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Published March 2010 | Submitted
Journal Article Open

Hunt for New Physics at the Large Hadron Collider

Abstract

The Large Hadron Collider presents an unprecedented opportunity to probe the realm of new physics in the TeV region and shed light on some of the core unresolved issues of particle physics. These include the nature of electroweak symmetry breaking, the origin of mass, the possible constituent of cold dark matter, new sources of CP violation needed to explain the baryon excess in the universe, the possible existence of extra gauge groups and extra matter, and importantly the path Nature chooses to resolve the hierarchy problem – is it supersymmetry or extra dimensions. Many models of new physics beyond the standard model contain a hidden sector which can be probed at the LHC. Additionally, the LHC will be a top factory and accurate measurements of the properties of the top and its rare decays will provide a window to new physics. Further, the LHC could shed light on the origin of neutralino masses if the new physics associated with their generation lies in the TeV region. Finally, the LHC is also a laboratory to test the hypothesis of TeV scale strings and D brane models. An overview of these possibilities is presented in the spirit that it will serve as a companion to the Technical Design Reports (TDRs) by the particle detector groups ATLAS and CMS to facilitate the test of the new theoretical ideas at the LHC. Which of these ideas stands the test of the LHC data will govern the course of particle physics in the subsequent decades.

Additional Information

© 2010 Elsevier B.V. Published by Elsevier B.V. Available online 5 May 2010. Fermilab is operated by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the United States Department of Energy. H.D. was supported by the US Department of Energy under Grant Contract DE-AC02-98CH10886. B.D. was supported in part by the DOE grant DE-FG02-95ER40917 and would like to thank his collaborators Richard Arnowitt, Adam Arusano, Rouzbeh Allahverdi, Alfredo Gurrola, Teruki Kamon, Nikolay Kolev, Abram Krislock, Anupam Mazumdar, Yukihiro Mimura and Dave Toback for the works related to this review. D.F. is supported in part by DOE grant DEFG92-95ER40899. H.G. is supported in part by NSF grant PHY-0757959 K.K. was supported by US Department of Energy contract DE-AC02-76SF00515. P.L. was supported by NSF grant PHY-0503584 and by the IBM Einstein Fellowship. G.L. is partially supported by the U.S. Department of Energy under Grant No. DE-FG02-91ER40688. Z.L. is supported in part by NSF grant PHY-0653342 P.N. is supported in part by NSF grant PHY-0757959. SUSY09 and Pre-SUSY09 were supported by NSF PHY-0834022 and de-sc0001075. B.D.N. was supported by National Science Foundation Grant PHY-0653587. E.P. was supported by the U.S. Department of Energy under contract DE-FG02-92ER-40699. J.S. is funded by MICINN and projects FPA2006-05294, FQM101, FQM437 and FQM03048. T.T. is supported in part by NSF grant PHY-0757959. X.T. thanks the UW IceCube Group for making his visit to Wisconsin, where this report was prepared, possible. This research was supported in part by the United States Department of Energy. Work of J.F.W.V. supported by the US National Science Foundation under grant No. PHY-0652363, by European Union ITN UNILHC (PITN-GA-2009-237920), by the Consolider Multidark project CSD2009-00064 (MICIIN), by the FPA2008-00319/FPA grant (MICIIN), by the PROMETEO/2009/091 grant (Generalitat Valenciana), by German Ministry of Education and Research (BMBF) contract 05HT6WWA, and by Colombian grant UdeA Sostenibilidad 2009-2010. C.E.M.W.'s work at ANL is supported in part by the U.S. Department of Energy (DOE), Div. of HEP, Contract DE-AC02-06CH11357.

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Created:
August 19, 2023
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October 20, 2023