CERN-PH-TH/2012-307Implications of LHC Higgs and SUSY searchesfor MSSM

                                                                                                                            Cern-Ph-Th/2012-307
Implications of LHC Higgs and SUSY searches for MSSM

Abstract

The implications of the LHC SUSY searches as well as the discovery of a new bosonic state compatible with the lightest Higgs boson will be discussed in the context of constrained and general MSSM scenarios. Exploring the MSSM through the Higgs sector is an alternative and complementary path to direct searches, and tight constraints on the MSSM parameter space can be obtained.

\ShortTitle

Implications of LHC Higgs and SUSY searches for MSSM \FullConference36th International Conference on High Energy Physics
4-11 July 2012
Melbourne, Australia

1 Introduction

The search for Higgs and supersymmetry (SUSY) are the main focus of ATLAS and CMS experiments. Although before the start of the LHC the expectation for an early discovery of supersymmetric partners of the Standard Model (SM) particles was very high (mainly driven by the studies in the constrained SUSY scenarios), no SUSY particle has been observed yet. On the other hand, ATLAS and CMS collaborations have reported the discovery of a new bosonic state with a mass of around 126 GeV, compatible with the SM-Higgs [1, 2]. These results have significant implications for the Minimal Supersymmetric Standard Model (MSSM). In the following, we discuss the consequences of the latest SUSY and Higgs search results in the context of the MSSM.

2 Implication of SUSY searches

To study the implication of the LHC SUSY searches we consider the unconstrained phenomenological MSSM (pMSSM) with 19 parameters [3]. Most of the previous studies considered the highly constrained models with a small number of free parameters. However, these models are not representative of a generic MSSM scenario where the particle mass parameters are independent. As we will see below, the results can be very different in such generic scenarios.

To explore the pMSSM, we perform a flat scan over the parameters in the ranges given in Table 1. The particle spectra are generated for more than 100M points using SOFTSUSY [4] and SUSPECT [5]. We impose the SUSY and Higgs mass limits from LEP and Tevatron as described in [6]. The flavour observables, muon anomalous magnetic moment and relic density are computed with SuperIso Relic [7], and we apply the constraints given in Table 2. We do not discuss here the consequences of the dark matter direct detection results which are discussed thoroughly in [8].

    Parameter           Range     Parameter           Range
[1, 60] [50, 2500]
[50, 2000] [50, 2500]
[-2500, 2500] [50, 2500]
[-2500, 2500] [50, 2500]
[50, 2500] [50, 2500]
[-10000, 10000] [50, 2500]
[-10000, 10000] [50, 2500]
[-10000, 10000] [50, 2500]
[-1000, 2000] [50, 2500]
[50, 2500]
Table 1: SUSY parameter ranges (in GeV when applicable).

To evaluate the consequences of the SUSY searches, we compute the supersymmetric particle decay rates with SDECAY [9] and we use PYTHIA 6 [10] for event generation of inclusive SUSY production in interactions. The generated events are then passed through fast detector simulation using Delphes [11]. The Higgs decay rates are computed with HDECAY [13] and the gluon fusion and VBF cross sections of the lightest CP-even Higgs with HIGLU [14] and FeynHiggs [15]. More details can be found in [6, 12].

Table 2: Constraints applied in our pMSSM analysis. The points passing all the constrained are called “accepted points”.

We consider the consequences of the SUSY searches in all hadronic events with [16], in same-sign isolated dilepton events with jets [17] and missing energy and in opposite-sign dilepton events with missing transverse energy [18] in the CMS detector at 7 TeV with 1 fb of data, and extrapolate to the 8 TeV run with 15 fb of data. In Fig. 1 we show the consequences on the masses of the lightest squark of the first two generations, the lightest neutralino and , where the distribution of the points compatible with SUSY searches with 1 fb at 7 TeV and the projections for 15 fb at 7 and 8 TeV data are displayed.

Figure 1: Fraction of accepted pMSSM points with 111 GeV, not excluded by the SUSY searches with 1 fb of 7 TeV data (red), and by a projection of 15 fb at 7 TeV (blue) and 15 fb at 8 TeV (green), as functions of the masses of the lightest squark of the first two generations (left panel), the lightest neutralino (central panel) and (right panel).

We notice that with 15 fb of data at 8 TeV, more than 30% of the points with squark masses below 1 TeV will still be allowed. The spectrum of the weakly interacting particles will be even less affected as there is basically no sensitivity for neutralino masses above 700 GeV. The spectrum of is also rather flat. The full set of the results can be found in [12]. These results in the unconstrained pMSSM are very different from those obtained in highly constrained scenarios such as mSUGRA.

3 Implication of Higgs searches

An alternative way to efficiently constrain SUSY is using the information from the Higgs sector. In the following, we consider that the new boson discovered at the LHC corresponds to the lightest CP-even Higgs boson. The combination of the Higgs search results presented by ATLAS and CMS are given in Table 3.

Parameter Value Experiment
125.92.1 GeV ATLAS [1] + CMS [2]
1.710.33 ATLAS [19] + CMS [20]
0.950.40 ATLAS [21] + CMS [22]
1.64 (95% C.L.) CMS [23]
1.06 (95% C.L.) CMS [24]
Table 3: Input parameters used for the pMSSM study.

In [25, 26], we have shown that the Higgs mass measurement has strong implications on the constrained MSSM scenarios. This is demonstrated in Fig. 2, where the maximal value of the light Higgs mass is given in mAMSB, mGMSB, mSUGRA and some of its variants, as a function of and the SUSY scale .

Figure 2: The maximal mass value as functions of (left) and (right) in the mASMB, mGMSB as well as in mSUGRA and some of its variants.

The parameters of the models are varied within the ranges given in [26], and the top quark mass is taken to be GeV, and is limited to 3 TeV. While mSUGRA and NUHM provide solutions compatible with a Higgs mass 126 GeV, it is clear that the minimal versions of GMSB and AMSB, and the even more constrained mSUGRA scenarios (VCMSSM, no-scale) are disfavoured.

Figure 3: Maximal Higgs mass in mSUGRA, mAMSB and mGMSB, as a function of for the top quark mass varied in the range GeV.

It should be noted that the value of top mass has a significant impact on the maximal Higgs mass, in particular in constrained scenarios, where also enters in the evaluation of the soft SUSY breaking parameters and the minimisation of the scalar potential. This effect is demonstrated in Fig. 3 for the minimal SUGRA, AMSB and GMSB models.

We turn now to the pMSSM and in Fig. 4 we show the distribution of points compatible with SUSY searches with 15 fb of 7 TeV data as well as the Higgs mass constraints and the and signal strengths given in Table 3, as functions of the masses of the lightest squark of the first two generations, the lightest neutralino and .

Figure 4: Fraction of accepted pMSSM points, with 123 127 GeV (filled squares), not excluded by the SUSY searches with 15 fb of 7 TeV data as functions of the masses of the lightest squark of the first two generations (left panel), the lightest neutralino (central panel) and (right panel). The open square points show the fraction of pMSSM points after imposing the additional requirements on the Higgs rates and .

A comparison with Fig. 1 reveals first that the Higgs constraints strongly reduce the statistics. The squark and neutralino distribution shapes are quite unaffected, but the small region (below 15) is now more constrained.

In Fig. 5 we present the distribution of pMSSM points compatible with the boson mass and the observed yields given, in the , , and , parameter planes. To do so, we combined all the constraints in Table 3 with a combination. We notice first that small values of are clearly disfavoured, and that stop masses as low as 400 GeV are still compatible with the data. This is mainly the results of the Higgs mass measurement which calls for non minimal mixing in the stop sector. Second, the negative region is favoured by the rate constraints. This can be explained by the fact that a decrease in the rate, generated in particular by negative , would result in an increase of , which is favoured by present data. Similarly, negative are favoured since a reduced rate is more likely to be consistent with the current limit. Finally, GeV values are strongly disfavoured by the Higgs mass and rate measurements for any value of , and therefore the decoupling regime seems to be favoured by the data.

Figure 5: Distributions of the pMSSM points in the (upper left), (upper right), (lower left) and , (lower right) parameter planes. The black dots show the accepted pMSSM points, those in light (dark) grey the same points compatible at 68% (90%) C.L. with the Higgs constraints of Table 3.

4 Conclusion

We have considered the results from SUSY and Higgs searches at the LHC in the context of the MSSM. Contrary to the constrained MSSM scenarios, in the pMSSM the current LHC limits from the SUSY searches still leave a substantial room for low energy SUSY. This conclusion does not change when we include in addition the information from the Higgs sector, namely the mass and signal yields of the new boson. However, the current Higgs data already point to specific regions of the MSSM, in particular to the decoupling regime with large stop and negative sbottom and stau mixings. With more data becoming available, and more precise experimental results on the Higgs boson properties, more important impacts on the parameter regions of the SUSY scenarios are to be expected.

References

  1. G. Aad et al. [ATLAS Collaboration], Phys. Lett. B 716 (2012) 1 [arXiv:1207.7214].
  2. S. Chatrchyan et al. [CMS Collaboration], Phys. Lett. B 716 (2012) 30 [arXiv:1207.7235].
  3. A. Djouadi et al. [MSSM Working Group Collaboration], hep-ph/9901246.
  4. B. C. Allanach, Comput. Phys. Commun. 143 (2002) 305 [hep-ph/0104145].
  5. A. Djouadi, J.L. Kneur and G. Moultaka, Comput. Phys. Commun. 176 (2007) 426 [hep-ph/0211331].
  6. A. Arbey, M. Battaglia and F. Mahmoudi, Eur. Phys. J. C 72 (2012) 1906 [arXiv:1112.3032].
  7. F. Mahmoudi, Comput. Phys. Commun. 178 (2008) 745 [arXiv:0710.2067]; Comput. Phys. Commun. 180 (2009) 1579 [arXiv:0808.3144]; A. Arbey and F. Mahmoudi, Comput. Phys. Commun. 181 (2010) 1277 [arXiv:0906.0369].
  8. A. Arbey, M. Battaglia and F. Mahmoudi, Eur. Phys. J. C 72 (2012) 2169 [arXiv:1205.2557].
  9. M. Muhlleitner, A. Djouadi and Y. Mambrini, Comput. Phys. Commun. 168 (2005) 46 [hep-ph/0311167].
  10. T. Sjostrand, S. Mrenna and P. Z. Skands, JHEP 0605 (2006) 026 [hep-ph/0603175].
  11. S. Ovyn, X. Rouby and V. Lemaitre, arXiv:0903.2225 [hep-ph].
  12. A. Arbey, M. Battaglia and F. Mahmoudi, Eur. Phys. J. C 72 (2012) 1847 [arXiv:1110.3726].
  13. A. Djouadi, J. Kalinowski and M. Spira, Comput. Phys. Commun. 108 (1998) 56 [hep-ph/9704448].
  14. M. Spira, hep-ph/9510347.
  15. S. Heinemeyer, W. Hollik and G. Weiglein, Comput. Phys. Commun. 124 (2000) 76 [hep-ph/9812320].
  16. [CMS Collaboration], CMS PAS SUS-11-003.
  17. [CMS Collaboration], CMS PAS SUS-11-010.
  18. [CMS Collaboration], CMS PAS SUS-11-011.
  19. [ATLAS Collaboration], Note ATLAS-CONF-2012-091.
  20. [CMS Collaboration], Note CMS PAS HIG-2012-015.
  21. [ATLAS Collaboration], Note ATLAS-CONF-2012-092.
  22. [CMS Collaboration], Note CMS PAS HIG-2012-016.
  23. [CMS Collaboration], Note CMS PAS HIG-2012-019.
  24. [CMS Collaboration], Note CMS PAS HIG-2012-018.
  25. A. Arbey, M. Battaglia, A. Djouadi, F. Mahmoudi and J. Quevillon, Phys. Lett. B 708 (2012) 162 [arXiv:1112.3028].
  26. A. Arbey, M. Battaglia, A. Djouadi and F. Mahmoudi, JHEP 1209 (2012) 107 [arXiv:1207.1348].
Comments 0
Request Comment
You are adding the first comment!
How to quickly get a good reply:
  • Give credit where it’s due by listing out the positive aspects of a paper before getting into which changes should be made.
  • Be specific in your critique, and provide supporting evidence with appropriate references to substantiate general statements.
  • Your comment should inspire ideas to flow and help the author improves the paper.

The better we are at sharing our knowledge with each other, the faster we move forward.
""
The feedback must be of minimum 40 characters and the title a minimum of 5 characters
   
Add comment
Cancel
Loading ...
304799
This is a comment super asjknd jkasnjk adsnkj
Upvote
Downvote
""
The feedback must be of minumum 40 characters
The feedback must be of minumum 40 characters
Submit
Cancel

You are asking your first question!
How to quickly get a good answer:
  • Keep your question short and to the point
  • Check for grammar or spelling errors.
  • Phrase it like a question
Test
Test description