@article{863b53228ffa4d2691a5461f1978a880,
title = "Recommendations on presenting LHC searches for missing transverse energy signals using simplified s-channel models of dark matter",
abstract = "This document summarises the proposal of the LHC Dark Matter Working Group on how to present LHC results on s-channel simplified dark matter models and to compare them to direct (indirect) detection experiments.",
author = "Antonio Boveia and Oliver Buchmueller and Giorgio Busoni and Francesco D'Eramo and {De Roeck}, Albert and {De Simone}, Andrea and Caterina Doglioni and Dolan, {Matthew J.} and Genest, {Marie Helene} and Kristian Hahn and Ulrich Haisch and Harris, {Philip C.} and Jan Heisig and Valerio Ippolito and Felix Kahlhoefer and Khoze, {Valentin V.} and Suchita Kulkarni and Greg Landsberg and Steven Lowette and Sarah Malik and Michelangelo Mangano and Christopher McCabe and Stephen Mrenna and Priscilla Pani and {du Pree}, Tristan and Antonio Riotto and David Salek and Kai Schmidt-Hoberg and William Shepherd and Tait, {Tim M.P.} and Wang, {Lian Tao} and Steven Worm and Kathryn Zurek",
note = "Funding Information: This document is part of a project that has received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (grant agreement No 679305). The work of AB is partially supported by the Department of Energy Award DE-SC0011726. The work of OB is supported in part by the London Centre for Terauniverse Studies (LCTS), using funding from the European Research Council via the Advanced Investigator Grant 267352. UH acknowledges the hospitality and support of the CERN theory division. SK is supported by the New Frontiers program of the Austrian Academy of Sciences. The work of CM is part of the research programme of the Foundation for Fundamental Research on Matter (FOM), which is part of the Netherlands Organisation for Scientific Research (NWO). TMPT acknowledges support from National Science Foundation (NSF) grant PHY-1316792 and UCI through a Chancellor's Fellowship. Funding Information: This document is part of a project that has received funding from the European Research Council (ERC) under the European Union{\textquoteright}s Horizon 2020 research and innovation programme (grant agreement No 679305 ). The work of AB is partially supported by the Department of Energy Award DE-SC0011726 . The work of OB is supported in part by the London Centre for Terauniverse Studies (LCTS) , using funding from the European Research Council via the Advanced Investigator Grant 267352 . UH acknowledges the hospitality and support of the CERN theory division. SK is supported by the New Frontiers program of the Austrian Academy of Sciences . The work of CM is part of the research programme of the Foundation for Fundamental Research on Matter (FOM) , which is part of the Netherlands Organisation for Scientific Research (NWO) . TMPT acknowledges support from National Science Foundation (NSF) grant PHY-1316792 and UCI through a Chancellor{\textquoteright}s Fellowship. Publisher Copyright: {\textcopyright} 2019 The Authors",
year = "2020",
month = jan,
doi = "10.1016/j.dark.2019.100365",
language = "English (US)",
volume = "27",
journal = "Physics of the Dark Universe",
issn = "2212-6864",
publisher = "Elsevier BV",
}