The Scientific Data and Computing Center At

Total Page:16

File Type:pdf, Size:1020Kb

The Scientific Data and Computing Center At The Scientific Data and Computing Center at BNL Benedikt Hegner, CERN SFT Group Meeting, Nov 2 2019 Outline ● Brookhaven National Laboratory ● Particle Physics at BNL ● Scientific Data and Computing Center New York BNL ~ 100 km 2 Brookhaven National Laboratory (BNL) Founded in 1947 it is the oldest national lab not rooting in the Manhattan project ● First a facility for finding peaceful uses for nuclear power, they quickly decided in ‘48 to build the first proton-accelerator worldwide - the Cosmotron reached its full design energy of 3.3 GeV in 1953 ● Since then one of the leading HEP and NP labs in the US with the Alternating Gradient Synchrotron (AGS) and the Relativistic Heavy Ion Collider (RHIC) ● Based on the accelerator experience, two light sources (NSLS and NSLS-II) ● BNL nowadays is a multi-disciplinary lab covering plenty of High Flux Beam sciences Reactor 3 BNL in numbers ● 21 square kilometers ● 2750 staff ● 4000 guest scientists annually ● > 600M US$ annual budget ● Plenty of facilities ○ RHIC ○ National Synchrotron Light Source II ○ Center for Functional Nanomaterials ○ NASA Space Radiation Laboratory ○ Scientific Data and Computing Center ○ Long Island Solar Farm ○ Accelerator Test Facility ○ Linac Isotope Producer ○ Tandem Van de Graaf Facility ● Coordinating US ATLAS contributions 4 Nobel Prizes connected to BNL in Physics ● 1957 – Chen Ning Yang and Tsung-Dao Lee – parity laws based on Cosmotron measurements in ‘56 ● 1976 – Samuel C. C. Ting – J/Psi particle at the AGS published in ‘74 ● 1980 – James Cronin and Val Logsdon Fitch – CP-violation with the AGS published in ‘63 ● 1988 – Leon M. Lederman, Melvin Schwartz, Jack Steinberger – Muon neutrino with AGS published in `62 ● 2002 – Raymond Davis, Jr. – Solar neutrino detection 5 Nobel Prizes connected to BNL in Chemistry ● 2003 – Roderick MacKinnon – Ion channel with measurements at the NSLS ● 2009 – Venkatraman Ramakrishnan and Thomas A. Steitz – Ribosome function with measurements at the NSLS 6 The First Video Game - Tennis for Two Prepared for an outreach event in 1958 on an analog computer 7 BNL’s Relativistic Heavy-Ion Collider (RHIC) Started in 2000 200 - 500 GeV depending on kind of beam (p or heavy-ion) STAR and PHENIX as major experiments 8 ● Part of the NPP directorate and the Computational Science Initiative (CSI) ● About 40 FTE ● Currently moving from a NPP focussed facility to serving all science communities at BNL ● Extending to supporting more and more off-site efforts ● New, bigger data center in the works [* formerly known as RHIC and ATLAS Computing Facility - RACF] 9 Provided Computing Resources High-Throughput Computing ● ~ 2000 nodes w/ 65000 logical cores ● ~ 970mkHSpec High-Performance Computing ● “Institutional Cluster” ○ 216 * Dual Intel Xeon E5-2695v4 CPUs @ 2.1 GHz - 256 GB DDR4-2400 MHz RAM ○ Dual Tesla K80 GPUs in 1/2 the systems - Dual P100 GPUs in the other half ○ EDR Infiniband ● KNL cluster ○ 142 * Intel Xeon Phi 7230 CPU @ 1.3 GHz - 192 GB DDR4-1200 MHz RAM ○ EDR Infiniband ● ML Cluster ○ 5 * Dual Intel Xeon Gold 6248 CPUs @ 2.5 GHz - 768 GB DDR-2933 MHz RAM ○ EDR Infiniband ML Cluster ○ 8 V100 GPUs (per node) 4kW per node 10 Provided Storage Central Disk Storage ● GPFS based 14 PB with > 1 billion files for HEP & NP ● NSLS-II with additional 1 PB of storage in GPFS ● Based on license cost changes, considering migration to Lustre dCache/XROOTD ● dCache with > 50 PB for ATLAS, Belle II, Phenix and Simons Foundation ● XROOTD with ~ 11 PB total for STAR Tape storage ● ~165 PB total data on tape managed by HPSS Tape Statistics (from Oct 04 - Oct 19) 11 SDCC activities in Particle Physics Serving host-lab experiments at RHIC as Tier-0 ● STAR Data taking ● PHENIX analysis and sPHENIX preparations for 2023 ● Simulation studies for the Electron-Ion Collider (EIC) ○ Decision on site (BNL or Jefferson Lab) still pending ○ Start planned for late 2020s Serving remote experiments ● Tier 1 and Tier 3 for ATLAS at CERN ● (sole) Tier 1 for Belle II at KEK ● Contributions to DUNE Computing 12 What did I do over there? From September 2018 to October 2019 on a sabbatical in Brookhaven serving as ● Deputy Director of the Scientific Data and Computing Center ● US-Belle II Computing Coordinator and Belle II Conditions DB Convener And enjoyed life in busy New York and calm https://www.bnl.gov/newsroom/news.php?a=214486 Long Island :-) about Belle II activities at BNL 13 Belle II Belle II is a b-physics experiment located at KEK in Japan ● Data taking started in 2018 ● Still in ramp-up phase ● Computing Model drastically more distributed than LHC ○ Central services like Data Management and Conditions DB hosted off-site at BNL ○ Collaborative tools and user management served by DESY If there is interest I can talk a bit more about Belle II in a later presentation 14 SDCC Vision for the Future Based on the experience as host-lab and with providing services to off-site experiments, SDCC aims to become a Remote Host Lab/Superfacility for future Physics Experiments, providing ● CPU and Storage Resources ● (Quasi-) online streaming ● (Interactive) Analysis Facilities ● Collaborative Tools Possible future projects are LSST, DUNE or other smaller scale projects 15 Collaborative Tools Last year the SDCC increased the emphasis on collaborative tools, providing and developing for Invenio, Indico, BNLBox, Gitea, Mattermost, remote authentication, JupyterLab Rucio as data management tool for NSLS-II Feature article about Collaborative Tools efforts: Community not yet a notion of https://www.bnl.gov/newsroom/news.php?a=216638 big-data and big-data management 16 JupyterHub I/II Providing JupyterHub instances for several of supported experiments - Both on HTC/HTCondor and HPC/Slurm resources HTCondor batch-spawned instance online for NSLS-II ● Most light-source analysis uses Python-based library developed at BNL ● Link-based notebook sharing/copying between users functional Question of kernel management still under discussion at BNL ● Maintenance by SDCC or experiments/groups? ● Base environment provided, plus custom additions? ○ Could play CVMFS a role here? 17 JupyterHub II/II Example for nanomaterial analysis 18 CVMFS at BNL Based on the various user communities, BNL provides ● A Stratum One with 26 TB of data in 81 replicated repositories ● A Stratum Zero for local experiments and groups ○ 12 local repositories for local experiments and groups ○ Some of the local repository content has now been re-published to OSG via sphenix.opensciencegrid.org ● Service running extremely well, and as expected the Stratum Zero sees almost no direct load from remote ● Other (soon to be) data intense communities at BNL will hopefully take advantage of CVMFS too ○ Part of an effort to exchange knowledge between science domains 19 Interaction between CERN and BNL - Invenio Invenio V3 based custom applications for two different scientific communities National Nuclear Security Administration (NNSD) ● SET, Smuggling Detection and Deterrence Science and Engineering Team (btw - one of the reasons why Cyber Security is so big at BNL) Materials Science community ● GENESIS (Next-Generation Synthesis Center) Expect sPHENIX to utilize Invenio as well Invenio V3 Research Data Management (RDM) SDCC is working to build a research data management platform called InvenioRDM along with CERN and ten other multidisciplinary and commercial institutions 20 Single Sing-On and Federated Access ● The most basic functionality to serve as remote host lab ● The most difficult one to set up ○ Rules, regulations, trust relationships, technical implementations, cyber security ○ Every app behaves differently ○ Kerberos/Shibboleth increasingly difficult ■ Replaced consistently with IPA ● Deployed Keycloak as an SSO/Federated access solution ○ FreeOTP MFA AuthN for interactive apps and services ○ Allows use of ActiveDirectory accounts, IPA accounts, and federated ID via CILogon ● Pioneering interaction with InCommon / CILogon for science community in the US ● A topic of its own being relevant for CERN soon ○ Removal of Microsoft products and active directory will require some rethinking More details in a recent HEPiX presentation by Mizuki Karawasa 21 Other interesting CS activities on Long Island BNL ● Computational Science Initiative invests heavily in GPU research ○ Dedicated GPU training and hackathon once a year ○ Constant consultation for interested users ● Physics Department has a new NPP Software Group focussing on improving exchange between BNL’s physics user groups ○ Sort of BNL’s SFT group ○ Lead by Torre Wenaus Stony Brook University (SBU) ● Institute for Advanced Computational Science covers various fields from Ecology, Materials Science, Physics, Linguistics, … and their data science problems ○ Quite a thrilling atmosphere with plenty of interdiscipliary discussions ○ Since this year I am adjunct professor at the Institute 22 Lessons Learned - a random remark In a computing facility you have a very different view on scientific applications ● You do not care about what it produces, but whether it behaves correctly ● An application is just a state-machine, which you can start/stop/kill/pause/… - and inspect for its status ○ Rarely an application behaves in a sane way ⇒ that’s why containers come so handy ;-) ○ Checkpointing anyone? ● If an application uses 100 % CPU, you want to know, whether ○ It hangs and does crap ○ It is extremely efficient in using resources ● If it crashes, you need to have proper logs to know whether ○ The application crashed (application problem) ○ The computing node or storage system had a problem (site problem) ○ Or some weird combination of the two resulted in a problem ● Let’s try to help our computing colleagues in having an easier life… 23 Comments and Questions? My street at my last day - Halloween :-) 24.
Recommended publications
  • The Physical Tourist Physics and New York City
    Phys. perspect. 5 (2003) 87–121 © Birkha¨user Verlag, Basel, 2003 1422–6944/05/010087–35 The Physical Tourist Physics and New York City Benjamin Bederson* I discuss the contributions of physicists who have lived and worked in New York City within the context of the high schools, colleges, universities, and other institutions with which they were and are associated. I close with a walking tour of major sites of interest in Manhattan. Key words: Thomas A. Edison; Nikola Tesla; Michael I. Pupin; Hall of Fame for GreatAmericans;AlbertEinstein;OttoStern;HenryGoldman;J.RobertOppenheimer; Richard P. Feynman; Julian Schwinger; Isidor I. Rabi; Bronx High School of Science; StuyvesantHighSchool;TownsendHarrisHighSchool;NewYorkAcademyofSciences; Andrei Sakharov; Fordham University; Victor F. Hess; Cooper Union; Peter Cooper; City University of New York; City College; Brooklyn College; Melba Phillips; Hunter College; Rosalyn Yalow; Queens College; Lehman College; New York University; Courant Institute of Mathematical Sciences; Samuel F.B. Morse; John W. Draper; Columbia University; Polytechnic University; Manhattan Project; American Museum of Natural History; Rockefeller University; New York Public Library. Introduction When I was approached by the editors of Physics in Perspecti6e to prepare an article on New York City for The Physical Tourist section, I was happy to do so. I have been a New Yorker all my life, except for short-term stays elsewhere on sabbatical leaves and other visits. My professional life developed in New York, and I married and raised my family in New York and its environs. Accordingly, writing such an article seemed a natural thing to do. About halfway through its preparation, however, the attack on the World Trade Center took place.
    [Show full text]
  • Of Charles D. Ferguson, on Behalf Of
    FEDERATION OF AMERICAN SCIENTISTS T: 202/546-3300 1725 DeSales Street, NW 6th Floor Washington, DC 20036 www.fas.org F: 202/675-1010 [email protected] PRM-70-9 DOCKETED Board of Sponsors (75FR80730) USNRC (PartialList) March 4, 2011 March 7, 2011 (10:30 am) •Pacr Agre * SidnheyAman * Philip W. Anderson *Kenneth J. Arrow To: Secretary, U.S. Nuclear Regulatory Commission OFFICE OF SECRETARY * David Baltimore RULEMAKINGS AND * Bamj Be.....ea Washington, DC 20555-0001 SPaulBerg ADJUDICATIONS STAFF * J. Michael Bishop AT-TN: Rulemakings and Adjudications Staff * Guther Blobel * Nicolaas Bloensbergen * Paul Boyce Ann Pitts Carter Subject: Comment on Docket ID NRC-2010-0372, "Petition for Rulemaking, * Stanley Cohen * Leon N. Cooper Francis Slakey on Behalf of the American Physical Society" * E. J. Corey 'James Cronin * Johann Deismehofer ArmDruyan *RenatoDulbeomo As Board Members of the Federation of American Scientists, an independent, Paul L Ehrlich George Field nonpartisan think tank, we strongly support the petition submitted by the Vat L. Fitch * JeromeI. Friedman American Physical Society that requests proliferation risk assessments become a * Riccardo Giacoani * Walter Gilbert required part of the NRC licensing process. * Alfed G. Gilman " Donald Glaser * Sheldon L. Glashow Marvin L. Goidhergr * Joseph L. Goldstein Emerging nuclear fuel technologies such as laser enrichment of uranium can pose Roger C. L. Gaillemin * L[land H. Hartwell significant proliferation risks due to difficulties in detecting facilities using these * Herbert A. Hauptman " Dudley RKHIaechach technologies. If such technologies are developed without a clear, objective, and * Roald Hoff-aan John P. Hoidren detailed assessment, they can dangerously undermine U.S. nuclear * -l Robert Horvitz * David H.
    [Show full text]
  • Download This Article in PDF Format
    The Second Lepton Family Klaus Winter, CERN The Nobel Prize for Physics for 1988 was awarded to L. Lederman, M. Schwartz and J. Steinberger for work on neutrinos in the early 1960s. In a letter [1] addressed to the "dear radioactive ladies and gentlemen", writ­ ten in December 1930, Wolfgang Pauli proposed, as a "desperate remedy" to save the principle of conservation of energy in beta-decay, the idea of the neutrino, a neutral particle of spin 1/2 and with a mass not larger than 0.01 proton mass. "The continuous beta-spectrum [2] would then become understandable by the assumption that in beta-decay a neutrino is emitted together with the electron, in such a way that the sum of the energies of the neutrino and electron is constant." Pauli did not specify at that time Fig. 1 — A recent photograph taken at CERN of Leon Lederman (left), whether the neutrino was to be ejected Jack Steinberger (centre) and Melvin Schwartz. or created. In his famous paper "An attempt of a theory of beta-decay" [3] the muon not decay into e + at the rate ween 1 and 2 GeV should be achievable. E. Fermi used the neutrino concept of predicted if such a non-locality exis­ Would these synchrotrons though, deli­ Pauli together with the concept of the ted ? ". On this view the muon would vir­ ver enough neutrinos? According to nucleon of Heisenberg. He assumed tually dissociate into W + v, the charged their specifications they should accele­ that in beta-decay a pair comprising an W would radiate a and W + v would rate 1011 protons per second, an unpre­ electron and a neutrino is created, analo­ recombine to an electron.
    [Show full text]
  • CERN Courier Is Distributed to Member-State Governments, Institutes and Laboratories Affiliated with CERN, and to Their Personnel
    I n t e r n at I o n a l J o u r n a l o f H I g H - e n e r g y P H y s I c s CERN COURIERV o l u m e 4 6 n u m b e r 9 n o V e m b e r 2 0 0 6 OPERA makes its grand debut ACCELERATORS COMPUTING NEWS INTERVIEW Laser-wakefield device Business signs up to Stephen Hawking pays reaches 1 GeV p5 work with EGEE p12 a visit to CERN p28 CCENovCover1.indd 1 18/10/06 08:53:59 CERN & ProCurve Networking 15 petabytes of data And a network that can handle it “CERN uses ProCurve Switches because we generate a colossal amount of data, making dependability a top priority.” —David Foster, Communication Systems Group Leader, CERN CERN has joined with ProCurve to build their network based on high-performance security, reliability and flexibility, along with a lifetime warranty.* From the world’s largest applications, to a company-wide email, just think what ProCurve could do for your network. Get a closer look at CERN and the world’s biggest physics experiment. Visit www.hp.com/eur/procurvecern1 *For as long as you own the product, with next-business-day advance replacement (available in most countries). For details, refer to the ProCurve Software License, Warranty and Support booklet at www.hp.com/rnd/support/warranty/index.htm The ProCurve Routing Switch 9300m series, ProCurve Routing Switch 9408sl, ProCurve Switch 8100fl series, and the ProCurve Access Control Server 745wl have a one-year- warranty with extensions available.
    [Show full text]
  • Date: To: September 22, 1 997 Mr Ian Johnston©
    22-SEP-1997 16:36 NOBELSTIFTELSEN 4& 8 6603847 SID 01 NOBELSTIFTELSEN The Nobel Foundation TELEFAX Date: September 22, 1 997 To: Mr Ian Johnston© Company: Executive Office of the Secretary-General Fax no: 0091-2129633511 From: The Nobel Foundation Total number of pages: olO MESSAGE DearMrJohnstone, With reference to your fax and to our telephone conversation, I am enclosing the address list of all Nobel Prize laureates. Yours sincerely, Ingr BergstrSm Mailing address: Bos StU S-102 45 Stockholm. Sweden Strat itddrtSMi Suircfatan 14 Teleptelrtts: (-MB S) 663 » 20 Fsuc (*-«>!) «W Jg 47 22-SEP-1997 16:36 NOBELSTIFTELSEN 46 B S603847 SID 02 22-SEP-1997 16:35 NOBELSTIFTELSEN 46 8 6603847 SID 03 Professor Willis E, Lamb Jr Prof. Aleksandre M. Prokhorov Dr. Leo EsaJki 848 North Norris Avenue Russian Academy of Sciences University of Tsukuba TUCSON, AZ 857 19 Leninskii Prospect 14 Tsukuba USA MSOCOWV71 Ibaraki Ru s s I a 305 Japan 59* c>io Dr. Tsung Dao Lee Professor Hans A. Bethe Professor Antony Hewlsh Department of Physics Cornell University Cavendish Laboratory Columbia University ITHACA, NY 14853 University of Cambridge 538 West I20th Street USA CAMBRIDGE CB3 OHE NEW YORK, NY 10027 England USA S96 014 S ' Dr. Chen Ning Yang Professor Murray Gell-Mann ^ Professor Aage Bohr The Institute for Department of Physics Niels Bohr Institutet Theoretical Physics California Institute of Technology Blegdamsvej 17 State University of New York PASADENA, CA91125 DK-2100 KOPENHAMN 0 STONY BROOK, NY 11794 USA D anni ark USA 595 600 613 Professor Owen Chamberlain Professor Louis Neel ' Professor Ben Mottelson 6068 Margarldo Drive Membre de rinstitute Nordita OAKLAND, CA 946 IS 15 Rue Marcel-Allegot Blegdamsvej 17 USA F-92190 MEUDON-BELLEVUE DK-2100 KOPENHAMN 0 Frankrike D an m ar k 599 615 Professor Donald A.
    [Show full text]
  • 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!
    [Show full text]
  • Scientific and Related Works of Chen Ning Yang
    Scientific and Related Works of Chen Ning Yang [42a] C. N. Yang. Group Theory and the Vibration of Polyatomic Molecules. B.Sc. thesis, National Southwest Associated University (1942). [44a] C. N. Yang. On the Uniqueness of Young's Differentials. Bull. Amer. Math. Soc. 50, 373 (1944). [44b] C. N. Yang. Variation of Interaction Energy with Change of Lattice Constants and Change of Degree of Order. Chinese J. of Phys. 5, 138 (1944). [44c] C. N. Yang. Investigations in the Statistical Theory of Superlattices. M.Sc. thesis, National Tsing Hua University (1944). [45a] C. N. Yang. A Generalization of the Quasi-Chemical Method in the Statistical Theory of Superlattices. J. Chem. Phys. 13, 66 (1945). [45b] C. N. Yang. The Critical Temperature and Discontinuity of Specific Heat of a Superlattice. Chinese J. Phys. 6, 59 (1945). [46a] James Alexander, Geoffrey Chew, Walter Salove, Chen Yang. Translation of the 1933 Pauli article in Handbuch der Physik, volume 14, Part II; Chapter 2, Section B. [47a] C. N. Yang. On Quantized Space-Time. Phys. Rev. 72, 874 (1947). [47b] C. N. Yang and Y. Y. Li. General Theory of the Quasi-Chemical Method in the Statistical Theory of Superlattices. Chinese J. Phys. 7, 59 (1947). [48a] C. N. Yang. On the Angular Distribution in Nuclear Reactions and Coincidence Measurements. Phys. Rev. 74, 764 (1948). 2 [48b] S. K. Allison, H. V. Argo, W. R. Arnold, L. del Rosario, H. A. Wilcox and C. N. Yang. Measurement of Short Range Nuclear Recoils from Disintegrations of the Light Elements. Phys. Rev. 74, 1233 (1948). [48c] C.
    [Show full text]
  • 1 Restoring Scientific Integrity in Policy Making February 18, 2004
    Restoring Scientific Integrity in Policy Making February 18, 2004 Science, like any field of endeavor, relies on freedom of inquiry; and one of the hallmarks of that freedom is objectivity. Now, more than ever, on issues ranging from climate change to AIDS research to genetic engineering to food additives, government relies on the impartial perspective of science for guidance. President George H.W. Bush, April 23, 1990 Successful application of science has played a large part in the policies that have made the United States of America the world’s most powerful nation and its citizens increasingly prosperous and healthy. Although scientific input to the government is rarely the only factor in public policy decisions, this input should always be weighed from an objective and impartial perspective to avoid perilous consequences. Indeed, this principle has long been adhered to by presidents and administrations of both parties in forming and implementing policies. The administration of George W. Bush has, however, disregarded this principle. When scientific knowledge has been found to be in conflict with its political goals, the administration has often manipulated the process through which science enters into its decisions. This has been done by placing people who are professionally unqualified or who have clear conflicts of interest in official posts and on scientific advisory committees; by disbanding existing advisory committees; by censoring and suppressing reports by the government’s own scientists; and by simply not seeking independent scientific advice. Other administrations have, on occasion, engaged in such practices, but not so systematically nor on so wide a front. Furthermore, in advocating policies that are not scientifically sound, the administration has sometimes misrepresented scientific knowledge and misled the public about the implications of its policies.
    [Show full text]
  • Melvin Schwartz 1932-2006
    MELVIN SCHWARTZ 1932-2006 A Biographical Memoir by N. P. SAMIOS AND P. YAMIN © 2012 The National Academy of Sciences Any opinions expressed in this memoir are those of the authors and do not necessarily reflect the views of the National Academy of Sciences. MELVIN SCHWARTZ Courtesy of Brookhaven National Laboratories. November 2, 1932–August 28, 2006 BY N. P. SAMIOS AND P. YAMIN MEL SCHWARTZ DIED ON August 28, 2006, in Twin Falls, Idaho. He was born on 1 November 2, 1932, in New York City. He grew up in the Great Depression, but with a sense of optimism and desire to use his mind for the betterment of human- kind. He entered the Bronx High School of Science in the fall of 1945. It was there that his interest in physics began and that he recognized the importance of interactions with peers in determining his sense of direction in life. One of his classmates and future colleagues recalled that “even then” he wanted a Nobel Prize. Mel noted: My interest in physics began at the age of 12 when I entered the Bronx High School of Science. The four years I spent there were certainly among the most exciting and stimulating in my life, mostly because of the interaction with the other students of similar background, interest, and ability. MELVIN SCHWARTZ MELVIN On Sunday afternoons he attended a school run by the secular and Zionist Yiddish and many others. As Mel commented, “This faculty [was] at this time unmatched by any in the world, largely Nationaler Arbeter Farband (Jewish National Workers Alliance).
    [Show full text]
  • Dzhelepov Laboratory of Nuclear Problems
    Dzhelepov Laboratory of Nuclear Problems Dmitry V.Naumov Presented by O.Smirnov Dubna JINR New elements 102, {103, 104, 105(Db), 107}, 114, 115, 116, 117, 118 are synthesized Hypothesis of neutrino oscillations (1957г.) New particles: anti-sigma- minus hyperon And many other discoveries JINR Employed ~ 5000: 1200 - scientists, 2000 - engineers 7 labs. Each lab is as a big research institute 18 member-states and 6 associated members 1500 scientific publications Collaboration with 700 scientific centers and universities in 64 countries Expected budget in 2017-2023 1, 472 billion USD History ● May, 7 1946. First discussion of «construction of a power cyclotron» at special committee of the government ● 18 August 1946. Soviet government approved the proposal of Academician Igor Kurchatov to construct in USSR „the installation M” for fundamental studies in nuclear physics. ● 14 December 1949. The 480 MeV proton synchrocyclotron started operation at the Hydrotechnical Laboratory in Dubna, the most powerful accelerator in the world at that time. ● 26 March 1956. Laboratory of Nuclear Problems of JINR has been founded. M.G.Meshcheryakov Synchrocyclotron 680 MeV (1953) Discoveries Half of discoveries (37) in physics recorded in Soviet Union belongs to JINR 15 of these belongs to LNP Nowadays DLNP researchers are also awarded for important discoveries. Discoveries → New Technologies→ Discoveries LNP a laboratory with largest diversity → origin of most of laboratories in JINR Institute of Nuclear Problems (now DLNP) + Electrophysical laboratory (now
    [Show full text]
  • Muonium Gravity Seminar Wichita-6-17
    Antimatter Gravity MICE-U.S. Plans withDaniel Muons M. Kaplan US Spokesperson, MICE Collaboration Daniel M. Kaplan Physics Seminar WichitaMuTAC State Review Univ. June Fermilab16, 2017 16–17 March, 2006 Outline • Dramatis Personae • A Bit of History - antimatter, the baryon asymmetry of the universe, and all that... • The Ideas, The Issues, The Opportunities • Required R&D • Conclusions Our story’s a bit complicated, so please bear with me! ...and stop me if you have a question! D. M. Kaplan, IIT An#ma&er Gravity Seminar 2/41 Matter & Energy • After many decades of experimentation with subatomic particles, we now know whatDramatis everything is made of... Personae Baryons & antibaryons : p== uud & p uud ΛΛ==uds & uds ... Mesons : K00== ds & K ds B00== db & B db B+ == ub & B− ub ... ∓ ∓ ∓ Leptons : e , µ , τ , ν’s D. M. Kaplan, IIT An#ma&er Gravity Seminar 3/41 Matter & Energy • After many decades of experimentation with subatomic particles, we now know whatDramatis everything is made of... Personae “Imperfect mirror” Baryons & antibaryons : Antip== uud & p uud ΛΛ==uds & uds ... Mesons : Anti K00== ds & K ds B00== db & B db Anti B+ == ub & B− ub ... Antimatter Leptons : e∓, µ∓, τ∓, ν’s • And, don’t forget: antimatter and matter annihilate on contact D. M. Kaplan, IIT An#ma&er Gravity Seminar 3/41 Outline • Dramatis Personae ➡ • A Bit of History - antimatter, the baryon asymmetry of the universe, and all that... • The Ideas, The Issues, The Opportunities • Muonium Gravity Experiment • Required R&D • Conclusions D. M. Kaplan, IIT An#ma&er Gravity Seminar 4/41 Our story begins with..
    [Show full text]
  • Liste Der Nobelpreisträger
    Physiologie Wirtschafts- Jahr Physik Chemie oder Literatur Frieden wissenschaften Medizin Wilhelm Henry Dunant Jacobus H. Emil von Sully 1901 Conrad — van ’t Hoff Behring Prudhomme Röntgen Frédéric Passy Hendrik Antoon Theodor Élie Ducommun 1902 Emil Fischer Ronald Ross — Lorentz Mommsen Pieter Zeeman Albert Gobat Henri Becquerel Svante Niels Ryberg Bjørnstjerne 1903 William Randal Cremer — Pierre Curie Arrhenius Finsen Bjørnson Marie Curie Frédéric John William William Mistral 1904 Iwan Pawlow Institut de Droit international — Strutt Ramsay José Echegaray Adolf von Henryk 1905 Philipp Lenard Robert Koch Bertha von Suttner — Baeyer Sienkiewicz Camillo Golgi Joseph John Giosuè 1906 Henri Moissan Theodore Roosevelt — Thomson Santiago Carducci Ramón y Cajal Albert A. Alphonse Rudyard \Ernesto Teodoro Moneta 1907 Eduard Buchner — Michelson Laveran Kipling Louis Renault Ilja Gabriel Ernest Rudolf Klas Pontus Arnoldson 1908 Metschnikow — Lippmann Rutherford Eucken Paul Ehrlich Fredrik Bajer Theodor Auguste Beernaert Guglielmo Wilhelm Kocher Selma 1909 — Marconi Ostwald Ferdinand Lagerlöf Paul Henri d’Estournelles de Braun Constant Johannes Albrecht Ständiges Internationales 1910 Diderik van Otto Wallach Paul Heyse — Kossel Friedensbüro der Waals Allvar Maurice Tobias Asser 1911 Wilhelm Wien Marie Curie — Gullstrand Maeterlinck Alfred Fried Victor Grignard Gerhart 1912 Gustaf Dalén Alexis Carrel Elihu Root — Paul Sabatier Hauptmann Heike Charles Rabindranath 1913 Kamerlingh Alfred Werner Henri La Fontaine — Robert Richet Tagore Onnes Theodore
    [Show full text]