First International Four Seas Conference

Total Page:16

File Type:pdf, Size:1020Kb

First International Four Seas Conference CERN 97-06 31 July 1997 XC98FK266 ORGANISATION EUROPEENNE POUR LA RECHERCHE NUCLEAIRE CERN EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH FIRST INTERNATIONAL FOUR SEAS CONFERENCE Trieste, Italy 26 June-1 July 1995 PROCEEDINGS Editors: A.K. Gougas, Y. Lemoigne, M. Pepe-Altarelli, P. Petroff, C.E. Wulz GENEVA 1997 CERN-Service d'information scientifique-RD/975-200O-juiUet 1997 d) Copyright CKRN, Genève. IW7 Propriété littéraire et si'icnlirii|iic réservée Literary and scientific copyrights reserved in all pour tous les pays du monde. Ce document ne countries of the world. This report, or any part peut être reproduit ou traduit en tout ou en of it, may not be reprinted or translated partie sans l'autorisation écrite du Directeur without written permission of the copyright général du CHRN. titulaire du droit d'auteur. holder, the l)irector-(ieneral of CHRN. Dans les cas appropriés, et s'il s'agit d'utiliser However, permission will he freely granted for le document à des lins non commerciales, cette appropriate noncommercial use. autorisation sera volontiers accordée. II any patentable invention or registrable design l.c CHRN ne revendique pas la propriété des is described in the report, (T!RN makes no inventions hrevclablcs et dessins ou modèles claim to properly rights in it but offers it for the susceptibles de dépôt qui pourraient être free use of research institutions, manu- décrits dans le présent document; ceux-ci peu- facturers and others. CHRN, however, may vent être librement utilisés par les instituts de oppose any attempt by a user to claim any recherche, les industriels et autres intéressés. proprietary or patent rights in such inventions Cependant, le CHRN se réserve le droit de or designs as may be described in the present s'opposer à toute revendication qu'un usager document. pourrait faire de la propriété scientifique ou industrielle de toute invention et tout dessin ou modèle décrits dans le présent document. ISSN «007 -X.12X ISHN Ill Abstract The First International Four Seas Conference was held in Trieste, Italy, from June 25th to July 1st, 1995. The principal aim of the Conference was to bring together physicists from the wider Balkan region along with their colleagues from the rest of the world. An overview of the current and future major European and World Physics projects (along with latest experimental results) was presented. Topics included: Physics at FNAL (collider and fixed target), LEP Physics, B and CP violation, presentations from the LHC experiments, AstroParticle Physics, Heavy Ion & Neutrino Physics. Special sessions were devoted to instrumentation projects, to spin-off applications of Particle Physics, while the final session was devoted to presentations connecting Physics and Society. NEXT Introduction Prof. Georges Charpak The idea of this conference was born in the minds of young particle physicists working at CERN. Because of the war in ex-Yugoslavia they witnessed the severing of most links between the physicists from that region of Europe and the rest of the world physics community. They imagined, maybe with some idealism or naivete, that they could help their ex-Yugoslav colleagues, by organizing, as soon as possible, a conference where the physicists of the region would have the possibility to get acquainted with the latest developments in physics and have the opportunity to meet their colleagues who are active in the most important particle physics projects. They did not intend to re-web a network of scientists of the old Yugoslavia but rather to give the physicists in that region the opportunity to renew ties with the world's scientific community. The initiative was well received in general and the immediate agreement by the President of the European Commission, Jacques Delors, gave them a substantive financial support, which permitted the materialization of their idea when it was combined with the logistic support from CERN, the generous help from the local organizations of Trieste and the enthusiastic personal investment of work by a group of people, scientists and non-scientists, at CERN and in some other European laboratories. The organizers thought that the conference would be the first post-war conference. Unfortunately it occurs at a moment when the war is at its peak, so we had to resort to a "neutral" but still symbolic place like Trieste to organize it. Research in physics, like all other cultural activities, is embedded in the people, and the level of grief or hatred reached in this region of Europe is not clearly perceived by those who have been living in peace for fifty years. When I accepted to join the initiators of this venture, I was acutely aware of this major problem because in my youth much reading and personal reflection on the First World War had contributed to the elaboration of my political sensitivity. I had been fascinated by the ease with which leaders entered into the most destructive wars, although they very often shared the same spiritual values, or were even of the same religion, and I had developed when I was young a great respect for the very few who resisted the chauvinistic social pressure. The most inspiring example for a physicist was indeed Albert Einstein. In 1922 he was invited by Paul Langevin to give a series of lectures in Paris. He refused because of his feeling of solidarity with German physicists who were being boycotted by the French. It was under the pressure of his German colleagues that he finally accepted the invitation of his friend Paul Langevin. During his visit to France, he discovered the hostility of the so-called "patriots" who were perturbing his lectures because he came from Berlin. At that time he had long been a Swiss citizen. After having left Germany at the turn of the century because of his deep hostility to the military discipline existing in German high schools, he had studied in Zurich. After fundamental discoveries, he came back to Germany, which by then was the cradle of modern physics, and was a member of the Prussian Academy of Sciences when the 1914 war broke out. He refused to sign an appeal of the Academy of Sciences in support of the noble goals of the coalition led by Germany and had to leave a hostile country. He came back after the war and was made world famous among the public at large by the verification of his theory of general relativity. This irritated strongly a chauvinist fraction of the German public and he was violently attacked for the corruption he introduced into German science with his Jewish physics. A very large meeting hostile to A. Einstein was convened at the Concert Hall of the Berlin Philharmonic Orchestra. It was chaired by Philip Van Lenard, Nobel Prize for Physics in 1905! And it is in these surroundings that Einstein was fighting against the boycott of the German scientists by the scientists of the winning countries. He was giving a beautiful example of intellectual freedom and attachment to principles. At the same time, he was a member of a Committee within the "Society of Nations" in Geneva which was in charge of bringing to light the crimes committed by both sides engaged in the war. VI I like the idea that Albert Einstein is the predecessor of the young physicists who at CERN in 1993 decided to hold this conference. It was necessary to mark a big leap forward to repair this part of Europe which was being destroyed. It was a monstrous cancer which we had to help cure by finding medicines. CERN was ideally placed for these physicists to meet and discuss the problem. At CERN we never ever asked anybody what his father or uncle was doing during the war. As long as he himself was not a war criminal we did not see why anybody in Europe should be denied an equal right to have a creative life. This was the credo of all the people who tried to create a European Community and, despite present difficulties, I believe that a great step forward has been achieved in the last fifty years. A week ago I read a striking article about the son of A. Eichmann, one of the main artisans of the enterprise of the Jews' extermination. He was captured by the Israelis and hung. His son is a respected professor at the University of Heidelberg and a very decent man. He did not try to hide himself or deny the reality as "negationists" do. I cannot imagine anybody aggressing him for deeds beyond his personal responsibility. The collective responsibility of the German people and the German State is something different. It is because present Germany acknowledged the crimes of the German State during World War II that it is now a respected member of the democratic nations. It is in fact a good example for many other nations who are bearing a very strong responsibility in the desperate state of some parts of the world because of brutal behaviour during the times of slavery, colonial conquests, colonial wars, ruthless economic imperialism, and so on. But who would ever admit that their responsibility bears with it some moral obligation for solidarity and repair? This is why I personally consider that the United Nations are rendering a great service to the peoples of the ex-Yugoslavia by instituting a tribunal for war crimes. It is relatively unimportant whether they can catch the criminals and punish them. But in ten, twenty years they will enable the new generations to distance themselves from criminal acts which can be justified by no decent cause. The organizing committee has had to meet the difficulty of bringing together, in a purely scientific conference, peoples from the different regions of ex-Yugoslavia.
Recommended publications
  • Detection of Geoneutrinos: Can We Make the Gnus Work For
    Detection of Geoneutrinos: Can We Make the Gnus Work for Us? John G. Learned Department of Physics and Astronomy, University of Hawaii, 2505 Correa Road, Honolulu, HI 96822 USA The detection of electron anti-neutrinos from natural radioactivity in the earth has been a goal of neutrino researchers for about half a century[21, 22, 23, 24, 25, 26]. It was accomplished by the KamLAND Collaboration in 2005[27], and opens the way towards studies of the Earth’s radioactive content, with very important implications for geology. New detectors are operating (KamLAND[3] and Borexino[2]), building (SNO+[4]) and being proposed (Hanohano, LENA, Earth and others) that will go beyond the initial observation and allow interesting geophysical and geochemical re- search, in a means not otherwise possible. Herein we describe the approaches being taken (large liquid scintillation instruments), the experimental and technical challenges (optical detectors, direc- tionality), and prospects for growth of this field. There is related spinoff in particle physics (neutrino oscillations and hierarchy determination), astrophysics (solar neutrinos, supernovae, exotica), and in the practical matter of remote monitoring of nuclear reactors. PACS numbers: I. INTRODUCTION: GEONEUTRINO STUDIES tivity required demands employment of expensive liquid STARTED scintillators in order to produce significant light (yielding 30-50 times that from a Cherenkov detector) and further, The preceding paper, “Why Geoneutrinos are almost all neutrino directionality is lost. Further, delicate Interesting”[1], really sets the stage for this contribu- care must be taken for radiopurity, now well understood tion to NU2008. McDonough explains that the flux of but not easy. geoneutrinos coming mainly from the natural radioactive The process employed for detection of the anti- decay chains of Uranium and Thorium from throughout neutrinos is the inverse beta decay, used by researchers the earth, serves as a tag for the abundance and loca- since the initial observations of these neutrinos by Cowan tion of these rare isotopes.
    [Show full text]
  • Name Street City ABABULUGU, BIFTU a 309 CAMPUS DR UNIT 3
    Name Street City ABABULUGU, BIFTU A 309 CAMPUS DR UNIT 3 AMHERST NY 14226 ABALIGDI, AYESHA A 161 PRINCETON AVE UNIT 3 AMHERST NY 14226 ABAS, SELWA K 136 PRINCETON AVE UNIT 2 AMHERST NY 14226 ABAZAID, EMAN R 581 ALLENHURST RD UNIT A AMHERST NY 14226 ABBAS, AMMAR 288 ALLENHURST RD AMHERST NY 14226 ABBATE, JOSEPHINE A 166 THISTLE LEA WILLIAMSVILLE NY 14221 ABBATOY, DAVID M 535 BURROUGHS DR AMHERST NY 14226 ABBOTT, ELIZABETH F 293 SARATOGA RD AMHERST NY 14226 ABBOTT, GREGORY N 293 SARATOGA RD AMHERST NY 14226 ABBOTT, JACLYN K 216 BERRYMAN DR AMHERST NY 14226 ABBOTT, JAMES E 334 CALLODINE AVE AMHERST NY 14226 ABBOTT, MARY ROBERTA 519 GROVER CLEVELAND HWY AMHERST NY 14226 ABBOTT, MYLES M 293 SARATOGA RD AMHERST NY 14226 ABDALLAH, BAHI 591 ALLENHURST RD AMHERST NY 14226 ABDELLATIF, IHMAIDAN M 497 ALLENHURST RD AMHERST NY 14226 ABDEL-LATIF, RUBA 497 ALLENHURST RD UNIT A AMHERST NY 14226 ABDULJABBAR, ZAID 533 ALLENHURST RD UNIT B AMHERST NY 14226 ABED, JAWAD K 210 CAPEN BLVD AMHERST NY 14226 ABEDZADEAH, ANIS 72 MEADOW LEA DR AMHERST NY 14226 ABEDZADEH, YOUNES 72 MEADOW LEA DR AMHERST NY 14226 ABEEL, ASHLEY C 326 ROYCROFT BLVD AMHERST NY 14226 ABEEL, JOHN EDMUND 326 ROYCROFT BLVD AMHERST NY 14226 ABEL, BARBARA N 351 CAPEN BLVD AMHERST NY 14226 ABEL, JANE M 356 HUXLEY DR AMHERST NY 14226 ABEL, KEVIN S 356 HUXLEY DR AMHERST NY 14226 ABEL, NANCY J 356 HUXLEY DR AMHERST NY 14226 ABEL, RICHARD C 356 HUXLEY DR AMHERST NY 14226 ABEL-NEAL, SHERYL L 350 WASHINGTON HWY AMHERST NY 14226 ABELS, JOHN R 78 SARGENT DR AMHERST NY 14226 ABELS, LINDSAY E 78 SARGENT
    [Show full text]
  • 1.743 Editors-In-Chief: Juan Luis Gutiérrez-Ch
    Impact Factor: 1.743 May 2020, Vol. 27, No. 3, pp. 225–328 www.cardiologyjournal.org Cardiology Journal 2020, Vol. 27, No. 3, pp. 225–328 Editors-in-Chief: Juan Luis Gutiérrez-Chico Miłosz J. Jaguszewski Section Editors: Krzysztof J. Filipiak José Luis Zamorano Carlo Di Mario Paweł Buszman Heleen van Beusekom Philipp Sommer International Honorary Editor: Thomas F. Lüscher Fang-Yang Huang et al., see figure legend on page 319 ORIGINAL ARTICLES 272 Cardiac sarcoidosis and ventricular arrhythmias. A rare association of a rare disease. A retrospective 230 Reproducibility of quantitative flow ratio: An inter- cohort study from the National Inpatient Sample -core laboratory variability study — Y. Chang et al. and current evidence for management 238 Coronary plaque redistribution after stent — A. Salama et al. implantation is determined by lipid composition: A NIRS-IVUS analysis — T. Roleder et al. 278 Psoriasis is an independent predictor of increased risk of allergic reaction during 246 Echocardiographic assessment of left atrial percutaneous coronary interventions. morphology and function to predict maintenance Big data analysis from the Polish National of sinus rhythm after electrical cardioversion PCI Registry (ORPKI) — Z. Siudak et al. in patients with non-valvular persistent atrial fibrillation and normal function or mild dysfunction of left ventricle — P. Wałek et al. 285 MiR-1/133 attenuates cardiomyocyte apoptosis and electrical remodeling in mice with viral ISSN 1897–5593 254 Significance of congestive heart failure as a cause myocarditis — W. Li et al. of pleural effusion: Pilot data from a large multidisciplinary teaching hospital — P. Korczyński et al. 295 Characteristics of circulating endothelial cells 262 Association between mild thyroid dysfunction obtained from non-ST-segment elevation and clinical outcome in acute coronary syndrome myocardial infarction patients with additional undergoing percutaneous coronary intervention diastolic dysfunction of left ventricle observed — Q.
    [Show full text]
  • Coronary Microvascular Dysfunction
    Journal of Clinical Medicine Review Coronary Microvascular Dysfunction Federico Vancheri 1,*, Giovanni Longo 2, Sergio Vancheri 3 and Michael Henein 4,5,6 1 Department of Internal Medicine, S.Elia Hospital, 93100 Caltanissetta, Italy 2 Cardiovascular and Interventional Department, S.Elia Hospital, 93100 Caltanissetta, Italy; [email protected] 3 Radiology Department, I.R.C.C.S. Policlinico San Matteo, 27100 Pavia, Italy; [email protected] 4 Institute of Public Health and Clinical Medicine, Umea University, SE-90187 Umea, Sweden; [email protected] 5 Department of Fluid Mechanics, Brunel University, Middlesex, London UB8 3PH, UK 6 Molecular and Nuclear Research Institute, St George’s University, London SW17 0RE, UK * Correspondence: [email protected] Received: 10 August 2020; Accepted: 2 September 2020; Published: 6 September 2020 Abstract: Many patients with chest pain undergoing coronary angiography do not show significant obstructive coronary lesions. A substantial proportion of these patients have abnormalities in the function and structure of coronary microcirculation due to endothelial and smooth muscle cell dysfunction. The coronary microcirculation has a fundamental role in the regulation of coronary blood flow in response to cardiac oxygen requirements. Impairment of this mechanism, defined as coronary microvascular dysfunction (CMD), carries an increased risk of adverse cardiovascular clinical outcomes. Coronary endothelial dysfunction accounts for approximately two-thirds of clinical conditions presenting with symptoms and signs of myocardial ischemia without obstructive coronary disease, termed “ischemia with non-obstructive coronary artery disease” (INOCA) and for a small proportion of “myocardial infarction with non-obstructive coronary artery disease” (MINOCA). More frequently, the clinical presentation of INOCA is microvascular angina due to CMD, while some patients present vasospastic angina due to epicardial spasm, and mixed epicardial and microvascular forms.
    [Show full text]
  • Subject Categories
    Subject Categories Click on a Subject Category below: Anthropology Archaeology Astronomy and Astrophysics Atmospheric Sciences and Oceanography Biochemistry and Molecular Biology Business and Finance Cellular and Developmental Biology and Genetics Chemistry Communications, Journalism, Editing, and Publishing Computer Sciences and Technology Economics Educational, Scientific, Cultural, and Philanthropic Administration (Nongovernmental) Engineering and Technology Geology and Mineralogy Geophysics, Geography, and Other Earth Sciences History Law and Jurisprudence Literary Scholarship and Criticism and Language Literature (Creative Writing) Mathematics and Statistics Medicine and Health Microbiology and Immunology Natural History and Ecology; Evolutionary and Population Biology Neurosciences, Cognitive Sciences, and Behavioral Biology Performing Arts and Music – Criticism and Practice Philosophy Physics Physiology and Pharmacology Plant Sciences Political Science / International Relations Psychology / Education Public Affairs, Administration, and Policy (Governmental and Intergovernmental) Sociology / Demography Theology and Ministerial Practice Visual Arts, Art History, and Architecture Zoology Subject Categories of the American Academy of Arts & Sciences, 1780–2019 Das, Veena Gellner, Ernest Andre Leach, Edmund Ronald Anthropology Davis, Allison (William Gluckman, Max (Herman Leakey, Mary Douglas Allison) Max) Nicol Adams, Robert Descola, Philippe Goddard, Pliny Earle Leakey, Richard Erskine McCormick DeVore, Irven (Boyd Goodenough, Ward Hunt Frere Adler-Lomnitz, Larissa Irven) Goody, John Rankine Lee, Richard Borshay Appadurai, Arjun Dillehay, Tom D. Grayson, Donald K. LeVine, Robert Alan Bailey, Frederick George Dixon, Roland Burrage Greenberg, Joseph Levi-Strauss, Claude Barth, Fredrik Dodge, Ernest Stanley Harold Levy, Robert Isaac Bateson, Gregory Donnan, Christopher B. Greenhouse, Carol J. Levy, Thomas Evan Beall, Cynthia M. Douglas, Mary Margaret Grove, David C. Lewis, Oscar Benedict, Ruth Fulton Du Bois, Cora Alice Gumperz, John J.
    [Show full text]
  • History of High-Energy Neutrino Astronomy
    History of high-energy neutrino astronomy C. Spiering DESY, Platanenallee 6, D-15738 Zeuthen, Germany This talk sketches the main milestones of the path towards cubic kilometer neutrino telescopes. It starts with the first conceptual ideas in the late 1950s and describes the emergence of concepts for detectors with a realistic discovery potential in the 1970s and 1980s. After the pioneering project DUMAND close to Hawaii was terminated in 1995, the further development was carried by NT200 in Lake Baikal, AMANDA at the South Pole and ANTARES in the Mediterranean Sea. In 2013, more than half a century after the first concepts, IceCube has discovered extraterrestrial high-energy neutrinos and opened a new observational window to the cosmos { marking a milestone along a journey which is far from being finished. 1 From first concepts to the detection of atmospheric neutrinos The initial idea of neutrino astronomy beyond the solar system rested on two arguments: The first was the expectation that a supernova stellar collapse in our galaxy would be accompanied by an enormous burst of neutrinos in the 5-10 MeV range. The second was the expectation that fast rotating pulsars must accelerate charged particles in their Tera-Gauss magnetic fields. Either in the source or on their way to Earth they must hit matter, generate pions and neutrinos as decay products of the pions. The first ideas to detect cosmic high energy neutrinos underground or underwater date back to the late fifties (see 1 for a detailed history of cosmic neutrino detectors). In the 1960 Annual Review of Nuclear Science, K.
    [Show full text]
  • Characterizing the Diffuse Neutrino Flux with the Future Km3net/ARCA
    Characterizing the diffuse neutrino flux with the future KM3NeT/ARCA detector Charakterisierung des diffusen Neutrinoflusses mit dem zukunftigen¨ KM3NeT/ARCA-Neutrinoteleskop Der Naturwissenschaftlichen Fakultat¨ der Friedrich-Alexander-Universitat¨ Erlangen-Nurnberg¨ zur Erlangung des Doktorgrades Dr. rer. nat. vorgelegt von Thomas Gerhard Georg Heid aus Roth Als Dissertation genehmigt von der Naturwissenschaftlichen Fakultat¨ der Friedrich-Alexander-Universitat¨ Erlangen-Nurnberg¨ Tag der mundlichen¨ Prufung:¨ 13.12.2018 Vorsitzender des Promotionsorgans: Prof. Dr. Georg Kreimer Gutachter: Prof. Dr. Gisela Anton Dr. Paschal Coyle Contents 1 Introduction 6 2 Neutrino physics8 2.1 Neutrino properties...................................8 2.2 Neutrino production...................................8 2.2.1 Neutrinos from astrophysical sources.....................9 2.2.2 Neutrinos produced in the Earth’s atmosphere................. 11 2.3 Neutrino Oscillation................................... 12 2.4 Neutrino interaction................................... 13 2.4.1 Interactions of neutrinos of all kinds of flavor in the neutral current..... 15 2.4.2 Interaction of νe in the charged current..................... 15 2.4.3 Interaction of νµ in the charged current..................... 15 2.4.4 Interactions of ντ in the charged current.................... 16 3 KM3NeT: A worker for neutrino astronomy 18 3.1 KM3NeT........................................ 18 3.2 Future prospects of neutrino astronomy........................ 20 4 Detector Simulation 21 5 Atmospheric
    [Show full text]
  • Using Standard Syste
    PHYSICAL REVIEW D VOLUME 55, NUMBER 10 15 MAY 1997 Cumulative Author Index All authors of papers published so far in the current volume are listed alphabetically with the issue and page numbers following the dash. A more complete index, with the full title listed with each ®rst author's name and subsequent authors cross-referenced, is published in the last issue of the volume. A cumulative author and subject index covering Physical Review A through E, Physical Review Letters, and Reviews of Modern Physics is published annually under separate cover. Abashian, A.Ð͑9͒ 5667 Anderson, Paul R.Ð͑6͒ 3440; ͑10͒ 6116 Badgett, W.Ð͑3͒ 1142; ͑5͒ 2546; Abbasabadi, AliÐ͑9͒ 5647 Anderson, S.Ð͑3͒ R1119; ͑5͒ 2559; ͑9͒ R5263 Abe, F.Ð͑3͒ 1142; ͑5͒ 2546; ͑9͒ R5263 ͑7͒ R3919; ͑9͒ 5273 Baer, HowardÐ͑3͒ 1466; ͑5͒ 3201; Abe, K.Ð͑1͒ 19; ͑5͒ 2533, 2533 Andersson, NilsÐ͑2͒ 468 ͑7͒ 4463 Andreev, Yu. M.Ð͑3͒ 1233 Abel, S. A.Ð͑3͒ 1623 Bagdasarov, S.Ð͑3͒ 1142; ͑5͒ 2546; Anisovich, V. V.Ð͑5͒ 2918 Abney, MarkÐ͑2͒ 582 ͑9͒ R5263 Anninos, PeterÐ͑2͒ 829; ͑4͒ 1948 Abrahams, AndrewÐ͑2͒ 829 Bagger, JonathanÐ͑2͒ 1091 Anselmino, M.Ð͑9͒ 5841 Abt, I.Ð͑5͒ 2533 ͑ ͒ AntilloÂn, ArmandoÐ͑10͒ 6327 Bagger, Jonathan A.Ð 5 3188 Acharya, B. S.Ð͑8͒ R4521 Antoniadis, IgnatiosÐ͑8͒ 4756, 4770 Baier, R.Ð͑7͒ 4344 Achasov, N. N.Ð͑5͒ 2663, 2672 Antoniazzi, L.Ð͑7͒ 3927 Bailey, M. W.Ð͑3͒ 1142; ͑5͒ 2546; Adam, ChristophÐ͑10͒ 6299 Antos, J.Ð͑3͒ 1142; ͑5͒ 2546; ͑9͒ R5263 ͑9͒ R5263 Adhikari, RathinÐ͑6͒ 3836 Antunes, Nuno D.Ð͑2͒ 925 Baird, K. G.Ð͑5͒ 2533 Afanasev, AndreiÐ͑7͒ 4380 Anway-Wiese, C.Ð͑3͒ 1142; ͑5͒ 2546 Baker, JohnÐ͑2͒ 829 Ahlen, S.
    [Show full text]
  • List of Participants
    First name Last name Organization Position Rose Abdollahzadeh Chatham House Research Partnerships Manager David Abulafia Cambridge University Professor Of Mediterranean History Evangelia Achladi General Consulate Of Greece At Constantinople/Sismanoglio Megaro Greek Language Instructor - Librarian Babis Adamantidis Vasiliki Adamidou LIDL Hellas Corporate Communications and CSR Director Katerina Agorogianni The Greek Guiding Association Vice Chair of National Board Eleni Agouridi Stavros Niarchos Foundation Program Officer George Agouridis Stavros Niarchos Foundation Board Member & Group Chief Legal Counsel Kleopatra Alamantariotou Biomimicry Greece/ Nasa Challenge Greece Founder CEO Christina Albanou Spastics' Society of Northern Greece Director Eleni Alexaki US Embassy Cultural Affairs Specialist Maria Alexiou TITAN Cement SA Vasiliki Alexopoulos Stavros Niarchos Foundation Intern Georgios Alexopoulos European Research Institute on Cooperative and Social Enterprises Senior Researcher Ben Altshuler Institute for Digital Archaeology Director Mike Ammann Embassy Of Switzerland Deputy Head Of Mission Virginia Anagnos Goodman Media International Executive Vice President Dora Anastasiadou American Farm School of Thessaloniki -Perrotis College Despina Andrianopoulou American Embassy Protocol Specialist Mayor's Office Communications & Foteini Andrikopoulou City Of Athens Public Relations Advisor Elly Andriopoulou Stavros Niarchos Foundation SNFCC Grant Manager Anastasia Andritsou British Council Head Partnerships & Programmes Sophia Anthopoulou
    [Show full text]
  • Improving Event Classification at Km3net with Orcanet
    Improving event classification at KM3NeT with OrcaNet A thesis submitted in fulfillment of the requirements for Master in Experimental Physics at Universiteit Utrecht Author Enrique Huesca Santiago July, 2019 2 Abstract Neutrino telescopes such as KM3NeT are being built to detect these tiny, elusive particles. In the case of KM3NeT ORCA the aim is to determine the currently unknown neutrino mass hierarchy, which has far reaching implications for scientific research. Distinguishing between the different types of neutrino flavour interactions seen in the detector is critical for this goal. In order to achieve this, Deep-Learning algorithms such as the OrcaNet framework for KM3NeT are being developed and tested. This work consists of an exploration of the performance of this tool for the concrete case of event identification in KM3NeT, and its implications for determining the neutrino mass hierarchy. Here, clear evidence is presented that there is potential for event classification and identification beyond the current binary track-shower scheme, including up to 40% separation for electron neutrino charged current events. Para mamá y papá, los mejores científicos que nunca han sido. Student number: 6310141 Thesis Research Project: 60 ECTS Contact: [email protected] Supervisor: Paul de Jong First Examiner: Raimond Snellings Second Examiner: Alessandro Grelli Word Count: 24966 3 Contents 1 Introduction6 1.1 Motivation.................................6 1.2 Neutrino classification.......................... 10 1.3 Cherenkov Radiation........................... 11 2 Neutrino Physics 12 2.1 Neutrino Discovery............................ 12 2.2 Neutrino Oscillations........................... 14 2.2.1 Neutrino Mixing Formalism................... 14 2.2.2 The Solar Neutrino Problem................... 16 2.2.3 3 flavour neutrino oscillations.................
    [Show full text]
  • Origin and Propagation of Extremely High Energy Cosmic Rays
    To appear in Physics Reports E-Print astro-ph/9811011 Origin and Propagation of Extremely High Energy Cosmic Rays Pijushpani Bhattacharjee1 Indian Institute of Astrophysics, Bangalore-560 034, India. G¨unter Sigl2 Astronomy & Astrophysics Center, Enrico Fermi Institute, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA Abstract Cosmic ray particles with energies in excess of 1020 eV have been detected. The sources as well as the physical mechanism(s) responsible for endowing cosmic ray particles with such enormous energies are unknown. This report gives a review of the physics and astrophysics associated with the questions of origin and propagation of these Extremely High Energy (EHE) cosmic rays in the Universe. After a brief review of the observed cosmic rays in general and their possible sources and acceleration mechanisms, a detailed discussion is given of possible “top-down” (non-acceleration) scenarios of origin of EHE cosmic rays through decay of sufficiently massive particles originating from processes in the early Universe. The massive particles can come from collapse and/or annihilation of cosmic topological defects (such as monopoles, cosmic strings, etc.) associated with Grand Unified Theories or they could be some long- lived metastable supermassive relic particles that were created in the early Universe and are decaying in the current epoch. The highest energy end of the cosmic ray spectrum can thus be used as a probe of new fundamental physics beyond Standard Model. We discuss the role of existing and proposed cosmic ray, gamma-ray and neutrino experiments in this context. We also discuss how observations with next generation experiments of images and spectra of EHE cosmic ray sources can be used to obtain new information on Galactic and extragalactic magnetic fields and possibly their origin.
    [Show full text]
  • An Overview of the Experimental High Energy Activities in Greece Chara
    An overview of the Experimental High Energy Activities in Greece Chara Petridou, Aristotle University of Thessaloniki, Greece [email protected] The Activities An overview of the Experimental High Energy Activities in Greece Greek Experimental HEP Activities Chara Petridou Aristotle University of Thessaloniki Accelarator Non-Accelerator Detector/Acceleratotor Experiments Experiments R&D PhD's 44 PhD's 12 PhD's 3 PhD-students 30 PhD-students 4 PhD-students 2 Accelerator Physics Experiments Accelerator Physics Activities CERN Fermilab Experiments DESY Experiments LHC Exper imen ts nTOF Tevatron-CDF Neutrino Physics HERA-H1/ZEUS PhD's 1 ATLAS CMS ALICE PhD's 1 PhD's 3 PhD-students 2 PhD's 18 PhD's 17 PhD's 3 PhD-students 1 PhD-students 1 PhD-students 10 PhD-students 10 PhD-students 5 Non-Accelerator Physics The Greek ATLAS Project Experiments NKUoA, NTUA, AUTh all three institutes collaborated for the construction of the BIS chambers of the ATLAS Muon sSpectrometer, consisting of 128 MTD Muon chambers Experiments in Greece Experiments at CERN All chambers installed in the ATLAS pit since Dec 2006 NESTOR HELYCON CAST PhD's 4 PhD's 3 PhD's 4 PhD-students 2 PhD-students 2 All chambers commissioned with cosmic rays Ready for data taking C. Kourkoumelis This Conference 3 Demokritos University National Center for University The Greek ATLAS Project CMS in Greece of Athens Scientific Research of Ioannina Preshower • Muon studies: 2008: 17 PhD physicists Participation: Endcap • CMS Preshower (DEMOKRITOS-UoI) ECAL DCS and HV/LV, Bfield control
    [Show full text]