Imperial College London


Faculty of Natural SciencesDepartment of Physics

Professor of Experimental Astrophysics



+44 (0)20 7594 7552t.sumner




1108Blackett LaboratorySouth Kensington Campus






BibTex format

author = {Abdallah, J and Araujo, H and Arbey, A and Ashkenazi, A and Belyaev, A and Berger, J and Boehm, C and Boveia, A and Brennan, A and Brooke, J and Buchmueller, O and Buckley, M and Busoni, G and Calibbi, L and Chauhan, S and Daci, N and Davies, G and De, Bruyn I and De, Jong P and De, Roeck A and de, Vries K and Del, Re D and De, Simone A and Di, Simone A and Doglioni, C and Dolan, M and Dreiner, HK and Ellis, J and Eno, S and Etzion, E and Fairbairn, M and Feldstein, B and Flaecher, H and Feng, E and Fox, P and Genest, M-H and Gouskos, L and Gramling, J and Haisch, U and Harnik, R and Hibbs, A and Hoh, S and Hopkins, W and Ippolito, V and Jacques, T and Kahlhoefer, F and Khoze, VV and Kirk, R and Korn, A and Kotov, K and Kunori, S and Landsberg, G and Liem, S and Lin, T and Lowette, S and Lucas, R and Malgeri, L and Malik, S and McCabe, C and Mete, AS and Morgante, E and Mrenna, S and Nakahama, Y and Newbold, D and Nordstrom, K and Pani, P and Papucci, M and Pataraia, S and Penning, B a},
doi = {10.1016/j.dark.2015.08.001},
journal = {Physics of the Dark Universe},
pages = {8--23},
title = {Simplified models for dark matter searches at the LHC},
url = {},
volume = {9-10},
year = {2015}

RIS format (EndNote, RefMan)

AB - This document a outlines a set of simplified models for dark matter and its interactions with Standard Model particles. It is intended to summarize the main characteristics that these simplified models have when applied to dark matter searches at the LHC, and to provide a number of useful expressions for reference. The list of models includes both s-channel and t-channel scenarios. For s-channel, spin-0 and spin-1 mediations are discussed, and also realizations where the Higgs particle provides a portal between the dark and visible sectors. The guiding principles underpinning the proposed simplified models are spelled out, and some suggestions for implementation are presented.
AU - Abdallah,J
AU - Araujo,H
AU - Arbey,A
AU - Ashkenazi,A
AU - Belyaev,A
AU - Berger,J
AU - Boehm,C
AU - Boveia,A
AU - Brennan,A
AU - Brooke,J
AU - Buchmueller,O
AU - Buckley,M
AU - Busoni,G
AU - Calibbi,L
AU - Chauhan,S
AU - Daci,N
AU - Davies,G
AU - De,Bruyn I
AU - De,Jong P
AU - De,Roeck A
AU - de,Vries K
AU - Del,Re D
AU - De,Simone A
AU - Di,Simone A
AU - Doglioni,C
AU - Dolan,M
AU - Dreiner,HK
AU - Ellis,J
AU - Eno,S
AU - Etzion,E
AU - Fairbairn,M
AU - Feldstein,B
AU - Flaecher,H
AU - Feng,E
AU - Fox,P
AU - Genest,M-H
AU - Gouskos,L
AU - Gramling,J
AU - Haisch,U
AU - Harnik,R
AU - Hibbs,A
AU - Hoh,S
AU - Hopkins,W
AU - Ippolito,V
AU - Jacques,T
AU - Kahlhoefer,F
AU - Khoze,VV
AU - Kirk,R
AU - Korn,A
AU - Kotov,K
AU - Kunori,S
AU - Landsberg,G
AU - Liem,S
AU - Lin,T
AU - Lowette,S
AU - Lucas,R
AU - Malgeri,L
AU - Malik,S
AU - McCabe,C
AU - Mete,AS
AU - Morgante,E
AU - Mrenna,S
AU - Nakahama,Y
AU - Newbold,D
AU - Nordstrom,K
AU - Pani,P
AU - Papucci,M
AU - Pataraia,S
AU - Penning,B
AU - Pinna,D
AU - Polesello,G
AU - Racco,D
AU - Re,E
AU - Riotto,AW
AU - Rizzo,T
AU - Salek,D
AU - Sarkar,S
AU - Schramm,S
AU - Skubic,P
AU - Slone,O
AU - Smirnov,J
AU - Soreq,Y
AU - Sumner,T
AU - Tait,TMP
AU - Thomas,M
AU - Tomalin,I
AU - Tunnell,C
AU - Vichi,A
AU - Volansky,T
AU - Weiner,N
AU - West,SM
AU - Wielers,M
AU - Worm,S
AU - Yavin,I
AU - Zaldivar,B
AU - Zhou,N
AU - Zurek,K
DO - 10.1016/j.dark.2015.08.001
EP - 23
PY - 2015///
SN - 2212-6864
SP - 8
TI - Simplified models for dark matter searches at the LHC
T2 - Physics of the Dark Universe
UR -
UR -
VL - 9-10
ER -