CERN Accelerating science

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Preprint
Report number arXiv:2203.08033
Title A Muon Collider Facility for Physics Discovery
Author(s)

Stratakis, D. (Fermilab) ; Mokhov, N. (Fermilab) ; Palmer, M. (Brookhaven) ; Pastrone, N. (INFN, Turin) ; Raubenheimer, T. (SLAC) ; Rogers, C. (Rutherford) ; Schulte, D. (CERN) ; Shiltsev, V. (Fermilab) ; Tang, J. (Zhongshan U. ; Beijing, Inst. High Energy Phys.) ; Aimè, C. (Pavia U. ; INFN, Pavia) ; Mahmoud., M.A. (Fayoum U.) ; Bartosik, N. (INFN, Turin) ; Barzi, E. (Fermilab ; Ohio State U.) ; Bersani, A. (INFN, Genoa) ; Bertolin, A. (INFN, Padua) ; Bonesini, M. (INFN, Italy ; INFN, Milan Bicocca ; Milan Bicocca U.) ; Caiffi, B. (INFN, Genoa) ; Casarsa, M. (INFN, Trieste) ; Catanesi, M.G. (INFN, Bari) ; Cerri, A. (Sussex U.) ; Curatolo, C. (INFN, Italy) ; Dam, M. (INFN, Italy) ; Damerau, H. (CERN) ; De Matteis, E. (Milan U.) ; Denizli, H. (Abant Izzet Baysal U.) ; Di Micco, B. (Rome III U. ; INFN, Rome3) ; Dorigo, T. (INFN, Padua) ; Farinon, S. (INFN, Genoa) ; Filthaut, F. (Nijmegen U.) ; Fiorina, D. (INFN, Pavia) ; Giove, D. (Milan U.) ; Greco, M. (Rome III U.) ; Grojean, C. (DESY ; Humboldt U., Berlin) ; Han, T. (Pittsburgh U.) ; Jindariani, S. (Fermilab) ; Koppenburg, P. (NIKHEF, Amsterdam) ; Krizka, K. (LBNL, Berkeley) ; Li, Q. (Peking U.) ; Liu, Z. (Minnesota U.) ; Long, K.R. (Imperial Coll., London ; Rutherford) ; Lucchesi, D. (INFN, Padua ; Padua U.) ; Mariotto, S. (Milan U.) ; Meloni, F. (DESY) ; Merlassino, C. (U. Oxford (main)) ; Métral, E. (CERN) ; Montella, A. (INFN, Trieste) ; Musenich, R. (INFN, Genoa) ; Nardecchia, M. (U. Rome La Sapienza (main) ; INFN, Rome) ; Nardi, F. (INFN, Padua ; Padua U.) ; Neuffer, D. (Fermilab) ; Griso, S.Pagan (LBNL, Berkeley) ; Potamianos, K. (U. Oxford (main)) ; Prioli, M. (Milan U.) ; Radicioni, E. (INFN, Bari) ; Reina, L. (Florida U.) ; Riccardi, C. (Pavia U. ; INFN, Pavia) ; Ristori, L. (Fermilab) ; Rossi, L. (Milan U.) ; Salvini, P. (INFN, Pavia) ; Santiago, J. (Granada U. ; CAFPE, Granada ; Granada U., Theor. Phys. Astrophys.) ; Senol, A. (Abant Izzet Baysal U.) ; Sestini, L. (INFN, Padua) ; Sorbi, M. (Milan U.) ; Stark, G. (UC, Santa Cruz, Inst. Part. Phys. ; UC, Santa Cruz) ; Statera, M. (Milan U.) ; Sun, X. (Peking U., SKLNPT) ; Vai, I. (INFN, Pavia) ; Agashe, K. (Maryland U.) ; Allanach, B.C. (Cambridge U., DAMTP) ; Apresyan, A. (Fermilab) ; Asadi, P. (MIT, Cambridge, CTP) ; Athanasakos, D. (YITP, Stony Brook) ; Azatov, A. (SISSA, Trieste ; INFN, Trieste) ; Batsch, F. (CERN) ; Biagini, M.E. (Frascati) ; Black, K.M. (Wisconsin U., Madison) ; Braghieri, A. (INFN, Pavia) ; Bross, A. (Fermilab) ; Buonincontri, L. (INFN, Padua ; Padua U.) ; Buttazzo, D. (INFN, Pisa) ; Calderini, G. (Paris U., VI-VII) ; Calzaferri, S. (INFN, Pavia) ; Canepa, A. (Fermilab) ; Capdevilla, R. (Perimeter Inst. Theor. Phys. ; Toronto U.) ; Castelli, L. (INFN, Padua ; Padua U.) ; Cesarotti, C. (Harvard U., Phys. Dept.) ; Chachamis, G. (LIP, Lisbon) ; Chacko, Z. (Maryland U.) ; Chancé, A. (IRFU, Saclay) ; Chen, S. (EPFL, Lausanne, LPTP) ; Chien, Y.-T. (Georgia State U.) ; Colaleo, A. (Bari U. ; INFN, Bari) ; Costa, M. (Pisa, Scuola Normale Superiore ; INFN, Pisa) ; Craig, N. (UC, Santa Barbara) ; Cui, Y. (UC, Riverside (main)) ; Curtin, D. (Toronto U.) ; D'Agnolo, R.T. (IPhT, Saclay) ; Da Molin, G. (INFN, Padua ; Padua U.) ; Dasu, S. (Wisconsin U., Madison) ; de Blas, J. (Granada U., Theor. Phys. Astrophys.) ; Deandrea, A. (IP2I, Lyon) ; Delahaye, J. (CERN) ; Delgado, A. (Notre Dame U.) ; Dermisek, R. (Indiana U.) ; Di Petrillo, K.F. (Fermilab) ; Dickinson, J. (Fermilab) ; Dracos, M. (Strasbourg, IPHC ; Louis Pasteur U., Strasbourg I) ; Errico, F. (Bari U. ; INFN, Bari) ; Everaerts, P. (Wisconsin U., Madison) ; Everett, L. (Wisconsin U., Madison) ; Ferretti, G. (Goteborg, ITP ; CERN) ; Forslund, M. (YITP, Stony Brook) ; Franceschini, R. (Rome III U. ; INFN, Rome3) ; Gabrielli, E. (SISSA, Trieste ; INFN, Trieste) ; Garosi, F. (European Southern Observ.) ; Giambastiani, L. (Padua U. ; INFN, Padua) ; Giraldin, C. (INFN, Padua ; Padua U.) ; Glioti, A. (EPFL, Lausanne, LPTP) ; Gray, L. (Fermilab) ; Greljo, A. (Bern U. ; U. Bern, AEC) ; Gu, J. (Fudan U.) ; Haber, H.E. (UC, Santa Cruz, Inst. Part. Phys. ; UC, Santa Cruz) ; Han, C. (SYSU, Guangzhou) ; Hauptman, J. (Iowa State U.) ; Henning, B. (EPFL, Lausanne, LPTP) ; Hermanek, K. (Indiana U.) ; Herndon, M. (Wisconsin U., Madison) ; Holmes, T.R. (Tennessee U.) ; Homiller, S. (Harvard U., Phys. Dept.) ; Jana, S. (Heidelberg, Max Planck Inst.) ; Jia, H. (Wisconsin U., Madison) ; Kahn, Y. (Illinois U., Urbana) ; Kaplan, D.M. (MIT) ; Kilian, W. (Siegen U.) ; Kong, K. (Kansas U.) ; Krintiras, G.K. (Kansas U.) ; Krnjaic, G. (Fermilab) ; Losito, R. (CERN) ; Lee, L. (Tennessee U.) ; Li, W. (Rice U.) ; Low, I. (Argonne ; Northwestern U.) ; Lu, Q. (Harvard U., Phys. Dept.) ; Ma, Y. (Pittsburgh U.) ; Maltoni, F. (Louvain U., CP3 ; Bologna U.) ; Mantani, L. (Cambridge U., DAMTP) ; Marzocca, D. (INFN, Trieste) ; Mastrapasqua, P. (Louvain U., CP3) ; Matchev, K. (Florida U.) ; Mazzacane, A. (Fermilab) ; McGinnis, N. (TRIUMF) ; Meade, P. (YITP, Stony Brook) ; Mele, B. (INFN, Rome) ; Merkel, P. (Fermilab) ; Mescia, F. (Barcelona, IFAE ; ICC, Barcelona U.) ; Mishra, R.K. (Harvard U., Phys. Dept.) ; Mohammadi, A. (Wisconsin U., Madison) ; Mohapatra, R. (Maryland U.) ; Montagna, P. (Pavia U. ; INFN, Pavia) ; Neufeld, N. (CERN) ; Newman, H. (Caltech) ; Nomura, Y. (UC, Berkeley ; LBL, Berkeley) ; Ojalvo, I. (Princeton U.) ; Panci, P. (INFN, Pisa) ; Pagani, D. (INFN, Bologna) ; Paradisi, P. (Padua U. ; INFN, Padua) ; Pellecchia, A. (Bari U. ; INFN, Bari) ; Perloff, A. (Colorado u.) ; Piccinini, F. (INFN, Pavia) ; Pierini, M. (CERN) ; Procura, M. (Vienna U.) ; Radogna, R. (Bari U. ; INFN, Bari) ; Raubenheimer, T. (Brookhaven ; SLAC) ; Redigolo, D. (INFN, Florence) ; Reuter, J. (DESY) ; Riva, F. (Geneva U., Dept. Theor. Phys.) ; Robens, T. (Boskovic Inst., Zagreb) ; Queiroz, F.S. (IIP, Brazil) ; Sala, F. (Paris, LPTHE) ; Salko, J. (Bern U. ; U. Bern, AEC) ; Salvioni, E. (Padua U. ; INFN, Padua) ; Sarra, I. (Maryland U.) ; Schieck, J. (Vienna, OAW ; Vienna, Tech. U., Atominst.) ; Selvaggi, M. (CERN) ; Sharma, V. (Wisconsin U., Madison) ; Simone, F.M. (Bari U. ; INFN, Bari) ; Stamerra, A. (Bari U. ; INFN, Bari) ; Stolarski, D. (Ottawa Carleton Inst. Phys.) ; Stupak, J. (Oklahoma U.) ; Su, S. (Arizona U.) ; Sundrum, R. (Maryland U.) ; Swiatlowski, M. (TRIUMF) ; Sytov, A. (INFN, Ferrara) ; Tait, T. (UC, Irvine) ; Thompson, E.A. (DESY) ; Torre, R. (INFN, Genoa) ; Tortora, L. (INFN, Rome3 ; CERN) ; Trifinopoulos, S. (INFN, Trieste) ; Valente, M. (TRIUMF) ; Valle, N. (Pavia U. ; INFN, Pavia) ; Venditti, R. (Bari U. ; INFN, Bari) ; Verwilligen, P. (INFN, Bari) ; Vittorio, L. (Pisa, Scuola Normale Superiore ; INFN, Pisa) ; Vitulo, P. (Pavia U. ; INFN, Pavia) ; Vryonidou, E. (Manchester U.) ; Vuosalo, C. (Wisconsin U., Madison) ; Weber, H. (Humboldt U., Berlin) ; Wu, Y. (Oklahoma State U.) ; Wulzer, A. (INFN, Padua ; Padua U.) ; Xie, K. (Pittsburgh U.) ; Yonehara, K. (Fermilab) ; Yu, H.-B. (UC, Riverside (main)) ; Zaza, A. (Bari U. ; INFN, Bari) ; Zheng, Y.J. (Kansas U.) ; Zuliani, D. (INFN, Padua ; Padua U.) ; Zurita, J. (U. Valencia (main))

Imprint 2022-03-15
Number of pages 23
Note 23 pages, 3 figures. arXiv admin note: text overlap with arXiv:2201.07895
Presented at 2021 Snowmass Summer Study, Seattle, WA, United States, 11 - 20 July 2021
Subject category physics.acc-ph ; Accelerators and Storage Rings
Study IMCC
Abstract Muon colliders provide a unique route to deliver high energy collisions that enable discovery searches and precision measurements to extend our understanding of the fundamental laws of physics. The muon collider design aims to deliver physics reach at the highest energies with costs, power consumption and on a time scale that may prove favorable relative to other proposed facilities. In this context, a new international collaboration has formed to further extend the design concepts and performance studies of such a machine. This effort is focused on delivering the elements of a $\sim$10 TeV center of mass (CM) energy design to explore the physics energy frontier. The path to such a machine may pass through lower energy options. Currently a 3 TeV CM stage is considered. Other energy stages could also be explored, e.g. an s-channel Higgs Factory operating at 125 GeV CM. We describe the status of the R&D; and design effort towards such a machine and lay out a plan to bring these concepts to maturity as a tool for the high energy physics community.
Other source Inspire
Copyright/License preprint: (License: CC BY 4.0)



 


 Registro creado el 2022-09-16, última modificación el 2024-10-30


Texto completo:
2203.08033 - Descargar el texto completoPDF
1d831c5ff49dc5c77ab54a52485f652b - Descargar el texto completoPDF
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