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@article{Khachatryan:2017:10.1103/PhysRevD.95.012003,
author = {Khachatryan, V and Sirunyan, AM and Tumasyan, A and Adam, W and Asilar, E and Bergauer, T and Brandstetter, J and Brondolin, E and Dragicevic, M and Eroe, J and Flechl, M and Friedl, M and Fruehwirth, R and Ghete, VM and Hartl, C and Hoermann, N and Hrubec, J and Jeitler, M and Koenig, A and Kraetschmer, I and Liko, D and Matsushita, T and Mikulec, I and Rabady, D and Rad, N and Rahbaran, B and Rohringer, H and Schieck, J and Strauss, J and Treberer-Treberspurg, W and Waltenberger, W and Wulz, C-E and Mossolov, V and Shumeiko, N and Gonzalez, JS and Alderweireldt, S and De, Wolf EA and Janssen, X and Lauwers, J and Van, De Klundert M and Van, Haevermaet H and Van, Mechelen P and Van, Remortel N and Van, Spilbeeck A and Abu, Zeid S and Blekman, F and D'Hondt, J and Daci, N and De, Bruyn I and Deroover, K and Heracleous, N and Lowette, S and Moortgat, S and Moreels, L and Olbrechts, A and Python, Q and Tavernier, S and Van, Doninck W and Van, Mulders P and Van, Parijs I and Brun, H and C},
doi = {10.1103/PhysRevD.95.012003},
journal = {Physical Review D},
title = {Inclusive search for supersymmetry using razor variables in pp collisions at root s=13 TeV},
url = {http://dx.doi.org/10.1103/PhysRevD.95.012003},
volume = {95},
year = {2017}
}

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TY  - JOUR
AB  - An inclusive search for supersymmetry using razor variables is performed in events with four or more jets and no more than one lepton. The results are based on a sample of proton-proton collisions corresponding to an integrated luminosity of 2.3  fb−1 collected with the CMS experiment at a center-of-mass energy of √s=13  TeV. No significant excess over the background prediction is observed in data, and 95% confidence level exclusion limits are placed on the masses of new heavy particles in a variety of simplified models. Assuming that pair-produced gluinos decay only via three-body processes involving third-generation quarks plus a neutralino, and that the neutralino is the lightest supersymmetric particle with a mass of 200 GeV, gluino masses below 1.6 TeV are excluded for any branching fractions for the individual gluino decay modes. For some specific decay mode scenarios, gluino masses up to 1.65 TeV are excluded. For decays to first- and second-generation quarks and a neutralino with a mass of 200 GeV, gluinos with masses up to 1.4 TeV are excluded. Pair production of top squarks decaying to a top quark and a neutralino with a mass of 100 GeV is excluded for top squark masses up to 750 GeV.
AU  - Khachatryan,V
AU  - Sirunyan,AM
AU  - Tumasyan,A
AU  - Adam,W
AU  - Asilar,E
AU  - Bergauer,T
AU  - Brandstetter,J
AU  - Brondolin,E
AU  - Dragicevic,M
AU  - Eroe,J
AU  - Flechl,M
AU  - Friedl,M
AU  - Fruehwirth,R
AU  - Ghete,VM
AU  - Hartl,C
AU  - Hoermann,N
AU  - Hrubec,J
AU  - Jeitler,M
AU  - Koenig,A
AU  - Kraetschmer,I
AU  - Liko,D
AU  - Matsushita,T
AU  - Mikulec,I
AU  - Rabady,D
AU  - Rad,N
AU  - Rahbaran,B
AU  - Rohringer,H
AU  - Schieck,J
AU  - Strauss,J
AU  - Treberer-Treberspurg,W
AU  - Waltenberger,W
AU  - Wulz,C-E
AU  - Mossolov,V
AU  - Shumeiko,N
AU  - Gonzalez,JS
AU  - Alderweireldt,S
AU  - De,Wolf EA
AU  - Janssen,X
AU  - Lauwers,J
AU  - Van,De Klundert M
AU  - Van,Haevermaet H
AU  - Van,Mechelen P
AU  - Van,Remortel N
AU  - Van,Spilbeeck A
AU  - Abu,Zeid S
AU  - Blekman,F
AU  - D'Hondt,J
AU  - Daci,N
AU  - De,Bruyn I
AU  - Deroover,K
AU  - Heracleous,N
AU  - Lowette,S
AU  - Moortgat,S
AU  - Moreels,L
AU  - Olbrechts,A
AU  - Python,Q
AU  - Tavernier,S
AU  - Van,Doninck W
AU  - Van,Mulders P
AU  - Van,Parijs I
AU  - Brun,H
AU  - Caillol,C
AU  - Clerbaux,B
AU  - De,Lentdecker G
AU  - Delannoy,H
AU  - Fasanella,G
AU  - Favart,L
AU  - Goldouzian,R
AU  - Grebenyuk,A
AU  - Karapostoli,G
AU  - Lenzi,T
AU  - Leonard,A
AU  - Luetic,J
AU  - Maerschalk,T
AU  - Marinov,A
AU  - Randle-conde,A
AU  - Seva,T
AU  - Vander,Velde C
AU  - Vanlaer,P
AU  - Yonamine,R
AU  - Zenoni,F
AU  - Zhang,F
AU  - Cimmino,A
AU  - Cornelis,T
AU  - Dobur,D
AU  - Fagot,A
AU  - Garcia,G
AU  - Gul,M
AU  - Poyraz,D
AU  - Salva,S
AU  - Schofbeck,R
AU  - Tytgat,M
AU  - Van,Driessche W
AU  - Yazgan,E
AU  - Zaganidis,N
AU  - Bakhshiansohi,H
AU  - Beluffi,C
AU  - Bondu,O
AU  - Brochet,S
AU  - Bruno,G
AU  - Caudron,A
AU  - De,Visscher S
AU  - Delaere,C
AU  - Delcourt,M
AU  - Francois,B
AU  - Giammanco,A
AU  - Jafari,A
AU  - Jez,P
AU  - Komm,M
AU  - Lemaitre,V
AU  - Magitteri,A
AU  - Mertens,A
AU  - Musich,M
AU  - Nuttens,C
AU  - Piotrzkowski,K
AU  - Quertenmont,L
AU  - Selvaggi,M
AU  - Marono,MV
AU  - Wertz,S
AU  - Beliy,N
AU  - Alda,Junior WL
AU  - Alves,FL
AU  - Alves,GA
AU  - Brito,L
AU  - Hensel,C
AU  - Moraes,A
AU  - Pol,ME
AU  - Rebello,Teles P
AU  - Belchior,Batista Das Chagas E
AU  - Carvalho,W
AU  - Chinellato,J
AU  - Custodio,A
AU  - Da,Costa EM
AU  - Da,Silveira GG
AU  - De,Jesus Damiao D
AU  - De,Oliveira Martins C
AU  - Fonseca,De Souza S
AU  - Huertas,Guativa LM
AU  - Malbouisson,H
AU  - Matos,Figueiredo D
AU  - Mora,Herrera C
AU  - Mundim,L
AU  - Nogima,H
AU  - Prado,Da Silva WL
AU  - Santoro,A
AU  - Sznajder,A
AU  - Tonelli,Manganote EJ
AU  - Vilela,Pereira A
AU  - Ahuja,S
AU  - Bernardes,CA
AU  - Dogra,S
AU  - Fernandez,Perez Tomei TR
AU  - Gregores,EM
AU  - Mercadante,PG
AU  - Moon,CS
AU  - Novaes,SF
AU  - Padula,SS
AU  - Abad,DR
AU  - Ruiz,Vargas JC A
DO  - 10.1103/PhysRevD.95.012003
PY  - 2017///
SN  - 1550-7998
TI  - Inclusive search for supersymmetry using razor variables in pp collisions at root s=13 TeV
T2  - Physical Review D
UR  - http://dx.doi.org/10.1103/PhysRevD.95.012003
UR  - http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000391314300001&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
UR  - http://hdl.handle.net/10044/1/44989
VL  - 95
ER  -

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