The Scientific Work of Ettore Majorana
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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. -
Ettore Majorana: Genius and Mystery
«ETTORE MAJORANA» FOUNDATION AND CENTRE FOR SCIENTIFIC CULTURE TO PAY A PERMANENT TRIBUTE TO GALILEO GALILEI, FOUNDER OF MODERN SCIENCE AND TO ENRICO FERMI, THE "ITALIAN NAVIGATOR", FATHER OF THE WEAK FORCES ETTORE MAJORANA CENTENARY ETTORE MAJORANA: GENIUS AND MYSTERY Antonino Zichichi ETTORE MAJORANA: GENIUS AND MYSTERY Antonino Zichichi ABSTRACT The geniality of Ettore Majorana is discussed in the framework of the crucial problems being investigated at the time of his activity. These problems are projected to our present days, where the number of space-time dimensions is no longer four and where the unification of the fundamental forces needs the Majorana particle: neutral, with spin ½ and identical to its antiparticle. The mystery of the way Majorana disappeared is restricted to few testimonies, while his geniality is open to all eminent physicists of the XXth century, who had the privilege of knowing him, directly or indirectly. 3 44444444444444444444444444444444444 ETTORE MAJORANA: GENIUS AND MYSTERY Antonino Zichichi CONTENTS 1 LEONARDO SCIASCIA’S IDEA 5 2 ENRICO FERMI: FEW OTHERS IN THE WORLD COULD MATCH MAJORANA’S DEEP UNDERSTANDING OF THE PHYSICS OF THE TIME 7 3 RECOLLECTIONS BY ROBERT OPPENHEIMER 19 4 THE DISCOVERY OF THE NEUTRON – RECOLLECTIONS BY EMILIO SEGRÉ AND GIANCARLO WICK 21 5 THE MAJORANA ‘NEUTRINOS’ – RECOLLECTIONS BY BRUNO PONTECORVO – THE MAJORANA DISCOVERY ON THE DIRAC γ- MATRICES 23 6 THE FIRST COURSE OF THE SUBNUCLEAR PHYSICS SCHOOL (1963): JOHN BELL ON THE DIRAC AND MAJORANA NEUTRINOS 45 7 THE FIRST STEP TO RELATIVISTICALLY DESCRIBE PARTICLES WITH ARBITRARY SPIN 47 8 THE CENTENNIAL OF THE BIRTH OF A GENIUS – A HOMAGE BY THE INTERNATIONAL SCIENTIFIC COMMUNITY 53 REFERENCES 61 4 44444444444444444444444444444444444 Ettore Majorana’s photograph taken from his university card dated 3rd November 1923. -
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. -
Vol 15 No 2, Spring 2009
Search Lites Vol. 15 No. 2, Spring 2009 The Quarterly Newsletter of The SETI League, Inc. Offices: 433 Liberty Street Alpha Centauri, Here We Come PO Box 555 by Paul Gilster, Tau Zero Foundation Little Ferry NJ 07643 USA I'm always fascinated with the way the media handle nearby stars and the plan- ets that may orbit them, especially as our inventory of confirmed planets continues Phone: to grow. A recent National Geographic television special is a case in point. The (201) 641-1770 show's graphics were superb, its narration gripping. But how puzzling to run into a Facsimile: (201) 641-1771 fundamental misunderstanding about our nearest stellar neighbors. Email: [email protected] In "Journey to the Edge of the Universe," putative travelers have moved out Web: through the Solar System, passing (an ingenious touch) the various probes and arti- www.setileague.org facts we humans have scattered from Mercury out to the Kuiper Belt. As we move President/Registered Agent: to the nearest stars, we pass what is obviously the red dwarf Proxima Centauri and Richard Factor make for the binaries Centauri A and B. Describing them, the narrator says, "Not Secretary/Treasurer: one but three stars, spinning around each other locked in a celestial standoff, each A. Heather Wood star's gravity attracting the other, their blazing orbital speed keeping them apart." Executive Director Emeritus: H. Paul Shuch, Ph.D. And then this: "Get between them and we'd be vaporized." Trustee: Not a chance. We don't yet know whether there are planets around Centauri A Martin Schreiber, CPA or B. -
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. -
Friends and Colleagues Look at Aspects of Cocconi's Lifelong Interest in the Cosmos and Recent Developments in Modern Physics
TRIBUTE Giuseppe Cocconi and his love of the cosmos Friends and colleagues look at aspects of Cocconi’s lifelong interest in the cosmos and recent developments in modern physics, revealing a physicist of remarkable perception. In 1938 Giuseppe Cocconi published his first paper, “On the spectrum of cosmic radiation”. His last unpublished note of December 2005 bore the title “Arguments in favour of a personal interpre- tation of extra galactic cosmic rays”. No better indication could be given of his deep interest in astronomy and astrophysics, which lasted until he died in November 2008 aged 94 (CERN Courier March 2009 p36). The fields that he pioneered are now witnessing exciting new developments. Over the past six months they have reminded us of his many contributions to physics; his simple, direct way to conceive and perform experiments; and his unique way of presenting the sub- jects that he loved. In this article we describe some of these events and recall what Giuseppe contributed to the various fields. Ultra-high-energy cosmic rays Giuseppe and Vanna Cocconi check cosmic-ray shower detectors. This Giuseppe’s interest in the cosmos began when he was in his teens. photograph appeared in an article in the world famous magazine Life in He would design sundials for friends’ villas around his home town of November 1948. (Courtesy Time & Life Pictures/Getty Images.) Como, observe the sky and read as much about it as he could. Late one evening, he happened to observe the fall of some Perseid mete- and little about their composition. ors at an unexpected time. -
Antonino Cattaneo
ANTONINO CATTANEO Presidente European Brain Research Institute Roma [email protected] After obtaining a degree in biophysics, Antonino Cattaneo worked as a PhD student at the Scuola Normale Superiore (Pisa) with Lamberto Maffei and as a postdoc and staff scientist with Rita Levi-Montalcini (Nobel Laureate for the discovery of NGF) at the CNR Institute of Neurobiology in Rome. He later worked with Cesar Milstein (Nobel Prize laureate for the discovery of monoclonal antibodies) and Michael Neuberger at the MRC Laboratory of Molecular Biology (Cambridge, UK). From 1991 to 2008, he was Full Professor of Biophysics at the International School for Advanced Studies (SISSA) in Trieste (Italy), where he was Head of the Biophysics Department from 1991 to 1995 and the Deputy Director of SISSA from 1996 to 2001. Since 2008 he is Professor of Neurobiology at the Scuola Normale Superiore (Pisa), where he is also the Director of the Biology Lab Bio@SnS. Antonino Cattaneo is author of more than 200 publications in peer-reviewed international scientific journals and is recipient of several awards including Domenico Marotta Prize (Accademia Nazionale delle Scienze detta XL), the W. Jansenius Medal (Slovak Academy of Sciences) and the “G. Tartufari” International Prize for Biology (Accademia Nazionale dei Lincei). He is a member of EMBO (European Molecular Biology Organization) and member of the Accademia Nazionale delle Scienze detta XL, the Academia Europaea and of the Accademia Nazionale dei Lincei. Since 2018 he is President of the European Brain Research -
How US Physicists First Came to Work at CERN
CERN-US COLLABORATION How US physicists first came to work at CERN After help from an eminent US figure, CERN was founded in the 1950s to provide a European stage for physics. Once the curtain was up, US physicists found the new laboratory increasingly attractive. In the first of two articles, Gordon Fraser traces the history of CERN-US collaboration from the post-war era to the advent of collider physics in the 1970s. In the late 1940s, Europe was major role in establishing the US struggling to emerge from the ruins Brookhaven National Laboratory. of the Second World War. The US The establishment of an analo had played a vital role in the con gous European laboratory was to flict, but had been less affected mat Rabi a natural and vital need. erially, and a shining vision of life However, on arrival in Florence he across the Atlantic was a beacon of was disturbed to find that there was hope for millions of Europeans liv no mention of this idea on the ing in austerity, if not misery. agenda. Two Europeans, Pierre i In a speech at Harvard on 5 June Auger (then UNESCO's director of 1947, US Secretary of State George exact and natural sciences) and C Marshall said that the US should Edoardo Amaldi, who was to be a help to "assist in the return of nor constant driving force, helped Rabi mal economic health in the world". Playing a key role in the post-Second World War through the intricacies of European North American "Marshall aid" was groundwork for what would become CERN was US physicist committee formalities. -
Majorana Returns Frank Wilczek in His Short Career, Ettore Majorana Made Several Profound Contributions
perspective Majorana returns Frank Wilczek In his short career, Ettore Majorana made several profound contributions. One of them, his concept of ‘Majorana fermions’ — particles that are their own antiparticle — is finding ever wider relevance in modern physics. nrico Fermi had to cajole his friend Indeed, when, in 1928, Paul Dirac number of electrons minus the number of Ettore Majorana into publishing discovered1 the theoretical framework antielectrons, plus the number of electron Ehis big idea: a modification of the for describing spin-½ particles, it seemed neutrinos minus the number of antielectron Dirac equation that would have profound that complex numbers were unavoidable neutrinos is a constant (call it Le). These ramifications for particle physics. Shortly (Box 2). Dirac’s original equation contained laws lead to many successful selection afterwards, in 1938, Majorana mysteriously both real and imaginary numbers, and rules. For example, the particles (muon disappeared, and for 70 years his modified therefore it can only pertain to complex neutrinos, νμ) emitted in positive pion (π) + + equation remained a rather obscure fields. For Dirac, who was concerned decay, π → μ + νμ, will induce neutron- − footnote in theoretical physics (Box 1). with describing electrons, this feature to-proton conversion νμ + n → μ + p, Now suddenly, it seems, Majorana’s posed no problem, and even came to but not proton-to-neutron conversion + concept is ubiquitous, and his equation seem an advantage because it ‘explained’ νμ + p → μ + n; the particles (muon is central to recent work not only in why positrons, the antiparticles of antineutrinos, ν¯ μ) emitted in the negative − − neutrino physics, supersymmetry and dark electrons, exist. -
Luisa Bonolis 2
LuisaM<html><head></head><body><pre Bonolis style="word-wrap:Address: Via Cavalese break-word; 13, 00135 Rome white-space: pre-wrap;"> Address: Koserstraße 23, 14195 Berlin </pre></body></html>Curriculum Vitae Email: [email protected] Email: [email protected] www: https://www.luisabonolis.it/ 12 January 2015 www: https://www.mpiwg-berlin.mpg.de/users/lbonolis Education and Qualifications 1993 Master Degree in Physics, Rome University Sapienza 1994 Post graduate specialization diploma in Physics, Sapienza University, Rome, Italy 2006 Ph.D. Scholarship, History of Sciences, Seminario di Storia della Scienza, Bari University, Italy 2009 Ph.D. in History of Science (with distinction). Title of dissertation: Bruno Rossi and Cosmic Rays: From Earth Laboratories to Physics in Space 2018 National Scientific Habilitation in History of Physics for the role of Associate Professor from the Italian Ministry of Education, University and Research Language Skills Italian: Mother tongue English: Fluent German: Working knowledge French: Proficient Spanish: Working knowledge Professional and research experience 1993–1995 Editor for book publishers Shakespeare & Company Futura, Florence. 1996–2002 Collaboration with the Society for Oral History on a project funded by the National Re- search Council regarding the realization of a series of oral history interviews to leading figures of the 20th century Italian physics to be preserved at the National State Archive. 1996–2003 Scientific Consultant and collaborator at Quadrofilm Company for the realization of a series of documentaries on the history of science, produced for RAI Italian Television (See Docufilms & Television Series). 2000–2002 Contract with the Physics Department of Rome University La Sapienza and the Ro- me branch of the National Institute for Nuclear Physics: research activities and collaboration with the National Committee and with the executive Council for the celebrations of Enrico Fermi’s birth centennial. -
Double-Beta Decay and the Search for (Elementary) Majorana Particles
Double-beta decay and the search for (elementary) Majorana particles Giorgio Gratta Physics Dept. Stanford University Summer Undergraduate Program, Aug Neutrinos - Gratta 1 2020 Summer Undergraduate Program, Aug Neutrinos - Gratta 2 2020 For the first ~50 years since the neutrino was invented by Pauli, its properties could be fairly well described by quoting just 2 papers: Neutrinos really exist! Summer Undergraduate Program, Aug Neutrinos - Gratta 3 2020 Neutrinos are left handed particles Summer Undergraduate Program, Aug Neutrinos - Gratta 4 2020 Helicity is the property that correlates the spin of a particle to its momentum Because of special relativity the helicity of a particle is related to its mass The observer above sees a neutrino passing-by and reports its helicity (the scalar product between spin vector and momentum vector) as negative (left-handed) Summer Undergraduate Program, Aug Neutrinos - Gratta 5 2020 Helicity is the property that correlates the spin of a particle to its momentum Because of special relativity the helicity of a particle is related to its mass Now the observer is cruising in the same direction of the neutrinos, at higher speed. While overtaking the neutrino he will claim that its helicity is positive! Summer Undergraduate Program, Aug Neutrinos - Gratta 6 2020 Helicity is the property that correlates the spin of a particle to its momentum Because of special relativity the helicity of a particle is related to its mass But if the neutrino has zero mass nothing can overtake it Neutrinos with fixed helicity -
Edoardo Amaldi
Edoardo Amaldi Inventario sommario dell'archivio conservato presso il Dipartimento di fisica dell'Università La Sapienza di Roma 1927 – 1990 a cura di Giovanni Battimelli, Lucia Orlando e Giovanni Paoloni (1994) Informatizzazione e indicizzazione a cura di Nicoletta Valente svolte nel corso del 2015-2016 con il finanziamento della Direzione generale ArcHivi del Ministero dei beni culturali e ambientali e del turismo Sommario Premessa, cenni biografici, nota arcHivistica 1 Inventario 3 Indici dei nomi 73 Premessa Le carte di Amaldi, recuperate nel suo studio e in altri locali del Dipartimento di fisica dell'Università "La Sapienza" di Roma, in aggiunta al corposo versamento del 1991 da parte della famiglia Amaldi al Gruppo di storia della fisica, fanno dell'Archivio del grande fisico piacentino il maggiore tra gli archivi degli scienziati posseduti dall'Università di Roma. L'inventario sommario che segue è relativo ai fascicoli personali (1927-1990) prove- nienti dal Dipartimento e redatto dagli autori a metà degli anni '90. Il suo recupero in- formatico (tramite il software GEA.4 in uso presso il Dipartimento di fisica), lo Ha reso omogeneo alla gran parte dei fondi arcHivistici conservati presso il Dipartimento stesso.1 Cenni biografici Edoardo Amaldi nacque a Carpaneto Piacentino il 5 settembre 1908, figlio di Ugo Amal- di, professore universitario di Matematica. Fu tra i primi allievi di Enrico Fermi a Roma e fece parte del leggendario gruppo dei ''ragazzi di Via Panisperna'', nucleo originario del- la Scuola di Fisica romana. Tra i risultati più importanti ottenuti dal Gruppo romano, cui Amaldi contribuì attivamente, sono da ricordare gli studi pionieristici sulla radioattività e sulla fisica dei nuclei, cHe fecero guadagnare ai componenti del gruppo i più alti rico- noscimenti mondiali, culminati nel Nobel per la Fisica attribuito a Fermi nel 1938.