T2K Presents Hint of CP Violation by Neutrinos August 4, 2017 (Strict Press Embargo Until Aug 4, 2017 11:00 JST) Last Updated 02/08/2017 10:33 BST
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Development of an Electron Gun for the Kek Positron Generator
Particle Accelerators, 1990, Vol. 27, pp. 145-149 © 1990 Gordon and Breach, Science Publishers, Inc. Reprints available directly from the publisher Printed in the United States of America Photocopying permitted by license only DEVELOPMENT OF AN ELECTRON GUN FOR THE KEK POSITRON GENERATOR HIDEKI IWATA, YUJIRO OOAWA*, SATOSIll OHSAWA*, HITOSHI KOBAYASHI*, MITUHIRO YOKOTA*, SHIGEKI FUKUDA* and AKIRA ASAMI* Ishikawajima-harima Heavy Industries Co., Ltd. * National Laboratory for High Energy Physics(KEK) 1-1 Oho, Tsukuba-shi, Ibaraki-ken, 305 Japan Abstract In the KEK Positron Generator, a semi-long pulsed beam (-40ns) has turned out to be suitable for effective positron injection into the PF storage ring. However, to use the semi-long pulsed beam, there was a problem concerning the cathode lifetime of the gun. Thus, a new gun has been developed with a dispenser cathode, Y-796(EIMAC); the characteristics of this gun have been investigated. This new gun has been used since October 1988 and has continued to produce constant current of about 12 A without having to exchange its cathode. Thus, the cathode lifetime has been remarkably improved. INTRODUCTION Positrons had so far been utilized only in the e+-e- colliding experiments of TRISTAN, which began in November 1986. Since 1988, however, it had started to use positrons also in the Photon Factory storage ring. It had been confinned that a positron beam with a width of -40 ns was suitable for the PF ring to reduce the injection time. t ,2,3 However, to use this semi-long pulsed beam, there was a problem regarding the cathode lifetime of the old gun, the cathode of which was an oxide-coated type.4 Therefore, a new gun with a dispenser cathode, Y-796(EIMAC), has been developed to achieve a long lifetime of the cathode and to obtain a larger anode current. -
Participants
PARTICIPANTS Abbott, Richard [email protected] California Institute of Technology Aldach, Jackie [email protected] Stanford Linear Accelerator Center Allen, Christopher [email protected] Los Alamos National Laboratory Allison, Stephanie [email protected] Stanford Linear Accelerator Center Allison, Trent [email protected] Thomas Jefferson National Accelerator Facility Anicic, Damir [email protected] Paul Scherrer Institut PSI Armstrong, Dennis [email protected] Isaac Newton Group Bacher, Reinhard [email protected] DESY Backman, Raymond H. [email protected] Mega Industries, L.L.C. Baek, Sulhee [email protected] Samsung Advanced Institute of Technology Baer, Ralph C. [email protected] GSI Darmstadt Bartlett, J. Frederick [email protected] Fermi National Accelerator Laboratory Bec, Matthieu [email protected] Gemini Observatory Bernstein, Dorel [email protected] Stanford Linear Accelerator Center Bevins, Brian [email protected] Thomas Jefferson National Accelerator Facility Bickley, Matthew [email protected] Thomas Jefferson National Accelerator Facility Biocca, Alan [email protected] Lawrence Berkeley National Laboratory Birke, Thomas [email protected] Los Alamos National Laboratory PARTICIPANTS 8th International Conference on Accelerator & Large Experimental Physics Control Systems Bjorklund, Eric [email protected] Spallation Neutron Source Blumer, Thomas [email protected] Paul Scherrer Institut PSI Bolkhovityanov, Dmitry [email protected] Budker Institute of Nuclear Physics Bolshakov, Timofei [email protected] Fermi National Accelerator Laboratory Bookwalter, Valerie [email protected] Thomas Jefferson National Accelerator Facility Boriskin, Victor [email protected] Kharkov Institute Physics & Technology Bork, Rolf [email protected] California Institute of Technology Brazier, John [email protected] Brazier Systems & Consultants Ltd. -
FROM KEK-PS to J-PARC Yoshishige Yamazaki, J-PARC, KEK & JAEA, Japan
FROM KEK-PS TO J-PARC Yoshishige Yamazaki, J-PARC, KEK & JAEA, Japan Abstract target are located in series. Every 3 s or so, depending The user experiments at J-PARC have just started. upon the usage of the main ring (MR), the beam is JPARC, which stands for Japan Proton Accelerator extracted from the RCS to be injected to the MR. Here, it Research Complex, comprises a 400-MeV linac (at is ramped up to 30 GeV at present and slowly extracted to present: 180 MeV, being upgraded), a 3-GeV rapid- Hadron Experimental Hall, where the kaon-production cycling synchrotron (RCS), and a 50-GeV main ring target is located. The experiments using the kaons are (MR) synchrotron, which is now in operation at 30 GeV. conducted there. Sometimes, it is fast extracted to The RCS will provide the muon-production target and the produce the neutrinos, which are sent to the Super spallation-neutron-production target with a beam power Kamiokande detector, which is located 295-km west of of 1 MW (at present: 120 kW) at a repetition rate of 25 the J-PARC site. In the future, we are conceiving the Hz. The muons and neutrons thus generated will be used possibility of constructing a test facility for an in materials science, life science, and others, including accelerator-driven nuclear waste transmutation system, industrial applications. The beams that are fast extracted which was shifted to Phase II. We are trying every effort from the MR generate neutrinos to be sent to the Super to get funding for this facility. -
Baryogenesis and Dark Matter from B Mesons: B-Mesogenesis
Baryogenesis and Dark Matter from B Mesons: B-Mesogenesis Miguel Escudero Abenza [email protected] arXiv:1810.00880, PRD 99, 035031 (2019) with: Gilly Elor & Ann Nelson Based on: arXiv:2101.XXXXX with: Gonzalo Alonso-Álvarez & Gilly Elor New Trends in Dark Matter 09-12-2020 The Universe Baryonic Matter 5% 26% Dark Matter 69% Dark Energy Planck 2018 1807.06209 Miguel Escudero (TUM) B-Mesogenesis New Trends in DM 09-12-20 !2 Theoretical Understanding? Motivating Question: What fraction of the Energy Density of the Universe comes from Physics Beyond the Standard Model? 99.85%! Miguel Escudero (TUM) B-Mesogenesis New Trends in DM 09-12-20 !3 SM Prediction: Neutrinos 40% 60% Photons Miguel Escudero (TUM) B-Mesogenesis New Trends in DM 09-12-20 !4 The Universe Baryonic Matter 5% 26% Dark Matter 69% Dark Energy Planck 2018 1807.06209 Miguel Escudero (TUM) B-Mesogenesis New Trends in DM 09-12-20 !5 Baryogenesis and Dark Matter from B Mesons: B-Mesogenesis arXiv:1810.00880 Elor, Escudero & Nelson 1) Baryogenesis and Dark Matter are linked 2) Baryon asymmetry directly related to B-Meson observables 3) Leads to unique collider signatures 4) Fully testable at current collider experiments Miguel Escudero (TUM) B-Mesogenesis New Trends in DM 09-12-20 !6 Outline 1) B-Mesogenesis 1) C/CP violation 2) Out of equilibrium 3) Baryon number violation? 2) A Minimal Model & Cosmology 3) Implications for Collider Experiments 4) Dark Matter Phenomenology 5) Summary and Outlook Miguel Escudero (TUM) B-Mesogenesis New Trends in DM 09-12-20 !7 Baryogenesis -
Design Study of a Superconducting Insertion Quadrupole Magnet for the Large Hadron Collider
EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH European Laboratory for Particle Physics Large Hadron Collider Project LHC Project Report 75 DESIGN STUDY OF A SUPERCONDUCTING INSERTION QUADRUPOLE MAGNET FOR THE LARGE HADRON COLLIDER G. Kirby, R. Ostojic, and T. M. Taylor A. Yamamoto*, K. Tsuchiya*, N. Higashi*, T. Nakamoto*, T. Ogitsu*, N. Ohuchi*, T. Shintomi*, and A. Terashima* Abstract The conceptual design study of a high gradient superconducting insertion quadrupole magnet has been carried out in collaboration between KEK and CERN for the Large Hadron Collider (LHC) to be built at CERN. A model magnet design has been optimized to provide a nominal design field gradient of 240 T/m with a bore aperture of 70 mm and an operational field gradient of 225 T/m at 1.9 K under radiation environment with a beam energy deposit of several watts per meter in the superconducting coils. The design and its optimization process are discussed. LHC Division *National Laboratory for High Energy Physics (KEK), Tsukuba, Ibaraki, 305, Japan ASC Pittsburg ‘96 Administrative Secretariat LHC Division CERN CH - 1211 Geneva 23 Switzerland Geneva, 12 November 1996 Design Study of a Superconducting Insertion Quadrupole Magnet for The Large Hadron Collider A. Yamamoto, K. Tsuchiya, N. Higashi, T. Nakamoto T. Ogitsu, N. Ohuchi, T. Shintomi, and A. Terashima National Laboratory [or High Energy Physics (KEK), Tsukuba, Ibaraki, 305, Japan G. Kirby*, R. Ostojic, and T. M. Taylor European Laboratory for Particle Physics (CERN), 23 Geneva, CH-1211, Switzerland Abstract---The conceptual design study of a 111. MODEL MAGNET DESIGN high gradient superconducting insertion quadrupole magnet has been carried out i n A. -
Development of Pulsed Neutron Sources パルス中性子源の開発
23/12/2020 Development of Pulsed Neutron Sources パルス中性子源の開発 Yoshiaki Kiyanagi 鬼柳善明 Nagoya University 名古屋大学工学研究科 1 History of Pulsed Neutron Sources (Change of plans from 1990) ESS SNS J-PARC (2022?) (2006) (2008) (1982) (1985) IPNS(1981) KENS(1980) 136MeV 1971 1959 300MeV 45MeV Hokkaido 1973 45MeV 2 Accelerator-driven Neutron Sources before KENS established in 1980 (Electron Acc.) (Except for nuclear data measurements) Hokkaido University The Gaerttner Linear Accelerator Center at Rensselaer Polytechnic Institute (RPI) Harwell Linac Linac at Laboratory of Nuclear Science at (opposite present ISIS) Tohoku University (LNS) (Present: Research Center for Electron Photon Science) 3 National Laboratory for High Energy Physics: KEK (Now, High Energy Accelerator Research Organization) Booster Synchrotron Utilization Facility KENS:KEK Neutron Source (KEK中性子源) Green area Proton therapy Muon https://www2.kek.jp/openhouse/1996/image/BSF/BSF7.gif 4 Coupling of Target-Moderator- Reflector research Late Prof. Watanabe performed experiments using a RI neutron source. スパレーション・パルス中性子源KENSとそれによる中性子散乱 渡邊昇、佐々木寛、石川義和 日本原子力学会誌 Vol. 23, No. 6 (1981) 389-398 5 Development of a Methane Cold Moderator at Hokkaido University Cylindrical shape Neutron Energy Spectra Spectra Energy Neutron moderator with a re-entrant hole Neutron Energy (eV) K. Inoue, N. Otomo, H. Iwasa and Y. Kiyanagi, J. Nuclear Science and Technology, Vol.11, No.5, pp.228-229, (1974) 6 KENS Neutron source Cold source Co-existence Thermal source The first cold neutron source set at a dedicated neutron scattering experimental facility. (There was an opinion a cold source was not necessary for neutron sources based on accelerators) A wise decision by Professors Watanabe and Ishikawa 渡邊昇, 石川義和: 物理学会誌, 39, 826 (1984). -
Peering Into the Universe and Its Ele Mentary
A gigantic detector to explore elementary particle unification theories and the mysteries of the Universe’s evolution Peering into the Universe and its ele mentary particles from underground Ultrasensitive Photodetectors The planned Hyper-Kamiokande detector will consist of an Unified Theory and explain the evolution of the Universe order of magnitude larger tank than the predecessor, Super- through the investigation of proton decay, CP violation (the We have been developing the world’s largest photosensors, which exhibit a photodetection Kamiokande, and will be equipped with ultra high sensitivity difference between neutrinos and antineutrinos), and the efficiency two times greater than that of the photosensors. The Hyper-Kamiokande detector is both a observation of neutrinos from supernova explosions. The Super-Kamiokande photosensors. These new “microscope,” used to observe elementary particles, and a Hyper-Kamiokande experiment is an international research photosensors are able to perform light intensity “telescope”, used to study the Sun and supernovas through project aiming to become operational in the second half of and timing measurements with a much higher neutrinos. Hyper-Kamiokande aims to elucidate the Grand the 2020s. precision. The new Large-Aperture High-Sensitivity Hybrid Photodetector (left), the new Large-Aperture High-Sensitivity Photomultiplier Tube (right). The bottom photographs show the electron multiplication component. A megaton water tank The huge Hyper-Kamiokande tank will be used in order to obtain in only 10 years an amount of data corresponding to 100 years of data collection time using Super-Kamiokande. This Experimental Technique allows the observation of previously unrevealed The photosensors on the tank wall detect the very weak Cherenkov rare phenomena and small values of CP light emitted along its direction of travel by a charged particle violation. -
Baryogenesis and Dark Matter from B Mesons
Baryogenesis and Dark Matter from B mesons Abstract: In [1] a new mechanism to simultaneously generate the baryon asymmetry of the Universe and the Dark Matter abundance has been proposed. The Standard Model of particle physics succeeds to describe many physical processes and it has been tested to a great accuracy. However, it fails to provide a Dark Matter candidate, a so far undetected component of matter which makes up roughly 25% of the energy budget of the Universe. Furthermore, the question arises why there is a more matter (or baryons) than antimatter in the Universe taking into account that cosmology predicts a Universe with equal parts matter and anti-matter. The mechanism to generate a primordial matter-antimatter asymmetry is called baryogenesis. Any successful mechanism for baryogenesis needs to satisfy the three Sakharov conditions [2]: • violation of charge symmetry and of the combination of charge and parity symmetry • violation of baryon number • departure from thermal equilibrium In this paper [1] a new mechanism for the generation of a baryon asymmetry together with Dark Matter production has been proposed. The mechanism proposed to explain the observed baryon asymetry as well as the pro- duction of dark matter is developed around a fundamental ingredient: a new scalar particle Φ. The Φ particle is massive and would dominate the energy density of the Universe after inflation but prior to the Bing Bang nucleosynthesis. The same particle will directly decay, out of thermal equilibrium, to b=¯b quarks and if the Universe is cool enough ∼ O(10 MeV), the produced b quarks can hadronize and form B-mesons. -
Atomic Electric Dipole Moments and Cp Violation
261 ATOMIC ELECTRIC DIPOLE MOMENTS AND CP VIOLATION S.M.Barr Bartol Research Institute University of Delaware Newark, DE 19716 USA Abstract The subject of atomic electric dipole moments, the rapid recent progress in searching for them, and their significance for fundamental issues in particle theory is surveyed. particular it is shown how the edms of different kinds of atoms and molecules, as well Inas of the neutron, give vital information on the nature and origin of CP violation. Special stress is laid on supersymmetric theories and their consequences. 262 I. INTRODUCTION In this talk I am going to discuss atomic and molecular electric dipole moments (edms) from a particle theorist's point of view. The first and fundamental point is that permanent electric dipole moments violate both P and T. If we assume, as we are entitled to do, that OPT is conserved then we may speak equivalently of T-violation and OP-violation. I will mostly use the latter designation. That a permanent edm violates T is easily shown. Consider a proton. It has a magnetic dipole moment oriented along its spin axis. Suppose it also has an electric edm oriented, say, parallel to the magnetic dipole. Under T the electric dipole is not changed, as the spatial charge distribution is unaffected. But the magnetic dipole changes sign because current flows are reversed by T. Thus T takes a proton with parallel electric and magnetic dipoles into one with antiparallel moments. Now, if T is assumed to be an exact symmetry these two experimentally distinguishable kinds of proton will have the same mass. -
High Energy Accelerator Research Organization Research Institute of Japan’S Largest Accelerator Science That Unravels the Mysteries of Universe, Matter and Life
Inter-University Research Institute Corporation High Energy Accelerator Research Organization Research institute of Japan’s largest accelerator science that unravels the mysteries of universe, matter and life Director General Masanori Yamauchi Particle accelerator has played extremely important roles in progress of our understanding of nature, since its history started in 1930’s. It has provided essential methodology to study nuclei, elementary particles, condensed matter and even life sciences. Also, role of particle accelerators is really outstanding in their industrial and medical applications. There is no doubt that progress of par- ticle accelerators has substantially contributed to the modern science. Technologies of particle accelerators are still advancing rapidly, and drive frontier of science and applied research. KEK has established its credit as one of the leading accelerator laboratories in the world, and is making substantial contributions to the basic sciences in the various fields. It serves as one of the inter-university research organizations to offer opportunities of fron- tier research to scientists and students in the Japanese universities, and contributes to progress of scientific research in Japan. More than 20,000 scientists visit KEK every year from abroad to carry out research program extensively at the accelerator facilities here. This provides extraordinary opportunity especially to young scientists to compete with each other internationally. Accomplishments of those international collaborations include: confirmation of Kobayashi-Maskawa theory, discoveries of many exotic compound par- ticles and clarification of neutrino oscillation. Remarkable achievements have been obtained in material and life science as well, such as structure determination of novel superconductors and protein-drug complexes, and studies of novel properties induced by hydro- gen atoms, spins and electrons in condensed matter. -
Session: Neutrino Astronomy
Session: Neutrino Astronomy Chair: Takaaki Kajita, Institute for Cosmic Ray Research, Univ. of Tokyo Basic natures of neutrinos Neutrino was introduced in 1930 by W. Pauli in order to save the energy conservation law in nuclear beta decay processes, in which the emitted electron exhibits a continuous energy spectrum. It was assumed that the penetration power of neutrinos is much higher than that of the gamma rays. More than 20 years later, the existence of neutrinos was experimentally confirmed by an experiment that measured neutrinos produced by a nuclear power reactor. Since then, the basic nature of neutrinos has been understood through various theoretical and experimental studies: Neutrinos interact with matter extremely weakly. The number of neutrino species is three. They are called electron-neutrino, muon-neutrino and tau-neutrino. In addition, recent neutrino experiments discovered that neutrinos have very small masses. Observing the Universe by neutrinos (1) Because of the extremely high penetration power of neutrinos, neutrinos produced at the center of a star easily penetrate to the outer space. Theories of astrophysics predict that there are various processes that neutrinos play an essential role at the center of stars. For example, the Sun is generating its energy by nuclear fusion processes in the central region. In these processes, low energy electron neutrinos with various energy spectra are generated. Thus the observation of solar neutrinos directly probes the nuclear fusion reactions in the Sun. Another example is the supernova explosion. While the optical measurements observe an exploding star, what is happening in the central region of the star is the collapse of the core of a massive star. -
Carsten Rott Curriculum Vitae Feb 2018
Carsten Rott Curriculum Vitae Feb 2018 Department of Physics, Sungkyunkwan University, Suwon 16419, Korea Tel: +82-31-290-5902 E-mail:[email protected] Experimental astro-particle physics, particle physics, geophysics, neutri- Research nos physics Focus Languages German, English; Elementary: French, Japanese, and Korean Employment 2017 { 2018 Honorary Fellow at Wisconsin IceCube Particle Astrophysics Center (WIPAC) (Sabbatical), University of Wisconsin Madison, USA 2017 { now Associate Professor, Sungkyunkwan University, Korea 2013 { 2017 Assistant Professor, Sungkyunkwan University, Korea 2016 Visiting Researcher (3-month), University of Tokyo, Japan 2009 { 2013 Senior Fellow of the Center for Cosmology and AstroParticle Physics (CCAPP) (5-year term), The Ohio State University, USA 2008 { 2009 CCAPP Fellow (3-year term), The Ohio State University, USA 2005 { 2008 Postdoctoral Fellow, Pennsylvania State University, USA Education 1998 { 2004 Purdue University, Indiana, USA Ph.D in Experimental Particle Physics (December 2004) Title : \Search for Scalar Bottom Quarks from Gluino Decays" at CDF Thesis Adviser : Prof. Daniela Bortoletto 1995 { 1998 Universit¨atHannover, Hannover, Germany Honors and Awards 2011 Recipient of NSF Antarctica Service Medal 2005 \Fermilab's Result of the Week" (FermiNews, August 11, 2005) 2004 George W. Tautfest Award, Purdue University 1998 { 1999 University of Hannover { Purdue University direct exchange fellowship Funds and Grants 2017 { present NRF Midscale Research Fund (PI), Korea { NRF-2017R1A2B2003666 2017 { present Foreign Facility Fund (PI of 7 sub-PIs) { NRF-2017K1A3A7A09015973 2016 { present NRF SRC Korea Neutrino Research Center (KNRC) (Co-I), Korea 2016 { 2017 NRF Individual Researcher (PI), Korea { NRF-2016R1D1A1B03931688 2013 { present BrainKorea (BK21plus) participant, Korea 2013 { 2016 NRF Individual Researcher (PI), Korea { NRF-2013R1A1A1007068 2013 { 2014 SKKU Intramural Faculty Fund Award, Korea 2013 { 2014 Fermi GI Cycle 6 (Co-I with Prof.