SUSYNLONNLLCrossSections27TeVHinoN2C1 < LHCPhysics

---+ NLO-NNLL higgsino-like !N2C1 cross sections

The following cross sections are for higgsino-like chargino-neutralino pair production (sum of &#967;&#771;<sup>+</sup><sub>1</sub>&#967;&#771;<sup>0</sup><sub>2</sub> and &#967;&#771;<sup>-</sup><sub>1</sub>&#967;&#771;<sup>0</sup><sub>2</sub>, and also for each subprocess individually). They have been calculated for sqrt(s) = 27 !TeV at NLO-NNLL using Resummino 2.0.1 from B. Fuks et al. The Monte Carlo PDF set with 100 replicas !PDF4LHC15_mc is used, which is a statistical combination of CT14, MMHT14 and NNPDF3.0, all using &alpha;<sub>s</sub>(m<sub>Z</sub><sup>2</sup>) = 0.118. The use of this combination of PDF sets is recommended for searches for new Physics by the !PDF4LHC Working Group. See https://arxiv.org/abs/1510.03865 for more details.

The cross sections are computed for degenerate charginos and neutralinos. The mass is denoted as m<sub>&#967;&#771;</sub>. The following sentence describes all the assumptions in the cross section calculations and is suitable to be included in the description of the interpretation of your results:

<verbatim>
The production cross sections are computed at NLO plus
next-to-next-to-leading-log (NNLL) precision in a limit of mass-degenerate
higgsino $\chiz_2$, $\chipm_1$, and $\chiz_1$ with all the other sparticles
assumed to be heavy and decoupled.
</verbatim>

When using these cross sections, some references have to be cited. They can be found below in bibtex format. The [[https://twiki.cern.ch/twiki/pub/LHCPhysics/SUSYNLONNLLCrossSections13TeVHinoN2C1/CMS-SUS-Cross-Sections.bib][references can also be downloaded]] from this Twiki, see attachments at the bottom.

%TWISTY{mode="div" showlink="Show References " hidelink="Hide References " firststart="hide" showimgright="%ICONURLPATH{toggleopen-small}%" hideimgright="%ICONURLPATH{toggleclose-small}%"}%

Resummino:

<verbatim>
@article{Debove:2010kf,
      author         = "Debove, Jonathan and Fuks, Benjamin and Klasen, Michael",
      title          = "{Threshold resummation for gaugino pair production at
                        hadron colliders}",
      journal        = "Nucl. Phys. B",
      volume         = "842",
      year           = "2011",
      pages          = "51-85",
      doi            = "10.1016/j.nuclphysb.2010.08.016",
      eprint         = "1005.2909",
      archivePrefix  = "arXiv",
      primaryClass   = "hep-ph",
      reportNumber   = "IPHC-PHENO-10-02, LPSC-10-050",
      SLACcitation   = "%%CITATION = ARXIV:1005.2909;%%"
}
@article{Fuks:2012qx,
      author         = "Fuks, Benjamin and Klasen, Michael and Lamprea, David R.
                        and Rothering, Marcel",
      title          = "{Gaugino production in proton-proton collisions at a
                        center-of-mass energy of 8 TeV}",
      journal        = "JHEP",
      volume         = "10",
      pages          = "081",
      doi            = "10.1007/JHEP10(2012)081",
      year           = "2012",
      eprint         = "1207.2159",
      archivePrefix  = "arXiv",
      primaryClass   = "hep-ph",
      reportNumber   = "IPHC-PHENO-12-07, MS-TP-12-05",
      SLACcitation   = "%%CITATION = ARXIV:1207.2159;%%",
}
@article{Fuks:2013vua,
      author         = "Fuks, Benjamin and Klasen, Michael and Lamprea, David R.
                        and Rothering, Marcel",
      title          = "{Precision predictions for electroweak superpartner
                        production at hadron colliders with {\sc Resummino}}",
      journal        = "Eur. Phys. J. C",
      volume         = "73",
      pages          = "2480",
      doi            = "10.1140/epjc/s10052-013-2480-0",
      year           = "2013",
      eprint         = "1304.0790",
      archivePrefix  = "arXiv",
      primaryClass   = "hep-ph",
      reportNumber   = "CERN-PH-TH-2013-064, IPHC-PHENO-13-02, MS-TP-13-06",
      SLACcitation   = "%%CITATION = ARXIV:1304.0790;%%",
}
@article{Fiaschi:2018hgm,
      author         = "Fiaschi, Juri and Klasen, Michael",
      title          = "{Neutralino-chargino pair production at NLO+NLL with
                        resummation-improved parton density functions for LHC Run
                        II}",
      journal        = "Phys. Rev. D",
      volume         = "98",
      year           = "2018",
      number         = "5",
      pages          = "055014",
      doi            = "10.1103/PhysRevD.98.055014",
      eprint         = "1805.11322",
      archivePrefix  = "arXiv",
      primaryClass   = "hep-ph",
      reportNumber   = "MS-TP-18-19",
      SLACcitation   = "%%CITATION = ARXIV:1805.11322;%%"
}
</verbatim>

LHAPDF:

<verbatim>
@article{Buckley:2014ana,
      author         = "Buckley, Andy and Ferrando, James and Lloyd, Stephen and
                        Nordström, Karl and Page, Ben and Rüfenacht, Martin and
                        Schönherr, Marek and Watt, Graeme",
      title          = "{LHAPDF6: parton density access in the LHC precision
                        era}",
      journal        = "Eur. Phys. J.",
      volume         = "C75",
      year           = "2015",
      pages          = "132",
      doi            = "10.1140/epjc/s10052-015-3318-8",
      eprint         = "1412.7420",
      archivePrefix  = "arXiv",
      primaryClass   = "hep-ph",
      reportNumber   = "GLAS-PPE-2014-05, MCNET-14-29, IPPP-14-111, DCPT-14-222",
      SLACcitation   = "%%CITATION = ARXIV:1412.7420;%%"
}
</verbatim>

!PDF4LHC:

<verbatim>
@article{Butterworth:2015oua,
      author         = "Butterworth, Jon and others",
      title          = "{PDF4LHC recommendations for LHC Run II}",
      journal        = "J. Phys.",
      volume         = "G43",
      year           = "2016",
      pages          = "023001",
      doi            = "10.1088/0954-3899/43/2/023001",
      eprint         = "1510.03865",
      archivePrefix  = "arXiv",
      primaryClass   = "hep-ph",
      reportNumber   = "OUTP-15-17P, SMU-HEP-15-12, TIF-UNIMI-2015-14,
                        LCTS-2015-27, CERN-PH-TH-2015-249",
      SLACcitation   = "%%CITATION = ARXIV:1510.03865;%%"
}
@article{Carrazza:2015hva,
      author         = "Carrazza, Stefano and Latorre, José I. and Rojo, Juan
                        and Watt, Graeme",
      title          = "{A compression algorithm for the combination of PDF
                        sets}",
      journal        = "Eur. Phys. J.",
      volume         = "C75",
      year           = "2015",
      pages          = "474",
      doi            = "10.1140/epjc/s10052-015-3703-3",
      eprint         = "1504.06469",
      archivePrefix  = "arXiv",
      primaryClass   = "hep-ph",
      reportNumber   = "TIF-UNIMI-2015-2, OUTP-15-01P, IPPP-15-22, DCPT-15-44",
      SLACcitation   = "%%CITATION = ARXIV:1504.06469;%%"
}
@article{Watt:2012tq,
      author         = "Watt, G. and Thorne, R. S.",
      title          = "{Study of Monte Carlo approach to experimental
                        uncertainty propagation with MSTW 2008 PDFs}",
      journal        = "JHEP",
      volume         = "08",
      year           = "2012",
      pages          = "052",
      doi            = "10.1007/JHEP08(2012)052",
      eprint         = "1205.4024",
      archivePrefix  = "arXiv",
      primaryClass   = "hep-ph",
      reportNumber   = "CERN-PH-TH-2012-132, LCTS-2012-11",
      SLACcitation   = "%%CITATION = ARXIV:1205.4024;%%"
}
</verbatim>

CT14:

<verbatim>
@article{Dulat:2015mca,
      author         = "Dulat, Sayipjamal and Hou, Tie-Jiun and Gao, Jun and
                        Guzzi, Marco and Huston, Joey and Nadolsky, Pavel and
                        Pumplin, Jon and Schmidt, Carl and Stump, Daniel and Yuan,
                        C. P.",
      title          = "{New parton distribution functions from a global analysis
                        of quantum chromodynamics}",
      journal        = "Phys. Rev.",
      volume         = "D93",
      year           = "2016",
      number         = "3",
      pages          = "033006",
      doi            = "10.1103/PhysRevD.93.033006",
      eprint         = "1506.07443",
      archivePrefix  = "arXiv",
      primaryClass   = "hep-ph",
      SLACcitation   = "%%CITATION = ARXIV:1506.07443;%%"
}
</verbatim>

MMHT14:

<verbatim>
@article{Harland-Lang:2014zoa,
      author         = "Harland-Lang, L. A. and Martin, A. D. and Motylinski, P.
                        and Thorne, R. S.",
      title          = "{Parton distributions in the LHC era: MMHT 2014 PDFs}",
      journal        = "Eur. Phys. J.",
      volume         = "C75",
      year           = "2015",
      number         = "5",
      pages          = "204",
      doi            = "10.1140/epjc/s10052-015-3397-6",
      eprint         = "1412.3989",
      archivePrefix  = "arXiv",
      primaryClass   = "hep-ph",
      reportNumber   = "LCTS-2014-47, IPPP-14-97, DCPT-14-194",
      SLACcitation   = "%%CITATION = ARXIV:1412.3989;%%"
}
</verbatim>

NNPDF:

<verbatim>
@article{Ball:2014uwa,
      author         = "Ball, Richard D. and others",
      title          = "{Parton distributions for the LHC Run II}",
      collaboration  = "NNPDF",
      journal        = "JHEP",
      volume         = "04",
      year           = "2015",
      pages          = "040",
      doi            = "10.1007/JHEP04(2015)040",
      eprint         = "1410.8849",
      archivePrefix  = "arXiv",
      primaryClass   = "hep-ph",
      reportNumber   = "EDINBURGH-2014-15, IFUM-1034-FT, CERN-PH-TH-2013-253,
                        OUTP-14-11P, CAVENDISH-HEP-14-11",
      SLACcitation   = "%%CITATION = ARXIV:1410.8849;%%"
}
</verbatim>

%ENDTWISTY%

To calculate these cross sections, [[https://github.com/basilschneider/cross-section-calculator][this repository]] can be used. The !SLHA files can be found there as well: [[https://github.com/basilschneider/cross-section-calculator/blob/master/condor/wino.in][wino.in]] and [[https://github.com/basilschneider/cross-section-calculator/blob/master/condor/hino.in][hino.in]].

Should cross section information be needed for a mass that is not tabulated below, one can obtain it by using the ROOT macros provided under:

<verbatim>
/afs/cern.ch/user/a/amete/public/EWKGauginoCrossSections_13TeV
</verbatim> 

For this specific grid one needs to do:
<verbatim>
root -l 'get_gaugino.C("C1N2", "hino", mass)' 
</verbatim> 

where mass is the mass of the sparticle in !GeV. The result of the interpolation can be seen <a href="https://twiki.cern.ch/twiki/pub/LHCPhysics/SUSYCrossSections13TeVn2x1hino/c1n2_hino.pdf" />here</a>.

<!-- 
    Cross section table generated with Cross Section Calculator 
    https://github.com/basilschneider/cross-section-calculator 
    Input directory: eoscopy/resummino_c720883/hino_27TeV_1000023_1000024 
    Input directory: eoscopy/resummino_c720884/hino_27TeV_1000023_m1000024 
    Date: 14-11-2018 07:34:02 
--> 
 
---+++ NLO+NNLL Higgsino cross sections for combined &#967;&#771;<sup>0</sup><sub>2</sub>&#967;&#771;<sup>+</sup><sub>1</sub> and &#967;&#771;<sup>0</sup><sub>2</sub>&#967;&#771;<sup>-</sup><sub>1</sub> production at sqrt(s) = 27 !TeV 
 
%TABLE{ tableborder="0" cellpadding="4" cellspacing="3" cellborder="1" headerrows="1" columnwidths="80, 125, 125" headeralign="center" dataalign="right" headercolor="#FFFFFF" headerbg="#437B58" databg="#A1C2B1, #CFDFD5" datacolor="#000000"}% 
 
 | *m<sub>&#967;&#771;</sub> [GeV]* | *&sigma; [fb]*  | *uncertainty [fb]* | 
 | 50 | 248000 | 372 | 
 | 75 | 38748 | 50.4 | 
 | 100 | 13687.1 | 16.893 | 
 | 125 | 6358.6 | 7.569 | 
 | 150 | 3428.3 | 3.966 | 
 | 175 | 2034.98 | 2.3011 | 
 | 200 | 1292.74 | 1.4437 | 
 | 225 | 864.28 | 0.9468 | 
 | 250 | 601.26 | 0.6465 | 
 | 275 | 431.87 | 0.4609 | 
 | 300 | 318.47 | 0.3344 | 
 | 325 | 240.051 | 0.24967 | 
 | 350 | 184.35 | 0.18924 | 
 | 375 | 143.873 | 0.14732 | 
 | 400 | 113.865 | 0.11576 | 
 | 425 | 91.231 | 0.09168 | 
 | 450 | 73.896 | 0.07345 | 
 | 475 | 60.438 | 0.05945 | 
 | 500 | 49.853 | 0.04919 | 
 | 525 | 41.463 | 0.04023 | 
 | 550 | 34.724 | 0.03338 | 
 | 575 | 29.2685 | 0.027895 | 
 | 600 | 24.8164 | 0.023453 | 
 | 625 | 21.1554 | 0.019842 | 
 | 650 | 18.1247 | 0.016864 | 
 | 675 | 15.5975 | 0.014031 | 
 | 700 | 13.4826 | 0.012051 | 
 | 725 | 11.7005 | 0.010394 | 
 | 750 | 10.1915 | 0.009002 | 
 | 775 | 8.9078 | 0.007824 | 
 | 800 | 7.8109 | 0.006824 | 
 | 825 | 6.8697 | 0.005972 | 
 | 850 | 6.0596 | 0.005284 | 
 | 875 | 5.3589 | 0.004649 | 
 | 900 | 4.7513 | 0.004122 | 
 | 925 | 4.2225 | 0.003647 | 
 | 950 | 3.7608 | 0.0032334 | 
 | 975 | 3.3568 | 0.0028737 | 
 | 1000 | 3.00214 | 0.002559 | 
 | 1025 | 2.69019 | 0.0022841 | 
 | 1050 | 2.41499 | 0.0020423 | 
 | 1075 | 2.17147 | 0.0018294 | 
 | 1100 | 1.9554 | 0.0016408 | 
 | 1125 | 1.76392 | 0.0014754 | 
 | 1150 | 1.59401 | 0.0013151 | 
 | 1175 | 1.4421 | 0.0011861 | 
 | 1200 | 1.30651 | 0.0010713 | 
 | 1225 | 1.18467 | 0.0009682 | 
 | 1250 | 1.07592 | 0.0008769 | 
 | 1275 | 0.97832 | 0.0007952 | 
 | 1300 | 0.89057 | 0.000722 | 
 | 1325 | 0.81158 | 0.0006562 | 
 | 1350 | 0.74036 | 0.0005972 | 
 | 1375 | 0.67607 | 0.0005441 | 
 | 1400 | 0.61785 | 0.000496 | 
 | 1425 | 0.56524 | 0.0004527 | 
 | 1450 | 0.51816 | 0.0004147 | 
 | 1475 | 0.47495 | 0.00038048 | 
 | 1500 | 0.4357 | 0.00034852 | 
 | 1525 | 0.40002 | 0.00031948 | 
 | 1550 | 0.367563 | 0.00029329 | 
 | 1575 | 0.337986 | 0.00026948 | 
 | 1600 | 0.310934 | 0.00024803 | 
 | 1625 | 0.286227 | 0.00022766 | 
 | 1650 | 0.263666 | 0.00021048 | 
 | 1675 | 0.243063 | 0.00019374 | 
 | 1700 | 0.224209 | 0.0001785 | 
 | 1725 | 0.206933 | 0.00016452 | 
 | 1750 | 0.191093 | 0.00015234 | 
 | 1775 | 0.17657 | 0.0001402 | 
 | 1800 | 0.163251 | 0.00012953 | 
 | 1825 | 0.150992 | 0.00011976 | 
 | 1850 | 0.139724 | 0.00011094 | 
 | 1875 | 0.129355 | 0.00010305 | 
 | 1900 | 0.119797 | 9.531e-05 | 
 | 1925 | 0.110987 | 8.815e-05 | 
 | 1950 | 0.102871 | 8.158e-05 | 
 | 1975 | 0.095392 | 7.559e-05 | 
 | 2000 | 0.088497 | 7.009e-05 | 
<!-- 
    Cross section table generated with Cross Section Calculator 
    https://github.com/basilschneider/cross-section-calculator 
    Input directory: eoscopy/resummino_c720883/hino_27TeV_1000023_1000024 
    Date: 14-11-2018 07:34:30 
--> 
 
---+++ NLO+NNLL Higgsino cross sections for &#967;&#771;<sup>0</sup><sub>2</sub>&#967;&#771;<sup>+</sup><sub>1</sub> production at sqrt(s) = 27 !TeV 
 
%TABLE{ tableborder="0" cellpadding="4" cellspacing="3" cellborder="1" headerrows="1" columnwidths="80, 125, 125" headeralign="center" dataalign="right" headercolor="#FFFFFF" headerbg="#437B58" databg="#A1C2B1, #CFDFD5" datacolor="#000000"}% 
 
 | *m<sub>&#967;&#771;</sub> [GeV]* | *&sigma; [fb]*  | *uncertainty [fb]* | 
 | 50 | 1.4089e+05 | 215.2 | 
 | 75 | 22420 | 29.97 | 
 | 100 | 8029.9 | 10.22 | 
 | 125 | 3774.8 | 4.64 | 
 | 150 | 2056.6 | 2.458 | 
 | 175 | 1232.4 | 1.442 | 
 | 200 | 789.66 | 0.9167 | 
 | 225 | 532.22 | 0.6056 | 
 | 250 | 373.05 | 0.416 | 
 | 275 | 269.85 | 0.2999 | 
 | 300 | 200.34 | 0.2187 | 
 | 325 | 151.97 | 0.1634 | 
 | 350 | 117.41 | 0.1245 | 
 | 375 | 92.159 | 0.09789 | 
 | 400 | 73.338 | 0.07688 | 
 | 425 | 59.07 | 0.06115 | 
 | 450 | 48.089 | 0.0492 | 
 | 475 | 39.522 | 0.03999 | 
 | 500 | 32.75 | 0.03342 | 
 | 525 | 27.364 | 0.02712 | 
 | 550 | 23.017 | 0.02259 | 
 | 575 | 19.483 | 0.01895 | 
 | 600 | 16.587 | 0.01599 | 
 | 625 | 14.196 | 0.01358 | 
 | 650 | 12.209 | 0.01158 | 
 | 675 | 10.546 | 0.009698 | 
 | 700 | 9.1492 | 0.008356 | 
 | 725 | 7.9679 | 0.00723 | 
 | 750 | 6.9641 | 0.006281 | 
 | 775 | 6.1072 | 0.005475 | 
 | 800 | 5.3726 | 0.004789 | 
 | 825 | 4.7401 | 0.004203 | 
 | 850 | 4.1941 | 0.003742 | 
 | 875 | 3.7202 | 0.003301 | 
 | 900 | 3.308 | 0.002921 | 
 | 925 | 2.9482 | 0.002591 | 
 | 950 | 2.6332 | 0.002303 | 
 | 975 | 2.3567 | 0.002052 | 
 | 1000 | 2.1133 | 0.001832 | 
 | 1025 | 1.8986 | 0.001639 | 
 | 1050 | 1.7087 | 0.001469 | 
 | 1075 | 1.5402 | 0.001319 | 
 | 1100 | 1.3902 | 0.001186 | 
 | 1125 | 1.257 | 0.001069 | 
 | 1150 | 1.1386 | 0.000956 | 
 | 1175 | 1.0324 | 0.0008641 | 
 | 1200 | 0.93739 | 0.0007822 | 
 | 1225 | 0.85168 | 0.0007086 | 
 | 1250 | 0.77511 | 0.0006431 | 
 | 1275 | 0.70623 | 0.0005844 | 
 | 1300 | 0.64416 | 0.0005317 | 
 | 1325 | 0.58816 | 0.0004842 | 
 | 1350 | 0.53756 | 0.0004415 | 
 | 1375 | 0.49179 | 0.000403 | 
 | 1400 | 0.45022 | 0.0003681 | 
 | 1425 | 0.41261 | 0.0003366 | 
 | 1450 | 0.37905 | 0.000309 | 
 | 1475 | 0.34805 | 0.0002843 | 
 | 1500 | 0.31983 | 0.0002609 | 
 | 1525 | 0.29413 | 0.0002396 | 
 | 1550 | 0.27071 | 0.0002204 | 
 | 1575 | 0.24933 | 0.0002029 | 
 | 1600 | 0.22972 | 0.0001868 | 
 | 1625 | 0.21177 | 0.0001718 | 
 | 1650 | 0.19535 | 0.0001591 | 
 | 1675 | 0.18034 | 0.0001467 | 
 | 1700 | 0.16658 | 0.0001354 | 
 | 1725 | 0.15395 | 0.000125 | 
 | 1750 | 0.14236 | 0.0001156 | 
 | 1775 | 0.1317 | 0.0001069 | 
 | 1800 | 0.12192 | 9.893e-05 | 
 | 1825 | 0.1129 | 9.163e-05 | 
 | 1850 | 0.1046 | 8.489e-05 | 
 | 1875 | 0.096946 | 7.908e-05 | 
 | 1900 | 0.089877 | 7.324e-05 | 
 | 1925 | 0.08335 | 6.783e-05 | 
 | 1950 | 0.07733 | 6.286e-05 | 
 | 1975 | 0.071777 | 5.832e-05 | 
 | 2000 | 0.066652 | 5.415e-05 | 
<!-- 
    Cross section table generated with Cross Section Calculator 
    https://github.com/basilschneider/cross-section-calculator 
    Input directory: eoscopy/resummino_c720884/hino_27TeV_1000023_m1000024 
    Date: 14-11-2018 07:34:35 
--> 
 
---+++ NLO+NNLL Higgsino cross sections for &#967;&#771;<sup>0</sup><sub>2</sub>&#967;&#771;<sup>-</sup><sub>1</sub> production at sqrt(s) = 27 !TeV 
 
%TABLE{ tableborder="0" cellpadding="4" cellspacing="3" cellborder="1" headerrows="1" columnwidths="80, 125, 125" headeralign="center" dataalign="right" headercolor="#FFFFFF" headerbg="#437B58" databg="#A1C2B1, #CFDFD5" datacolor="#000000"}% 
 
 | *m<sub>&#967;&#771;</sub> [GeV]* | *&sigma; [fb]*  | *uncertainty [fb]* | 
 | 50 | 1.0711e+05 | 156.8 | 
 | 75 | 16328 | 20.43 | 
 | 100 | 5657.2 | 6.673 | 
 | 125 | 2583.8 | 2.929 | 
 | 150 | 1371.7 | 1.508 | 
 | 175 | 802.58 | 0.8591 | 
 | 200 | 503.08 | 0.527 | 
 | 225 | 332.06 | 0.3412 | 
 | 250 | 228.21 | 0.2305 | 
 | 275 | 162.02 | 0.161 | 
 | 300 | 118.13 | 0.1157 | 
 | 325 | 88.081 | 0.08627 | 
 | 350 | 66.94 | 0.06474 | 
 | 375 | 51.714 | 0.04943 | 
 | 400 | 40.527 | 0.03888 | 
 | 425 | 32.161 | 0.03053 | 
 | 450 | 25.807 | 0.02425 | 
 | 475 | 20.916 | 0.01946 | 
 | 500 | 17.103 | 0.01577 | 
 | 525 | 14.099 | 0.01311 | 
 | 550 | 11.707 | 0.01079 | 
 | 575 | 9.7855 | 0.008945 | 
 | 600 | 8.2294 | 0.007463 | 
 | 625 | 6.9594 | 0.006262 | 
 | 650 | 5.9157 | 0.005284 | 
 | 675 | 5.0515 | 0.004333 | 
 | 700 | 4.3334 | 0.003695 | 
 | 725 | 3.7326 | 0.003164 | 
 | 750 | 3.2274 | 0.002721 | 
 | 775 | 2.8006 | 0.002349 | 
 | 800 | 2.4383 | 0.002035 | 
 | 825 | 2.1296 | 0.001769 | 
 | 850 | 1.8655 | 0.001542 | 
 | 875 | 1.6387 | 0.001348 | 
 | 900 | 1.4433 | 0.001201 | 
 | 925 | 1.2743 | 0.001056 | 
 | 950 | 1.1276 | 0.0009304 | 
 | 975 | 1.0001 | 0.0008217 | 
 | 1000 | 0.88884 | 0.000727 | 
 | 1025 | 0.79159 | 0.0006451 | 
 | 1050 | 0.70629 | 0.0005733 | 
 | 1075 | 0.63127 | 0.0005104 | 
 | 1100 | 0.5652 | 0.0004548 | 
 | 1125 | 0.50692 | 0.0004064 | 
 | 1150 | 0.45541 | 0.0003591 | 
 | 1175 | 0.4097 | 0.000322 | 
 | 1200 | 0.36912 | 0.0002891 | 
 | 1225 | 0.33299 | 0.0002596 | 
 | 1250 | 0.30081 | 0.0002338 | 
 | 1275 | 0.27209 | 0.0002108 | 
 | 1300 | 0.24641 | 0.0001903 | 
 | 1325 | 0.22342 | 0.000172 | 
 | 1350 | 0.2028 | 0.0001557 | 
 | 1375 | 0.18428 | 0.0001411 | 
 | 1400 | 0.16763 | 0.0001279 | 
 | 1425 | 0.15263 | 0.0001161 | 
 | 1450 | 0.13911 | 0.0001057 | 
 | 1475 | 0.1269 | 9.618e-05 | 
 | 1500 | 0.11587 | 8.762e-05 | 
 | 1525 | 0.10589 | 7.988e-05 | 
 | 1550 | 0.096853 | 7.289e-05 | 
 | 1575 | 0.088656 | 6.658e-05 | 
 | 1600 | 0.081214 | 6.123e-05 | 
 | 1625 | 0.074457 | 5.586e-05 | 
 | 1650 | 0.068316 | 5.138e-05 | 
 | 1675 | 0.062723 | 4.704e-05 | 
 | 1700 | 0.057629 | 4.31e-05 | 
 | 1725 | 0.052983 | 3.952e-05 | 
 | 1750 | 0.048733 | 3.674e-05 | 
 | 1775 | 0.04487 | 3.33e-05 | 
 | 1800 | 0.041331 | 3.06e-05 | 
 | 1825 | 0.038092 | 2.813e-05 | 
 | 1850 | 0.035124 | 2.605e-05 | 
 | 1875 | 0.032409 | 2.397e-05 | 
 | 1900 | 0.02992 | 2.207e-05 | 
 | 1925 | 0.027637 | 2.032e-05 | 
 | 1950 | 0.025541 | 1.872e-05 | 
 | 1975 | 0.023615 | 1.727e-05 | 
 | 2000 | 0.021845 | 1.594e-05 | 



-- Main.BasilSchneider - 2018-11-14
This topic: LHCPhysics > WebHome > SUSYCrossSections > SUSYNLONNLLCrossSections27TeVHinoN2C1
Topic revision: r3 - 2019-01-23 - BasilSchneider
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