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CERN Courier – Digital Edition Welcome to the Digital Edition of the January/February 2013 Issue of CERN Courier – the First Digital Edition of This Magazine
I NTERNATIONAL J OURNAL OF H IGH -E NERGY P HYSICS CERNCOURIER WELCOME V OLUME 5 3 N UMBER 1 J ANUARY /F EBRUARY 2 0 1 3 CERN Courier – digital edition Welcome to the digital edition of the January/February 2013 issue of CERN Courier – the first digital edition of this magazine. CERN Courier dates back to August 1959, when the first issue appeared, consisting of eight black-and-white pages. Since then it has seen many changes in design and layout, leading to the current full-colour editions of more than 50 pages on average. It went on the web for the High luminosity: first time in October 1998, when IOP Publishing took over the production work. Now, we have taken another step forward with this digital edition, which provides yet another means to access the content beyond the web the heat is on and print editions, which continue as before. Back in 1959, the first issue reported on progress towards the start of CERN’s first proton synchrotron. This current issue includes a report from the physics frontier as seen by the ATLAS experiment at the laboratory’s current flagship, the LHC, as well as a look at work that is under way to get the most from this remarkable machine in future. Particle physics has changed a great deal since 1959 and this is reflected in the article on the emergence of QCD, the theory of the strong interaction, in the early 1970s. To sign up to the new issue alert, please visit: http://cerncourier.com/cws/sign-up To subscribe to the print edition, please visit: http://cerncourier.com/cws/how-to-subscribe LHC PHYSICS FERMILAB FRONTIER Using monojets Oddone to retire to point the way after eight PHYSICS EDITOR: CHRISTINE SUTTON, CERN to new physics fruitful years Opening up DIGITAL EDITION CREATED BY JESSE KARJALAINEN/IOP PUBLISHING, UK p7 p35 interdisciplinarity p33 CERNCOURIER www. -
Switching Neutrinos
Research in Progress Physics Fl avor- -Switching Neutrinos rof. Ewa Rondio from the National P Center for Nuclear Research (NCBJ) explains the nature of neutrinos, the measurements taken by the Super-Kamiokande detector, and the involvement of Polish scientists in the project. MIJAKOWSKI PIOTR ACADEMIA: What are neutrinos? What is the difference between the neutrinos that PROF. EWA RONDIO: Literally translated, the word come from space and the neutrinos created on Earth? “neutrino” means “little neutral one.” The name was Neutrinos arriving from space are almost as abundant first suggested when the existence of neutrinos was as photons in the cosmic background radiation, but proposed to patch up the law of conservation of en- their energies are so small that we’re unable to detect ergy. It had turned out that without postulating their them. We can’t see them, even though there are so existence we could not explain why the spectrum of many of them. We can only observe higher-energy energy in beta decay is continuous, whereas two-body neutrinos, for example those arriving from the Sun. decay should give a single constant value. Back then, At first glance, they do not differ in any way from that postulate was considered very risky, because it those made on Earth. However, they have somewhat was believed that such particles would be impossible different energies. Also, those arriving from space are to observe. Experimental physicists have nowadays predominantly neutrinos, whereas those we produce managed that, although it took them quite a long time. on Earth produce are chiefly antineutrinos. -
Radiochemical Solar Neutrino Experiments, "Successful and Otherwise"
BNL-81686-2008-CP Radiochemical Solar Neutrino Experiments, "Successful and Otherwise" R. L. Hahn Presented at the Proceedings of the Neutrino-2008 Conference Christchurch, New Zealand May 25 - 31, 2008 September 2008 Chemistry Department Brookhaven National Laboratory P.O. Box 5000 Upton, NY 11973-5000 www.bnl.gov Notice: This manuscript has been authored by employees of Brookhaven Science Associates, LLC under Contract No. DE-AC02-98CH10886 with the U.S. Department of Energy. The publisher by accepting the manuscript for publication acknowledges that the United States Government retains a non-exclusive, paid-up, irrevocable, world-wide license to publish or reproduce the published form of this manuscript, or allow others to do so, for United States Government purposes. This preprint is intended for publication in a journal or proceedings. Since changes may be made before publication, it may not be cited or reproduced without the author’s permission. DISCLAIMER This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of their employees, nor any of their contractors, subcontractors, or their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or any third party’s use or the results of such use of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise, does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof or its contractors or subcontractors. -
Kavli IPMU Annual 2014 Report
ANNUAL REPORT 2014 REPORT ANNUAL April 2014–March 2015 2014–March April Kavli IPMU Kavli Kavli IPMU Annual Report 2014 April 2014–March 2015 CONTENTS FOREWORD 2 1 INTRODUCTION 4 2 NEWS&EVENTS 8 3 ORGANIZATION 10 4 STAFF 14 5 RESEARCHHIGHLIGHTS 20 5.1 Unbiased Bases and Critical Points of a Potential ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙20 5.2 Secondary Polytopes and the Algebra of the Infrared ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙21 5.3 Moduli of Bridgeland Semistable Objects on 3- Folds and Donaldson- Thomas Invariants ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙22 5.4 Leptogenesis Via Axion Oscillations after Inflation ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙23 5.5 Searching for Matter/Antimatter Asymmetry with T2K Experiment ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ 24 5.6 Development of the Belle II Silicon Vertex Detector ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙26 5.7 Search for Physics beyond Standard Model with KamLAND-Zen ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙28 5.8 Chemical Abundance Patterns of the Most Iron-Poor Stars as Probes of the First Stars in the Universe ∙ ∙ ∙ 29 5.9 Measuring Gravitational lensing Using CMB B-mode Polarization by POLARBEAR ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ 30 5.10 The First Galaxy Maps from the SDSS-IV MaNGA Survey ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙32 5.11 Detection of the Possible Companion Star of Supernova 2011dh ∙ ∙ ∙ ∙ ∙ ∙ -
Searching for Lightweight Dark Matter in Nova Near Detector
Searching for Lightweight Dark Matter in NOvA Near Detector PoS(FPCP2017)056 Filip Jediný* Czech Technical University in Prague Brehova 7, Prague, Czech Republic E-mail: [email protected] Athanasios Hatzikoutelis University of Tennessee Knoxville Knoxville, TN, USA E-mail: [email protected] Sergey Kotelnikov Fermi National Accelerator Laboratory Kirk and Pine st., Batavia, IL, USA E-mail: [email protected] Biao Wang Southern Methodist University Dallas, TX, USA E-mail: [email protected] The NOvA long-baseline neutrino oscillation experiment is receiving record numbers of 120GeV protons on target from Fermilab's NuMI neutrino beam. We take advantage of our experiment’s sophisticated particle identification algorithms to search for Lightweight Dark Matter (LDM) in the first year of data from the Near Detector of NOvA (300-ton low-Z mass, placed off the beam axis) during the experiment’s first physics runs. Theoretical models of LDM predict that bellow- 10GeV candidates produced in the NuMI target might scatter or decay in the NOvA Near Detector. We simulate an example of the Neutral Vector Portal model with the sensitivity estimate of 10-39 cm2, which corresponds to O(10) LDM candidates per three years of data, looking at single electromagnetic showers between 5 and 15 GeV in a model independent way. The 15th International Conference on Flavor Physics & CP Violation 5-9 June, 2017 Prague, Czech Republic * Speaker Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0). http://pos.sissa.it/ Searching for LDM in NOvA ND Filip Jediný 1. -
Neutrino Oscillations: T2k and Na61 Experiments, R&D
NEUTRINO OSCILLATIONS: T2K AND NA61 EXPERIMENTS, R&D TOWARDS A FUTURE NEUTRINO PROGRAM 1 Research Plan The field of neutrino physics is certainly one of the most active in particle physics today. It is by now well established that neutrinos have mass and that the three families mix. In the minimal Standard Model, neutrinos are massless; massive neutrinos require either a new ad- hoc conservation law or new phenomena beyond the present framework, with a possible link to the grand unification scale via the see-saw mechanism. A deep field of research is thus open, that could last several decades and culminate with the discovery of leptonic CP violation – a key ingredient in the understanding of the baryon- anti-baryon asymmetry of the universe. Because observation of CP violation in neutrino oscillations requires appearance experiments, accessible at accelerators only, an important investment in accelerator-based neutrino beams and experiments is called for. The CHIPP Roadmap considers neutrino physics as one of the three pillars of particle physics in Switzerland, and so does the 15 years research plan of the DPNC at University of Geneva1. The neutrino group at DPNC has been actively involved in this quest since the nomination of Prof. A. Blondel in early 2000, where participation in the HARP experiment at CERN led us to the K2K experiment in Japan, in which the first observation of neutrino oscillation with a neutrino beam was achieved. The group received an added boost with the nomination of Alessandro Bravar (MER) in 2006. The research program comprises a progression of on- going experiments and far-reaching R&D activity as described in the SNF reports of October 2007 and October 2008. -
Long Baseline Neutrino Oscillation Experiments 1 Introduction 2
Long Baseline Neutrino Oscillation Experiments Mark Thomson Cavendish Laboratory Department of Physics JJ Thomson Avenue Cambridge, CB3 0HE United Kingdom 1 Introduction In the last ten years the study of the quantum mechanical e®ect of neutrino os- cillations, which arises due to the mixing of the weak eigenstates fºe; º¹; º¿ g and the mass eigenstates fº1; º2; º3g, has revolutionised our understanding of neutrinos. Until recently, this understanding was dominated by experimental observations of at- mospheric [1, 2, 3] and solar neutrino [4, 5, 6] oscillations. These measurements have been of great importance. However, the use of naturally occuring neutrino sources is not su±cient to determine fully the flavour mixing parameters in the neutrino sector. For this reason, many of the current and next generation of neutrino experiments are based on high intensity accelerator generated neutrino beams. The ¯rst generation of these long-baseline (LBL) neutrino oscillation experiments, K2K, MINOS and CNGS, are the main subject of this review. The next generation of LBL experiments, T2K and NOºA, are also discussed. 2 Theoretical Background For two neutrino weak eigenstates fº®; º¯g related to two mass eigenstates fºi; ºjg, by a single mixing angle θij, it is simple to show that the survival probability of a neutrino of energy Eº and flavour ® after propagating a distance L through the vacuum is à ! 2 2 2 2 1:27¢mji(eV )L(km) P (º® ! º®) = 1 ¡ sin 2θij sin ; (1) Eº(GeV) 2 2 2 where ¢mji is the di®erence of the squares of the neutrino masses, mj ¡ mi . -
Measurements of Hadronic Cross Section for Precise Determination of Neutrino Beam Properties in T2K Oscillation Experiment
University of Warsaw Faculty of Physics Institute of Experimental Physics Measurements of Hadronic Cross Section for Precise Determination of Neutrino Beam Properties in T2K Oscillation Experiment Magdalena Zofia Posiadała Ph.D. thesis written under supervision of prof. dr hab. Danuta Kiełczewska Warsaw, 2011 Abstract Differential cross sections and mean multiplicities in production processes for low momentum charged pion mesons and protons in p+C interactions at 31 GeV/c measured with the large acceptance NA61/SHINE spectrometer at the CERN SPS are presented. A set of data col- lected during the first NA61/SHINE run in 2007 with a thin graphite target was used for the analysis. The results are presented as a function of laboratory momentum in 10 intervals of the laboratory polar angle covering the range from 0 up to 420 mrad. The spectra are compared with predictions of several hadron production models. Measurements for π+ and π− mesons are used by the T2K experiment to tune neutrino beam simulations and reduce uncertainties on charged pion production. Contents List of Figures vii List of Tables xi Acknowledgments xii Introduction 1 1 Neutrinos 4 1.1 Neutrino oscillation mechanism . .5 1.2 The Current Situation in Neutrino Oscillation Physics . .7 2 T2K experiment and its prerequisites for NA61/SHINE measurements 18 2.1 The T2K long baseline neutrino oscillation experiment . 18 2.2 J-PARC facility . 20 2.2.1 J-PARC accelerator . 20 2.2.2 Primary and secondary T2K beamline . 20 2.2.3 Near detector complex . 23 2.3 Overview of the Super-Kamiokande detector . 24 2.4 T2K physical goals . -
A Brief Overview of Neutrino Oscillabon Results and Future Prospects
A brief overview of neutrino oscillaon results and future prospects Trevor Stewart On behalf of the T2K collaboraon Rutherford Appleton Laboratory ICNFP 2016 01/01/2015 Trevor Stewart, RAL 1 The Nobel Prize in Physics 2015 Takaaki Kajita, Arthur B. McDonald “for the discovery of neutrino oscillaons, which shows that neutrinos have mass" 06/07/2016 Trevor Stewart, RAL 2 Intoduc2on • This talk will discuss recent neutrino oscillaon results and how they contribute to our overall understanding of the physics of neutrinos • Will present results from current experiments such as T2K, NOνA, Daya Bay, RENO, and Double Chooz • Discuss future experiments such as Hyper- Kamiokande, DUNE, and JUNO • If I do not men2on your favourite experiment then please forgive me, it is for the sake of brevity 01/01/2015 Trevor Stewart, RAL 3 Two-flavour neutrino oscillaons ⌫ cos✓ sin✓ ⌫ • e = 1 Two sets of eigenstates for ⌫µ sin✓ cos✓ ⌫2 neutrinos ✓ ◆ ✓− ◆✓ 2 ◆ - Flavour states which 2 2 ⎛ Δm L ⎞ P(ν →ν ) = sin (2θ )sin ⎜ ⎟ interact µ e ⎜ 4E ⎟ ∆m2 = m2 m2 ⎝ ⎠ - Mass states which 2 − 1 propagate ⌫µ ⌫1, ⌫2 ⌫µ or ⌫e • Measure • Result probabili2es – Mixing angle(s) – Disappearance – Mass differences – Appearance 01/01/2015 Trevor Stewart, RAL 4 The Pontecorvo-Maki-Nakagawa-Sakata (PMNS) mixing matrix ⌫e ⌫1 • Unfortunately things are not as ⌫ = U ⌫ 0 µ1 0 21 simple as the 2-flavour mixing ⌫⌧ ⌫3 shown on the previous slide @ A @ A • 3-flavour mixing Flavour eigenstates Mass eigenstates - Three independent mixing (coupling to the W, Z) (definite masses) angles and CP violang -
Measurement of Hadron-Carbon Interactions for Better Understanding of Air Showers with NA61/SHINE
33RD INTERNATIONAL COSMIC RAY CONFERENCE,RIO DE JANEIRO 2013 THE ASTROPARTICLE PHYSICS CONFERENCE Measurement of hadron-carbon interactions for better understanding of air showers with NA61/SHINE H. P. DEMBINSKI1 FOR THE NA61/SHINE COLLABORATION2. 1 Institut fur¨ Kernphysik, KIT Karlsruhe, Postfach 3640, D - 76021 Karlsruhe 2 Full author list: https: // na61. web. cern. ch/ na61/ pages/ storage/ authors_ list. pdf [email protected] Abstract: The interpretation of air shower measurements requires the detailed simulation of hadronic particle production over a wide range of energies and the forward phase space of secondary particles. In air showers, the bulk of particles is produced at later stages of the shower development and at equivalent beam energies in the sub-TeV range. NA61/SHINE is a fixed target experiment using secondary beams produced at the SPS at 1 CERN. Hadron-hadron interactions have been recorded at beam momenta between 13 and 350 GeVc− with a wide-acceptance spectrometer. In this article we present measurements of the inelastic cross-section and secondary particle yields of pion-carbon interactions, which are essential for modelling air showers. Keywords: hadron interaction, QCD, air shower, pion 1 Hadronic interactions in air showers Cosmic rays initiate extensive air showers (EAS) when they collide with nuclei of the atmosphere. The EAS data recorded by experiments like the Pierre Auger Observa- tory [1], KASCADE [2] or IceTop [3], is used to infer their properties. The interpretation relies on simulations of the shower development during which electromagnetic and hadronic particle interactions are followed from primary 20 9 energies of & 10 eV down to energies of 10 eV. -
NA61/SHINE Facility at the CERN SPS: Beams and Detector System
Preprint typeset in JINST style - HYPER VERSION NA61/SHINE facility at the CERN SPS: beams and detector system N. Abgrall11, O. Andreeva16, A. Aduszkiewicz23, Y. Ali6, T. Anticic26, N. Antoniou1, B. Baatar7, F. Bay27, A. Blondel11, J. Blumer13, M. Bogomilov19, M. Bogusz24, A. Bravar11, J. Brzychczyk6, S. A. Bunyatov7, P. Christakoglou1, T. Czopowicz24, N. Davis1, S. Debieux11, H. Dembinski13, F. Diakonos1, S. Di Luise27, W. Dominik23, T. Drozhzhova20 J. Dumarchez18, K. Dynowski24, R. Engel13, I. Efthymiopoulos10, A. Ereditato4, A. Fabich10, G. A. Feofilov20, Z. Fodor5, A. Fulop5, M. Ga´zdzicki9;15, M. Golubeva16, K. Grebieszkow24, A. Grzeszczuk14, F. Guber16, A. Haesler11, T. Hasegawa21, M. Hierholzer4, R. Idczak25, S. Igolkin20, A. Ivashkin16, D. Jokovic2, K. Kadija26, A. Kapoyannis1, E. Kaptur14, D. Kielczewska23, M. Kirejczyk23, J. Kisiel14, T. Kiss5, S. Kleinfelder12, T. Kobayashi21, V. I. Kolesnikov7, D. Kolev19, V. P. Kondratiev20, A. Korzenev11, P. Koversarski25, S. Kowalski14, A. Krasnoperov7, A. Kurepin16, D. Larsen6, A. Laszlo5, V. V. Lyubushkin7, M. Mackowiak-Pawłowska´ 9, Z. Majka6, B. Maksiak24, A. I. Malakhov7, D. Maletic2, D. Manglunki10, D. Manic2, A. Marchionni27, A. Marcinek6, V. Marin16, K. Marton5, H.-J.Mathes13, T. Matulewicz23, V. Matveev7;16, G. L. Melkumov7, M. Messina4, St. Mrówczynski´ 15, S. Murphy11, T. Nakadaira21, M. Nirkko4, K. Nishikawa21, T. Palczewski22, G. Palla5, A. D. Panagiotou1, T. Paul17, W. Peryt24;∗, O. Petukhov16 C.Pistillo4 R. Płaneta6, J. Pluta24, B. A. Popov7;18, M. Posiadala23, S. Puławski14, J. Puzovic2, W. Rauch8, M. Ravonel11, A. Redij4, R. Renfordt9, E. Richter-Wa¸s6, A. Robert18, D. Röhrich3, E. Rondio22, B. Rossi4, M. Roth13, A. Rubbia27, A. Rustamov9, M. -
Neutrino Book
The challenge of neutrinos Preparing the Gargamelle bubble chamber at CERN in 1969. In 1973 the chamber took the first historic photographs of neutral current interactions. (Photo CERN 409.9.69) Neutrino book Gargamelle and Neutral Currents - The Story of a Vital Discovery by Andre Rousset Andre Rousset's book (in French - Gargamelle et les Courants Neutres - Ecole des Mines de Paris) tells the story of Gargamelle and the discov ery at CERN in 1973 of neutral currents, the cornerstone of the electroweak theory. This vital discov ery helped to give credence to the Standard Model of particle physics. Rousset is both an observer and one of the key figures in the story. His book is lively and well docu mented; in it he uses archive material to ensure the accuracy of his infor mation on dates, choices and deci sions. ously" to the project was probably in an interesting manner the theo After an introduction to particle what swung the decision. rists' "green light", giving the go- physics which puts into perspective Construction took five years, during ahead to the experimentalists. In fact, the electroweak theory unifying weak which many problems were encoun the European collaboration (Aachen, and electromagnetic interactions, tered, right up to the fault in the main Brussels, CERN, Ecole Polytechni Rousset comes straight to the point. part of the chamber which caused que, Milan, Orsay, UC London) was From the late 1950s onwards he was delays and, a few years later, was to divided between a study of the quark- involved in the construction of the prove fatal to the detector.