@article{a83df90166e444999897e5b5ef1aa0cb,
title = "Simulations of supercollider physics",
abstract = "The Standard Model of particle physics makes it possible to simulate complete events for physics signatures and their backgrounds in high-energy collisions. A knowledge of how the produced particles interact with the materials in a detector makes it possible to simulate the response of any particular detector design of these events and so determine whether the detector could observe the signal. The combination of these techniques has played an important role in the design of new detectors, particularly those for hadron supercolliders where the high rates and small signal cross sections make the experiments difficult. The technique is reviewed here and illustrated using the simulation of the GEM detector proposed for the Superconducting Super Collider. Although the simulations and results described here are somewhat detector-specific, we believe that they can serve as a useful model for this component of detector design for future hadron supercolliders.",
keywords = "GEM detector, Simulation, Standard model",
author = "Lane, {K. D.} and Paige, {F. E.} and T. Skwarnicki and Womersley, {W. J.}",
note = "Funding Information: The resultss ummarizedh ere representt he hard work of a large and dedicatedg roup of our GEM colleaguesM: elynda Brooks, Jim Brau, Rob Carey, Peter Dingus, Yuri Efremenko,Y uri Fisyak, Geoff Forden, Ray Frey, Mitch Golden, Yuri Kamyshkov,M ikhail Leltchouk,H ong Ma, Ken McFarlane, Shawn McKee, Roger McNeil, Geoff Mills, Mohammad Mohammadi, Steve Mrenna, Harvey Newman, Fred Olness, Sasha Savin, Irwin Sheer, Sergei Shevchenko, Xiaorong Shi, Mike Shupe, Kostya Shmakov, Liz Simmons,J enny Thomas, Henk Uijterwaal, SashaV anyashin,T orre Wenaus,D avid Worrick, Hiro Yamamoto, Chiaki Yanagisawa,Y anlin Ye, Bing Zhou, and Ren-yuan Zhu. We also acknowledget he contributionst o the experiment madeb y the whole GEM collaborationu ndert he leadershipo f the spokesmenB, arry Barish and Bill Willis. Finally, we would like to thank Holly Durden and the SSCL technicasl tafff or theirh elp in the preparationo f the GEM Technical Design Report, from which many of the plots presented herea re drawn. K.D.L. was supportedi n part by the US Departmento f Energy under Grant No. DE-FGOZ 91ER40676a nd by the Texas National ResearchL aboratory Commission under Grant Nos. RGFY91-B6, RGFY92-B6, and RGFY93-278. F.E.P. was supportedi n part by the US Department of Energy under Contract DE-AC02-76CH00016T. .S. was supportedi n part by the US Departmento f Energy under Contract DE-FG05-92ER40722T. .S. also thanks the Outstanding Junior Investigatorp rogram of DOE and the SSC Fellowship program of the Texas National ResearchL aboratoryC ommission.F ermilabi s operatedb y the UniversitiesR esearchA ssociation Inc. for the US Departmento f Energy.",
year = "1997",
month = jan,
doi = "10.1016/S0370-1573(96)00018-X",
language = "English (US)",
volume = "278",
pages = "291--371",
journal = "Physics Report",
issn = "0370-1573",
publisher = "Elsevier",
number = "5-6",
}