for SUSY masses, and show that they may be significantly lighter in the pMSSM10 than in the CMSSM, NUHM1 and NUHM2. We discuss the discovery potential of future LHC runs, e+e colliders and direct detection experiments.
The SLHA files of our benchmark points can be obtained from here:
Full text at
arXiv:1504.03260 [hepph].
The CMSSM and NUHM1 after LHC Run 1 [Dec 18, 2013]
We analyze the impact of data from the full Run 1 of the LHC at 7 and 8 TeV on the CMSSM with μ>0 and μ<0 and the NUHM1 with μ>0,
incorporating the constraints imposed by other experiments such as precision electroweak measurements, flavour measurements,
the cosmological density of cold dark matter and the direct search for the scattering of dark matter particles in the LUX experiment.
We use the following results from the LHC experiments: ATLAS searches for events with MET accompanied by jets with the full 7 and 8 TeV data,
the ATLAS and CMS measurements of the mass of the Higgs boson, the CMS searches for heavy neutral Higgs bosons and a combination of the LHCb
and CMS measurements of B
_{s}→μμ and B
_{d}→μμ.
Full text at
arXiv:1312.5250 [hepph].
Supersymmetry in light of LUX [October 31st, 2013]
On October 30th the LUX Collaboration announced the first results of its direct search for spinindependent WIMP dark matter scattering on Xenon,
which are significantly more sensitive than previous such experiments, particularly in the region of low WIMP masses.
We present here some preliminary results from a global analysis of the parameter spaces of simple supersymmetric models in light of LUX.
These results also incorporate the (negative) results of ATLAS searches for events with jets and missing transverse energy at the LHC
with ∼20/fb of luminosity at 8 TeV, as well as the CMS and LHCb measurements of B
_{s}→μμ decay.
We also include the implications for supersymmetric models of the measurements by the ATLAS and CMS Collaborations of the mass of the Higgs boson,
as interpreted using the latest version of the
FeynHiggs code,
which yields an improved calculation leading to somewhat larger light Higg boson masses than previous versions
for the same values of the supersymmetric model input parameters.


The (m_{χ},σ_{p}^{SI}) planes in the CMSSM (left panel) and the NUHM1 (right panel).
The Δχ^{2} = 2.30(5.99) contours, corresponding to the 68(95)% CL are coloured red (blue).
The solid (dashed) lines are for global fits including (excluding) the new LUX results. The new bestfit points are indicated by a solid green star.
The 90% CL exclusion lines of LUX and XENON100 are also shown. Note that the global fit contours include an additional systematic uncertainty on
σ_{p}^{SI}. 
Implications of the first evidence of the B_{s}→μμ decay! [November 12, 2012]
After the
publication of the first measurement of the B
_{s}→μμ branching fraction
by the
LHCb experiment,
we update our frequentist analysis of the parameter space of the CMSSM and NUHM1 models. The following results
are based on a (nonofficial)
combination of the ATLAS, CDF, CMS, and LHCb results yielding:
BR(B
_{s}→μμ) ≈ 3.0
_{1.1}^{+1.2} x 10
^{9}.
The new measurement provides a valuable new constraint on the supersymmetric parameter space, but
the observation of a Standard Modellike branching fraction for the B_{s}→μμ decay is quite consistent with supersymmetry.
In fact, a Standard Modellike branching fraction of this decay was expected in constrained supersymmetric models like
the CMSSM or NUHM1 (see, e.g., the
recent MasterCode results for further details).
As a result, the favoured regions in the parameter space of these models do not change significantly after the inclusion of the new constraint.

Combination of BR(B_{s}→μμ) measurements: ATLAS (cyan, Winter 2012), CDF (dark blue, ASPEN 2012),
CMS (red, Winter 2012), LHCb (blue, HCP 2012). The combined likelihood is shown in green. 


Prediction for BR(B_{s}→μμ) in the (m_{0},m_{1/2}) plane, in the (left) CMSSM and (right) NUHM1 models.
The red (blue) contour shows the 68% (95%) C.L. exclusion, after including the already published
constraints from the LHC and XENON100, as well as the new LHCb result. 


68% and 95% C.L. contours in the (m_{0},m_{1/2}) plane, in the (left) CMSSM and (right) NUHM1 models.
The dashed lines include the already published constraints from the LHC and XENON100,
the solid lines include the new LHCb result in addition. 


Prediction for BR(B_{s}→μμ) in the (M_{A},tanβ) plane, in the (left) CMSSM and (right) NUHM1 models.



68% and 95% C.L. contours in the (M_{A},tanβ) plane, in the (left) CMSSM and (right) NUHM1 models.



Δχ^{2} distributions for BR(B_{s}→μμ) normalized to SM expectation in the (left) CMSSM and (right) NUHM1 models,
after (solid line) and before (dashed line) the new LHCb result.



Δχ^{2} distributions for the gluino mass in the (left) CMSSM and (right) NUHM1 models,
after (solid line) and before (dashed line) the new LHCb result.

Grand summary of 2011 searches [Summer 2012]
We make a frequentist analysis of the parameter space of the CMSSM and NUHM1, using a Markov Chain Monte Carlo (MCMC)
with 95 (221) million points to sample the CMSSM (NUHM1) parameter spaces.
Our analysis includes the ATLAS search for supersymmetric jets + MET signals using ∼5/fb of LHC data at 7 TeV,
which we apply using PYTHIA and a Delphes implementation that we validate in the relevant parameter regions of the CMSSM and NUHM1.
Our analysis also includes the constraint imposed by searches for B
_{s}→μμ by LHCb, CMS, ATLAS and CDF,
and the limit on spinindependent dark matter scattering from 225 live days of XENON100 data.
We assume M_h ∼ 125 GeV, and use a full set of electroweak precision and other flavourphysics observables,
as well as the cold dark matter density constraint.
The ATLAS 5/fb constraint has relatively limited effects on the 68 and 95% CL regions in the (m_0, m_1/2) planes of
the CMSSM and NUHM1. The new B
_{s}→μμ constraint has greater impacts on these CL regions, and also impacts significantly
the 68 and 95% CL regions in the (M_A, tanβ) planes of both models, reducing the bestfit values of tanβ.
The recent XENON100 data eliminate the focuspoint region in the CMSSM and affect the 68 and 95% CL regions in the NUHM1.
In combination, these new constraints reduce the bestfit values of m_0, m_1/2 in the CMSSM, and increase the global
χ
^{2} from 31.0 to 32.8, reducing the pvalue from 12% to 8.5%.
In the case of the NUHM1, they have little effect on the bestfit values of m_0, m_1/2,
but increase the global χ
^{2} from 28.9 to 31.3, thereby reducing the pvalue from 15% to 9.1%.
More information:
→ The CMSSM and NUHM1 in Light of 7 TeV LHC, B_{s}→μ^{+}μ^{} and XENON100 Data
New results including 1/fb of LHC data [October 11, 2011]
We update previous frequentist analyses of the CMSSM and NUHM1 parameter spaces to include the public results of searches for supersymmetric signals using
~1/fb of LHC data recorded by ATLAS and CMS and ~0.3/fb of data recorded by LHCb in addition to electroweak precision and Bphysics observables.
We also include the constraints imposed by the cosmological dark matter density and the XENON100 search for spinindependent dark matter scattering.
The LHC data set includes ATLAS and CMS searches for jets + missing ET events and for the heavier MSSM Higgs bosons, and the upper limits on
B
_{s}→μμ from LHCb and CMS. The absences of jets + missing ET signals in the LHC data favour heavier mass spectra than in our previous analyses
of the CMSSM and NUHM1, which may be reconciled with (g2)
_{μ} if tanβ ~40, a possibility that is however under pressure from heavy Higgs searches and
the upper limits on B
_{s}→μμ. As a result, the
pvalue for the CMSSM fit is reduced to ~15 (38)%, and that for the NUHM1 to ~16 (38)%, to be compared
with ~9 (49)% for the Standard Model limit of the CMSSM for the same set of observables (dropping (g2)
_{μ}), ignoring the dark matter relic density in both cases.
We discuss the sensitivities of the fits to the (g2)
_{μ} and b→sγ constraints, contrasting fits with and without the (g2)
_{μ} constraint,
and combining
the theoretical and experimental errors for b→sγ linearly or in quadrature. We present predictions for m
_{gluino}, B
_{s}→μμ,
M
_{h} and M
_{A},
and update predictions for spinindependent dark matter scattering, stressing again the importance of taking into account the uncertainty in the pinucleon
sigma term, Σ
_{πN}.
Finally, we present predictions based on our fits for the likely thresholds for sparticle pair production in ee collisions in the CMSSM and NUHM1.
More information:
→ Supersymmetry in Light of 1/fb of LHC Data
→ A selection of results
MasterCode's "red band plots" on the front page of EPJC! [September 6, 2011]
A figure of our
most recent paper, displaying the prediction for the lightest Higgs mass
in various constrained versions of the MSSM, was selected as a cover picture for
EPJC vol. 71, no. 8.
EPS 2011 update
The ATLAS and CMS Collaborations have recently presented at the EPS conference in Grenoble
(
http://epshep2011.eu/)
new results from more powerful allhadronic SUSY searches, using about 1/fb of 2011 LHC data.
(
http://epshep2011.eu/) new results of their powerful
allhadronic SUSY searches:
In addition, the CMS, LHCb, and CDF Collaborations have also presented stringent new limits
on the branching fraction for the B
_{s}→μμ decay:
Here we incorporate this new information in an update of our recent frequentist global analysis
of the parameter spaces of the CMSSM and NUHM1:
arXiv:1106.2529 [hepph].
In that reference we incorporated a combination of the B
_{s}→μμ constraints from LHCb and D0,
and also the previous CDF constraint, as well as the available LHC 2010 and XENON100 constraints,
as well as other observables including the LEP Higgs limit, b→sγ decay, g
_{μ}2,
the relic cold dark matter density, precision electroweak observables. Details of our analysis can be found there.
In the absences of official combinations of the new limits, we use in each case the single most constraining limit.
For the allhadronic searches we use the CMS result up to m
_{0} = 1 TeV and the ATLAS limit
for m
_{0} > 1 TeV. In case of BR(B
_{s}→μμ) we use the limit from LHCb.
We display first the (m
_{0}, m
_{1/2}) planes of the CMSSM (
Figure 1)
and NUHM1 (
Figure 2), showing bestfit points (green stars), 68% CL boundaries (red lines)
and 95% CL boundaries (blue lines). The dotted (solid) lines are before (after) including the new constraints
presented at EPS. To further illustrate the impact of the new limits on the allowed parameter space, we also
show in the same plotting format the correlation of the spinindependent dark matter scattering cross section with
the mass of the lightest supersymmetric particle (neutralino) in these models (
Figure 3 CMSSM
and
Figure 4 NUHM1).
In both models, the bestfit point changes significantly due to the tight constraints from the new direct
allhadronic SUSY searches. The overall χ
^{2} increases from 26.2 to 30.2 in the CMSSM
and from 24.2 to 27.0 in the NUHM1, yielding a χ
^{2}probability of about
11% for the CMSSM and 17% for NUHM1.
The tension on the parameter space of these constrained SUSY models is more visible when
displaying the χ
^{2}probability in (m
_{0},m
_{1/2}) planes. As can be
seen in
Figure 5, the CMSSM still exhibits a rather large region in the parameter
space with a goodness of fit probability of better then 5% (green region) but since the best fit
probability is only 11%, overall the portion of parameter space of this model still allowed possesses
only rather a low chi2 probability, as given above.
The situation is slightly better in the case of the less constrained NUHM1 (
Figure 6),
but also here the overall probability of 17% is also significantly lower than before the EPS conference.
Finally, we display the 1dimensional χ
^{2} functions for B
_{s}→μμ
in the CMSSM (in green,
Figure 7)
and NUHM1 (in purple,
Figure 8), showing the pre (post)EPS predictions as dotted (solid) lines.
We await with interest the results on the combination of B
_{s}→μμ results and will update
arXiv:1106.2529 [hepph] more fully at that time.
The update will also discuss the impacts of different treatments of the g
_{μ}2 and b→sγ
constraints on global fits.
Today:  
Yesterday:  
Last week:  
Last month:  
Total:  