Advanced Proton Driven Plasma Wakefield Acceleration Experiment at CERN
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CERN Courier–Digital Edition
CERNMarch/April 2021 cerncourier.com COURIERReporting on international high-energy physics WELCOME CERN Courier – digital edition Welcome to the digital edition of the March/April 2021 issue of CERN Courier. Hadron colliders have contributed to a golden era of discovery in high-energy physics, hosting experiments that have enabled physicists to unearth the cornerstones of the Standard Model. This success story began 50 years ago with CERN’s Intersecting Storage Rings (featured on the cover of this issue) and culminated in the Large Hadron Collider (p38) – which has spawned thousands of papers in its first 10 years of operations alone (p47). It also bodes well for a potential future circular collider at CERN operating at a centre-of-mass energy of at least 100 TeV, a feasibility study for which is now in full swing. Even hadron colliders have their limits, however. To explore possible new physics at the highest energy scales, physicists are mounting a series of experiments to search for very weakly interacting “slim” particles that arise from extensions in the Standard Model (p25). Also celebrating a golden anniversary this year is the Institute for Nuclear Research in Moscow (p33), while, elsewhere in this issue: quantum sensors HADRON COLLIDERS target gravitational waves (p10); X-rays go behind the scenes of supernova 50 years of discovery 1987A (p12); a high-performance computing collaboration forms to handle the big-physics data onslaught (p22); Steven Weinberg talks about his latest work (p51); and much more. To sign up to the new-issue alert, please visit: http://comms.iop.org/k/iop/cerncourier To subscribe to the magazine, please visit: https://cerncourier.com/p/about-cern-courier EDITOR: MATTHEW CHALMERS, CERN DIGITAL EDITION CREATED BY IOP PUBLISHING ATLAS spots rare Higgs decay Weinberg on effective field theory Hunting for WISPs CCMarApr21_Cover_v1.indd 1 12/02/2021 09:24 CERNCOURIER www. -
CERN Celebrates Discoveries
INTERNATIONAL JOURNAL OF HIGH-ENERGY PHYSICS CERN COURIER VOLUME 43 NUMBER 10 DECEMBER 2003 CERN celebrates discoveries NEW PARTICLES NETWORKS SPAIN Protons make pentaquarks p5 Measuring the digital divide pl7 Particle physics thrives p30 16 KPH impact 113 KPH impact series VISyN High Voltage Power Supplies When the objective is to measure the almost immeasurable, the VISyN-Series is the detector power supply of choice. These multi-output, card based high voltage power supplies are stable, predictable, and versatile. VISyN is now manufactured by Universal High Voltage, a world leader in high voltage power supplies, whose products are in use in every national laboratory. For worldwide sales and service, contact the VISyN product group at Universal High Voltage. Universal High Voltage Your High Voltage Power Partner 57 Commerce Drive, Brookfield CT 06804 USA « (203) 740-8555 • Fax (203) 740-9555 www.universalhv.com Covering current developments in high- energy physics and related fields worldwide CERN Courier (ISSN 0304-288X) is distributed to member state governments, institutes and laboratories affiliated with CERN, and to their personnel. It is published monthly, except for January and August, in English and French editions. The views expressed are CERN not necessarily those of the CERN management. Editor Christine Sutton CERN, 1211 Geneva 23, Switzerland E-mail: [email protected] Fax:+41 (22) 782 1906 Web: cerncourier.com COURIER Advisory Board R Landua (Chairman), P Sphicas, K Potter, E Lillest0l, C Detraz, H Hoffmann, R Bailey -
A Spectrometer for Proton Driven Plasma Accelerated Electrons at Awake - Recent Developments∗
Proceedings of IPAC2016, Busan, Korea WEPMY024 A SPECTROMETER FOR PROTON DRIVEN PLASMA ACCELERATED ELECTRONS AT AWAKE - RECENT DEVELOPMENTS∗ Lawrence Charles Deacon, Simon Jolly, Fearghus Keeble, UCL, London Aurélie Goldblatt, Stefano Mazzoni, Alexey Petrenko, CERN, Geneva Bartolomej Biskup, CERN, Geneva; Czech Technical University, Prague 6 Matthew Wing, UCL, London; DESY, Hamburg; University of Hamburg, Hamburg Abstract SPECTROMETER DESIGN The AWAKE experiment is to be constructed at the CERN Neutrinos to Gran Sasso facility (CNGS). This will be the first experiment to demonstrate proton-driven plasma wake- field acceleration. The 400 GeV proton beam from the CERN SPS will excite a wakefield in a plasma cell several meters in length. To probe the plasma wakefield, electrons of 10–20 MeV will be injected into the wakefield follow- ing the head of the proton beam. Simulations indicate that electrons will be accelerated to GeV energies by the plasma wakefield. The AWAKE spectrometer is intended to measure both the peak energy and energy spread of these accelerated electrons. Results of beam tests of the scintillator screen Figure 1: A 3D CAD image of the spectrometer system output are presented, along with tests of the resolution of annotated with distances along the z direction from the exit the proposed optical system. The results are used together of the plasma cell to the magnetic centers of magnets, and with a BDSIM simulation of the spectrometer system to pre- the center of the scintillator screen. dict the spectrometer performance for a range of possible accelerated electron distributions. INTRODUCTION RESOLUTION Proton bunches are the most promising drivers of wake- Optical System fields to accelerate electrons to the TeV energy scale in a The resolution of the energy spectrometer will ultimateley single stage. -
Proton Driven Plasma Wakefield Acceleration in AWAKE
Proton Driven Plasma Article submitted to journal Wakefield Acceleration in Subject Areas: AWAKE Plasma Wakefield Acceleration, 1 1 Proton Driven, Electron Acceleration E. Gschwendtner , M. Turner , **Author List Continues Next Page** Keywords: AWAKE, Plasma Wakefield Acceleration, Seeded Self Modulation In this article, we briefly summarize the experiments Author for correspondence: performed during the first Run of the Advanced Insert corresponding author name Wakefield Experiment, AWAKE, at CERN (European e-mail: [email protected] Organization for Nuclear Research). The final goal of AWAKE Run 1 (2013 - 2018) was to demonstrate that 10-20 MeV electrons can be accelerated to GeV- energies in a plasma wakefield driven by a highly- relativistic self-modulated proton bunch. We describe the experiment, outline the measurement concept and present first results. Last, we outline our plans for the future. 1 Continued Author List 2 E. Adli2,A. Ahuja1,O. Apsimon3;4,R. Apsimon3;4, A.-M. Bachmann1;5;6,F. Batsch1;5;6 C. Bracco1,F. Braunmüller5,S. Burger1,G. Burt7;4, B. Buttenschön8,A. Caldwell5,J. Chappell9, E. Chevallay1,M. Chung10,D. Cooke9,H. Damerau1, L.H. Deubner11,A. Dexter7;4,S. Doebert1, J. Farmer12, V.N. Fedosseev1,R. Fiorito13;4,R.A. Fonseca14,L. Garolfi1,S. Gessner1, B. Goddard1, I. Gorgisyan1,A.A. Gorn15;16,E. Granados1,O. Grulke8;17, A. Hartin9,A. Helm18, J.R. Henderson7;4,M. Hüther5, M. Ibison13;4,S. Jolly9,F. Keeble9,M.D. Kelisani1, S.-Y. Kim10, F. Kraus11,M. Krupa1, T. Lefevre1,Y. Li3;4,S. Liu19,N. Lopes18,K.V. Lotov15;16, M. Martyanov5, S. -
A Time of Great Growth
Newsletter | Spring 2019 A Time of Great Growth Heartfelt greetings from the UC Riverside Department of Physics and Astronomy. This is our annual newsletter, sent out each Spring to stay connected with our former students, retired faculty, and friends in the wider community. The Department continues to grow, not merely in size but also in stature and reputation. For the 2018-2019 academic year, we were pleased to welcome two new faculty: Professors Thomas Kuhlman and Barry Barish. Professor Kuhlman was previously on the faculty at the University of Illinois at Urbana-Champaign. He joins our efforts in the emerging field of biophysics. His research lies in the quantitative imaging and theoretical modeling of biological systems. He works on genome dynamics, quantification of the activity of transposable elements in living cells, and applications to the engineering of genome editing. Professor Barry Barish, who joins us from Caltech, is the winner of the 2017 Nobel Prize in Physics. He brings great prestige to our Department. Along with Professor Richard Schrock of the Department of Chemistry, who also joined UCR in 2018, UCR now has two Nobel Prize winners on its faculty. Professor Barish is an expert on the detection and physics of gravitational waves. He has been one of the key figures in the conception, construction, and operation of the LIGO detector, where gravitational waves were first discovered in 2015, and which led to his Nobel Prize. He is a member of the National Academy of Sciences and the winner of many other prestigious awards. The discovery of gravitational waves is one of the most exciting developments in physics so far this century. -
Swapan Chattopadhyay Course Syllabus
NIU PHYSICS 659: Special Problems in Physics, Winter 2016 Instructor: Swapan Chattopadhyay Course Syllabus This is an independent study course involving personalized study, research, problem searching and problem solving in the field of Physics of Beams and Accelerator Science. The enrolled student will perform literature search via the web, available libraries, and references provided by the instructor and identify relevant publications and current up-to-date status of the fields/topics mentioned below, search for potential areas for further exploratory research and list and quantify a limited set of graduate dissertation areas/topics that are mature for getting engaged in. The areas/topics suggested for study/research in this semester are: 1. Theoretical, computational and experimental aspects of nonlinear dynamics of high intensity space-charge dominated proton beams as relevant for future proton accelerators for exploring neutrino physics and possibilities of scaled experiments at the Integrated Optics Test Accelerator (IOTA), under construction at Fermilab. The topics could address theoretical modelling or computer simulation or experimental measurements of nonlinear dynamics, dynamical diffusion, beam halo formation and resonance dynamics in general. 2. Explore and investigate possible research into the design and development of the 100 TeV- class proton collider as envisioned in the Future Circular Collider (FCC) design study at CERN and identify beam dynamics issues relevant for further research e.g. coherent beam instabilities; beam injection dynamics; beam-environment interaction via electromagnetic impedance, beam luminosity, beam lifetime and ring lattice. 3. Explore and investigate possible research into the proton-driven plasma wakefield experiment, AWAKE, under development at CERN. The possible research areas could be around beam-plasma high fidelity simulations, beam injection dynamics, beam and plasma diagnostics and scaling from present experiments to a proper collider. -
The AWAKE Acceleration Scheme for New Particle Physics Experiments at CERN
AWAKE++: the AWAKE Acceleration Scheme for New Particle Physics Experiments at CERN W. Bartmann1, A. Caldwell2, M. Calviani1, J. Chappell3, P. Crivelli4, H. Damerau1, E. Depero4, S. Doebert1, J. Gall1, S. Gninenko5, B. Goddard1, D. Grenier1, E. Gschwendtner*1, Ch. Hessler1, A. Hartin3, F. Keeble3, J. Osborne1, A. Pardons1, A. Petrenko1, A. Scaachi3, and M. Wing3 1CERN, Geneva, Switzerland 2Max Planck Institute for Physics, Munich, Germany 3University College London, London, UK 4ETH Zürich, Switzerland 5INR Moscow, Russia 1 Abstract The AWAKE experiment reached all planned milestones during Run 1 (2016-18), notably the demon- stration of strong plasma wakes generated by proton beams and the acceleration of externally injected electrons to multi-GeV energy levels in the proton driven plasma wakefields. During Run 2 (2021 - 2024) AWAKE aims to demonstrate the scalability and the acceleration of elec- trons to high energies while maintaining the beam quality. Within the Physics Beyond Colliders (PBC) study AWAKE++ has explored the feasibility of the AWAKE acceleration scheme for new particle physics experiments at CERN. Assuming continued success of the AWAKE program, AWAKE will be in the position to use the AWAKE scheme for particle physics ap- plications such as fixed target experiments for dark photon searches and also for future electron-proton or electron-ion colliders. With strong support from the accelerator and high energy physics community, these experiments could be installed during CERN LS3; the integration and beam line design show the feasibility of a fixed target experiment in the AWAKE facility, downstream of the AWAKE experiment in the former CNGS area. The expected electrons on target for fixed target experiments exceeds the electrons on target by three to four orders of magnitude with respect to the current NA64 experiment, making it a very promising experiment in the search for new physics. -
Barry Barish and the Gde: Mission Achievable
INTERVIEW Barry Barish and the GDE: mission achievable The head of the Global Design Effort for a future International Linear Collider talks about challenges past, present and future. Barry Barish likes a challenge. He admits to a complete tendency to go for the difficult in his research – in his view, life is an adventure. Some might say that his most recent challenge would fit well with a certain famous TV series: “Your mission, should you choose to accept it… is to produce a design for the International Linear Collider that includes a detailed design concept, performance assessments, reliable international costing, an industrialization plan, and siting analysis, as well as detector concepts and scope.” Barish did indeed accept the challenge in March 2005, when he became director of the Global Design Effort (GDE) for a proposed International Linear Collider (ILC). He started in a directorate of one – himself – at the head of a “virtual” laboratory of hundreds of physicists and engineers around the globe. To run the “lab” he has set up a small executive committee, which includes three regional directors (for the Americas, Asia and Europe), three project manag- ers and two leading accelerator experts. There are also boards for R&D, change control and design cost. Barish operates from his base at Caltech, where he has been since 1962 and ultimately became Linde Professor of Physics (now emeri- tus). His taste for research challenges became evident in the 1970s, when he was co-spokesperson with Frank Sciulli (also at Caltech) of the “narrow band” neutrino experiment at Fermilab that studied Barish became director of the Global Design Effort for the International weak neutral currents and the quark substructure of the nucleon. -
Gravitational Waves from the Early Universe
Gravitational Waves from the Early Universe Lecture 1A: Gravitational Waves, Theory Kai Schmitz (CERN) Chung-Ang University, Seoul, South Korea j June 2 – 4 1/21 ◦ 1916: Albert Einstein predicts GWs based on his general theory of relativity ◦ 2016: The LIGO/Virgo Collaboration announces the detection of GW150914 ◦ 2017: Nobel Prize in Physics awarded to Rainer Weiss, Barry Barish, and Kip Thorne → Milestone in fundamental physics, triumph of general relativity → Discovery of a new class of astrophysical objects: heavy black holes in binary systems First direct detection of gravitational waves [Nicolle Rager Fuller for sciencenews.org] 2/21 ◦ 2016: The LIGO/Virgo Collaboration announces the detection of GW150914 ◦ 2017: Nobel Prize in Physics awarded to Rainer Weiss, Barry Barish, and Kip Thorne → Milestone in fundamental physics, triumph of general relativity → Discovery of a new class of astrophysical objects: heavy black holes in binary systems First direct detection of gravitational waves [Nicolle Rager Fuller for sciencenews.org] ◦ 1916: Albert Einstein predicts GWs based on his general theory of relativity 2/21 ◦ 2017: Nobel Prize in Physics awarded to Rainer Weiss, Barry Barish, and Kip Thorne → Milestone in fundamental physics, triumph of general relativity → Discovery of a new class of astrophysical objects: heavy black holes in binary systems First direct detection of gravitational waves [Nicolle Rager Fuller for sciencenews.org] ◦ 1916: Albert Einstein predicts GWs based on his general theory of relativity ◦ 2016: The LIGO/Virgo -
The Future Circular Collider (FCC) Project and Its Cryogenic Challenges
The Future Circular Collider (FCC) project and its cryogenic challenges Laurent Tavian, CERN ECD 2017, Karlsruhe, 13 September 2017 Content • Introduction: Scope of the FCC study • FCC-hh tunnel cryogenics and user heat loads • FCC-hh cryogenics layout and architecture • FCC-hh cool-down and nominal operation • FCC-hh electrical consumption and helium inventory • Conclusion Scope of FCC Study International FCC collaboration (CERN as host lab) to study: • pp-collider (FCC-hh) main emphasis, defining infrastructure requirements ~16 T ⇒ 100 TeV pp in 100 km • ~100 km tunnel infrastructure in Geneva area, site specific • e+e- collider (FCC-ee), as potential first step • p-e (FCC-he) option, integration one IP, e from ERL • HE-LHC with FCC-hh technology • CDR for end 2018 Luminosity vs energy of colliders Conventional He I He II 1.E+36 x 7 FCC 1.E+35 HL-LHC ] x 30 1 - LHC 2017 .s 2 1.E+34 - LHC (design) 1.E+33 ISR 1.E+32 LEP2 HERA TeVatron Luminosity [cm LEP1 1.E+31 SppS 1.E+30 0.01 0.1 1 10 100 Centr-of-mass energy [TeV] CERN Collider plan 1980 1985 1990 1995 2000 2005 2010 2015 2020 2025 2030 2035 2040 Construction Physics Upgr LEP Design Proto Construction Physics LHC Design Construction Physics HL-LHC Future Collider Design Proto Construction Physics ~25 years FCC-hh baseline parameters Parameter LHC HL-LHC FCC-hh c.m. energy [TeV] 14 100 Nb3Sn superconducting dipole magnet field [T] 8.33 16 magnets cooled at 1.9 K circumference [km] 26.7 100 luminosity [1034 cm-2.s-1] 1 5 5 29 bunch spacing [ns] 25 25 event / bunch crossing 27 135 170 ~50 mm bunch population [1011] 1.15 2.2 1 norm. -
AWAKE! Allen Caldwell Even Larger Accelerators ?
Swapan Chattopadhyay Symposium April 30, 2021 AWAKE! Allen Caldwell Even larger Accelerators ? Energy limit of circular proton collider given by magnetic field strength. P B R / · Energy gain relies in large part on magnet development Linear Electron Collider or Muon Collider? proton P P Leptons preferred: Collide point particles rather than complex objects But, charged particles radiate energy when accelerated. Power α (E/m)4 Need linear electron accelerator or m large (muon 200 heavier than electron) A plasma: collection of free positive and negative charges (ions and electrons). Material is already broken down. A plasma can therefore sustain very high fields. C. Joshi, UCLA E. Adli, Oslo An intense particle beam, or intense laser beam, can be used to drive the plasma electrons. Plasma frequency depends only on density: Ideas of ~100 GV/m electric fields in plasma, using 1018 W/cm2 lasers: 1979 T.Tajima and J.M.Dawson (UCLA), Laser Electron Accelerator, Phys. Rev. Lett. 43, 267–270 (1979). Using partice beams as drivers: P. Chen et al. Phys. Rev. Lett. 54, 693–696 (1985) Energy Budget: Introduction Witness: Staging Concepts 1010 particles @ 1 TeV ≈ few kJ Drivers: PW lasers today, ~40 J/Pulse FACET (e beam, SLAC), 30J/bunch SPS@CERN 20kJ/bunch Leemans & Esarey, Phys. Today 62 #3 (2009) LHC@CERN 300 kJ/bunch Dephasing 1 LHC driven stage SPS: ~100m, LHC: ~few km E. Adli et al. arXiv:1308.1145,2013 FCC: ~ 1<latexit sha1_base64="TR2ZhSl5+Ed6CqWViBcx81dMBV0=">AAAB7XicbZBNS8NAEIYn9avWr6pHL4tF8FQSEeyx4MVjBfsBbSib7aZdu9mE3YkQQv+DFw+KePX/ePPfuG1z0NYXFh7emWFn3iCRwqDrfjuljc2t7Z3ybmVv/+DwqHp80jFxqhlvs1jGuhdQw6VQvI0CJe8lmtMokLwbTG/n9e4T10bE6gGzhPsRHSsRCkbRWp2BUCFmw2rNrbsLkXXwCqhBodaw+jUYxSyNuEImqTF9z03Qz6lGwSSfVQap4QllUzrmfYuKRtz4+WLbGbmwzoiEsbZPIVm4vydyGhmTRYHtjChOzGptbv5X66cYNvxcqCRFrtjyozCVBGMyP52MhOYMZWaBMi3sroRNqKYMbUAVG4K3evI6dK7qnuX761qzUcRRhjM4h0vw4AaacActaAODR3iGV3hzYufFeXc+lq0lp5g5hT9yPn8Avy+PMg==</latexit> A. Caldwell and K. V. Lotov, Phys. -
Accelerator Programme Evaluation Report
OFFICIAL Accelerator Programme Evaluation Report ACCELERATOR PROGRAMME EVALUATION REPORT 1. Executive Summary 1.1. Accelerator science (i) enables advanced facilities that underpin fields as diverse as nuclear and particle physics, and physical and life sciences; and (ii) develops novel techniques that could revolutionise future research and lead to a wealth of applications. 1.2. Accelerator science within STFC is supported within the National Laboratories and by the Programmes Directorate (PD) programme. The PD programme funds accelerator R&D in universities via the UK’s two accelerator institutes (the Cockcroft and John Adams Institutes), and by fixed contribution to the Accelerator Science and Technology Centre (ASTeC) National Laboratory. 1.3. This review has evaluated the STFC PD funded Accelerators Programme under three financial scenarios (flat cash, and ±10%). The review includes a consideration of the breadth and balance of the programme and its sustainability. 1.4. We find that the UK performs world class accelerator science and is a valued and sought-after international partner. UK scientists lead international collaborations and working groups, develop innovative techniques, produce high impact papers, and leverage international investment in projects. UK accelerator institutes and universities provide world-class training and skilled graduates that move into industry and the public sector, 1.5. This world-leading expertise provides a basis to successfully leverage support and lead work in future projects. For example, the UK’s track record in cryomodules and targetry enabled the UK to successfully bid for BEIS funding and lead this work at Fermilab’s Long Baseline Neutrino Facility (LBNF). We note that this investment dwarfs PD’s total accelerator science budget, and that participation would not otherwise have been possible.