Industrial Patents and the Production of Isotopes, 1930-1960
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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. -
The Accademia Nazionale Dei Lincei Founded in 1603, the Accademia
THE XXI EDOARDO AMALDI CONFERENCE INTERNATIONAL COOPERATION FOR ENHANCING NUCLEAR SAFETY, SECURITY, SAFEGUARDS AND NON-PROLIFERATION ACCADEMIA NAZIONALE DEI LINCEI ROME, 7 – 8 OCTOBER 2019 ITALY The Accademia Nazionale dei Lincei Founded in 1603, the Accademia Nazionale dei Lincei is the oldest academy in the world which included, among many other prestigious names, Galileo Galilei. The Accademia Nazionale dei Lincei is within the sphere of the Italian Ministry of Cultural Heritage and is considered the highest Italian cultural institution. The Accademia Nazionale dei Lincei is a scientific consultant to the President of the Italian Republic and has recently been granted his High Permanent Patronage. The Accademia Nazionale dei Lincei mission is to promote, coordinate, integrate and spread scientific knowledge in its highest expressions, in the frame of cultural unity and universality. To this end, the Accademia Nazionale dei Lincei organises national and international conferences, meetings and seminars. The United States National Academy of Sciences Established by an Act of Congress signed by President Abraham Lincoln in 1863, the National Academy of Sciences is charged with providing independent, objective advice to the nation on matters related to science and technology. The National Academy of Sciences is committed to furthering science in America, and its members are active contributors to the international scientific community. Nearly 500 members of the National Academy of Sciences have won Nobel Prizes, and the Proceedings of the National Academy of Sciences, founded in 1914, is today one of the premier international journals publishing the results of original research. The National Academy of Sciences also encourage education and research, recognize outstanding contributions to knowledge, and increase public understanding in matters of science. -
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. -
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. -
Bruno Pontecorvo 1913-1993
Bruno Pontecorvo 1913-1993. Bruno Pontecorvo 1913-1993 External Academician Bruno Pontecorvo, one correspondents of the outstanding physicists of our times, died on 24 September 1993 at Argonne National Laboratory, (USA) the age of 80. He was bom on 22 D. Ayres August 1913 in Pisa, Italy. As a Brookhaven, National Laboratory, (USA) student he was noticed by Enrico P. Yamin Fermi and admitted to his world- CEBAF Laboratory, (USA) famous group in 1933, where he S. Corneliussen participated in the classical investiga Cornell University, (USA) tions of slow neutrons which paved D. G. Cassel the way for practical applications of DESY Laboratory, (Germany) nuclear power. P. Waloschek In 1936 Pontecorvo joined Joliot- Fermi National Accelerator Laboratory, (USA) Curie's group in Paris, again partici J. Cooper, J. Holt pating in research which laid a GSI Darmstadt, (Germany) foundation for modern nuclear G. Siegert physics, and making significant INFN, (Italy) discoveries of his own. From 1940- his idea to look for muon neutrinos. A. Pascolini 42 he worked in the USA, where he This involved using high energy IHEP, Beijing, (China) devised and introduced a neutron Qi Nading accelerators to produce pions, which logging technique which is still used decay predominantly into muons and JINR Dubna, (Russia) in oil prospecting. Then he worked in neutrinos, and so obtain an artificial B. Starchenko Canada, the UK (Harwell), and in beam of high energy neutrinos. This KEK National Laboratory, (Japan) S. Iwata 1950 moved to the Soviet Union, led to the classic experiment at immediately joining the research at Lawrence Berkeley Laboratory, (USA) Brookhaven by Leon Lederman, Jack B. -
Neutrino Physics
0 Neutrino Physics Zhi-zhong Xing ★ Neutrino’s history & lepton families (IHEP, Beijing) ★ Dirac & Majorana neutrino masses ★ Lepton flavor mixing & CP violation ★ Neutrino oscillation phenomenology ★ Seesaw & leptogenesis mechanisms ★ Extreme corners in the neutrino sky Lecture A @ the 2nd Asia-Europe-Pacific School of HEP, 11/2014, Puri, India Neutrinos everywhere 1 SM Properties: charge = 0 spin = ½ mass = 0 Big Bang speed = c neutrinos Galaxy Human Supernova Sun Earth Reactor Accelerator Neutrinos: witness and participant 1 in the evolution of the Universe 3 2 < 1% Some open questions 3 . the absolute mass scale? . the mass hierarchy? . the flavor desert? . leptonic CP violation? . the Majorana nature? . How many species? . cosmic background? . supernova & stellar ’s? . UHE cosmic ’s? . warm dark matter? . matter-antimatter asymmetry… Lecture A1 ★ Neutrinos from new physics ★ Interactions and discoveries ★ Flavors / families of leptons Beta decays in 1930 5 2-body Energy crisis = New physics ? decays J. Chadwick 1914/C. Ellis 1920-1927 What to do? Two ways out? 6 . giving up sth . adding in sth Niels Bohr Wolfgang Pauli (1930) Pauli put forward this idea in a letter instead of a paper….. Solvay 1933 7 Pauli gave a talk on his neutrino proposal in this congress. Fermi’s theory 8 Enrico Fermi assumed a new force for I will be remembered decay by combining 3 new concepts: for this paper. ------ Fermi in Italian ★ Pauli’s idea: neutrinos Alps, Christmas 1933 ★ Dirac’s idea: creation of particles ★ Heisenberg’s idea: isospin symmetry Fermi’s paper 9 This is Fermi’s best theoretical work! ---- C.N. Yang Published first in this journal and later in Z. -
Bruno Pontecorvo in Dubna — Recollections by a Former Student
IL NUOVO CIMENTO Vol. 37 C, N. 3 Maggio-Giugno 2014 DOI 10.1393/ncc/i2014-11758-6 Colloquia: Pontecorvo100 Bruno Pontecorvo in Dubna — Recollections by a former student G. Mitselmakher University of Florida - Gainesville, FL, USA Fig. 1. – On the back of the picture: “2+2=4! You have to know this! B.P.”. Dubna, 1978. Bruno arrived to Dubna in 1950, soon after departure with his family to the Soviet Union. This was well before my time in Dubna, I came to Dubna in 1966. From starting the research institute in the area in 1947, and until 1956 Dubna was a “secret” city. The scientific Institute in Dubna was run by the so called “Ministry for the Medium Machinery”, the code name for the Atomic Ministry in the Soviet Union. The secrecy was at the level comparable to military research places, despite the physics institute there has been built solely for the fundamental physics research. The best (in the world!) cyclotron (480 MeV) was secretly built and commissioned in Dubna in 1949. After arrival in 1950, Bruno became one of the first users of this machine. The institute had very young personnel, Bruno at the age of 37 years was one of the oldest, his nickname was the “Professor”. The documents which have been declassified since, show that he was doing elementary particles research. Here are some pictures of the documents related to Bruno’s work in USSR in Dubna after arrival to USSR (Figs. 2, 3). Bruno continued to work on elementary particle research. Being contained in the Soviet Union, he collaborated almost exclusively with physicists from the Soviet Union. -
IRPS Home Page
IRPS Home Page ARCHIVE EDITION OF IRPS BULLETIN Volume 19 No 1 June, 2005 Office Bearers : 2003 - 2006 Editorial President's Report Member's Paper Member's Report Junior Radiation Physics Medal Awards : Abstracts from Papers Return to Archive Home Page file:////warsaw/www/irps/archives/vol19no1/welcome.html [19/09/2013 3:01:07 PM] Untitled OFFICE BEARERS : 2003 - 2006 President: Regional Vice Executive Presidents: Councillors: R.H. Pratt Dept. of Physics North America: P. Bergstrom (U.S.A.) Univ Pittsburgh, PA J. Hubbell (USA) 15260 USA L. South and Central Gerward (Denmark) Secretariat: America: J.E. Fernandez (Italy) D.A. Bradley A. Paschoa (Brazil) R.T. School of Physics, Mainardi (Argentina) University of Exeter Africa and Middle East: Stocker Road J. O'Meara (Canada) Exeter EX4 4QL UK D.T.L. Jones (South K. Singh Thind (India) Africa) Treasurer: D. McLean (Australia) East Europe A. Ljubicic L. Musilek (Czech Rudjer Boskovic Institute T. Nakamura (Japan) Republic) Bijenicka 54 Zagreb 41000 Croatia F.S.U A.V. Korol (Russia) Chair, Advisory Board Western Europe: M.J. Cooper Department of Physics M.J. Farquharson (U. University of Warwick K.) Coventry CV4 7AL U.K. S.E. Asia : S.C. Roy (India) Australasia : D.C. Creagh (Australia) North East Asia: Luo Zhengming (PR China) EDITORIAL BOARD Editor : P.M. Bergstrom (U.S.A.) Editorial Committee : D.C. Creagh (Australia) S.A. McKeown (Australia) file:////warsaw/www/irps/archives/vol19no1/officers.html (1 of 2) [19/09/2013 3:01:07 PM] Untitled Home Page file:////warsaw/www/irps/archives/vol19no1/officers.html (2 of 2) [19/09/2013 3:01:07 PM] Untitled EDITORIAL Welcome to Vol.