This paper was converted on www.awesomepapers.org from LaTeX by an anonymous user.
Want to know more? Visit the Converter page.

11institutetext: Faculty of Sciences and Techniques, Abdelmalek Essaadi University, B.P. 416, Tanger, Morocco 22institutetext: Centro de Física Teórica e Computacional, Faculdade de Ciências, Universidade de Lisboa, Campo Grande, Edifício C8, 1749-016 Lisboa, Portugal 33institutetext: MSISM Team, Faculté Polydisciplinaire de Safi, Sidi Bouzid, B.P. 4162, Safi, Morocco 44institutetext: School of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ, United Kingdom 55institutetext: ARC Center of Excellence for Particle Physics at the Terascale, Department of Physics, University of Adelaide, 5005 Adelaide, South Australia 66institutetext: ISEL - Instituto Superior de Engenharia de Lisboa, Instituto Politécnico de Lisboa, 1959-007 Lisboa, Portugal

Scattering Interference effects on H+tb¯H^{+}\to t\bar{b} Signals in MSSM Benchmark Scenarios

\firstnameAbdesslam \lastnameArhrib\fnsep 11    \firstnameDuarte \lastnameAzevedo\fnsep 22    \firstnameRachid \lastnameBenbrik\fnsep 33    \firstnameHicham \lastnameHarouiz\fnsep 33    \firstnameStefano \lastnameMoretti\fnsep 44    \firstnameRiley \lastnamePatrick\fnsep 55    \firstnameRui \lastnameSantos\fnsep 2266
Abstract

In this talk an investigation into the interference effects between the process ppt¯bH+pp\to\bar{t}bH^{+} followed by the decay H+tb¯H^{+}\to t\bar{b} and the background process pptt¯bb¯pp\to t\bar{t}b\bar{b} is presented. The level of interference in parts of the parameter space is shown to be high and as such it may spoil the results of typical analyses which treat signal and background as independent. This is shown for two benchmarks of the MSSM.

1 Introduction

The selection of benchmark is important as the chosen parameter point must provide both a non-negligible cross section and high width-to-mass ratio of the signal particle - in this case the charged Higgs. Two areas of the MSSM parameter space of interest to experimentalists are the hMSSM and the mhmod+m_{h}^{\rm mod+} models, for reviews of these see Refs. Djouadi:2013uqa and Heinemeyer:1999zf respectively. We utilize these models as a vehicle for study of interference effects and hone in further on specific choices of MSSM parameters in the next section.

2 Benchmark Selection

To generate our benchmark points a scan of the MSSM parameter space is undertaken using FeynHiggs Heinemeyer:1998yj Hahn:2009zz interfaced with HiggsBounds-5.2.0beta Bechtle:2008jh Bechtle:2011sb Bechtle:2013wla Bechtle:2015pma and HiggsSignals-2.2.0beta Bechtle:2013xfa to obtain constraints.

Refer to caption
Refer to caption
Refer to caption
Refer to caption
Figure 1: Δχ2\Delta\chi^{2} (top-left) and the charged Higgs total width (top-right) in the (mAMA0m_{A}\equiv M_{A^{0}}, tanβ\tan\beta) plane. The best fit point is located at MA01M_{A^{0}}\approx 1 TeV and tanβ2\tan\beta\approx 2. The green lines show the exclusion limits from HiggSignals at 1σ1\sigma (solid) and 2σ2\sigma (dashed) while the gray area is ruled out by the various LHC searches implemented in HiggsBounds. The ratio ΓH±/MH±\Gamma_{H^{\pm}}/M_{H^{\pm}} as a function of the charged Higgs mass is shown in the bottom-left panel while in the bottom-right one it is presented as a function of the charged Higgs production cross section.

Fig 1 displays various three dimensional slices of the parameter space for the hMSSM model. We wish to choose a point which has high width-to-mass ratio, so as to generate high levels of interference, as well as a non-negligible cross section and high branching ratio of H+tb¯H^{+}\to t\bar{b} to preserve that cross section. Utilizing a scan of the parameter space with these goals in mind the best point found has MH±=633.91M_{H^{\pm}}=633.91 GeV and tanβ=1.01\tan\beta=1.01.

Refer to caption
Refer to caption
Refer to caption
Refer to caption
Figure 2: Allowed parameter region in the mhmod+m_{h}^{\rm mod+} scenario over the (mAMA0m_{A}\equiv M_{A^{0}}, tanβ\tan\beta) plane with colour showing Δχ2\Delta\chi^{2} (top-left) and the charged Higgs boson mass (top-right). The LHC Higgs searches constraints are included. The light green contours are HiggsSignals exclusion limits at 1σ1\sigma (solid) and 2σ2\sigma (dashed). The light gray area is excluded by HiggsBounds at 2σ2\sigma. The solid brown lines are contours for the lighter CP-even scalar h0h^{0} mass. The best fit point is located at MH±1M_{H^{\pm}}\approx 1 TeV and tanβ=20\tan\beta=20. In the two bottom panels of Fig. 2 we present tanβ\tan\beta as a function of ΓH±/MH±\Gamma_{H^{\pm}}/M_{H^{\pm}} with the colour code showing the charged Higgs mass (left) and the charged Higgs production cross section (right).

Fig 2 displays various three dimensional slices of the parameter space for the mhmod+m_{h}^{\rm mod+}. In this case we choose a point which has a much lower width-to-mass ratio but a higher cross section and thus we may see lower levels of interference prior to cuts. It is possible however that interference may grow after cuts. Utilizing a scan of the parameter space with these goals in mind the best point found has MH±=303.08M_{H^{\pm}}=303.08 GeV and tanβ=3.42\tan\beta=3.42.

3 Results

For this analysis two independent samples were generated for both the hMSSM and mhmod+m_{h}^{\rm mod+} at leading order and at 13 TeV CoM energy at the LHC. The first sample contained 20,000,000 parton level events to provide a Monte Carlo sample with sufficiently low statistical error on the interference term. This sample was generated using MadGraph Alwall:2014hca . The second sample contained 500,000 events generated in MadGraph, then passed to Pythia Sjostrand:2014zea for hadronization/fragmentation and then to Delphes deFavereau:2013fsa for detector smearing.

Model S (pb) B (pb) S+B (pb) I (pb)
hhMSSM σ\sigma 0.0324020.032402 13.07813.078 13.13913.139 0.0280.028
Δσ\Delta\sigma 1.4×1051.4\times 10^{-5} 0.0020.002 0.0010.001 0.0030.003
mhmod+m^{\rm{mod+}}_{{h}} σ\sigma 0.0885360.088536 13.09513.095 13.19713.197 0.0140.014
Δσ\Delta\sigma 3.3×1053.3\times 10^{-5} 0.0010.001 0.0010.001 0.0020.002
Table 1: Parton level results for the hhMSSM and mhmod+m^{\rm mod+}_{\rm h} benchmarks.

This process was undertaken for the signal (“S”), defined as all processes in the MSSM that generate tt¯bb¯t\bar{t}b\bar{b} mediated by H±H^{\pm}, the background (“B”), defined as all processes in the MSSM that generate tt¯bb¯t\bar{t}b\bar{b} that are not mediated by H±H^{\pm}, and the signal plus background - from here out called total (“T”) - that contains all processes in the MSSM that can generate tt¯bb¯t\bar{t}b\bar{b}.

The three samples were then used to quantify the interference using the relationship I=TSBI=T-S-B. As all three amplitudes have the same phase space then this equation isolates the interference term of the full scattering amplitude. The parton level results can be seen in Tab 1.

3.1 Event Reconstruction

We choose the final state with exactly 1-lepton, thus allowing us to calculate the longitudinal momentum of missing energy. This is done via solving the following quadratic equation:

pνz=12pT2(AWpz±EAW2±4pT2EνT2)\displaystyle p_{\nu}^{z}=\frac{1}{2p_{\ell T}^{2}}\left(A_{W}p^{z}_{\ell}\pm E_{\ell}\sqrt{A_{W}^{2}\pm 4p^{2}_{\ell T}E^{2}_{\nu T}}\right) (1)

where, AW=MW±2+2pTEνTA_{W}=M^{2}_{W^{\pm}}+2p_{\ell T}\cdot E_{\nu T}. If both of these solutions are non-real we veto the event.

We then perform a full event reconstruction by simultaneous minimisation of the following equations by permuting through all combinations of jets in the process and the two solutions for neutrino momentum,

χhad2=(MνMW)2ΓW2+(MjjMW)2ΓW2+(MνjMT)2ΓT2+(MjjjMT)2ΓT2+(MjjjjMH±)2ΓH±2\displaystyle\chi^{2}_{\rm had}=\frac{\left(M_{\ell\nu}-M_{W}\right)^{2}}{\Gamma^{2}_{W}}+\frac{\left(M_{jj}-M_{W}\right)^{2}}{\Gamma^{2}_{W}}+\frac{\left(M_{\ell\nu j}-M_{T}\right)^{2}}{\Gamma^{2}_{T}}+\frac{\left(M_{jjj}-M_{T}\right)^{2}}{\Gamma^{2}_{T}}+\frac{\left(M_{jjjj}-M_{H^{\pm}}\right)^{2}}{\Gamma^{2}_{H^{\pm}}} (2)

and

χlep2=(MνMW)2ΓW2+(MjjMW)2ΓW2+(MνjMT)2ΓT2+(MjjjMT)2ΓT2+(MνjjMH±)2ΓH±2\displaystyle\chi^{2}_{\rm lep}=\frac{\left(M_{\ell\nu}-M_{W}\right)^{2}}{\Gamma^{2}_{W}}+\frac{\left(M_{jj}-M_{W}\right)^{2}}{\Gamma^{2}_{W}}+\frac{\left(M_{\ell\nu j}-M_{T}\right)^{2}}{\Gamma^{2}_{T}}+\frac{\left(M_{jjj}-M_{T}\right)^{2}}{\Gamma^{2}_{T}}+\frac{\left(M_{\ell\nu jj}-M_{H^{\pm}}\right)^{2}}{\Gamma^{2}_{H^{\pm}}} (3)

The results of this reconstruction can be found in Figs. 3 and 5, normalised to unit area.

After this we apply a very simple set of cuts to calculate the behaviour of interference under cutflow. The full set of cuts are exactly one lepton, five or more light jets, two (three) or more b-jets, missing energy greater than 5050 GeV and finally, the transverse mass of missing energy and the lepton must be higher than 60 GeV. Specifically, mTW=(x+x)2+(y+y)2>60m^{W}_{T}=\sqrt{(\not{E}_{x}+\ell_{x})^{2}+(\not{E}_{y}+\ell_{y})^{2}}>60 GeV. The results of these cutflows can be found in Tabs 2 and 3.

3.2 The hMSSM analysis

The parton level interference relative to signal in the hMSSM scenario was 86.486.4%, an alarmingly high level of interference before cuts. The 2 b-tag cut flow served to increase this to 225.6225.6% and the 3 b-tag scenario to increase it to 277.8277.8%. In all three of these subsets of the phase space the interference appears to be sufficiently large to motivate quantifying it in a full analysis. It should be noted however that the error on the interference is of roughly the same order, and so these results should be considered with this in mind.

Fig 4 presents an example of the shape of the interference distribution, specifically in the tt¯bb¯t\bar{t}b\bar{b} reconstructed invariant mass plane. This was undertaken using the large parton level sample so as to ensure the per-bin error was sufficiently low. It can be seen that there is a significant off-peak positive contribution of the interference.

Refer to caption
Figure 3: Invariant mass distributions for reconstructed particles in the hhMSSM benchmark.
Cut S B S+B I ΔI\Delta\text{I}
No cuts: 97206 39235500 39417000 84294 111369
N=1N_{\ell}=1: 21601 9059869 9083647 2177 53488
NJ5N_{J}\geq 5: 19380 6256492 6296865 20991 44499
NBJ2N_{BJ}\geq 2: 15112 4058520 4091878 18246 35861
>20\not{E}>20 GeV: 14356 3736396 3776148 25395 34430
+mTW>60\not{E}+m_{T}^{W}>60 GeV: 14129 3639484 3685489 31874 33997
Cut S B S+B I ΔI\Delta\text{I}
NBJ3N_{BJ}\geq 3: 8263 1715768 1733953 9921 23335
>20\not{E}>20 GeV: 7851 1581190 1607425 18383 22435
+mTW>60\not{E}+m_{T}^{W}>60 GeV: 7729 1540778 1569979 21471 22160
Table 2: Cut flow results presented in expected event yield with 3000 fb-1 of luminosity for the hhMSSM benchmark.
Refer to caption
Figure 4: The charged Higgs invariant mass distribution of the signal, background and total samples (left) and interference and signal (right) at parton level and without cuts in the hhMSSM scenario.

3.3 The mhmod+m_{h}^{\rm mod+} analysis

The mhmod+m_{h}^{\rm mod+} results begin with a smaller parton level interference relative to signal of 15.0315.03%, reduce to 3.03.0% in the 2 b-tag scenario and increase to 58.758.7% in the 3 b-tag scenario. However it should be noted that the interference in this case is far smaller than the level of error, and so strong conclusions from this result are not possible.

Fig 6 presents an example of the shape of the interference distribution, again specifically in the tt¯bb¯t\bar{t}b\bar{b} reconstructed invariant mass plane. This was also undertaken using the large parton level sample and it can be seen that there is a non-negligible positive contribution from interference off-peak.

Refer to caption
Figure 5: Invariant mass distributions for reconstructed particles in the mhmod+m_{h}^{\rm mod+} benchmark.
Cut S B S+B I ΔI\Delta\text{I}
No cuts: 265620 39285000 39591000 40380 111923
N=1N_{\ell}=1: 60173 9031228 9109097 17695 53673
NJ5N_{J}\geq 5: 49641 6249064 6308825 10119 44671
NBJ2N_{BJ}\geq 2: 37040 4069533 4107962 1388 36057
>20\not{E}>20 GeV: 34323 3754074 3788858 460 34630
+mTW>60\not{E}+m_{T}^{W}>60 GeV: 33422 3658612 3693048 1013 34188
Cut S B S+B I ΔI\Delta\text{I}
NBJ3N_{BJ}\geq 3: 18946 1728147 1761007 13913 23561
>20\not{E}>20 GeV: 17578 1594185 1626002 14238 22635
+mTW>60\not{E}+m_{T}^{W}>60 GeV: 17124 1557257 1584431 10049 22357
Table 3: Cut flow results presented in expected event yield with 3000fb-1 of luminosity for the mhmod+m_{h}^{\rm mod+} benchmark.
Refer to caption
Figure 6: The charged Higgs invariant mass distribution of the signal, background and total samples (left) and interference and signal (right) at parton level and without cuts in the mhmod+m_{h}^{\rm mod+} scenario.

4 Conclusion

This talk presented the phenomenological analysis of the size of signal to background interference in the production of t¯bH+\bar{t}bH^{+} decaying via H+tb¯H^{+}\to t\bar{b} and the associated background production of tt¯bb¯t\bar{t}b\bar{b} at the 13 TeV LHC.

We utilize two benchmarks of the MSSM with heavy charged Higgs, and find that at parton level in both scenarios the interference is non-negligible. Furthermore the shape of the interference distribution and its associated impacts are not necessarily the same as the signal and so a simple rescaling of signal may not be feasible.

Furthermore, while the associated error on the detector level cutflow results is large, the results imply that the interference is sensitive to cuts and can reasonably increase significantly relative to the signal through a simple cutflow.

References

  • (1) A. Djouadi, L. Maiani, G. Moreau, A. Polosa, J. Quevillon and V. Riquer, Eur. Phys. J. C 73, 2650 (2013) [arXiv:1307.5205 [hep-ph]].
  • (2) S. Heinemeyer, W. Hollik and G. Weiglein, JHEP 0006 (2000) 009 [hep-ph/9909540].
  • (3) S. Heinemeyer, W. Hollik and G. Weiglein, Comput. Phys. Commun.  124, 76 (2000) [hep-ph/9812320].
  • (4) T. Hahn, S. Heinemeyer, W. Hollik, H. Rzehak and G. Weiglein, Comput. Phys. Commun.  180, 1426 (2009). See:: http://www.feynhiggs.de.
  • (5) P. Bechtle, O. Brein, S. Heinemeyer, G. Weiglein and K. E. Williams, Comput. Phys. Commun.  181, 138 (2010) [arXiv:0811.4169 [hep-ph]].
  • (6) P. Bechtle, O. Brein, S. Heinemeyer, G. Weiglein and K. E. Williams, Comput. Phys. Commun.  182, 2605 (2011) [arXiv:1102.1898 [hep-ph]].
  • (7) P. Bechtle, O. Brein, S. Heinemeyer, O. Stål, T. Stefaniak, G. Weiglein and K. E. Williams, Eur. Phys. J. C 74, no. 3, 2693 (2014) [arXiv:1311.0055 [hep-ph]].
  • (8) P. Bechtle, S. Heinemeyer, O. Stål, T. Stefaniak and G. Weiglein, Eur. Phys. J. C 75, no. 9, 421 (2015) [arXiv:1507.06706 [hep-ph]].
  • (9) P. Bechtle, S. Heinemeyer, O. Stål, T. Stefaniak and G. Weiglein, Eur. Phys. J. C 74, no. 2, 2711 (2014) [arXiv:1305.1933 [hep-ph]].
  • (10) J. Alwall et al., JHEP 1407, 079 (2014) [arXiv:1405.0301 [hep-ph]].
  • (11) T. Sjöstrand et al., Comput. Phys. Commun.  191, 159 (2015) [arXiv:1410.3012 [hep-ph]].
  • (12) J. de Favereau et al. [DELPHES 3 Collaboration], JHEP 1402, 057 (2014) [arXiv:1307.6346 [hep-ex]].