\begin{document}$\rm fb^{-1}$\end{document}, the 5 σ discovery prospect of \begin{document}$3l+ {jets} + {{\not {E_T}}}$\end{document} for \begin{document}$M_{\tilde{g}}=1.8$\end{document} TeV in the wino type model is promising. The study also presents various other models that may emerge at the early stage of LHC RUN-III. Wino type models in the scenario where left squarks are light and right squarks are heavy exhibit the best prospect of discovering gluinos in multi-lepton channels in the LHC RUN-III experiment. The findings of this study provide crucial insights into the potential discovery of gluinos in multi-lepton channels."> Prospects of gluino searches in multi-lepton channels in light of the ongoing LHC RUN-III -
  • [1]

    H. P. Nilles, Phys. Rept.110, 1 (1984)

  • [2]

    J. Bagger and J. Wess,Supersymmetry and Supergravity: Revised Ed, Princeton University Press Mar 23, 1992

  • [3]

    J. D. Lykken,Introduction to supersymmetry,inTheoretical Advanced Study Institute in Elementary Particle Physics (TASI 96): Fields, Strings, and Duality 1996, arXiv:hep-th/9612114

  • [4]

    S. P. Martin, Adv. Ser. Direct. High Energy Phys.18, 1 (1998), arXiv:hep-ph/9709356

  • [5]

    D. J. H. Chung, L. L. Everett, G. L. Kaneeet al., Phys. Rept.407, 1 (2005), arXiv:hep-ph/0312378

  • [6]

    M. Drees, R. Godbole, and P. Roy,Theory And Phenomenology Of Sparticles: An Account Of Four-dimensional N=1 Supersymmetry In High Energy Physics, (World Scientific Publishing Company 2005)

  • [7]

    P. Fayet, Nucl. Phys. B90, 104 (1975)

  • [8]

    P. Fayet,Introduction to Supersymmetry and Its Applications to Particle Interactions,inFundamentals of Microprocessing, 1977

  • [9]

    P. Fayet, Phys. Lett. B78, 417 (1978)

  • [10]

    P. Fayet, Stud. Nat. Sci.14, 413 (1978)

  • [11]

    H. Baer and X. Tata,Weak scale supersymmetry: From superfields to scattering events, (Cambridge University Press 2006)

  • [12]

    E. Gildener and S. Weinberg, Phys. Rev. D13, 3333 (1976)

  • [13]

    E. Gildener, Phys. Rev. D14, 1667 (1976)

  • [14]

    E. Witten, Nucl. Phys. B188, 513 (1981)

  • [15]

    S. Dimopoulos and H. Georgi, Phys. Lett. B117, 287 (1982)

  • [16]

    S. Dimopoulos and G. F. Giudice, Phys. Lett. B357, 573 (1995), arXiv:hep-ph/9507282

  • [17]

    N. Arkani-Hamed, S. Dimopoulos, and G. R. Dvali, Phys. Lett. B429, 263 (1998), arXiv:hep-ph/9803315

  • [18]

    J. R. Ellis, S. Kelley, and D. V. Nanopoulos, Phys. Lett. B260, 131 (1991)

  • [19]

    U. Amaldi, W. de Boer, and H. Furstenau, Phys. Lett. B260, 447 (1991)

  • [20]

    G. Jungman, M. Kamionkowski and K. Griest, Phys. Rept.267, 195 (1996), arXiv:hep-ph/9506380

  • [21]

    A. B. Lahanas, N. E. Mavromatos, and D. V. Nanopoulos, Int. J. Mod. Phys. D12, 1529 (2003), arXiv:hep-ph/0308251

  • [22]

    W. L. Freedman and M. S. Turner, Rev. Mod. Phys.75, 1433 (2003), arXiv:astro-ph/0308418

  • [23]

    L. Roszkowski, Pramana62, 389 (2004), arXiv:hep-ph/0404052

  • [24]

    G. Bertone, D. Hooper, and J. Silk, Phys. Rept.405, 279 (2005), arXiv:hep-ph/0404175

  • [25]

    K. A. Olive,TASI lectures on astroparticle physics,inTheoretical Advanced Study Institute in Elementary Particle Physics: Physics inD \begin{document}$\geqq$\end{document} 4 2005, arXiv:astro-ph/0503065

  • [26]

    H. Baer and X. Tata,Dark matter and the LHC 2009, arXiv:0805.1905[hep-ph]

  • [27]

    M. Drees and G. Gerbier,Mini-Review of Dark Matter: 2012, arXiv:1204.2373[hep-ph]

  • [28]

    S. Arrenberget al., Working Group Report: Dark Matter Complementarity,inCommunity Summer Study 2013: Snowmass on the Mississippi 2013, arXiv:1310.8621[hep-ph]

  • [29]

    T Javurek,et al. (ATLAS Collaboration), J. Phys. G Nucl. Partic.273-275, 2418 (2016)

  • [30]

    Aad Georges, Abbott B, Abdallah J,et al., J. High Energy Phys.2014(10), 1 (2014)

  • [31]

    Aad Georges, Abbott Brad, Abdallah Jalal,et al., J. High Energy Phys.2015(4), 1 (2015)

  • [32]

    Aad Georgeset al. (ATLAS), JHEP6, 035 (2014)

  • [33]

    G. Aadet al. (ATLAS),JHEP10, 130 (2013)[Erratum:JHEP01, 109 (2014)], arXiv:1308.1841[hep-ex]

  • [34]

    Aad Georgeset al. (ATLAS), JHEP09, 103 (2014)

  • [35]

    Khachatryan Vardanet al.(CMS), Phys. Rev. D91, 052018 (2015)

  • [36]

    G. Aadet al. (ATLAS), Phys. Rev. D94(3), 032003 (2016), arXiv:1605.09318[hep-ex

  • [37]

    G. Aadet al. (ATLAS), Eur. Phys. J. C76(10), 565 (2016), arXiv:1605.04285[hep-ex

  • [38]

    M. Aaboudet al. (ATLAS), Eur. Phys. J. C76(7), 392 (2016), arXiv:1605.03814[hep-ex

  • [39]

    G. Aadet al. (ATLAS), Eur. Phys. J. C76(5), 259 (2016), arXiv:1602.09058[hep-ex

  • [40]

    M. Aaboudet al. (ATLAS), Phys. Rev. D96(11), 112010 (2017), arXiv:1708.08232[hep-ex

  • [41]

    M. Aaboudet al. (ATLAS), JHEP12, 085 (2017), arXiv:1709.04183[hep-ex

  • [42]

    M. Aaboudet al. (ATLAS), JHEP09, 084 (2017), arXiv:1706.03731[hep-ex

  • [43]

    M. Aaboudet al. (ATLAS), Phys. Rev. D97(11), 112001 (2018), arXiv:1712.02332[hep-ex

  • [44]

    M. Aaboudet al. (ATLAS), JHEP06, 107 (2018), arXiv:1711.01901[hep-ex

  • [45]

    M. Aaboudet al. (ATLAS), Eur. Phys. J. C78(8), 625 (2018), arXiv:1805.11381[hep-ex

  • [46]

    M. Aaboudet al. (ATLAS), Phys. Rev. D99(1), 012009 (2019), arXiv:1808.06358[hep-ex

  • [47]

    G. Aadet al. (ATLAS), JHEP06, 046 (2020), arXiv:1909.08457[hep-ex

  • [48]

    G. Aadet al. (ATLAS), JHEP10, 062 (2020), arXiv:2008.06032[hep-ex

  • [49]

    G. Aadet al. (ATLAS),Search for new phenomena in events with an energetic jet and missing transverse momentum in \begin{document}$pp$\end{document} collisions at \begin{document}$\sqrt s = 13$\end{document} TeV with the ATLAS detector, arXiv:2102.10874[hep-ex]

  • [50]

    G. Aadet al. (ATLAS),Search for new phenomena in final states withb-jets and missing transverse momentum in \begin{document}$\sqrt s =13$\end{document} TeV \begin{document}$pp$\end{document} collisions with the ATLAS detector, arXiv:2101.12527[hep-ex]

  • [51]

    P. Fayet, Phys. Lett. B69, 489 (1977)

  • [52]

    K. Inoue, A. Kakuto, H. Komatsuet al., Prog. Theor. Phys.71, 413 (1984)

  • [53]

    L. E. Ibanez and C. Lopez, Nucl. Phys. B233, 511 (1984)

  • [54]

    G. Aadet al. (ATLAS), JHEP02, 143 (2021), arXiv:2010.14293[hep-ex

  • [55]

    G. Aadet al. (ATLAS),Search for squarks and gluinos in final states with one isolated lepton, jets, and missing transverse momentum at \begin{document}$\sqrt s =13$\end{document} TeVwith the ATLAS detector, arXiv:2101.01629[hep-ex]

  • [56]

    Searches for new phenomena in events with two leptons, jets, and missing transverse momentum in \begin{document}$139 \text{fb}^{-1}$\end{document} of \begin{document}$\sqrt s =13 $\end{document} TeV \begin{document}$pp$\end{document} collisions with the ATLAS detector, arXiv:2204.13072[hep-ex]

  • [57]

    A. Mukherjee, S. Niyogi, and S. Poddar,Revisiting the gluino mass limits in the pMSSM in the light of the latest LHC data and Dark Matter constraints, arXiv:2201.02531[hep-ph]

  • [58]

    T. J. LeCompte and S. P. Martin, Phys. Rev. D85, 035023 (2012), arXiv:1111.6897[hep-ph

  • [59]

    H. K. Dreiner, M. Kramer, and J. Tattersall, EPL99(6), 61001 (2012), arXiv:1207.1613[hep-ph

  • [60]

    B. Bhattacherjee and K. Ghosh,Degenerate SUSY search at the 8 TeV LHC, arXiv:1207.6289[hep-ph]

  • [61]

    B. Bhattacherjee, A. Choudhury, K. Ghoshet al., Phys. Rev. D89(3), 037702 (2014), arXiv:1308.1526[hep-ph

  • [62]

    T. Cohen, T. Golling, M. Hanceet al., JHEP04, 117 (2014), arXiv:1311.6480[hep-ph

  • [63]

    S. Mukhopadhyay, M. M. Nojiri, and T. T. Yanagida, JHEP10, 012 (2014), arXiv:1403.6028[hep-ph

  • [64]

    M. Low and L.-T. Wang, JHEP08, 161 (2014), arXiv:1404.0682[hep-ph

  • [65]

    M. Chakraborti, A. Datta, N. Gangulyet al., JHEP11, 117 (2017), arXiv:1707.04410[hep-ph

  • [66]

    M. Chakraborti, U. Chattopadhyay, A. Choudhuryet al., JHEP07, 019 (2014), arXiv:1404.4841[hep-ph

  • [67]

    M. Chakraborti, U. Chattopadhyay, A. Choudhuryet al., JHEP11, 050 (2015), arXiv:1507.01395[hep-ph

  • [68]

    A. Datta, N. Ganguly, and S. Poddar, Phys. Lett. B763, 213 (2016), arXiv:1606.04391[hep-ph

  • [69]

    A. Datta and N. Ganguly, JHEP01, 103 (2019), arXiv:1809.05129[hep-ph

  • [70]

    W. Adam and I. Vivarelli, Int. J. Mod. Phys. A37(2), 2130022 (2022), arXiv:2111.10180[hep-ex

  • [71]

    G. Aadet al. (ATLAS), JHEP05, 071 (2014), arXiv:1403.5294[hep-ex

  • [72]

    G. Aadet al. (ATLAS), JHEP04, 169 (2014), arXiv:1402.7029[hep-ex

  • [73]

    G. Aadet al. (ATLAS), JHEP10, 096 (2014), arXiv:1407.0350[hep-ex

  • [74]

    G. Aadet al. (ATLAS), Eur. Phys. J. C75(5), 208 (2015), arXiv:1501.07110[hep-ex

  • [75]

    D. Sabatta, A. S. Cornell, A. Goyalet al., Chin. Phys. C44(6), 063103 (2020), arXiv:1909.03969[hep-ph

  • [76]

    S. Buddenbrock, A. S. Cornell, Y. Fanget al., JHEP10, 157 (2019), arXiv:1901.05300[hep-ph

  • [77]

    Y. Hernandez, M. Kumar, A. S. Cornellet al., Eur. Phys. J. C81[4], 365 (2021), arXiv:1912.00699[hep-ph

  • [78]

    H. Baer, V. D. Barger, D. Karataset al., Phys. Rev. D36, 96 (1987)

  • [79]

    R. M. Barnett, J. F. Gunion, and H. E. Haber, Phys. Rev. D37, 1892 (1988)

  • [80]

    H. Baer, C.-h. Chen, F. Paigeet al., Phys. Rev. D53, 6241 (1996), arXiv:hep-ph/9512383

  • [81]

    H. Baer, C. Balazs, A. Belyaevet al., JHEP06, 054 (2003), arXiv:hep-ph/0304303

  • [82]

    N. Sakai, Z. Phys. C11, 153 (1981)

  • [83]

    R. K. Kaul and P. Majumdar, Nucl. Phys. B199, 36 (1982)

  • [84]

    R. Barbieri and G. F. Giudice, Nucl. Phys. B306, 63 (1988)

  • [85]

    J. L. Feng, K. T. Matchev, and T. Moroi, Phys. Rev. Lett.84, 2322 (2000), arXiv:hep-ph/9908309

  • [86]

    N. Arkani-Hamed, A. Delgado, and G. F. Giudice, Nucl. Phys. B741, 108 (2006), arXiv:hep-ph/0601041

  • [87]

    P. Athronet al. (GAMBIT), Eur. Phys. J. C79(5), 395 (2019), arXiv:1809.02097[hep-ph

  • [88]

    Y. Huang, G. E. Addison, J. L. Weilandet al., Astrophys. J.869(1), 38 (2018), arXiv:1804.05428[astro-ph.CO

  • [89]

    N. Aghanimet al. (Planck),Planck 2018 results. VI. Cosmological parameters,Astron. Astrophys.641, A6 (2020)[Erratum:Astron.Astrophys.652, C4 (2021)], arXiv:1807.06209[astro-ph.CO]

  • [90]

    M. Chakraborti, S. Heinemeyer, and I. Saha, Eur. Phys. J. C81(12), 1114 (2021), arXiv:2104.03287[hep-ph

  • [91]

    M. Chakraborti, S. Heinemeyer, and I. Saha, Moscow Univ. Phys. Bull.77(2), 116 (2022), arXiv:2201.03390[hep-ph

  • [92]

    M. Chakraborti, S. Iwamoto, J. S. Kimet al., JHEP08, 124 (2022), arXiv:2202.12928[hep-ph

  • [93]

    M. Chakraborti, S. Heinemeyer, and I. Saha, Int. J. Mod. Phys. A37(30), 2246010 (2022)

  • [94]

    B. Abiet al. (Muon g-2), Phys. Rev. Lett.126(14), 141801 (2021), arXiv:2104.03281[hep-ex

  • [95]

    D. A. Kosower, L. M. Krauss, and N. Sakai, Phys. Lett. B133, 305 (1983)

  • [96]

    T. C. Yuan, R. L. Arnowitt, A. H. Chamseddineet al., Z. Phys. C26, 407 (1984)

  • [97]

    G. Aadet al. (ATLAS), Eur. Phys. J. C80(2), 123 (2020), arXiv:1908.08215[hep-ex

  • [98]

    G. Aadet al. (ATLAS), Eur. Phys. J. C81(12), 1118 (2021), arXiv:2106.01676[hep-ex

  • [99]

    G. Aadet al. (ATLAS), Phys. Lett. B716, 1 (2012), arXiv:1207.7214[hep-ex

  • [100]

    S. Chatrchyanet al. (CMS), Phys. Lett. B716, 30 (2012), arXiv:1207.7235[hep-ex

  • [101]

    G. Degrassi, S. Heinemeyer, W. Holliket al., Eur. Phys. J. C28, 133 (2003), arXiv:hep-ph/0212020

  • [102]

    B. C. Allanach, A. Djouadi, J. L. Kneuret al., JHEP09, 044 (2004), arXiv:hep-ph/0406166

  • [103]

    K. C. Wonget al., Mon. Not. Roy. Astron. Soc.498(1), 1420 (2020), arXiv:1907.04869[astro-ph.CO

  • [104]

    A. Djouadi, M. Muhlleitner, and M. Spira, Acta Phys. Polon. B38, 635 (2007), arXiv:hep-ph/0609292

  • [105]

    G. Belanger, A. Mjallal, and A. Pukhov, Eur. Phys. J. C81(3), 239 (2021), arXiv:2003.08621[hep-ph

  • [106]

    J. Alwall, R. Frederix, S. Frixioneet al., JHEP07, 079 (2014), arXiv:1405.0301[hep-ph

  • [107]

    R. D. Ballet al., Nucl. Phys. B867, 244 (2013), arXiv:1207.1303[hep-ph

  • [108]

    T. Plehn, Czech. J. Phys.55, B213 (2005), arXiv:hep-ph/0410063

  • [109]

    T. Sjöstrand, S. Ask, J. R. Christiansenet al., Comput. Phys. Commun.191, 159 (2015), arXiv:1410.3012[hep-ph

  • [110]

    J. de Favereau, C. Delaere, P. Deminet al., JHEP02, 057 (2014), arXiv:1307.6346[hep-ex

  • [111]

    M. Cacciari, G. P. Salam, and G. Soyez, Eur. Phys. J. C72, 1896 (2012), arXiv:1111.6097[hep-ph

  • [112]

    H. Voss, A. Hocker, J. Stelzeret al., PoSACAT, 040 (2007)

  • [113]

    I. Antchevaet al., Comput. Phys. Commun.180, 2499 (2009), arXiv:1508.07749[physics.data-an

  • [114]

    G. Cowan, K. Cranmer, E. Grosset al., Eur. Phys. J. C71, 1554 (2011), arXiv:1007.1727[physics.data-an

  • [115]

    R. D. Cousins, J. T. Linnemann, and J. Tucker, Nucl. Instrum. Meth. A595(2), 480 (2008), arXiv:physics/0702156

  • [116]

    T. P. Li and Y. Q. Ma, Astrophys. J.272, 317 (1983)

  • [117]

    H. Baer, X. Tata, and J. Woodside, Phys. Rev. D45, 142 (1992)

  • [118]

    M. Guchait and D. P. Roy, Phys. Rev. D52, 133 (1995), arXiv:hep-ph/9412329

  • [119]

    A. Bartl, W. Porod, F. de Camposet al., Nucl. Phys. B502, 19 (1997), arXiv:hep-ph/9612436

  • [120]

    A. A. Sokolov, T. Lindblad, C. S. Lindseyet al., Nucl. Instrum. Meth. A416, 391 (1998)

  • [121]

    A. Alves, O. Eboli, and T. Plehn, Phys. Rev. D74, 095010 (2006), arXiv:hep-ph/0605067

  • [122]

    Y. G. Kim, Soryushiron Kenkyu Electron.116, A77 (2008)

  • [123]

    H. Baer, H. Prosper and H. Summy, Phys. Rev. D77, 055017 (2008), arXiv:0801.3799[hep-ph

  • [124]

    H. Baer, A. Lessa, and H. Summy, Phys. Lett. B674, 49 (2009), arXiv:0809.4719[hep-ph

  • [125]

    B. S. Acharya, P. Grajek, G. L. Kaneet al.,Identifying Multi-Top Events from Gluino Decay at the LHC, arXiv:0901.3367[hep-ph]

  • [126]

    Y. M. Andreev, N. V. Krasnikov, and A. N. Toropin, Mod. Phys. Lett. A24, 1317 (2009), arXiv:0902.0502[hep-ph

  • [127]

    E. Turlay, R. Lafaye, T. Plehnet al., J. Phys. G38, 035003 (2011), arXiv:1011.0759[hep-ph

  • [128]

    J. Reuter and D. Wiesler, Eur. Phys. J. C73(3), 2355 (2013), arXiv:1212.5559[hep-ph

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