Physics Beyond Colliders at CERN: Beyond the Standard Model Working Group Report
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Freeze-In Dark Matter from a Minimal B-L Model and Possible Grand
PHYSICAL REVIEW D 101, 115022 (2020) Freeze-in dark matter from a minimal B − L model and possible grand unification Rabindra N. Mohapatra1 and Nobuchika Okada 2 1Maryland Center for Fundamental Physics and Department of Physics, University of Maryland, College Park, Maryland 20742, USA 2Department of Physics and Astronomy, University of Alabama, Tuscaloosa, Alabama 35487, USA (Received 5 May 2020; accepted 5 June 2020; published 17 June 2020) We show that a minimal local B − L symmetry extension of the standard model can provide a unified description of both neutrino mass and dark matter. In our model, B − L breaking is responsible for neutrino masses via the seesaw mechanism, whereas the real part of the B − L breaking Higgs field (called σ here) plays the role of a freeze-in dark matter candidate for a wide parameter range. Since the σ particle is unstable, for it to qualify as dark matter, its lifetime must be longer than 1025 seconds implying that the B − L gauge coupling must be very small. This in turn implies that the dark matter relic density must arise from the freeze-in mechanism. The dark matter lifetime bound combined with dark matter relic density gives a lower bound on the B − L gauge boson mass in terms of the dark matter mass. We point out parameter domains where the dark matter mass can be both in the keV to MeV range as well as in the PeV range. We discuss ways to test some parameter ranges of this scenario in collider experiments. Finally, we show that if instead of B − L, we consider the extra Uð1Þ generator to be −4I3R þ 3ðB − LÞ, the basic phenomenology remains unaltered and for certain gauge coupling ranges, the model can be embedded into a five-dimensional SOð10Þ grand unified theory. -
Searches for the Dark Photon at Fixed Target Experiments
New Physics: Sae Mulli, Vol. 66, No. 8, August 2016, pp. 1036∼1044 http://dx.doi.org/10.3938/NPSM.66.1036 Searches for the Dark Photon at Fixed Target Experiments Suyong Choi∗ Department of Physics, Korea University, Seoul 02841, Korea (Received 3 July 2016 : revised 12 July 2016 : accepted 12 July 2016) Recent astrophysical observations provided indirect evidences for sub-GeV, light, dark-matter (DM). A new gauge particle in this mass range could exist as an extra U(1) gauge particle, called the dark photon. The dark photon can mix weakly with a ordinary photon and can mediate interactions of DM. If the dark photon is massive enough, it can decay into a pair of standard- model (SM) particles or DM particles. Light dark-matter particles in the MeV to GeV mass range, as well as in other mass ranges, have not been the subjects of intensive experimental researches. Large statistics is needed to search for dark-photon-mediated interactions. Therefore, high-power accelerators can be used to look for the dark photon. In this article, we review the current status of the experimental searches at various fixed-target experiments and the experiments planned in the near term future. PACS numbers: 12.60.-i, 14.70.Pw Keywords: Dark matter, Standard model, Dark photon, Accelerator, Fixed target experiment I. INTRODUCTION TO DARK PHOTON the regions of interest. Depending on the mass ranges, different experimental techniques are required. For the In 2008, PAMELA experiment reported on the rise WIMP DM, high-energy accelerators, such as the LHC, of the positron to electron ratio in cosmic rays start- are required to extend the mass reach and to have suf- ing from 10 GeV onwards, subsequently confirmed by ficiently high production cross-sections. -
Search for Dark Sector Physics with NA64 Arxiv:2003.07257V1 [Hep-Ph
Search for dark sector physics with NA64 S.N.Gninenko1, N.V. Krasnikov1;2 and V.A.Matveev1;2 1 INR RAS, 117312 Moscow, Russia 2 Joint Institute for Nuclear Research, 141980 Dubna, Russia Аннотация The NA64 experiment consists of two detectors which are planned to be located at the electron (NA64e) and muon (NA64µ) beams of the CERN SPS and start operation after the LHC long-stop 2 in 2021. Its main goals include searches for dark sector physics - particularly light dark matter (LDM), visible and invisible decays of dark photons (A0), and new light particles that could explain the 8Be and gµ − 2 anomalies. Here we review these physics goals, the current status of NA64 including recent results and perspectives of further searches, as well as other ongoing or planned experiments in this field. The main theoretical results on LDM, the problem of the origin of the γ − A0 mixing term and its connection to loop 0 corrections, possible existence of a new light Z coupled to Lµ − Lτ current are also discussed. arXiv:2003.07257v1 [hep-ph] 16 Mar 2020 1 1 Introduction At present the most striking evidence in favour of new physics beyond the Standard model (SM) is the observation of Dark Matter (DM) [1, 2]. The nature of DM is one of challenging questions in physics. If DM is a thermal relic from the hot early Universe then its existence motivates to look for models with nongravitational interactions between dark and ordinary matter. There is a lot of candidates for the role of dark matter [1, 2]. -
Physics Beyond Colliders at CERN: Beyond the Standard Model
EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH (CERN) CERN-PBC-REPORT-2018-007 Physics Beyond Colliders at CERN Beyond the Standard Model Working Group Report J. Beacham1, C. Burrage2,∗, D. Curtin3, A. De Roeck4, J. Evans5, J. L. Feng6, C. Gatto7, S. Gninenko8, A. Hartin9, I. Irastorza10, J. Jaeckel11, K. Jungmann12,∗, K. Kirch13,∗, F. Kling6, S. Knapen14, M. Lamont4, G. Lanfranchi4,15,∗,∗∗, C. Lazzeroni16, A. Lindner17, F. Martinez-Vidal18, M. Moulson15, N. Neri19, M. Papucci4,20, I. Pedraza21, K. Petridis22, M. Pospelov23,∗, A. Rozanov24,∗, G. Ruoso25,∗, P. Schuster26, Y. Semertzidis27, T. Spadaro15, C. Vallée24, and G. Wilkinson28. Abstract: The Physics Beyond Colliders initiative is an exploratory study aimed at exploiting the full scientific potential of the CERN’s accelerator complex and scientific infrastructures through projects complementary to the LHC and other possible future colliders. These projects will target fundamental physics questions in modern particle physics. This document presents the status of the proposals presented in the framework of the Beyond Standard Model physics working group, and explore their physics reach and the impact that CERN could have in the next 10-20 years on the international landscape. arXiv:1901.09966v2 [hep-ex] 2 Mar 2019 ∗ PBC-BSM Coordinators and Editors of this Report ∗∗ Corresponding Author: [email protected] 1 Ohio State University, Columbus OH, United States of America 2 University of Nottingham, Nottingham, United Kingdom 3 Department of Physics, University of Toronto, Toronto, -
FASER: Forward Search Experiment at the LHC
Input to the European Particle Physics Strategy Update 2018-2020 Submitted 18 December 2018 FASER FASER: ForwArd Search ExpeRiment at the LHC FASER Collaboration Akitaka Ariga, Tomoko Ariga, Jamie Boyd,∗ Franck Cadoux, David W. Casper, Yannick Favre, Jonathan L. Feng,y Didier Ferrere, Iftah Galon, Sergio Gonzalez-Sevilla, Shih-Chieh Hsu, Giuseppe Iacobucci, Enrique Kajomovitz, Felix Kling, Susanne Kuehn, Lorne Levinson, Hidetoshi Otono, Brian Petersen, Osamu Sato, Matthias Schott, Anna Sfyrla, Jordan Smolinsky, Aaron M. Soffa, Yosuke Takubo, Eric Torrence, Sebastian Trojanowski, and Gang Zhang Abstract FASER, the ForwArd Search ExpeRiment, is a proposed experiment dedicated to searching for light, extremely weakly-interacting particles at the LHC. Such particles may be produced in the LHC's high-energy collisions in large numbers in the far-forward region and then travel long distances through concrete and rock without interacting. They may then decay to visible particles in FASER, which is placed 480 m downstream of the ATLAS interaction point. In this work, we describe the FASER program. In its first stage, FASER is an extremely compact and inexpensive detector, sensitive to decays in a cylindrical region of radius R = 10 cm and length L = 1:5 m. FASER is planned to be constructed and installed in Long Shutdown 2 and will collect data during Run 3 of the 14 TeV LHC from 2021-23. If FASER is successful, FASER 2, a much larger successor with roughly R ∼ 1 m and L ∼ 5 m, could be constructed in Long Shutdown 3 and collect data during the HL-LHC era from 2026-35. -
Montecarlo Simulations Using GRID
UNIVERSITADEGLISTUDIDITORINO` Facolt`a di Scienze Matematiche, Fisiche e Naturali Dottorato di ricerca in Fisica XVII Ciclo Spin asymmetries for the reaction µD → µΛXat COMPASS: MonteCarlo simulations using GRID Candidato Antonio Amoroso Relatore Prof.ssa Maria Pia Bussa Coordinatore del ciclo Prof. Ezio Menichetti 2002-2004 0.1. Introduction i 0.1 Introduction COMPASS (COmmon Muon and Proton Apparatus for Structure and Spec- troscopy) [1] is a complex experimental apparatus assembled by an interna- tional collaboration of more than 20 Institutions. Two research physics pro- grams have been planned. One centered on muon physics and the other one on hadron physics. COMPASS is a fixed target experiment in the North Area site at CERN. It uses beams produced by the SPS accelerator. The experiment is placed in the EHN2 hall (Bldg. 888) in the Prevessin (F) site of CERN. The purpose of the experiment is the study of the structure and the spectroscopy of hadrons using different high intensity beams of lepton and hadrons with energies ranging from 100 to 200 GeV. The experiment aims to collect large samples of charmed particles. From the measurement of the cross section asymmetry for open charm production in deep inelastic scattering of polarized muons on polarized nucleons, the gluon polarization ∆G will be determined and compared with the available theoretical predictions. Hadron beams are used to study the semi-leptonic decays of charmed doubly charmed baryons. Both measurements will allow to study fundamental prob- lems regarding the hadron structure and to test Heavy Quark Effective Theory (HQET) calculations. Moreover the production of exotic states, which are fore- seen by the QCD but have not yet been established, will investigated. -
Book of Abstracts
WIN2019 The 27th International Workshop on Weak Interactions and Neutrinos. Sunday 02 June 2019 - Saturday 08 June 2019 Bari Book of Abstracts Contents On the interpretation of astrophysical neutrinos ....................... 1 Final results of the CUPID-0 Phase I experiment ....................... 1 The SHiP experiment at CERN ................................. 2 Results from the CUORE experiment ............................. 2 Study of TeV neutrinos in the FASER experiment at the LHC ................ 3 Physics prospects of JUNO ................................... 3 Study of tau-neutrino production at the CERN SPS ..................... 4 Design and Status of the JUNO Experiment .......................... 4 Probing New Physics with Germanium Detectors having sub-keV Sensitivity . 5 The Belle II experiment: early physics and prospect ..................... 5 Directional Dark Matter Search with Nuclear Emulsion ................... 6 Global fit to νµ disappearance data with sterile neutrinos .................. 6 Measurement of the neutron capture cross section on argon with ACED . 7 Status of the search for neutrinoless double-beta decay with GERDA ........... 7 Status of investigations of neutrino properties with the vGEN spectrometer at Kalinin Nu- clear Power Plant ...................................... 8 Relic neutrinos: clustering and consequences for direct detection ............. 8 The ENUBET project ...................................... 9 Atmospheric neutrino spectrum reconstruction with JUNO . 10 Dark Matter searches with Neutrino -
Cern: a European Laboratory for the World
CERN: A EUROPEAN LABORATORY FOR THE WORLD G.K. Mallot CERN THE BEGINNINGS 1949: Proposal by de Broglie to the Eur. Cult. Conf. "the creation of a laboratory or institution where it would be possible to do scientific work, but somehow beyond the framework of the different participating states” “undertake tasks, which, by virtue of their size and cost, were beyond the scope of individual countries" 1952: Interim council: Conseil Européen pour la Recherche Nucléaire left council members : Pierre Auger, Edoardo Amaldi and Lew Kowarski 1953: Geneva chosen as location G. K. Mallot Yamagata/ 24 September 2008 2 THE BEGINNINGS 1954: European Organization for Nuclear Research 12 founding European Member States Belgium, Denmark, France, the Federal Republic of Germany, Greece, Italy, the Netherlands, Norway, Sweden, Switzerland, the United Kingdom, and Yugoslavia foundation stone laying 10 June 1955 by DG Felix Mission: Bloch • provide for collaboration among European States in nuclear research of a pure scientific and fundamental character • have no concern with work for military requirements • the results of its experimental and theoretical work shall be published or otherwise made generally available . G. K. Mallot Yamagata/ 24 September 2008 3 A GOBAL ENDEAVOUR > half of world’s particle physicists G. K. Mallot Yamagata/ 24 September 2008 4 CERN IN NUMBERS 2500 staff 9000 users (192 from Japan) 800 fellows and associates 580 universities, 85 nations Budget 987MCHF (93 GJPY) 20 Member States: Austria, Belgium, Bulgaria, the Czech Republic, Denmark, Finland, France, Germany, Greece, Hungary, Italy, the Netherlands, Norway, Poland, Portugal, 7 Observers: the Slovak Republic, Spain, India, Israel, Japan, Sweden, Switzerland and the Russian Federation, Turkey, the United Kingdom. -
Physics Opportunities for the Fermilab Booster Replacement
FNAL Pub No. goes here Physics Opportunities for the Fermilab Booster Replacement John Arrington,1 Joshua Barrow,2 Brian Batell,3 Robert Bernstein,4 S. J. Brice,4 Ray Culbertson,4 Patrick deNiverville,5 Jeff Eldred,4 Angela Fava,4 Laura Fields,6 Alex 7 4 8 4, 4, 9 Friedland, Andrei Gaponenko, Stefania Gori, Roni Harnik, ∗ Richard J Hill, Daniel M. Kaplan,10 Kevin J. Kelly,4 Tom Kobilarcik,4 Gordan Krnjaic,4 Gabriel Lee,11, 12, 13 B. R. Littlejohn,10 W. C. Louis,5 Pedro Machado,4 William M. Morse,14 David Neuffer,4 Zarko Pavlovic,4 William Pellico,4 Ryan Plestid,4, 9 Maxim Pospelov,15 Eric Prebys,16 Yannis K. Semertzidis,17, 18 M. H. Shaevitz,19 P. Snopok,10 Rex Tayloe,20 R. T. Thornton,5 Oleksandr Tomalak,4, 9 M. Toups,4 Nhan Tran,4 Richard Van de Water,5 Katsuya Yonehara,4 Jacob Zettlemoyer,4 Yi-Ming Zhong,21 Robert Zwaska,4 and Anna Mazzacane4 1Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA 2The University of Tennessee at Knoxville, Department of Physics and Astronomy, 1408 Circle Drive, Knoxville, TN 37996, USA 3University of Pittsburgh, Pittsburgh, PA 15260 4Fermi National Accelerator Laboratory, Batavia, IL, 60510, USA 5Los Alamos National Laboratory, Los Alamos, NM 87545 6Notre Dame 7SLAC 8Department of Physics and Santa Cruz Institute for Particle Physics University of California, Santa Cruz, CA 95064, USA 9University of Kentucky, KY, 40506, USA 10Illinois Institute of Technology, Chicago, IL 60616, USA 11Department of Physics, LEPP, Cornell University, Ithaca, NY 14853, USA 12Department of Physics, Korea -
Simulation of Hydrodynamic Tunneling Induced by High-Energy Proton Beam in Copper by Coupling Computer Codes
PHYSICAL REVIEW ACCELERATORS AND BEAMS 22, 014501 (2019) Editors' Suggestion Simulation of hydrodynamic tunneling induced by high-energy proton beam in copper by coupling computer codes † ‡ Y. Nie,1,* C. Fichera,1 L. Mettler,1, F. Carra,1 R. Schmidt,1, N. A. Tahir,2 A. Bertarelli,1 and D. Wollmann1 1CERN, CH-1211 Geneva 23, Switzerland 2GSI Helmholtzzentrum für Schwerionenforschung, Planckstraße 1, 64291 Darmstadt, Germany (Received 18 October 2018; published 11 January 2019; corrected 31 January 2019) The design of machine protection systems for high-energy accelerators with high-intensity beams requires analyzing a large number of failures leading to beam loss. One of the most serious failures is an accidental impact of a large number of bunches at one location, for example, due to a deflection of the particle beams by the extraction kicker magnets with the wrong strength. The numerical assessment of such an event requires an iterative execution of an energy-deposition code and a hydrodynamic code, in case the hydrodynamic tunneling effect plays an important role in the beam-matter interactions. Such calculations have been performed for the CERN Large Hadron Collider (LHC), since the energy stored in the LHC beams exceeds previous accelerators by 2 orders of magnitude. This was done using the particle shower code FLUKA and the hydrodynamic code BIG2 [Tahir et al., Phys. Rev. STAccel. Beams 15, 051003 (2012)]. Later, simulations for a number of cases for other accelerators at CERN and the Future Circular Collider (FCC) were performed [Tahir et al., Phys. Rev. Accel. Beams 19, 081002 (2016)]. These simulations showed that the penetration depth of the beam in copper or graphite could be an order of magnitude deeper when considering the hydrodynamic tunneling, compared to a static approximation. -
ECFA Newsletter #6
ECFA Newsletter #6 Following the Plenary ECFA meeting, 19 and 20 November 2020 https://indico.cern.ch/event/966397/ Winter 2020 It was a great pleasure for ECFA to endorse the membership of the ECFA Early-Career Research Panel at its meeting on 19 November 2020. The panel, made up mainly of PhD students and postdocs, will discuss all aspects that contribute in a broad sense to the future of the research field of particle physics. To capture what is on their minds and to estaBlish a dialogue with ECFA members, a delegation of early-career researchers will Be invited to Plenary and Restricted ECFA, while the panel will also advise and inform ECFA through regular reports. During the Plenary ECFA meeting, we heard about the progress in developing the Accelerator and Detector R&D Roadmaps. The European Strategy for Particle Physics (ESPP) calls on ECFA to develop a detector R&D roadmap to support proposals at European and national levels, and to achieve the ESPP objectives in a timely manner. The ECFA roadmap panel will develop the roadmap taking into consideration the targeted R&D projects required, as well as transformational Blue-sky R&D relevant to the ESPP. Open symposia, in March or April 2021, are part of the consultation with the community. In parallel, with a view to stepping up accelerator R&D, the European Laboratory Directors Group (LDG) is developing an accelerator R&D roadmap that takes into account a variety of technologies for further development during this decade. The roadmap will set the course for R&D and technology demonstrators to enaBle the development of future facilities that support the scientific objectives of the ESPP. -
NCBJ Annual Report 2018
NARODOWE CENTRUM BADAŃ JĄDROWYCH NATIONAL CENTRE FOR NUCLEAR RESEARCH ANNUAL REPORT 2018 1 LOCATIONS Main site: 30 km from Warsaw 7 A.Sołtana street 05-400 Otwock-Świerk Warsaw site: (divisions BP1, BP2, BP3, BP4) 7 Pasteura street, 02-093 Warsaw Łódź site: (division BP4) 28 Płk. Strzelców Kaniowskich 69, 90-558 Łódź Editors: N. Keeley A. Malinowska Technical editors: G. Swiboda __________________________________________________________________________________________ PL-05-400 Otwock-Świerk, POLAND tel.: 048 22 273 10 01 fax: 048 22 779 34 81 e-mail: [email protected] http://www.ncbj.gov.pl ISSN 2299-2960 2 CONTENTS GENERAL INFORMATION MANAGEMENT OF THE INSTITUTE ............................................................................................................. 5 SCIENTIFIC COUNCIL ...................................................................................................................................... 5 DEPARTMENTS AND DIVISIONS OF THE INSTITUTE ............................................................................... 7 MAIN RESEARCH ACTIVITIES ....................................................................................................................... 8 SCIENTIFIC STAFF OF THE INSTITUTE ...................................................................................................... 10 PROJECTS ......................................................................................................................................................... 13 Grant projects for young Scientists ....................................................................................................................