PEOPLE Particle Physicists Recognized by APS Awards
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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. -
Prizes, Fellowships and Scholarships
ESEARCH OPPORTUNITIES ALERT Issue 26: Volume 2 R SCHOLARSHIPS, PRIZES AND FELLOWSHIPS (Quarter: July - September, 2016) A Compilation by the Scholarships & Prizes RESEARCH SERVICES UNIT Early/ Mid Career Fellowships OFFICE OF RESEARCH, INNOVATION AND DEVELOPMENT (ORID), UNIVERSITY OF GHANA Pre/ Post-Doctoral Fellowships Thesis/ Dissertation Funding JUNE 2016 Issue 26: Volume 2: Scholarships, Prizes and Fellowships (July – September, 2016) TABLE OF CONTENT OPPORTUNITIES FOR JULY 2016 DAVID ADLER LECTURESHIP AWARD ............................................................................................................ 15 HAYMAN PRIZE FOR PUBLISHED WORK PERTAINING TO TRAUMATISED CHILDREN AND ADULTS ..................................................................................................................................................................... 15 HANS A BETHE PRIZE ........................................................................................................................................... 16 TOM W BONNER PRIZE IN NUCLEAR PHYSICS ............................................................................................ 17 HERBERT P BROIDA PRIZE .................................................................................................................................. 18 OLIVER E BUCKLEY PRIZE IN CONDENSED MATTER PHYSICS ............................................................... 18 DANNIE HEINEMAN PRIZE FOR MATHEMATICAL PHYSICS.................................................................. -
Annual Report 2013.Pdf
ATOMIC HERITAGE FOUNDATION Preserving & Interpreting Manhattan Project History & Legacy preserving history ANNUAL REPORT 2013 WHY WE SHOULD PRESERVE THE MANHATTAN PROJECT “The factories and bombs that Manhattan Project scientists, engineers, and workers built were physical objects that depended for their operation on physics, chemistry, metallurgy, and other nat- ural sciences, but their social reality - their meaning, if you will - was human, social, political....We preserve what we value of the physical past because it specifically embodies our social past....When we lose parts of our physical past, we lose parts of our common social past as well.” “The new knowledge of nuclear energy has undoubtedly limited national sovereignty and scaled down the destructiveness of war. If that’s not a good enough reason to work for and contribute to the Manhattan Project’s historic preservation, what would be? It’s certainly good enough for me.” ~Richard Rhodes, “Why We Should Preserve the Manhattan Project,” Bulletin of the Atomic Scientists, May/June 2006 Photographs clockwise from top: J. Robert Oppenheimer, General Leslie R. Groves pinning an award on Enrico Fermi, Leona Woods Marshall, the Alpha Racetrack at the Y-12 Plant, and the Bethe House on Bathtub Row. Front cover: A Bruggeman Ranch property. Back cover: Bronze statues by Susanne Vertel of J. Robert Oppenheimer and General Leslie Groves at Los Alamos. Table of Contents BOARD MEMBERS & ADVISORY COMMITTEE........3 Cindy Kelly, Dorothy and Clay Per- Letter from the President..........................................4 -
2018 APS Prize and Award Recipients
APS Announces 2018 Prize and Award Recipients The APS would like to congratulate the recipients of these APS prizes and awards. They will be presented during APS award ceremonies throughout the year. Both March and April meeting award ceremonies are open to all APS members and their guests. At the March Meeting, the APS Prizes and Awards Ceremony will be held Monday, March 5, 5:45 - 6:45 p.m. at the Los Angeles Convention Center (LACC) in Los Angeles, CA. At the April Meeting, the APS Prizes and Awards Ceremony will be held Sunday, April 15, 5:30 - 6:30 p.m. at the Greater Columbus Convention Center in Columbus, OH. In addition to the award ceremonies, most prize and award recipients will give invited talks during the meeting. Some recipients of prizes, awards are recognized at APS unit meetings. For the schedule of APS meetings, please visit http://www.aps.org/meetings/calendar.cfm. Nominations are open for most 2019 prizes and awards. We encourage members to nominate their highly-qualified peers, and to consider broadening the diversity and depth of the nomination pool from which honorees are selected. For nomination submission instructions, please visit the APS web site (http://www.aps.org/programs/honors/index.cfm). Prizes 2018 APS MEDAL FOR EXCELLENCE IN PHYSICS 2018 PRIZE FOR A FACULTY MEMBER FOR RESEARCH IN AN UNDERGRADUATE INSTITUTION Eugene N. Parker University of Chicago Warren F. Rogers In recognition of many fundamental contributions to space physics, Indiana Wesleyan University plasma physics, solar physics and astrophysics for over 60 years. -
3.00Pm CET = 7.00 Am Pacific Time GRAVITATIONAL
PRESS RELEASE IN OCCASION OF THE START OF O3 Embargoed until March 26 – 3.00pm CET = 7.00 am Pacific time GRAVITATIONAL WAVE DETECTORS JOIN FORCES FOR A NEW YEAR-LONG SIGNAL HUNT Cascina (Pisa, Italy) - The Virgo and LIGO detectors are ready to start the new Observing run called O3, lasting a whole year. The hunt for gravitational waves is set to start on April 1st when the European Virgo detector, based in Italy at the European Gravitational Observatory (EGO), and the LIGO twin detectors, located in the state of Washington and Louisiana (USA), will start to take data becoming together the most sensitive gravitational wave observatory to date. During a one-year period the LIGO and Virgo Collaborations will register science data continuously, and the three detectors will operate as a global observatory. Since August 2017, the end of the second observation run O2, the two collaborations have intensively worked on their interferometers to improve the sensitivity and reliability. Scientists have also improved their offline and online data analysis and developed further the procedures for releasing Open Public Alerts: these will within minutes notify the physics and astronomy community when a potential gravitational-wave event is observed. “With our three detectors now operational at a significantly improved sensitivity, the global LIGO-Virgo detector network is expected to make several new detections. Moreover it will allow precise triangulation of the sources of gravitational waves. This will be an important step towards our quest of multi-messenger astronomy”, says Jo van den Brand of Nikhef (the Dutch National Institute for Subatomic Physics) and VU University Amsterdam, who is the spokesperson for the Virgo collaboration. -
New Aspera Roadmap
Astroparticle Physics for Europe ASPERA (& ApPEC) Roadmap Antonio Ferrer IFIC/MINECO Aspera-Spain Coordinator Benasque IMFP 1 June 2012 Astroparticle Physics for Europe > What is ApPEC ? > ApPEC is an European Consortium of funding agencies for Astroparticle Physics Coordination. Astroparticle Physics for Europe ApPEC created in 2001 by the national funding agencies of France, Germany, Italy, the Netherlands and UK. Since then Spain, Belgium, Portugal, Greece, Switzerland and Poland have joined ApPEC aims to Promote and facilitate co-operation within the European Particle Astrophysics (PA) community Develop and promulgate long term strategies for European PA, offering advice to national funding agencies and EU Assist in improving links and co-ordination between European PA and the scientific programmes of organisations such as CERN, ESA, and ESO Express their collective views on AP in appropriate international forums, such as OECD, UNESCO etc. Astroparticle Physics for Europe > What is ASPERA ? > ASPERA is an ERANET, a European network of national government agencies responsible for coordinating and funding research in astroparticle physics. > ASPERA is funded by the European Commission (FP 6) at the level of 2.5 Million € over a three years period. It started in July 2006. > ASPERA arises from the existence of ApPEC (Astroparticle Physics European Coordination). What is ASPERA ? Astroparticle Physics for Europe ‘per aspera ad astra’ www.aspera-eu.org ASPERA-I FP6 ERANET (July2006-July2009, 2.5 M€) Study APP personnel and funding -
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F N E E R W M S I FERMILAB AU.S. DEPARTMENT OF E NERGY L ABORATORY Millie Comes to Fermilab 2 Photo by Reidar Hahn Volume 23 INSIDE: Friday, October 20, 2000 Number 18 4 Saving the Day f 6 Keeping it Cool 10 Continuing Education in the Main Control Room 12 Famous in Sicily 14 Fermilab Award Winners Millie by Judy Jackson It was a special pleasure, Millie Dresselhaus said, to visit the physics f laboratory named in honor of her former teacher at the University of Chicago, Enrico Fermi. During her September 27-28 visit to Fermilab for an onsite DOE review of the laboratory, Dresselhaus, director of the Department of EnergyÕs Office of Science, spoke with respect and affection of the professor she knew during her years as a University of Chicago graduate student, She referred often to FermiÕs legendary concern for graduate students and young physicists. Comes to ItÕs a concern she clearly shares. ÒYoung people are excited about high-energy physics,Ó Dresselhaus said, Òbut there are serious career problems for youth. This is not just a Fermilab problem, but a problem for high-energy physics generally. It can be hard to Fermilab envision a career when there is such a long lead time for experiments. The community will have to address this.Ó As a step in that direction, she began her laboratory visit with a Òfocus groupÓ of Fermilab graduate students and young physicists, to hear what was on their minds and to assure them of her support. The students responded enthusiastically. -
Particle Detectors Lecture Notes
Lecture Notes Heidelberg, Summer Term 2011 The Physics of Particle Detectors Hans-Christian Schultz-Coulon Kirchhoff-Institut für Physik Introduction Historical Developments Historical Development γ-rays First 1896 Detection of α-, β- and γ-rays 1896 β-rays Image of Becquerel's photographic plate which has been An x-ray picture taken by Wilhelm Röntgen of Albert von fogged by exposure to radiation from a uranium salt. Kölliker's hand at a public lecture on 23 January 1896. Historical Development Rutherford's scattering experiment Microscope + Scintillating ZnS screen Schematic view of Rutherford experiment 1911 Rutherford's original experimental setup Historical Development Detection of cosmic rays [Hess 1912; Nobel prize 1936] ! "# Electrometer Cylinder from Wulf [2 cm diameter] Mirror Strings Microscope Natrium ! !""#$%&'()*+,-)./0)1&$23456/)78096$/'9::9098)1912 $%&!'()*+,-.%!/0&1.)%21331&10!,0%))0!%42%!56784210462!1(,!9624,10462,:177%&!(2;! '()*+,-.%2!<=%4*1;%2%)%:0&67%0%&!;1&>!Victor F. Hess before his 1912 balloon flight in Austria during which he discovered cosmic rays. ?40! @4)*%! ;%&! /0%)),-.&1(8%! A! )1,,%2! ,4-.!;4%!BC;%2!;%,!D)%:0&67%0%&,!(7!;4%! EC2F,1-.,%!;%,!/0&1.)%21331&10,!;&%.%2G!(7!%42%!*H&!;4%!A8)%,(2F!FH2,04F%!I6,40462! %42,0%))%2! J(! :K22%2>! L10&4(7! =4&;! M%&=%2;%0G! (7! ;4%! E(*0! 47! 922%&%2! ;%,! 9624,10462,M6)(7%2!M62!B%(-.04F:%40!*&%4!J(!.1)0%2>! $%&!422%&%G!:)%42%&%!<N)42;%&!;4%20!;%&!O8%&3&H*(2F!;%&!9,6)10462!;%,!P%&C0%,>!'4&;!%&! H8%&! ;4%! BC;%2! F%,%2:0G! ,6! M%&&42F%&0! ,4-.!;1,!1:04M%!9624,10462,M6)(7%2!1(*!;%2! -
Bright Prospects for Tevatron Run II
INTERNATIONAL JOURNAL OF HIGH-ENERGY PHYSICS CERN COURIER VOLUME 43 NUMBER 1 JANUARY/FEBRUARY 2003 Bright prospects for Tevatron Run II JLAB Virginia laboratory delivers terahertz light p6 ^^^J Modular and expandable power supplies WÊ H Communications via TCP/IP içert. n_.___910S.CAEN '^^^*aBOKS^^^^ • ÊÊÊ WÊÊÊSêSê É TÏSjj à OPC Server to ease integration in DCS J Directly interfaced to JCOP Framework p " j^pj ^ ^^^^ Wa9neticFie,dand^ ^^HTJHj^^^^^^^^^^^^^^^^^^^^^^E' ' tfHl far IM Éfefi-*il * CAEN: your largest choice of HV & LV )^ H MULTICHANNEL POWER SUPPLIES CONTENTS 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. Editors James Gillies and Christine Sutton CERN, 1211 Geneva 23, Switzerland Email [email protected] Fax+41 (22) 782 1906 Web cerncourier.com COURIER Advisory Board R Landua (Chairman), F Close, E Lillest0l, VOLUME 43 NUMBER 1 JANUARY/FEBRUARY 2003 H Hoffmann, C Johnson, K Potter, P Sphicas Laboratory correspondents: Argonne National Laboratory (US): D Ayres Brookhaven, National Laboratory (US): PYamin Cornell University (US): D G Cassel DESY Laboratory (Germany): Ilka Flegel, P Waloschek Fermi National Accelerator Laboratory (US): Judy Jackson GSI Darmstadt (Germany): G Siegert INFN -
A Half-Century with Solar Neutrinos*
REVIEWS OF MODERN PHYSICS, VOLUME 75, JULY 2003 Nobel Lecture: A half-century with solar neutrinos* Raymond Davis, Jr. Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA and Chemistry Department, Brookhaven National Laboratory, Upton, New York 11973, USA (Published 8 August 2003) Neutrinos are neutral, nearly massless particles that neutrino physics was a field that was wide open to ex- move at nearly the speed of light and easily pass through ploration: ‘‘Not everyone would be willing to say that he matter. Wolfgang Pauli (1945 Nobel Laureate in Physics) believes in the existence of the neutrino, but it is safe to postulated the existence of the neutrino in 1930 as a way say that there is hardly one of us who is not served by of carrying away missing energy, momentum, and spin in the neutrino hypothesis as an aid in thinking about the beta decay. In 1933, Enrico Fermi (1938 Nobel Laureate beta-decay hypothesis.’’ Neutrinos also turned out to be in Physics) named the neutrino (‘‘little neutral one’’ in suitable for applying my background in physical chemis- Italian) and incorporated it into his theory of beta decay. try. So, how lucky I was to land at Brookhaven, where I The Sun derives its energy from fusion reactions in was encouraged to do exactly what I wanted and get paid for it! Crane had quite an extensive discussion on which hydrogen is transformed into helium. Every time the use of recoil experiments to study neutrinos. I imme- four protons are turned into a helium nucleus, two neu- diately became interested in such experiments (Fig. -
Cornell Gets a New Chair
PEOPLE APPOINTMENTS & AWARDS Cornell gets a new chair Two prominent accelerator physicists and Cornell alumni, Helen T Edwards and her husband, Donald A Edwards, have endowed a chair in accelerator physics at Cornell.The chair is named after Boyce D McDaniel, pro fessor emeritus at Cornell. The first holder of the new chair is David L Rubin, professor of physics and director of accelerator physics at Cornell.The donors David Rubin is the first incumbent of the new Boyce McDaniel Chair of Physics at Cornell, asked that the new professorship should be endowed by Helen and Donald Edwards. The chair is named after Boyce D McDaniel. Left awarded to a Cornell faculty member whose to right: Boyce McDaniel, Donald Edwards, David Rubin, Helen Edwards and Maury Tigner, discipline is particle-beam physics and who director of Cornell's Laboratory of Nuclear Studies. would teach both graduate and undergradu ate students in addition to doing research. McDaniel, a previous director of nuclear ingthe commissioning of the Main Ring at Helen Edwards is a 1957 graduate of science at Cornell, was Helen Edwards' thesis Fermilab and providing advice for numerous Cornell, where she also earned her PhD in adviser. Initially a graduate student at Cornell, accelerator projects throughout the US, in 1966. She works at Fermilab and at DESY in he left during the Second World War to join the addition to his notable contributions to the Germany. She played a prominent role in the Manhattan Project and returned to complete accelerator and elementary particle physics construction of Fermilab'sTevatron and has his PhD, joining the faculty in 1946. -
Vol25-Issue6.Pdf
Vancouver Accelerator Conference Michael Craddock, Chairman of the Conference, and Accelerator Research Division Head at the TRIUMF Laboratory gives the opening address at the 1985 Particle Accelerator Conference in Vancouver. He and his colleagues are to be congratulated on the very smooth organization of such a large gathering. Anyone who contends that particle physics is conducted in an ivory tower, not contributing to other fields of science or to humanity at large, should have attended the 1985 Particle Accelerator Confer ence in Vancouver. Over a thou sand participants contributed 781 papers and only a fraction were actually related to accelerators for nigh energy physics. The majority of present developments are in the service of other fields of science, for alternative power sources, for medicine, for industrial applica tions, etc. Nevertheless, it is the spur of high energy physics that has dri ven accelerator technology along. As Burt Richter pointed out, in some fifty years since the first Cockcroft-Walton accelerators were built, accelerator physicists have increased peak machine energies by a factor of a million and have reduced the cost per GeV by a factor of over ten thou larly the machine diameter. ing problems, good cooling and sand. Conference Chairman Mike Though there are variants - with straightforward \)raddock rejoiced in his opening such as two-in-one (both beam ap manufacturing processes. Address that the contributions of ertures in a single yoke) or one-in- Paul Reardon reported on the al the accelerator community had one designs - there are essentially ternative high field type for which been so significantly recognized at two basic magnet types now un the initially separate proposals of the end of the last year with the der consideration.