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Acharya B, Alexandre J, Benes P, Bergmann B, Bertolucci S, Bevan A, Branzas H, Burian P, Campbell M, Cho YM, de Montigny M, De Roeck A, Ellis JR, Sawy ME, Fairbairn M, Felea D, Frank M, Gould O, Hays J, Hirt AM, Ho DLJ, Hung PQ, Janecek J, Kalliokoski M, Korzenev A, Lacarrère DH, Leroy C, Levi G, Lionti A, Maulik A, Margiotta A, Mauri N, Mavromatos NE, Mermod P, Millward L, Mitsou VA, Ostrovskiy I, Ouimet PP, Papavassiliou J, Parker B, Patrizii L, Păvălaş GE, Pinfold JL, Popa LA, Popa V, Pozzato M, Pospisil S, Rajantie A, de Austri RR, Sahnoun Z, Sakellariadou M, Santra A, Sarkar S, Semenoff G, Shaa A, Sirri G, Sliwa K, Soluk R, Spurio M, Staelens M, Suk M, Tenti M, Togo V, Tuszyn'ski JA, Upreti A, Vento V, Vives O. Search for magnetic monopoles produced via the Schwinger mechanism. Nature 2022; 602:63-67. [PMID: 35110756 DOI: 10.1038/s41586-021-04298-1] [Citation(s) in RCA: 7] [Impact Index Per Article: 3.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/18/2021] [Accepted: 12/01/2021] [Indexed: 11/09/2022]
Abstract
Electrically charged particles can be created by the decay of strong enough electric fields, a phenomenon known as the Schwinger mechanism1. By electromagnetic duality, a sufficiently strong magnetic field would similarly produce magnetic monopoles, if they exist2. Magnetic monopoles are hypothetical fundamental particles that are predicted by several theories beyond the standard model3-7 but have never been experimentally detected. Searching for the existence of magnetic monopoles via the Schwinger mechanism has not yet been attempted, but it is advantageous, owing to the possibility of calculating its rate through semi-classical techniques without perturbation theory, as well as that the production of the magnetic monopoles should be enhanced by their finite size8,9 and strong coupling to photons2,10. Here we present a search for magnetic monopole production by the Schwinger mechanism in Pb-Pb heavy ion collisions at the Large Hadron Collider, producing the strongest known magnetic fields in the current Universe11. It was conducted by the MoEDAL experiment, whose trapping detectors were exposed to 0.235 per nanobarn, or approximately 1.8 × 109, of Pb-Pb collisions with 5.02-teraelectronvolt center-of-mass energy per collision in November 2018. A superconducting quantum interference device (SQUID) magnetometer scanned the trapping detectors of MoEDAL for the presence of magnetic charge, which would induce a persistent current in the SQUID. Magnetic monopoles with integer Dirac charges of 1, 2 and 3 and masses up to 75 gigaelectronvolts per speed of light squared were excluded by the analysis at the 95% confidence level. This provides a lower mass limit for finite-size magnetic monopoles from a collider search and greatly extends previous mass bounds.
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Affiliation(s)
- B Acharya
- Theoretical Particle Physics & Cosmology Group, Physics Department, King's College London, London, UK
| | - J Alexandre
- Theoretical Particle Physics & Cosmology Group, Physics Department, King's College London, London, UK
| | - P Benes
- IEAP, Czech Technical University in Prague, Prague, Czech Republic
| | - B Bergmann
- IEAP, Czech Technical University in Prague, Prague, Czech Republic
| | | | - A Bevan
- School of Physics and Astronomy, Queen Mary University of London, London, UK
| | - H Branzas
- Institute of Space Science, Măgurele, Romania
| | - P Burian
- IEAP, Czech Technical University in Prague, Prague, Czech Republic
| | - M Campbell
- Experimental Physics Department, CERN, Geneva, Switzerland
| | - Y M Cho
- Center for Quantum Spacetime, Sogang University, Seoul, Korea
| | - M de Montigny
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - A De Roeck
- Experimental Physics Department, CERN, Geneva, Switzerland
| | - J R Ellis
- Theoretical Particle Physics & Cosmology Group, Physics Department, King's College London, London, UK.,Theoretical Physics Department, CERN, Geneva, Switzerland
| | - M El Sawy
- Experimental Physics Department, CERN, Geneva, Switzerland
| | - M Fairbairn
- Theoretical Particle Physics & Cosmology Group, Physics Department, King's College London, London, UK
| | - D Felea
- Institute of Space Science, Măgurele, Romania
| | - M Frank
- Department of Physics, Concordia University, Montreal, Quebec, Canada
| | - O Gould
- University of Nottingham, Nottingham, UK.,Helsinki Institute of Physics, University of Helsinki, Helsinki, Finland
| | - J Hays
- School of Physics and Astronomy, Queen Mary University of London, London, UK
| | - A M Hirt
- Department of Earth Sciences, Swiss Federal Institute of Technology, Zurich, Switzerland
| | - D L-J Ho
- Department of Physics, Imperial College London, London, UK
| | - P Q Hung
- Department of Physics, University of Virginia, Charlottesville, VA, USA
| | - J Janecek
- IEAP, Czech Technical University in Prague, Prague, Czech Republic
| | - M Kalliokoski
- Helsinki Institute of Physics, University of Helsinki, Helsinki, Finland
| | - A Korzenev
- Département de Physique Nucléaire et Corpusculaire, Université de Genève, Geneva, Switzerland
| | - D H Lacarrère
- Experimental Physics Department, CERN, Geneva, Switzerland
| | - C Leroy
- Département de Physique, Université de Montréal, Montreal, Quebec, Canada
| | - G Levi
- INFN, Section of Bologna, Bologna, Italy.,Department of Physics and Astronomy, University of Bologna, Bologna, Italy
| | - A Lionti
- Département de Physique Nucléaire et Corpusculaire, Université de Genève, Geneva, Switzerland
| | - A Maulik
- INFN, Section of Bologna, Bologna, Italy.,Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - A Margiotta
- Department of Physics and Astronomy, University of Bologna, Bologna, Italy
| | - N Mauri
- INFN, Section of Bologna, Bologna, Italy
| | - N E Mavromatos
- Theoretical Particle Physics & Cosmology Group, Physics Department, King's College London, London, UK
| | - P Mermod
- Département de Physique Nucléaire et Corpusculaire, Université de Genève, Geneva, Switzerland
| | - L Millward
- School of Physics and Astronomy, Queen Mary University of London, London, UK
| | - V A Mitsou
- IFIC, Universitat de València, CSIC, Valencia, Spain
| | - I Ostrovskiy
- Department of Physics and Astronomy, University of Alabama, Tuscaloosa, AL, USA.
| | - P-P Ouimet
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | | | - B Parker
- Institute for Research in Schools, Canterbury, UK
| | - L Patrizii
- INFN, Section of Bologna, Bologna, Italy
| | - G E Păvălaş
- Institute of Space Science, Măgurele, Romania
| | - J L Pinfold
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - L A Popa
- Institute of Space Science, Măgurele, Romania
| | - V Popa
- Institute of Space Science, Măgurele, Romania
| | - M Pozzato
- INFN, Section of Bologna, Bologna, Italy
| | - S Pospisil
- IEAP, Czech Technical University in Prague, Prague, Czech Republic
| | - A Rajantie
- Department of Physics, Imperial College London, London, UK
| | | | - Z Sahnoun
- INFN, Section of Bologna, Bologna, Italy
| | - M Sakellariadou
- Theoretical Particle Physics & Cosmology Group, Physics Department, King's College London, London, UK
| | - A Santra
- IFIC, Universitat de València, CSIC, Valencia, Spain
| | - S Sarkar
- Theoretical Particle Physics & Cosmology Group, Physics Department, King's College London, London, UK
| | - G Semenoff
- Department of Physics, University of British Columbia, Vancouver, British Columbia, Canada
| | - A Shaa
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - G Sirri
- INFN, Section of Bologna, Bologna, Italy
| | - K Sliwa
- Department of Physics and Astronomy, Tufts University, Medford, MA, USA
| | - R Soluk
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - M Spurio
- Department of Physics and Astronomy, University of Bologna, Bologna, Italy
| | - M Staelens
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - M Suk
- IEAP, Czech Technical University in Prague, Prague, Czech Republic
| | | | - V Togo
- INFN, Section of Bologna, Bologna, Italy
| | - J A Tuszyn'ski
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - A Upreti
- Department of Physics and Astronomy, University of Alabama, Tuscaloosa, AL, USA
| | - V Vento
- IFIC, Universitat de València, CSIC, Valencia, Spain
| | - O Vives
- IFIC, Universitat de València, CSIC, Valencia, Spain
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2
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Acharya B, Alexandre J, Benes P, Bergmann B, Bernabéu J, Bevan A, Branzas H, Burian P, Campbell M, Cecchini S, Cho YM, de Montigny M, De Roeck A, Ellis JR, El Sawy M, Fairbairn M, Felea D, Frank M, Hays J, Hirt AM, Janecek J, Kalliokoski M, Korzenev A, Lacarrère DH, Leroy C, Levi G, Lionti A, Mamuzic J, Maulik A, Margiotta A, Mauri N, Mavromatos NE, Mermod P, Mieskolainen M, Millward L, Mitsou VA, Orava R, Ostrovskiy I, Ouimet PP, Papavassiliou J, Parker B, Patrizii L, Păvălaş GE, Pinfold JL, Popa LA, Popa V, Pozzato M, Pospisil S, Rajantie A, Ruiz de Austri R, Sahnoun Z, Sakellariadou M, Santra A, Sarkar S, Semenoff G, Shaa A, Sirri G, Sliwa K, Soluk R, Spurio M, Staelens M, Suk M, Tenti M, Togo V, Tuszyński JA, Upreti A, Vento V, Vives O, Wall A. First Search for Dyons with the Full MoEDAL Trapping Detector in 13 TeV pp Collisions. Phys Rev Lett 2021; 126:071801. [PMID: 33666471 DOI: 10.1103/physrevlett.126.071801] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/02/2020] [Revised: 10/10/2020] [Accepted: 01/12/2021] [Indexed: 06/12/2023]
Abstract
The MoEDAL trapping detector consists of approximately 800 kg of aluminum volumes. It was exposed during run 2 of the LHC program to 6.46 fb^{-1} of 13 TeV proton-proton collisions at the LHCb interaction point. Evidence for dyons (particles with electric and magnetic charge) captured in the trapping detector was sought by passing the aluminum volumes comprising the detector through a superconducting quantum interference device (SQUID) magnetometer. The presence of a trapped dyon would be signaled by a persistent current induced in the SQUID magnetometer. On the basis of a Drell-Yan production model, we exclude dyons with a magnetic charge ranging up to five Dirac charges (5g_{D}) and an electric charge up to 200 times the fundamental electric charge for mass limits in the range 870-3120 GeV and also monopoles with magnetic charge up to and including 5g_{D} with mass limits in the range 870-2040 GeV.
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Affiliation(s)
- B Acharya
- Theoretical Particle Physics and Cosmology Group, Physics Department, King's College, London, United Kingdom
| | - J Alexandre
- Theoretical Particle Physics and Cosmology Group, Physics Department, King's College, London, United Kingdom
| | - P Benes
- IEAP, Czech Technical University in Prague, Prague, Czech Republic
| | - B Bergmann
- IEAP, Czech Technical University in Prague, Prague, Czech Republic
| | - J Bernabéu
- IFIC, Universitat de València-CSIC, Valencia, Spain
| | - A Bevan
- School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom
| | - H Branzas
- Institute of Space Science, Bucharest, Măgurele, Romania
| | - P Burian
- IEAP, Czech Technical University in Prague, Prague, Czech Republic
| | - M Campbell
- Experimental Physics Department, CERN, Geneva, Switzerland
| | - S Cecchini
- INFN, Section of Bologna, Bologna, Italy
| | - Y M Cho
- Center for Quantum Spacetime, Sogang University, Seoul, Korea
| | - M de Montigny
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - A De Roeck
- Experimental Physics Department, CERN, Geneva, Switzerland
| | - J R Ellis
- Theoretical Particle Physics and Cosmology Group, Physics Department, King's College, London, United Kingdom
- Theoretical Physics Department, CERN, Geneva, Switzerland
| | - M El Sawy
- Experimental Physics Department, CERN, Geneva, Switzerland
| | - M Fairbairn
- Theoretical Particle Physics and Cosmology Group, Physics Department, King's College, London, United Kingdom
| | - D Felea
- Institute of Space Science, Bucharest, Măgurele, Romania
| | - M Frank
- Department of Physics, Concordia University, Montréal, Québec, Canada
| | - J Hays
- School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom
| | - A M Hirt
- Department of Earth Sciences, Swiss Federal Institute of Technology, Zurich, Switzerland
| | - J Janecek
- IEAP, Czech Technical University in Prague, Prague, Czech Republic
| | - M Kalliokoski
- Physics Department, University of Helsinki, Helsinki, Finland
| | - A Korzenev
- Département de Physique Nucléaire et Corpusculaire, Université de Genève, Geneva, Switzerland
| | - D H Lacarrère
- Experimental Physics Department, CERN, Geneva, Switzerland
| | - C Leroy
- Département de Physique, Université de Montréal, Québec, Canada
| | - G Levi
- INFN, Section of Bologna and Department of Physics and Astronomy, University of Bologna, Bologna, Italy
| | - A Lionti
- Département de Physique Nucléaire et Corpusculaire, Université de Genève, Geneva, Switzerland
| | - J Mamuzic
- IFIC, Universitat de València-CSIC, Valencia, Spain
| | - A Maulik
- INFN, Section of Bologna, Bologna, Italy
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - A Margiotta
- INFN, Section of Bologna and Department of Physics and Astronomy, University of Bologna, Bologna, Italy
| | - N Mauri
- INFN, Section of Bologna, Bologna, Italy
| | - N E Mavromatos
- Theoretical Particle Physics and Cosmology Group, Physics Department, King's College, London, United Kingdom
| | - P Mermod
- Département de Physique Nucléaire et Corpusculaire, Université de Genève, Geneva, Switzerland
| | - M Mieskolainen
- Physics Department, University of Helsinki, Helsinki, Finland
| | - L Millward
- School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom
| | - V A Mitsou
- IFIC, Universitat de València-CSIC, Valencia, Spain
| | - R Orava
- Physics Department, University of Helsinki, Helsinki, Finland
| | - I Ostrovskiy
- Department of Physics and Astronomy, University of Alabama, Tuscaloosa, Alabama, USA
| | - P-P Ouimet
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | | | - B Parker
- Institute for Research in Schools, Canterbury, United Kingdom
| | - L Patrizii
- INFN, Section of Bologna, Bologna, Italy
| | - G E Păvălaş
- Institute of Space Science, Bucharest, Măgurele, Romania
| | - J L Pinfold
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - L A Popa
- Institute of Space Science, Bucharest, Măgurele, Romania
| | - V Popa
- Institute of Space Science, Bucharest, Măgurele, Romania
| | - M Pozzato
- INFN, Section of Bologna, Bologna, Italy
| | - S Pospisil
- IEAP, Czech Technical University in Prague, Prague, Czech Republic
| | - A Rajantie
- Department of Physics, Imperial College London, United Kingdom
| | | | - Z Sahnoun
- INFN, Section of Bologna, Bologna, Italy
| | - M Sakellariadou
- Theoretical Particle Physics and Cosmology Group, Physics Department, King's College, London, United Kingdom
| | - A Santra
- IFIC, Universitat de València-CSIC, Valencia, Spain
| | - S Sarkar
- Theoretical Particle Physics and Cosmology Group, Physics Department, King's College, London, United Kingdom
| | - G Semenoff
- Department of Physics, University of British Columbia, Vancouver, British Columbia, Canada
| | - A Shaa
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - G Sirri
- INFN, Section of Bologna, Bologna, Italy
| | - K Sliwa
- Department of Physics and Astronomy, Tufts University, Medford, Massachusetts, USA
| | - R Soluk
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - M Spurio
- INFN, Section of Bologna and Department of Physics and Astronomy, University of Bologna, Bologna, Italy
| | - M Staelens
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - M Suk
- IEAP, Czech Technical University in Prague, Prague, Czech Republic
| | | | - V Togo
- INFN, Section of Bologna, Bologna, Italy
| | - J A Tuszyński
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - A Upreti
- Department of Physics and Astronomy, University of Alabama, Tuscaloosa, Alabama, USA
| | - V Vento
- IFIC, Universitat de València-CSIC, Valencia, Spain
| | - O Vives
- IFIC, Universitat de València-CSIC, Valencia, Spain
| | - A Wall
- Department of Physics and Astronomy, University of Alabama, Tuscaloosa, Alabama, USA
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3
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Felea D, Mamuzic J, Masełek R, Mavromatos NE, Mitsou VA, Pinfold JL, de Austri RR, Sakurai K, Santra A, Vives O. Prospects for discovering supersymmetric long-lived particles with MoEDAL. Eur Phys J C Part Fields 2020; 80:431. [PMID: 32440256 PMCID: PMC7231802 DOI: 10.1140/epjc/s10052-020-7994-7] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Grants] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 01/21/2020] [Accepted: 04/30/2020] [Indexed: 06/11/2023]
Abstract
We present a study on the possibility of searching for long-lived supersymmetric partners with the MoEDAL experiment at the LHC. MoEDAL is sensitive to highly ionising objects such as magnetic monopoles or massive (meta)stable electrically charged particles. We focus on prospects of directly detecting long-lived sleptons in a phenomenologically realistic model which involves an intermediate neutral long-lived particle in the decay chain. This scenario is not yet excluded by the current data from ATLAS or CMS, and is compatible with astrophysical constraints. Using Monte Carlo simulation, we compare the sensitivities of MoEDAL versus ATLAS in scenarios where MoEDAL could provide discovery reach complementary to ATLAS and CMS, thanks to looser selection criteria combined with the virtual absence of background. It is also interesting to point out that, in such scenarios, in which charged staus are the main long-lived candidates, the relevant mass range for MoEDAL is compatible with a potential role of Supersymmetry in providing an explanation for the anomalous events observed by the ANITA detector.
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Affiliation(s)
- D. Felea
- Institute of Space Science, P.O. Box MG 23, 077125 Bucharest, Măgurele Romania
| | - J. Mamuzic
- Instituto de Física Corpuscular (IFIC), CSIC-Universitat de València, C/Catedrático José Beltrán 2, 46980 Paterna, Valencia Spain
| | - R. Masełek
- Institute of Theoretical Physics, Faculty of Physics, University of Warsaw, ul. Pasteura 5, 02093 Warsaw, Poland
| | - N. E. Mavromatos
- Theoretical Particle Physics and Cosmology Group, Department of Physics, King’s College London, Strand, London, WC2R 2LS UK
| | - V. A. Mitsou
- Instituto de Física Corpuscular (IFIC), CSIC-Universitat de València, C/Catedrático José Beltrán 2, 46980 Paterna, Valencia Spain
| | - J. L. Pinfold
- Physics Department, University of Alberta, Edmonton, AB T6G 2E4 Canada
| | - R. Ruiz de Austri
- Instituto de Física Corpuscular (IFIC), CSIC-Universitat de València, C/Catedrático José Beltrán 2, 46980 Paterna, Valencia Spain
| | - K. Sakurai
- Institute of Theoretical Physics, Faculty of Physics, University of Warsaw, ul. Pasteura 5, 02093 Warsaw, Poland
| | - A. Santra
- Instituto de Física Corpuscular (IFIC), CSIC-Universitat de València, C/Catedrático José Beltrán 2, 46980 Paterna, Valencia Spain
| | - O. Vives
- Instituto de Física Corpuscular (IFIC), CSIC-Universitat de València, C/Catedrático José Beltrán 2, 46980 Paterna, Valencia Spain
- Departament de Física Teòrica, Universitat de València, C/ Dr. Moliner 50, 46100 Burjassot, Valencia Spain
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4
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Acharya B, Alexandre J, Baines S, Benes P, Bergmann B, Bernabéu J, Bevan A, Branzas H, Campbell M, Cecchini S, Cho YM, de Montigny M, De Roeck A, Ellis JR, El Sawy M, Fairbairn M, Felea D, Frank M, Hays J, Hirt AM, Janecek J, Kim DW, Korzenev A, Lacarrère DH, Lee SC, Leroy C, Levi G, Lionti A, Mamuzic J, Margiotta A, Mauri N, Mavromatos NE, Mermod P, Mieskolainen M, Millward L, Mitsou VA, Orava R, Ostrovskiy I, Papavassiliou J, Parker B, Patrizii L, Păvălaş GE, Pinfold JL, Popa V, Pozzato M, Pospisil S, Rajantie A, Ruiz de Austri R, Sahnoun Z, Sakellariadou M, Santra A, Sarkar S, Semenoff G, Shaa A, Sirri G, Sliwa K, Soluk R, Spurio M, Staelens M, Suk M, Tenti M, Togo V, Tuszyński JA, Vento V, Vives O, Vykydal Z, Wall A, Zgura IS. Magnetic Monopole Search with the Full MoEDAL Trapping Detector in 13 TeV pp Collisions Interpreted in Photon-Fusion and Drell-Yan Production. Phys Rev Lett 2019; 123:021802. [PMID: 31386510 DOI: 10.1103/physrevlett.123.021802] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/21/2019] [Indexed: 06/10/2023]
Abstract
MoEDAL is designed to identify new physics in the form of stable or pseudostable highly ionizing particles produced in high-energy Large Hadron Collider (LHC) collisions. Here we update our previous search for magnetic monopoles in Run 2 using the full trapping detector with almost four times more material and almost twice more integrated luminosity. For the first time at the LHC, the data were interpreted in terms of photon-fusion monopole direct production in addition to the Drell-Yan-like mechanism. The MoEDAL trapping detector, consisting of 794 kg of aluminum samples installed in the forward and lateral regions, was exposed to 4.0 fb^{-1} of 13 TeV proton-proton collisions at the LHCb interaction point and analyzed by searching for induced persistent currents after passage through a superconducting magnetometer. Magnetic charges equal to or above the Dirac charge are excluded in all samples. Monopole spins 0, ½, and 1 are considered and both velocity-independent and-dependent couplings are assumed. This search provides the best current laboratory constraints for monopoles with magnetic charges ranging from two to five times the Dirac charge.
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Affiliation(s)
- B Acharya
- Theoretical Particle Physics and Cosmology Group, Physics Department, King's College London, United Kingdom
| | - J Alexandre
- Theoretical Particle Physics and Cosmology Group, Physics Department, King's College London, United Kingdom
| | - S Baines
- Theoretical Particle Physics and Cosmology Group, Physics Department, King's College London, United Kingdom
| | - P Benes
- IEAP, Czech Technical University in Prague, Czech Republic
| | - B Bergmann
- IEAP, Czech Technical University in Prague, Czech Republic
| | - J Bernabéu
- IFIC, Universitat de València-CSIC, Valencia, Spain
| | - A Bevan
- School of Physics and Astronomy, Queen Mary University of London, United Kingdom
| | - H Branzas
- Institute of Space Science, Bucharest-Măgurele, Romania
| | - M Campbell
- Experimental Physics Department, CERN, Geneva, Switzerland
| | - S Cecchini
- INFN, Section of Bologna, Bologna, Italy
| | - Y M Cho
- Physics Department, Konkuk University, Seoul, Korea
| | - M de Montigny
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - A De Roeck
- Experimental Physics Department, CERN, Geneva, Switzerland
| | - J R Ellis
- Theoretical Particle Physics and Cosmology Group, Physics Department, King's College London, United Kingdom
- Theoretical Physics Department, CERN, Geneva, Switzerland
| | - M El Sawy
- Experimental Physics Department, CERN, Geneva, Switzerland
| | - M Fairbairn
- Theoretical Particle Physics and Cosmology Group, Physics Department, King's College London, United Kingdom
| | - D Felea
- Institute of Space Science, Bucharest-Măgurele, Romania
| | - M Frank
- Department of Physics, Concordia University, Montréal, Québec, Canada
| | - J Hays
- School of Physics and Astronomy, Queen Mary University of London, United Kingdom
| | - A M Hirt
- Department of Earth Sciences, Swiss Federal Institute of Technology, Zurich, Switzerland-Associate member
| | - J Janecek
- IEAP, Czech Technical University in Prague, Czech Republic
| | - D-W Kim
- Physics Department, Gangneung-Wonju National University, Gangneung, Republic of Korea
| | - A Korzenev
- Département de Physique Nucléaire et Corpusculaire, Université de Genève, Geneva, Switzerland
| | - D H Lacarrère
- Experimental Physics Department, CERN, Geneva, Switzerland
| | - S C Lee
- Physics Department, Gangneung-Wonju National University, Gangneung, Republic of Korea
| | - C Leroy
- Département de Physique, Université de Montréal, Québec, Canada
| | - G Levi
- INFN, Section of Bologna and Department of Physics and Astronomy, University of Bologna, Italy
| | - A Lionti
- Département de Physique Nucléaire et Corpusculaire, Université de Genève, Geneva, Switzerland
| | - J Mamuzic
- IFIC, Universitat de València-CSIC, Valencia, Spain
| | - A Margiotta
- INFN, Section of Bologna and Department of Physics and Astronomy, University of Bologna, Italy
| | - N Mauri
- INFN, Section of Bologna, Bologna, Italy
| | - N E Mavromatos
- Theoretical Particle Physics and Cosmology Group, Physics Department, King's College London, United Kingdom
| | - P Mermod
- Département de Physique Nucléaire et Corpusculaire, Université de Genève, Geneva, Switzerland
| | - M Mieskolainen
- Physics Department, University of Helsinki, Helsinki, Finland
| | - L Millward
- School of Physics and Astronomy, Queen Mary University of London, United Kingdom
| | - V A Mitsou
- IFIC, Universitat de València-CSIC, Valencia, Spain
| | - R Orava
- Physics Department, University of Helsinki, Helsinki, Finland
| | - I Ostrovskiy
- Department of Physics and Astronomy, University of Alabama, Tuscaloosa, Alabama, USA
| | | | - B Parker
- Institute for Research in Schools, Canterbury, United Kingdom
| | - L Patrizii
- INFN, Section of Bologna, Bologna, Italy
| | - G E Păvălaş
- Institute of Space Science, Bucharest-Măgurele, Romania
| | - J L Pinfold
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - V Popa
- Institute of Space Science, Bucharest-Măgurele, Romania
| | - M Pozzato
- INFN, Section of Bologna, Bologna, Italy
| | - S Pospisil
- IEAP, Czech Technical University in Prague, Czech Republic
| | - A Rajantie
- Department of Physics, Imperial College London, United Kingdom
| | | | - Z Sahnoun
- INFN, Section of Bologna, Bologna, Italy
| | - M Sakellariadou
- Theoretical Particle Physics and Cosmology Group, Physics Department, King's College London, United Kingdom
| | - A Santra
- IFIC, Universitat de València-CSIC, Valencia, Spain
| | - S Sarkar
- Theoretical Particle Physics and Cosmology Group, Physics Department, King's College London, United Kingdom
| | - G Semenoff
- Department of Physics, University of British Columbia, Vancouver, British Columbia, Canada
| | - A Shaa
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - G Sirri
- INFN, Section of Bologna, Bologna, Italy
| | - K Sliwa
- Department of Physics and Astronomy, Tufts University, Medford, Massachusetts, USA
| | - R Soluk
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - M Spurio
- INFN, Section of Bologna and Department of Physics and Astronomy, University of Bologna, Italy
| | - M Staelens
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - M Suk
- IEAP, Czech Technical University in Prague, Czech Republic
| | | | - V Togo
- INFN, Section of Bologna, Bologna, Italy
| | - J A Tuszyński
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - V Vento
- IFIC, Universitat de València-CSIC, Valencia, Spain
| | - O Vives
- IFIC, Universitat de València-CSIC, Valencia, Spain
| | - Z Vykydal
- IEAP, Czech Technical University in Prague, Czech Republic
| | - A Wall
- Department of Physics and Astronomy, University of Alabama, Tuscaloosa, Alabama, USA
| | - I S Zgura
- Institute of Space Science, Bucharest-Măgurele, Romania
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5
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Acharya B, Alexandre J, Baines S, Benes P, Bergmann B, Bernabéu J, Branzas H, Campbell M, Caramete L, Cecchini S, de Montigny M, De Roeck A, Ellis JR, Fairbairn M, Felea D, Flores J, Frank M, Frekers D, Garcia C, Hirt AM, Janecek J, Kalliokoski M, Katre A, Kim DW, Kinoshita K, Korzenev A, Lacarrère DH, Lee SC, Leroy C, Lionti A, Mamuzic J, Margiotta A, Mauri N, Mavromatos NE, Mermod P, Mitsou VA, Orava R, Parker B, Pasqualini L, Patrizii L, Păvălaş GE, Pinfold JL, Popa V, Pozzato M, Pospisil S, Rajantie A, Ruiz de Austri R, Sahnoun Z, Sakellariadou M, Sarkar S, Semenoff G, Shaa A, Sirri G, Sliwa K, Soluk R, Spurio M, Srivastava YN, Suk M, Swain J, Tenti M, Togo V, Tuszyński JA, Vento V, Vives O, Vykydal Z, Whyntie T, Widom A, Willems G, Yoon JH, Zgura IS. Search for Magnetic Monopoles with the MoEDAL Forward Trapping Detector in 13 TeV Proton-Proton Collisions at the LHC. Phys Rev Lett 2017; 118:061801. [PMID: 28234515 DOI: 10.1103/physrevlett.118.061801] [Citation(s) in RCA: 8] [Impact Index Per Article: 1.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/22/2016] [Indexed: 06/06/2023]
Abstract
MoEDAL is designed to identify new physics in the form of long-lived highly ionizing particles produced in high-energy LHC collisions. Its arrays of plastic nuclear-track detectors and aluminium trapping volumes provide two independent passive detection techniques. We present here the results of a first search for magnetic monopole production in 13 TeV proton-proton collisions using the trapping technique, extending a previous publication with 8 TeV data during LHC Run 1. A total of 222 kg of MoEDAL trapping detector samples was exposed in the forward region and analyzed by searching for induced persistent currents after passage through a superconducting magnetometer. Magnetic charges exceeding half the Dirac charge are excluded in all samples and limits are placed for the first time on the production of magnetic monopoles in 13 TeV pp collisions. The search probes mass ranges previously inaccessible to collider experiments for up to five times the Dirac charge.
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Affiliation(s)
- B Acharya
- Physics Department, Theoretical Particle Physics & Cosmology Group, King's College, London, United Kingdom
- International Centre for Theoretical Physics, Trieste, Italy
| | - J Alexandre
- Physics Department, Theoretical Particle Physics & Cosmology Group, King's College, London, United Kingdom
| | - S Baines
- Formerly at School of Physics and Astronomy, The University of Manchester, Manchester, United Kingdom
| | - P Benes
- IEAP, Czech Technical University in Prague, Prague, Czech Republic
| | - B Bergmann
- IEAP, Czech Technical University in Prague, Prague, Czech Republic
| | - J Bernabéu
- IFIC, Universitat de València, CSIC, Valencia, Spain
| | - H Branzas
- Institute of Space Science, Bucharest, Măgurele, Romania
| | - M Campbell
- Experimental Physics Department, CERN, Geneva, Switzerland
| | - L Caramete
- Institute of Space Science, Bucharest, Măgurele, Romania
| | - S Cecchini
- INFN, Section of Bologna, Bologna, Italy
| | - M de Montigny
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - A De Roeck
- Experimental Physics Department, CERN, Geneva, Switzerland
| | - J R Ellis
- Physics Department, Theoretical Particle Physics & Cosmology Group, King's College, London, United Kingdom
- Theoretical Physics Department, CERN, Geneva, Switzerland
| | - M Fairbairn
- Physics Department, Theoretical Particle Physics & Cosmology Group, King's College, London, United Kingdom
| | - D Felea
- Institute of Space Science, Bucharest, Măgurele, Romania
| | - J Flores
- Formerly at Department of Physics and Astronomy, Stony Brook University, New York, New York, USA
| | - M Frank
- Department of Physics, Concordia University, Montréal, Québec, Canada
| | - D Frekers
- Physics Department, University of Muenster, Muenster, Germany
| | - C Garcia
- IFIC, Universitat de València, CSIC, Valencia, Spain
| | - A M Hirt
- Department of Earth Sciences, Swiss Federal Institute of Technology, Zurich, Switzerland
| | - J Janecek
- IEAP, Czech Technical University in Prague, Prague, Czech Republic
| | | | - A Katre
- Section de Physique, Université de Genève, Geneva, Switzerland
| | - D-W Kim
- Physics Department, Gangneung-Wonju National University, Gangneung, Republic of Korea
| | - K Kinoshita
- Physics Department, University of Cincinnati, Cincinnati, Ohio, USA
| | - A Korzenev
- Section de Physique, Université de Genève, Geneva, Switzerland
| | - D H Lacarrère
- Experimental Physics Department, CERN, Geneva, Switzerland
| | - S C Lee
- Physics Department, Gangneung-Wonju National University, Gangneung, Republic of Korea
| | - C Leroy
- Département de physique, Université de Montréal, Québec, Canada
| | - A Lionti
- Section de Physique, Université de Genève, Geneva, Switzerland
| | - J Mamuzic
- IFIC, Universitat de València, CSIC, Valencia, Spain
| | - A Margiotta
- INFN, Section of Bologna & Department of Physics & Astronomy, University of Bologna, Bologna, Italy
| | - N Mauri
- INFN, Section of Bologna, Bologna, Italy
| | - N E Mavromatos
- Physics Department, Theoretical Particle Physics & Cosmology Group, King's College, London, United Kingdom
| | - P Mermod
- Section de Physique, Université de Genève, Geneva, Switzerland
| | - V A Mitsou
- IFIC, Universitat de València, CSIC, Valencia, Spain
| | - R Orava
- Physics Department, University of Helsinki, Helsinki, Finland
| | - B Parker
- The Institute for Research in Schools, Canterbury, United Kingdom
| | - L Pasqualini
- INFN, Section of Bologna & Department of Physics & Astronomy, University of Bologna, Bologna, Italy
| | - L Patrizii
- INFN, Section of Bologna, Bologna, Italy
| | - G E Păvălaş
- Institute of Space Science, Bucharest, Măgurele, Romania
| | - J L Pinfold
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - V Popa
- Institute of Space Science, Bucharest, Măgurele, Romania
| | - M Pozzato
- INFN, Section of Bologna, Bologna, Italy
| | - S Pospisil
- IEAP, Czech Technical University in Prague, Prague, Czech Republic
| | - A Rajantie
- Department of Physics, Imperial College, London, United Kingdom
| | | | - Z Sahnoun
- INFN, Section of Bologna, Bologna, Italy
- Centre for Astronomy, Astrophysics and Geophysics, Algiers, Algeria
| | - M Sakellariadou
- Physics Department, Theoretical Particle Physics & Cosmology Group, King's College, London, United Kingdom
| | - S Sarkar
- Physics Department, Theoretical Particle Physics & Cosmology Group, King's College, London, United Kingdom
| | - G Semenoff
- Department of Physics, University of British Columbia, Vancouver, British Columbia, Canada
| | - A Shaa
- Formerly at Department of Physics and Applied Physics, Nanyang Technological University, Singapore, Singapore
| | - G Sirri
- INFN, Section of Bologna, Bologna, Italy
| | - K Sliwa
- Department of Physics and Astronomy, Tufts University, Medford, Massachusetts, USA
| | - R Soluk
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - M Spurio
- INFN, Section of Bologna & Department of Physics & Astronomy, University of Bologna, Bologna, Italy
| | - Y N Srivastava
- Physics Department, Northeastern University, Boston, Massachusetts, USA
| | - M Suk
- IEAP, Czech Technical University in Prague, Prague, Czech Republic
| | - J Swain
- Physics Department, Northeastern University, Boston, Massachusetts, USA
| | | | - V Togo
- INFN, Section of Bologna, Bologna, Italy
| | - J A Tuszyński
- Physics Department, University of Alberta, Edmonton, Alberta, Canada
| | - V Vento
- IFIC, Universitat de València, CSIC, Valencia, Spain
| | - O Vives
- IFIC, Universitat de València, CSIC, Valencia, Spain
| | - Z Vykydal
- IEAP, Czech Technical University in Prague, Prague, Czech Republic
| | - T Whyntie
- The Institute for Research in Schools, Canterbury, United Kingdom
- Queen Mary University of London, London, United Kingdom
| | - A Widom
- Physics Department, Northeastern University, Boston, Massachusetts, USA
| | - G Willems
- Physics Department, University of Muenster, Muenster, Germany
| | - J H Yoon
- Physics Department, Konkuk University, Seoul, Korea
| | - I S Zgura
- Institute of Space Science, Bucharest, Măgurele, Romania
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Ciuchini M, Masiero A, Silvestrini L, Vempati SK, Vives O. Grand unification of quark and lepton flavor changing neutral currents. Phys Rev Lett 2004; 92:071801. [PMID: 14995839 DOI: 10.1103/physrevlett.92.071801] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/22/2003] [Indexed: 05/24/2023]
Abstract
In the context of supersymmetric grand unified theories with soft breaking terms arising at the Planck scale, it is generally possible to link flavor changing neutral current and CP violating processes occurring in the leptonic and hadronic sectors. We study the correlation between flavor changing squark and slepton mass insertions in models à la SU(5). We show that the constraints coming from lepton flavor violation exhibit a strong impact on CP-violating B decays.
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Affiliation(s)
- M Ciuchini
- INFN, Sezione di Roma III and Dipartimento di Fisica, Università di Roma Tre, Via della Vasca Navale 84, I-00146 Rome, Italy
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8
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Masiero A, Vives O. CP Violation and Flavor Changing Effects in K and B Mesons from Nonuniversal Soft Breaking Terms. Phys Rev Lett 2001; 86:26-29. [PMID: 11136085 DOI: 10.1103/physrevlett.86.26] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 09/08/2000] [Indexed: 05/23/2023]
Abstract
We analyze CP violation and flavor changing effects in a minimal supersymmetric standard model with arbitrary nonuniversal soft breaking. Large flavor changing neutral current effects are naturally expected in the K system, even in the absence of quark-squark flavor misalignment. However, the B system is sensitive to new supersymmetric contributions only if nonuniversality implies, not only different soft terms for the three generations but also a large quark-squark misalignment. The only exceptions are processes with a leading chirality changing contribution proportional to tanbeta (as b-->sgamma).
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Affiliation(s)
- A Masiero
- SISSA-ISAS, Via Beirut 4, I-34013, Trieste, Italy and and INFN, Sezione di Trieste, Trieste, Italy
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9
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Barenboim G, Bernabéu J, Vives O. Left-Handed Neutrino Disappearance Probe of Neutrino Mass and Character. Phys Rev Lett 1996; 77:3299-3302. [PMID: 10062186 DOI: 10.1103/physrevlett.77.3299] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
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