Nobel Lecture by Toshihide Maskawa
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HOPE Meetings Are Held for Excellent Graduate Students and Young Researchers Specially Selected from Countries Around the 9Th Asia-Pacific and Africa Region
For Overseas Cooperating Institutions Objective HOPE Meetings are held for excellent graduate students and young researchers specially selected from countries around the 9th Asia-Pacific and Africa region. These meetings give an opportunity for the participants to engage in interdisciplinary discussions with Nobel laureates and other distinguished HOPE MEETING scientists pioneering the frontiers of knowledge. They also give the participants, who lodge together over the course of the event, a chance to make friends and form collegial networks with Nobel Laureates with peers from the regions. The title “HOPE Meeting” signifies the promise held for the future roles of young researchers and optimism for creating a bright S&T future within the global community. Date F ebruary 26- ■ Saturday, February 25: Orientation & Registration M arch 2, 2017 ■ Sunday, February 26: Nobel Prize Dialogue Tokyo 2017 Organizer Venue Tokyo , JAPAN Office of the HOPE Meetings, JSPS E-mail [email protected] Tel: +81-3-3263-2414 Fax:+81-3-3234-3700 HOPE MEETINGS with Nobel Laureates Organizing Committee of the HOPE Meetings ■ Chair Makoto Kobayashi <Nobel Laureate in Physics 2008> Honorary Professor Emeritus, High Energy Accelerator Research Organization (KEK) ■ Members Noriko Osumi Mitsuhiko Shionoya Tohoku University The University of Tokyo Takaaki Kajita <Nobel Laureate in Physics 2015> Yousuke Takahama The University of Tokyo Tokushima University Kazuhiro Kosuge Fumio Hanaoka Tohoku University Tsukuba University Program of the HOPE Meeting The program -
Ernest Rutherford and the Accelerator: “A Million Volts in a Soapbox”
Ernest Rutherford and the Accelerator: “A Million Volts in a Soapbox” AAPT 2011 Winter Meeting Jacksonville, FL January 10, 2011 H. Frederick Dylla American Institute of Physics Steven T. Corneliussen Jefferson Lab Outline • Rutherford's call for inventing accelerators ("million volts in a soap box") • Newton, Franklin and Jefferson: Notable prefiguring of Rutherford's call • Rutherfords's discovery: The atomic nucleus and a new experimental method (scattering) • A century of particle accelerators AAPT Winter Meeting January 10, 2011 Rutherford’s call for inventing accelerators 1911 – Rutherford discovered the atom’s nucleus • Revolutionized study of the submicroscopic realm • Established method of making inferences from particle scattering 1927 – Anniversary Address of the President of the Royal Society • Expressed a long-standing “ambition to have available for study a copious supply of atoms and electrons which have an individual energy far transcending that of the alpha and beta particles” available from natural sources so as to “open up an extraordinarily interesting field of investigation.” AAPT Winter Meeting January 10, 2011 Rutherford’s wish: “A million volts in a soapbox” Spurred the invention of the particle accelerator, leading to: • Rich fundamental understanding of matter • Rich understanding of astrophysical phenomena • Extraordinary range of particle-accelerator technologies and applications AAPT Winter Meeting January 10, 2011 From Newton, Jefferson & Franklin to Rutherford’s call for inventing accelerators Isaac Newton, 1717, foreseeing something like quarks and the nuclear strong force: “There are agents in Nature able to make the particles of bodies stick together by very strong attractions. And it is the business of Experimental Philosophy to find them out. -
Quantum Mechanics Quantum Chromodynamics (QCD)
Quantum Mechanics_quantum chromodynamics (QCD) In theoretical physics, quantum chromodynamics (QCD) is a theory ofstrong interactions, a fundamental forcedescribing the interactions between quarksand gluons which make up hadrons such as the proton, neutron and pion. QCD is a type of Quantum field theory called a non- abelian gauge theory with symmetry group SU(3). The QCD analog of electric charge is a property called 'color'. Gluons are the force carrier of the theory, like photons are for the electromagnetic force in quantum electrodynamics. The theory is an important part of the Standard Model of Particle physics. A huge body of experimental evidence for QCD has been gathered over the years. QCD enjoys two peculiar properties: Confinement, which means that the force between quarks does not diminish as they are separated. Because of this, when you do split the quark the energy is enough to create another quark thus creating another quark pair; they are forever bound into hadrons such as theproton and the neutron or the pion and kaon. Although analytically unproven, confinement is widely believed to be true because it explains the consistent failure of free quark searches, and it is easy to demonstrate in lattice QCD. Asymptotic freedom, which means that in very high-energy reactions, quarks and gluons interact very weakly creating a quark–gluon plasma. This prediction of QCD was first discovered in the early 1970s by David Politzer and by Frank Wilczek and David Gross. For this work they were awarded the 2004 Nobel Prize in Physics. There is no known phase-transition line separating these two properties; confinement is dominant in low-energy scales but, as energy increases, asymptotic freedom becomes dominant. -
Scaling Laws in Particle Physics and Astrophysics
SCALING LAWS IN PARTICLE PHYSICS AND ASTROPHYSICS RUDOLF MURADYAN Dedicated to the Golden Jubilee (1961-2011) of publication of the article by Geoffrey Chew and Steven Frautschi in Phys. Rev. Lett. 7, 394, 1961, where a celebrated scaling law J m2 has been conjectured for spin/mass dependence of hadrons. G. Chew S. Frautschi 1. INTRODUCTION: WHAT IS SCALING? Any polynomial power law f() x c xn , where constant c has a dimension dim f dimc (dimx )n exhibits the property of scaling or scale invariance. Usually n is called scaling exponent. The word scaling express the fact that function f is shape-invariant with respect to the dilatation transformation x x f ( x) c ( x)n n f() x and this transformation preserves the shape of function f . We say, following Leonhard Euler, that f is homogeneous of degree “n” if for any value of parameter f ( x) n f() x . Differentiating this relation with respect to and putting 1we obtain simple differential equation x f() x n f() x solution of which brings back to the polynomial power scaling law. There are tremendously many different scaling laws in Nature. The most important of them can be revealed by Google search of scaling site:nobelprize.org in the official site of Nobel Foundation, where nearly 100 results appears. Ten of them are shown below: 1. Jerome I. Friedman - Nobel Lecture 2. Daniel C. Tsui - Nobel Lecture 3. Gerardus 't Hooft - Nobel Lecture 4. Henry W. Kendall - Nobel Lecture 5. Pierre-Gilles de Gennes - Nobel Lecture 6. Jack Steinberger - Nobel Lecture 7. -
C11 Commission on Particles and Fields Fermilab MS 370 +1(630)840-8071
Patricia McBride C11 Commission on Particles and Fields Fermilab MS 370 +1(630)840-8071 His Excellency Mr. Tatsuo Kawabata Minister of Education, Culture, Sports, Science and Technology 3-2-2 Kasumigaseki, Chiyoda-ku Tokyo, 100-8959 Japan Your Excellency, The members of the International Union of Pure and Applied Physics (IUPAP) C11 Commission on Particles and Fields would like to acknowledge the significant and distinguished contributions of Japanese scientists and Japanese scientific research projects to the field of elementary particle physics. C11 promotes the exchange of information and views among the members of the international scientific community in the field of Particles and Fields. This field of science investigates the nature and properties of the fundamental constituents of matter and the forces acting between these constituents. In addition, the field encompasses the accelerators, detectors and techniques used in these investigations and the industrial applications of related technologies. Scientists working in Japan have made many major contributions to our field. The discovery of neutrino mass was heralded as one of the most important discoveries in elementary particle physics during the last quarter century. The first convincing evidence for neutrino masses came from Super-Kamiokande, a Japanese experiment. The Kamiokande experiment on the other hand, the predecessor of Super-Kamiokande, detected neutrinos coming from supernova 1987a. These detected neutrinos showed that we are able to understand the science of supernova explosions. In 2002, the Japanese scientist Masatoshi Koshiba won a Nobel Prize for his leading role in the Kamiokande and Super-Kamiokande experiments. The Japanese research center KEK and the American research center SLAC have studied the difference between the behavior of matter and antimatter at their facilities known as "B-Factories". -
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. -
Award Winning Research Kyoto University Is Acknowledged As One of the Most Accomplished Research-Oriented Universities in Asia
Award Winning Research Kyoto University is acknowledged as one of the most accomplished research-oriented universities in Asia. That reputation is 2016 testified by the accolades conferred on our alumni and researchers, most notably nine Nobel Prize laureates who undertook vital research during their time at the university. In addition to those awards, several other Kyoto University faculty members have received major accolades, including two Fields Medalists, one Gauss Prize winner, and five Lasker Award winners. Nobel Prize 1949, Physics 1965, Physics 1981, Chemistry 1987, Physiology and 2001, Chemistry Hideki Yukawa Shinichiro Tomonaga Kenichi Fukui Medicine Ryoji Noyori Susumu Tonegawa 2008, Physics 2008, Physics 2012, Physiology or 2014, Physics Makoto Kobayashi Toshihide Maskawa Medicine Isamu Akasaki Shinya Yamanaka Fields Medal Gauss Prize Kyoto Prize 1970, Mathematics 1990, Mathematics 2006, Mathematics 1995, Basic Sciences 1998, Basic Sciences 2004, 2010, Heisuke Hironaka Shigefumi Mori Kiyoshi Ito Chushiro Hayashi Kiyoshi Ito Advanced Technology Advanced Technology Alan Curtis Kay Shinya Yamanaka Japan Prize Lasker Award 2005, Information and 2005, Cell Biology 1987, Basic Medical 1989, Basic Medical 1998, Basic Medical 2009, Basic Medical 2014, Basic Medical Media Technology Masatoshi Takeichi Research Research Research Research Research Makoto Nagao Susumu Tonegawa Yasutomi Nishizuka Yoshio Masui Shinya Yamanaka Kazutoshi Mori *photos provided by the Japan Prize Foundation ©e Nobel Foundation2012 photo by Alexander Mahmoud Dr. Shinya Yamanaka, director of the Prof. Kayo Inaba, Kyoto University’s Prof. Kazutoshi Mori of Kyoto Center for iPS Cell Research and executive vice-president for gender University’s Graduate School of Science Application (CiRA), receives the 2012 equality, international affairs, and public receiving the 2014 Albert Lasker Award Nobel Prize in Physiology or Medicine. -
Arxiv:Hep-Ph/0703178V1 16 Mar 2007 Eta Eorn Huddcyt Htn I H Following the Via Photons to Decay Should S Mesotrons Force
FERMILAB-CONF-07-48-T Mesotron Decays and the Role of Anomalies William A. Bardeen Theoretical Physics Department Fermilab, MS 106, P.O. Box 500 Batavia, IL 60510, USA March 15, 2007 Puzzles associated with Yukawa’s mesotron theory of nuclear interactions led to the dis- covery of “anomalies” in quantum field theory. I will discuss some of the remarkable conse- quences of these anomalies in the physics of elementary particles. In 1935 Hideki Yukawa postulated that nuclear forces were ascribed to a new massive scalar field that coupled to neutrons to protons. To explain the saturation of the nuclear forces, the new mesotrons were required to have a mass of order 200 me, and a coupling a few times larger than that associated with the electric charge. The terms mesotron was used to describe a particle of intermediate mass, much heavier than the light electron and much lighter than the neutron and proton, the constituents of the atomic nucleus. Indeed, in 1937, a new meson of intermediate mass was discovered as the dominant part of the hard component of cosmic rays. It was natural to associate this meson with the field that Yukawa had proposed to explain the nuclear force. Shoichi Sakata played an important role in the struggle to understand the physics of the new Yukawa mesotrons and their relation to the new mesons seen in cosmic rays. arXiv:hep-ph/0703178v1 16 Mar 2007 Early estimates of the lifetime of the mesotron were based on Fermi’s theory of β-decay. These estimates, in the range of 10−8 to 10−7 sec, were considerably shorter than the lifetime observed for the cosmic ray mesons, ∼2 10−6 sec. -
HOPE MEETINGS with Nobel Laureates
For Overseas Cooperating Institutions HOPE MEETINGS with Nobel Laureates Objective HOPE Meetings are held for excellent graduate students and young 13th researchers specially selected from countries/areas around the Asia-Pacific and Africa regions. They give an opportunity for the HOPE participants to engage in interdisciplinary discussions with Nobel laureates and other distinguished scientists pioneering the frontiers of knowledge. They also give the participants, who lodge together MEETING over the course of the event, a chance to make friends and form with Nobel Laureates collegial networks with peers from the regions. https://www.jsps.go.jp/english/e-hope/index.html Nobel Prize Dialogue (NPD) Tokyo 2021 Reception for HOPE & NPD participants jointly hosted 17-21 by JSPS & Nobel Media AB ・ arch, 2021 Sunday, 21 March, 2021 M Venue (Tentative) Organizer Yokohama, Office of the HOPE Meetings, JSPS E-mail [email protected] JAPAN Tel: +81-3-3263-2414 Fax:+81-3-3234-3700 1 HOPE MEETINGS with Nobel Laureates Organizing Committee of the 13th HOPE Meeting ■Chair KAJITA Takaaki Nobel Laureate in Physics 2015 Director, Institute for Cosmic Ray Research (ICRR) Distinguished University Professor, The University of Tokyo ■Organizing Committee Members See: https://www.jsps.go.jp/english/e-hope/sosiki13.html Participants About 100 doctoral students and young researchers from the following countries/areas: Australia, Bangladesh, China, Egypt, India, Indonesia, Israel, Japan, Kenya, Korea, Malaysia, Mongolia, Myanmar, Nepal, New Zealand, Philippines, -
SAKURA Science High School Program Activity Report 2016 SAKURA Science High School Program Activity Report 2016
2016 Japan-Asia Youth Exchange Program in Science SAKURA Science High School Program Activity Report 2016 SAKURA Science High School Program Activity Report 2016 〈Table of Contents〉 About the SAKURA Science High School Program / Kazuki Okimura (Counselor to the President, Japan Science and Technology Agency) 2 Message to the Students / Dr. Toshihide Maskawa (Director General and Professor Emeritus, Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya University) 3 Outline of the SAKURA Science High School Program 2016 4 Courtesy visit to Mr. Hiroshi Hase, Minister of Education, Culture, Sports, Science and Technology 5 Group 1 Activity Report 6 Group 2 Activity Report 8 Group 3 Activity Report 10 Group 4 Activity Report 12 Group 5 Activity Report 14 Group 6 Activity Report 16 Group 7 Activity Report 18 Group 8 Activity Report 20 Special Program for India and Sri Lanka 22 Participant Survey Results 24 Acknowledgments 26 About the SAKURA Science High School Program Counselor to the President, Japan Science and Technology Agency (JST) About theSAKURA Science Director, Japan-Asia Youth Exchange Program in Science Promotion Office High SchoolProgram Kazuki Okimura The SAKURA Exchange Program in Science( SSP) aims to nurture the interest in science and technology among young people( high school students and adults under 41 years old) in Asia, by improving their levels of knowledge in these fields so that they may contribute to the development of their home countries and Asia. We expect to achieve these objectives by inviting these people to our country and providing them access to Japan’s science and technology. -
Neutrino Mass and Mixing – the Beginning and Future –
Nuclear Physics B Proceedings Supplement Nuclear Physics B Proceedings Supplement 00 (2012) 1–4 Neutrino mass and mixing – The beginning and future – M. Kobayashi High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan Abstract The early history of neutrino mixing will be discussed with a focus on the birth of the MNS theory. Keywords: two neutrinos, MNS matrix 1. Sakata Model Another important aspect of the Sakata model is the fact that the weak interactions of hadrons can be ex- The first evidence of strange particles was found in plained by two types of transitions among the funda- cosmic ray events in 1947. Much progress in under- mental triplets: standing these particles was made in the early 1950’s, in particular after the operation of accelerators started. p The discovery of strange particles made it difficult to ↑↓-& . (1) regard all of the known hadrons as fundamental objects n Λ since there were so many. This pattern of the weak interaction is similar to the In 1956, Sakata proposed a model known as the weak interaction of the leptons, Sakata model [1], in which all the hadrons, both strange and non-strange, are composite states of a fundamental ν triplet formed from the proton, the neutron, and the Λ ↑↓-& . (2) particle. e µ Shoichi Sakata was born in 1911. He was a collabora- tor of Yukawa for some time. He was appointed profes- At that time the neutrino was thought to consist of a sor of Nagoya University when its physics department single species. This similarity of the weak interaction was established in 1942. -
Teoretisk Fysik
1 Teoretisk fysik Institutionen för fysik Helsingfors Universitet 12.11. 2008 Paul Hoyer 530013 Presentation av de fysikaliska vetenskaperna (3 sp, 1 sv) Kursbeskrivning: I kursen presenteras de fysikaliska vetenskaperna med sina huvudämnen astronomi, fysik, geofysik, meteorologi samt teoretisk fysik. Den allmänna studiegången presenteras samt en inblick i arbetsmarkanden för utexaminerade fysiker ges. Kursens centrala innehåll: Kursen innehåller en presentation av de fysikaliska vetenskapernas huvudämnes uppbyggnad samt centrala forskningsobjekt. Presentationen ges av institutionens lärare samt av utomstående forskare och fysiker i industrin. Centrala färdigheter: Att kunna tillgodogöra sig en muntlig presentation sam föra en diskussion om det presenterade temat. Kommentarer: På kursen kan man även behandla speciella ämnesområden, såsom: speciella forskningsområden inom fysiken samt specifika önskemål inom studierna. 2 Bakgrund Den fortgående specialiseringen inom naturvetenskaperna ledde till att teoretisk fysik utvecklades till ett eget delområde av fysiken Professurer i teoretisk fysik år 1900: 8 i Tyskland, 2 i USA,1 i Holland, 0 i Storbritannien Professorer i teoretisk fysik år 2008: Talrika! Även forskningsinstitut för teoretisk fysik (Nordita @ Stockholm, Kavli @ Santa Barbara,...) Teoretisk fysik är egentligen en metod (jfr. experimentell och numerisk fysik) som täcker alla områden av fysiken: Kondenserad materie Optik Kärnfysik Högenergifysik,... 3 Kring nyttan av teoretisk fysik Rutherford 1910: “How can a fellow sit down at a table and calculate something that would take me, me, six months to measure in the laboratory?” 1928: Dirac realized that his equation in fact describes two spin-1/2 particles with opposite charge. He first thought the two were the electron and the proton, but it was then pointed out to him by Igor Tamm and Robert Oppenheimer that they must have the same mass, and the new particle became the anti-electron, the positron.