| Preprint | |
| Report number | hep-ph/0003154 ; FERMILAB-PUB-00-386-T |
| Title | Report of the SUGRA Working Group for Run II of the Tevatron |
| Related title | Supergravity |
| Author(s) |
Barger, V. (Wisconsin U., Madison) ; Kamon, T. (Texas A-M) ; Flattum, E. (Fermilab) ; Falk, T. (Wisconsin U., Madison) ; Abel, S. (CERN) ; Accomando, E. (Texas A-M) ; Anderson, G. (Northwestern U.) ; Arnowitt, R. (Texas A-M) ; Azzi, P. (INFN, Padua) ; Baer, H. (Florida State U.) ; Bagger, J. (Johns Hopkins U.) ; Beenakker, W. (Durham U.) ; Belyaev, A. (Sao Paulo, IFT) ; Berger, E. (Argonne) ; Berger, M. (Indiana U.) ; Brhlik, M. (Michigan U.) ; Blazek, T. (Hawaii U.) ; Blessing, S. (Florida State U.) ; Bokhari, W. (Pennsylvania U.) ; Bruner, N. (New Mexico U.) ; Carena, M. (Fermilab) ; Chakraborty, D. (SUNY, Stony Brook) ; Chang, D. (Taiwan, Natl. Tsing Hua U.) ; Chankowski, P. (Warsaw U.) ; Chen, C.H. (UC, Davis) ; Cheng, H.C. (Fermilab) ; Chertok, M. (Texas A-M) ; Cho, G.C. (KEK, Tsukuba) ; Claes, D. (Nebraska U., Omaha) ; Demina, R. (Fermilab) ; Done, J. (Texas A-M) ; Duflot, L. (Orsay, LAL) ; Dutta, Bhaskar (Texas A-M) ; Eboli, O.J.P. (Sao Paulo, IFT ; Wisconsin U., Madison) ; Eno, S. (Maryland U.) ; Feng, J. (LBL, Berkeley) ; Ganis, G. (Munich, Max Planck Inst.) ; Gold, M. (New Mexico U.) ; Gregores, E.M. (Wisconsin U., Madison) ; Hagiwara, K. (KEK, Tsukuba) ; Han, T. (Wisconsin U., Madison) ; Harris, B. (Florida State U.) ; Hikasa, K. (Tohoku U.) ; Holck, C. (Pennsylvania U.) ; Kao, C. (Wisconsin U., Madison) ; Kato, Y. (Osaka City U.) ; Klasen, M. (Argonne) ; Keung, W.Y. (Illinois U., Chicago) ; Kramer, M. (CERN) ; Lammel, S. (Fermilab) ; Li, T.J. (Wisconsin U., Madison) ; Lykken, J.D. (Fermilab) ; Magro, M. (Wisconsin U., Madison) ; Mani, S. (UC, Davis) ; Matchev, K.T. (Fermilab) ; Mangano, M. (CERN) ; Mercadante, P. (Hawaii U.) ; Mrenna, S. (Argonne) ; Nachtman, J. (UCLA) ; Nath, P. (Northeastern U.) ; Nojiri, M.M. (Kyoto U.) ; Nomerotski, A. (Florida U.) ; Norman, D. (Texas A-M) ; Oishi, R. (Tsukuba U.) ; Ono, K. (Tokyo U.) ; Paige, F. (Brookhaven) ; Paterno, M. (Fermilab) ; Parke, S. (Fermilab) ; Pierce, D. (Johns Hopkins U.) ; Pilaftsis, A. (CERN) ; Plehn, T. (Wisconsin U., Madison) ; Pompos, A. (Purdue U.) ; Polonksy, N. (Rutgers U., Piscataway) ; Pokorski, S. (Warsaw U.) ; Quintana, P. (Florida State U.) ; Roco, M. (Fermilab) ; Saltzberg, D. (UCLA) ; Savoy-Navarro, A. (Paris, LPTHE) ; Seiya, Y. (Tsukuba U.) ; Smith, C. (Johns Hopkins U.) ; Spira, M. (Hamburg U., Inst. Theor. Phys. II) ; Spiropulu, M. (Harvard U., Phys. Dept.) ; Sullivan, Z. (Argonne) ; Szalapski, R. (Rochester U.) ; Tannenbaum, B. (UCLA) ; Tait, T. (Michigan State U. ; Argonne) ; Wackeroth, D. (PSI, Villigen) ; Wang, Y. (Hawaii U.) ; White, J. (Texas A-M) ; Williams, H.H. (Pennsylvania U.) ; Worcester, M. (UCLA) ; Worm, S. (New Mexico U.) ; Zhang, R.J. (Wisconsin U., Madison) ; Zielinski, M. (Rochester U.) |
| Publication | 2000 |
| Imprint | 16 Mar 2000 |
| Number of pages | 173 |
| Note | Part 2 of physics at Run II SUSY/Higgs report: available as hep-ph/0003154 (part 2), hep-ph/0008070 (part 3), and hep-ph/9906224 (part 4), and hep-ph/0006162 (part 5), and hep-ph/0010338 (part 6) |
| Subject category | Particle Physics - Phenomenology |
| Abstract | We present an analysis of the discovery reach for supersymmetric particles at the upgraded Tevatron collider, assuming that SUSY breaking results in universal soft breaking parameters at the grand unification scale, and that the lightest supersymmetric particle is stable and neutral. We first present a review of the literature, including the issues of unification, renormalization group evolution of the supersymmetry breaking parameters and the effect of radiative corrections on the effective low energy couplings and masses of the theory. We consider the experimental bounds coming from direct searches and those arising indirectly from precision data, cosmology and the requirement of vacuum stability. The issues of flavor and CP-violation are also addressed. The main subject of this study is to update sparticle production cross sections, make improved estimates of backgrounds, delineate the discovery reach in the supergravity framework, and examine how this might vary when assumptions about universality of soft breaking parameters are relaxed. With 30 fb$^{-1}$ luminosity and one detector, charginos and neutralinos, as well as third generation squarks, can be seen if their masses are not larger than 200-250 GeV, while first and second generation squarks and gluinos can be discovered if their masses do not significantly exceed 400 GeV. We conclude that there are important and exciting physics opportunities at the Tevatron collider, which will be significantly enhanced by continued Tevatron operation beyond the first phase of Run II. |
| Other source | Inspire |
| Submitted by | [email protected] |
Element opprettet 2000-03-17, sist endret 2025-05-20
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