4 December 1996 BRUNO PONTECORVO
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Ninety Years of X-Ray Spectroscopy in Italy 1896-1986
Ninety years of X-ray spectroscopy in Italy 1896-1986 Vanda Bouché1,2, Antonio Bianconi1,3,4 1 Rome Int. Centre Materials Science Superstripes (RICMASS), Via dei Sabelli 119A, 00185Rome, Italy 2 Physics Dept., Sapienza University of Rome, P.le A. Moro 2, 00185 Rome, Italy 3 Institute of Crystallography of Consiglio Nazionale delle Ricerche, IC-CNR, Montero- tondo, Rome, Italy 4 National Research Nuclear University MEPhI (Moscow Engineering Physics Institute), Kashirskoeshosse 31, 115409 Moscow, Russia Ninety years of X-ray spectroscopy research in Italy, from the X-rays dis- covery (1896), and the Fermi group theoretical research (1922-1938) to the Synchrotron Radiation research in Frascati from 1963 to 1986 are here summarized showing a coherent scientific evolution which has evolved into the actual multidisciplinary research on complex phases of condensed mat- ter with synchrotron radiation 1. The early years of X-ray research The physics community was very quick to develop an intense research in Italy on X rays, after the discovery on 5th January, 1896 by Röngten in Munich. Antonio Garbasso in Pisa [1], and then in Rome Alfonso Sella, with Quirino Majorana, Pietro Blaserna and Garbasso, published several papers on Nuovo Cimento [2], starting the Italian experimental school on X-rays research in XIX century [3]. The focus was on the mechanism of the emission by the X-ray tubes, the nature of X-rays (wave or particles), the propagation characteristics in the matter, the absorption and diffusion. Cambridge and Edinburgh at the beginning of the XX century became the world hot spots of X-ray spectroscopy with Charles Barkla who demonstrated the electromagnetic wave nature of X-ray propagation in the vacuum, similar with light and Henry Moseley, who studied the X-ray emission spectra, recorded the X-ray emission lines of most of the elements of the Mendeleev atomic table. -
Franco Rasetti
Franco Rasetti Castiglione del Lago, Italy, 10 August 1901 – Waremme, Belgium, 5 December 2001 Title Professor of Physics, Johns Hopkins University, Baltimore, MD, USA Field Entomology, Physics, Paleontology, Botany Nomination 28 Oct. 1936 Download 1937 biography in Italian Most important awards, prizes and academies Honorary Doctor, Laval University, Quebec (Canada); Honorary Doctor of Law, University of Glasgow; Honorary Research Associate in Paleobiology, Smithsonian Institution (Washington); Socio Nazionale dell’Accademia Nazionale dei Lincei (since 1937); Socio dell’Accademia Nazionale delle Scienze, detta dei XL (since 1937); Medaglia Matteucci dell’Accademia Nazionale delle Scienze (1931); Premio Righi dell’Accademia delle Scienze di Bologna (1932); Premio Mussolini della Reale Accademia d’Italia (1938); Medaglia d’Oro dell’Associazione Laureati Ateneo Pisano (1972); Charles D. Walcott Medal and Award, National Academy of Sciences, Washington (1952); Medaglia dell’Accademia Nazionale delle Scienze (1984); Cavaliere di Gran Croce (1995). Summary of scientific research Professional Career: Doctor’s Degree in Physics, University of Pisa (1921); Assistant in the Physics Department, University of Florence (1921-25); Assistant in the Physics Department, University of Rome (1926-1930); Tenured Professor of Physics, University of Rome (1931-1939); Professor of Physics and Chairman of Physics Department at Laval University, Quebec, Canada (1939-1945); Full Professor of Physics, Johns Hopkins University, Baltimore, Maryland, USA (1946-1966). Summer Lecturer in Physics at Cornell University, Ithaca, N.Y. (1936); Washington University St. Louis, Missouri (1946); University of Washington, Seattle (1955); Instituto Venezolano de Investigaciones Científicas, Caracas (1957), University of Miami, Florida, (1958; 1961). Main publications A) Physics: Rasetti F., Il nucleo Atomico. Zanichelli, Bologna; Rasetti F., Elements of Nuclear Physics. -
Bruno Pontecorvo-Pioneer of Neutrino Oscillations
Bruno Pontecorvo-pioneer of neutrino oscillations S. Bilenky JINR(Dubna) 19.11.2013 I Bruno Pontecorvo was born on August 22 1913 in Pisa (Marina di Pisa) I His father was owner of a textile factory. The factory was founded by Pellegrino Pontecorvo, Bruno grandfather. I After the war during many years the factory was closed and the building was not used. Now the Pisa department of INFN is in the building of the Pontecorvo`s factory. The square before the building is called Largo Bruno Pontecorvo I There were 8 children in the family: 5 brothers and 3 sisters All of them were very successful I Three brothers became famous: I Biologist Guido (the eldest brother) I Physicist Bruno I Movie director Gillo I Bruno entered engineer faculty of Pisa University. However, after two years he decided to switch to physics I From his autobiography. My brother Guido declared authoritatively \Physics! I would like to say that you must go to Rome. In Rome there are Fermi and Rasetti". I Bruno passed through exam that was taken by Fermi and Rasetti and was accepted at the third year of the Faculty of Physics and Mathematics of the Rome University with specialization in experimental physics I First as a student and later as researcher from 1931 till 1936 Bruno worked in the Fermi group I The experiment performed by Amaldi and Pontecorvo lead to the discovery of the effect of slow neutrons, the most important discovery made by the Fermi`s group At that time Bruno was 21 I For the discovery of the effect of slow neutrons Fermi was awarded the Nobel Prize. -
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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. -
Fermi-Glast Rome U. Amaldi 9.5.11.Ppt
INFLUENCE OF FERMI AND HIS ROMAN GROUP ON NUCLEAR AND MEDICAL PHYSICS Ugo Amaldi Universitày Milano Bicocca and TERA Foundation Rome - 9.5.11 - U. Amaldi 1 Photo of a photo Enrico Fermi at 36 Edoardo Amaldi at 80 1936 1988 Rome - 9.5.11 - U. Amaldi 2 The discovery of neutron induced radioactivity Rome - 9.5.11 - U. Amaldi 3 January-March 1934 1933 Christmas holidays: Enrico Fermi and the other “ragazzi di Via Panisperna” at Santa Cristina March 1934: The Joliot-Curies discover artificial radioactivity induced by alfa particles The Institute of Via Panisperna Rome - 9.5.11 - U. Amaldi 4 1934 : Fermi discovery was made with a Be-Rn source. Radon extracted at Laboratorio Fisico della Sanità Pubblica The “Divine Providence” Rome - 9.5.11 - U. Amaldi 5 The third paper iodine isotopes used in nuclear medicine Rome - 9.5.11 - U. Amaldi 6 The efficacy of slow neutrons Rome - 9.5.11 - U. Amaldi 7 October 20, 1934 Rome - 9.5.11 - U. Amaldi 8 October 1934: discovery of artificial radioactivity induced by slow neutrons Discovery: Saturday 20.10.34 (*) First paper: Monday 22.10.34 Patent: Friday 26.10.34 (*) A. De Gregorio : not on October 22! O. D’Agostino E. Segrè E. Amaldi F. Rasetti E. Fermi Rome - 9.5.11 - U. Amaldi + B. Pontecorvo = The boys of Via Panisperna9 Writing the paper Emilio Segrè: “Enrico Fermi physicist” – 1970 Fermi dictated while I wrote. He stood by me; Rasetti, Amaldi and Pontecorvo paced the room excitedly, all making comments at the same time. The din was such that when we left, Amaldi’s maid discreetly asked whether the evening guests were tipsy. -
Dubna, 18 March. Meeting of the Committee of Plenipotentiaries of JINR Member States
Dubna, 18 March. Meeting of the Committee of Plenipotentiaries of JINR Member States Dubna, 21 January 2005. Professor Arthur B. McDonald (left) receives Bruno Pontecorvo Prize-2004 Dubna, 19 February. Meeting of the JINR Finance Committee Dubna, 15 January. The 95th session of the JINR Scientific Council Dubna, 19–20 April. Participants of the meeting of the Programme Advisory Committee for Condensed Matter Physics Dubna, 5–6 April. Meeting of the Programme Advisory Committee for Particle Physics Dubna, 16 April. CERN delegation, headed by CERN Director-General R. Aymar, visits JINR. N. Koulberg, R. Aymar and D. Ellis (first, second and third from right) at the JINR Directorate Minsk, 13 May. Participants of the meeting of the joint expert board on JINR–Belarus projects (from left to right): N. Kazak, V. Katrasev, I. Golutvin, A. Lesnikovich, A. Sissakian, N. Shumeiko, N. Russakovich Beijing (China), 19 August. JINR Director Academician V. Kadyshevsky and Director of the Institute of High Energy Physics (Beijing) Professor Chen Hesheng during the signing of an agreement on JINR–IHEP cooperation Dubna, 15 January. Extraordinary and Plenipotentiary of the South African Republic Mochubela J. Seekoe (second from right) visits JINR Dubna, 5 February. A delegation from Ukraine headed by Plenipotentiary of the Ukrainian government to JINR V. Stognij (second from left) on a visit to JINR Dubna, 10 August. JINR CP Chairman, Plenipotentiary of Belarus to JINR V. Nedilko signs a new edition of the documents that regulate the activities at the Institute Dubna, 17 February. Participants of the 14th meeting of the Joint Steering Committee on BMBF–JINR cooperation Dubna, 26 July. -
Accelerator Disaster Scenarios, the Unabomber, and Scientific Risks
Accelerator Disaster Scenarios, the Unabomber, and Scientific Risks Joseph I. Kapusta∗ Abstract The possibility that experiments at high-energy accelerators could create new forms of matter that would ultimately destroy the Earth has been considered several times in the past quarter century. One consequence of the earliest of these disaster scenarios was that the authors of a 1993 article in Physics Today who reviewed the experi- ments that had been carried out at the Bevalac at Lawrence Berkeley Laboratory were placed on the FBI's Unabomber watch list. Later, concerns that experiments at the Relativistic Heavy Ion Collider at Brookhaven National Laboratory might create mini black holes or nuggets of stable strange quark matter resulted in a flurry of articles in the popular press. I discuss this history, as well as Richard A. Pos- ner's provocative analysis and recommendations on how to deal with such scientific risks. I conclude that better communication between scientists and nonscientists would serve to assuage unreasonable fears and focus attention on truly serious potential threats to humankind. Key words: Wladek Swiatecki; Subal Das Gupta; Gary D. Westfall; Theodore J. Kaczynski; Frank Wilczek; John Marburger III; Richard A. Posner; Be- valac; Relativistic Heavy Ion Collider (RHIC); Large Hadron Collider (LHC); Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; CERN; Unabomber; Federal Bureau of Investigation; nuclear physics; accel- erators; abnormal nuclear matter; density isomer; black hole; strange quark matter; scientific risks. arXiv:0804.4806v1 [physics.hist-ph] 30 Apr 2008 ∗Joseph I. Kapusta received his Ph.D. degree at the University of California at Berkeley in 1978 and has been on the faculty of the School of Physics and Astronomy at the University of Minnesota since 1982. -
Sidney D. Drell Professional Biography
Sidney D. Drell Professional Biography Present Position Professor Emeritus, SLAC National Accelerator Laboratory, Stanford University (Deputy Director before retiring in 1998) Senior Fellow at the Hoover Institution since 1998 Present Activities Member, JASON, The MITRE Corporation Member, Board of Governors, Weizmann Institute of Science, Rehovot, Israel Professional and Honorary Societies American Physical Society (Fellow) - President, 1986 National Academy of Sciences American Academy of Arts and Sciences American Philosophical Society Academia Europaea Awards and Honors Prize Fellowship of the John D. and Catherine T. MacArthur Foundation, November (1984-1989) Ernest Orlando Lawrence Memorial Award (1972) for research in Theoretical Physics (Atomic Energy Commission) University of Illinois Alumni Award for Distinguished Service in Engineering (1973); Alumni Achievement Award (1988) Guggenheim Fellowship, (1961-1962) and (1971-1972) Richtmyer Memorial Lecturer to the American Association of Physics Teachers, San Francisco, California (1978) Leo Szilard Award for Physics in the Public Interest (1980) presented by the American Physical Society Honorary Doctors Degrees: University of Illinois (1981); Tel Aviv University (2001), Weizmann Institute of Science (2001) 1983 Honoree of the Natural Resources Defense Council for work in arms control Lewis M. Terman Professor and Fellow, Stanford University (1979-1984) 1993 Hilliard Roderick Prize of the American Association for the Advancement of Science in Science, Arms Control, and International Security 1994 Woodrow Wilson Award, Princeton University, for “Distinguished Achievement in the Nation's Service” 1994 Co-recipient of the 1989 “Ettore Majorana - Erice - Science for Peace Prize” 1995 John P. McGovern Science and Society Medalist of Sigma Xi 1996 Gian Carlo Wick Commemorative Medal Award, ICSC–World Laboratory 1997 Distinguished Associate Award of U.S. -
Neutrino Physics Was Certainly Major.'Xxii
Neutrino FRANK CLOSE OXFORD UNIVERSITY PRESS OXFORD UNIVERSITY PRESS Great Clarendon Street, Oxford ox2 6dp Oxford University Press is a department of the University of Oxford. It furthers the University's objective of excellence in research, scholarship, and education by publishing worldwide in Oxford New York Auckland Cape Town Dar es Salaam Hong Kong Karachi Kuala Lumpur Madrid Melbourne Mexico City Nairobi New Delhi Shanghai Taipei Toronto With offices in Argentina Austria Brazil Chile Czech Republic France Greece Guatemala Hungary Italy Japan Poland Portugal Singapore South Korea Switzerland Thailand Turkey Ukraine Vietnam Oxford is a registered trade mark of Oxford University Press in the UK and in certain other countries Published in the United States by Oxford University Press Inc., New York ©Frank Close 2010 The moral rights of the author have been asserted Database right Oxford University Press (maker) First published 2010 All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, without the prior permission in writing of Oxford University Press, or as expressly permitted by law, or under terms agreed with the appropriate reprographics rights organization. Enquiries concerning reproduction outside the scope of the above should be sent to the Rights Department, Oxford University Press, at the address above You must not circulate this book in any other binding or cover and you must impose the same condition on any acquirer British Library Cataloguing in Publication Data Data available Library of Congress Cataloging in Publication Data Library of Congress Control Number 2010930302 Typeset by SPI Publisher Services, Pondicherry, India Printed in Great Britain on acid-free paper by Clays Ltd, St Ives ISBN 978-0-19-957459-9 Contents Ray Davis Foreword 1. -
Enrico Fermi: Genius
ANNIVERSARY Enrico Fermi: genius This year marks the centenary of the birth of Enrico Fermi, one of the giants of 20th- • century science, and one of the last physicists to be both an accomplished experimentalist and an influential theorist. Here, Gianni Battimelli of the University of Rome "La Sapienza" traces the life of a genius. Enrico Fermi was born on 29 September 1901 in Rome to a family with no scientific traditions. His passion for natural sciences, and in particular for physics, was stimulated and guided in his school years by an engineer and family friend, Adolph Amidei, who recognized Fermi's exceptional intellectual abilities and suggested admission to Pisa's Scuola Normale Superiore. After finishing high-school studies in Rome, in 1918 Fermi progressed to the prestigious Pisa Institute, after producing for the admission exam an essay on the characteristics of the propagation of sound, the authenticity of which the commissioners initially refused to believe. Studies at Pisa did not pose any particular difficulties for the young Fermi, despite his having to be largely self-taught using mate rial in foreign languages because nothing existed at the time in Fermi's group discovered the Italian on the new physics emerging around relativity and quantum radioactivity induced by theory. In those years in Italy, these new theories were absent from university teaching, and only mathematicians likeTullio Levi-Civita neutrons, instead of the had the knowledge and insight to see their implications. alpha particles used in the Working alone, between 1919 and 1922, Fermi built up a solid competence in relativity, statistical mechanics and the applications Paris experiments. -
The Charm of Theoretical Physics (1958– 1993)?
Eur. Phys. J. H 42, 611{661 (2017) DOI: 10.1140/epjh/e2017-80040-9 THE EUROPEAN PHYSICAL JOURNAL H Oral history interview The Charm of Theoretical Physics (1958{ 1993)? Luciano Maiani1 and Luisa Bonolis2,a 1 Dipartimento di Fisica and INFN, Piazzale A. Moro 5, 00185 Rome, Italy 2 Max Planck Institute for the History of Science, Boltzmannstraße 22, 14195 Berlin, Germany Received 10 July 2017 / Received in final form 7 August 2017 Published online 4 December 2017 c The Author(s) 2017. This article is published with open access at Springerlink.com Abstract. Personal recollections on theoretical particle physics in the years when the Standard Theory was formed. In the background, the remarkable development of Italian theoretical physics in the second part of the last century, with great personalities like Bruno Touschek, Raoul Gatto, Nicola Cabibbo and their schools. 1 Apprenticeship L. B. How did your interest in physics arise? You enrolled in the late 1950s, when the period of post-war reconstruction of physics in Europe was coming to an end, and Italy was entering into a phase of great expansion. Those were very exciting years. It was the beginning of the space era. L. M. The beginning of the space era certainly had a strong influence on many people, absolutely. The landing on the moon in 1969 was for sure unforgettable, but at that time I was already working in Physics and about to get married. My interest in physics started well before. The real beginning was around 1955. Most important for me was astronomy. It is not surprising that astronomy marked for many people the beginning of their interest in science. -
Out from the Cold
books & arts Out from the cold Half-Life: The in Italy, this environment was the catalyst for MI5 started to take a keener interest in his Divided Life of shaping his communist beliefs. Pontecorvo political leanings. After concluding that it was Bruno Pontecorvo, also met his future wife, Marianne Nordblom. “difficult to regard a man with Pontecorvo’s Physicist or Spy War broke out soon after they had their first international outlook and family history child, and following the Nazi occupation of as reliable” for sensitive nuclear projects, a By Frank Close Paris they fled to the USA in 1940. face-saving solution was engineered, in the form of a professorship at the University of BASIC BOOKS: 2015. Liverpool. But Pontecorvo never took this 400 PP. £20 appointment: in that fateful summer of 1950, midway through a family holiday in Italy, he abruptly headed to Stockholm and onwards through Finland to the Soviet Union, only to runo Pontecorvo’s defection to the resurface publicly five years later. Soviet Union in 1950 is one of the more / ALAMY © RIA NOVOSTI What triggered Pontecorvo’s sudden flight? Bsingular events in the history of Cold War There is no smoking gun to prove that he ever science. A talented physicist who had been passed secrets to the Soviet Union. But Close involved in wartime nuclear research, his concludes that the kaleidoscopic body of abrupt decision to flee behind the Iron Curtain facts surrounding his defection only falls into with his family is shrouded in mystery. Was place once one accepts the hypothesis that Pontecorvo a Soviet spy or an idealist looking he had been a spy prior to 1950 — any other to escape anti-communist hysteria in the interpretation requires an unwieldy number of West, consciously choosing to live in Russia? additional explanations, akin to the epicycles In Half-Life, Frank Close, a professor of invoked by medieval astronomers looking to physics at the University of Oxford, sets In the USA, Pontecorvo developed the keep the geocentric model of the Solar System out to answer this question.