TRIUMF Shares the 2016 Breakthrough Prize in Fundamental Physics
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CERN Courier–Digital Edition
CERNMarch/April 2021 cerncourier.com COURIERReporting on international high-energy physics WELCOME CERN Courier – digital edition Welcome to the digital edition of the March/April 2021 issue of CERN Courier. Hadron colliders have contributed to a golden era of discovery in high-energy physics, hosting experiments that have enabled physicists to unearth the cornerstones of the Standard Model. This success story began 50 years ago with CERN’s Intersecting Storage Rings (featured on the cover of this issue) and culminated in the Large Hadron Collider (p38) – which has spawned thousands of papers in its first 10 years of operations alone (p47). It also bodes well for a potential future circular collider at CERN operating at a centre-of-mass energy of at least 100 TeV, a feasibility study for which is now in full swing. Even hadron colliders have their limits, however. To explore possible new physics at the highest energy scales, physicists are mounting a series of experiments to search for very weakly interacting “slim” particles that arise from extensions in the Standard Model (p25). Also celebrating a golden anniversary this year is the Institute for Nuclear Research in Moscow (p33), while, elsewhere in this issue: quantum sensors HADRON COLLIDERS target gravitational waves (p10); X-rays go behind the scenes of supernova 50 years of discovery 1987A (p12); a high-performance computing collaboration forms to handle the big-physics data onslaught (p22); Steven Weinberg talks about his latest work (p51); and much more. To sign up to the new-issue alert, please visit: http://comms.iop.org/k/iop/cerncourier To subscribe to the magazine, please visit: https://cerncourier.com/p/about-cern-courier EDITOR: MATTHEW CHALMERS, CERN DIGITAL EDITION CREATED BY IOP PUBLISHING ATLAS spots rare Higgs decay Weinberg on effective field theory Hunting for WISPs CCMarApr21_Cover_v1.indd 1 12/02/2021 09:24 CERNCOURIER www. -
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. -
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 ∙ ∙ ∙ ∙ ∙ ∙ -
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 . -
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 -
2019/20 Perimeter Institute Annual Report English
2020 ANNUAL REPORT VISION To create the world’s foremost centre for research, graduate training, and educational outreach in theoretical physics, uniting public and private partners, and the world’s best scientific minds, in a shared enterprise to achieve breakthroughs that will transform our future. Estelle Inack, Jason Iaconis, and Roger Melko, October 2019 CONTENTS Message from the Board Chair .............................................2 Message from the Institute Director ......................................3 How Perimeter Measures Up ................................................4 Research ...............................................................................6 Training ................................................................................26 Outreach ..............................................................................32 Our Future is Bright .............................................................38 Advancement ......................................................................40 Governance and Finance ....................................................44 Appendices .........................................................................51 This report covers the activities and finances of Perimeter Institute for Theoretical Physics from August 1, 2019, to July 31, 2020. TODAY'S THEORETICAL PHYSICS IS TOMORROW'S TECHNOLOGY MESSAGE FROM THE BOARD CHAIR The coronavirus has made the past year very difficult. The loss transform epidemiology, finance and insurance, risk of loved ones and the economic, -
The T2K Experiment Daniel I
The T2K Experiment Daniel I. Scully University of Warwick, Department of Physics, Coventry. UK Abstract. T2K is a long-baseline neutrino oscillation experiment built to make precision measurements of q13, q23 and 2 Dm 32. It achieves this by utilising an off-axis, predominantly nm , neutrino beam from J-PARC to Super-Kamiokande, and a near detector complex which constrains the beam’s direction, flux, composition and energy. To date T2K has published nm -disappearance and ne-appearance results, the latter excluding q13 = 0 at over 3s and therefore constituting first evidence for ne-appearance in a nm beam. In addition to oscillation physics, the on-axis (INGRID) and off-axis (ND280) near detectors provide the capability for a broad neutrino-nucleus interaction physics programme at neutrino energies below 1GeV. Keywords: T2K, ND280, neutrino, oscillations, cross sections PACS: 14.60.Lm, 13.15.+g T2K OVERVIEW The T2K experiment [1], based in Japan, is a long-baseline neutrino oscillation experiment built to make precision 2 measurements of q13, q23 and Dm 32. The first stage of the experiment is a neutrino beam generated at the J-PARC proton accelerator facility. 30 GeV protons are collided with a graphite target and three magnetic horns focus the resulting positive pions and kaons down a 110m decay tunnel. These decay in flight to produce a beam of predominantly nm , though some n m (≈ 6%), ne (≈ 1%) and ne (< 1%) are also produced (Figure 1a)[2]. (a) The contribution of each neutrino flavour to the flux through (b) The effect on the neutrino energy spectrum of moving off the ND280. -
Breakthrough Prize in Mathematics Awarded to Terry Tao
156 Breakthrough Prize in Mathematics awarded to Terry Tao Our congratulations to Australian Mathematician Terry Tao, one of five inaugu- ral winners of the Breakthrough Prizes in Mathematics, announced on 23 June. Terry is based at the University of California, Los Angeles, and has been awarded the prize for numerous breakthrough contributions to harmonic analysis, combi- natorics, partial differential equations and analytic number theory. The Breakthrough Prize in Mathematics was launched by Mark Zuckerberg and Yuri Milner at the Breakthrough Prize ceremony in December 2013. The other winners are Simon Donaldson, Maxim Kontsevich, Jacob Lurie and Richard Tay- lor. All five recipients of the Prize have agreed to serve on the Selection Committee, responsible for choosing subsequent winners from a pool of candidates nominated in an online process which is open to the public. From 2015 onwards, one Break- through Prize in Mathematics will be awarded every year. The Breakthrough Prizes honor important, primarily recent, achievements in the categories of Fundamental Physics, Life Sciences and Mathematics. The prizes were founded by Sergey Brin and Anne Wojcicki, Mark Zuckerberg and Priscilla Chan, and Yuri and Julia Milner, and aim to celebrate scientists and generate excitement about the pursuit of science as a career. Laureates will receive their trophies and $3 million each in prize money at a televised award ceremony in November, designed to celebrate their achievements and inspire the next genera- tion of scientists. As part of the ceremony schedule, they also engage in a program of lectures and discussions. See https://breakthroughprize.org and http://www.nytimes.com/2014/06/23/us/ the-multimillion-dollar-minds-of-5-mathematical-masters.html? r=1 for further in- formation.. -
Final Report for Studies in Elementary Particle Physics for the Period February 1, 2010 to April 30, 2013 Virginia Tech Tasks A, B, and N
Final Report for Studies in Elementary Particle Physics for the period February 1, 2010 to April 30, 2013 Virginia Tech Tasks A, B, and N Leo Piilonen Tatsu Takeuchi Djordje Minic Jonathan Link Center for Neutrino Physics, Department of Physics Virginia Polytechnic Institute and State University Blacksburg VA 24061-0435 Principal Investigator: Leo Piilonen Center for Neutrino Physics, Department of Physics 125 Robeson Hall Virginia Tech Blacksburg VA 24061-0435 (540)231-7472 [email protected] Office of High Energy Physics DOE/Science Program Office Technical Contact: Dr. Alan Stone DOE Grant Number: DE-FG05-92ER40709 1 Overview of the Virginia Tech HEP Program and Group This final report of DOE Grant DE-FG05-92ER40709 awarded to the Virginia Tech HEP group covers the period February 1, 2010 through April 30, 2013. The HEP program at Virginia Tech supported by this grant is organized into three tasks: A for theory (Profs. Tatsu Takeuchi and Djordje Minic), B for heavy flavor physics with the Belle and Belle II experiments (Prof. Leo Piilonen), and N for neutrino physics (Profs. Jonathan Link and Piilonen). There are several other HEP faculty members at Virginia Tech who were not supported by this grant through April 30, 2012 with whom we collaborated. Prof. Patrick Huber works in neutrino phenomenology and is supported by a separate ECRA grant from DOE. Prof. Eric Sharpe col- laborates with Minic and Takeuchi and is supported by the NSF. Prof. Camillo Mariani joined Virginia Tech in August 2012 as our newest neutrino experimentalist. Prof. Bruce Vogelaar is another neutrino experimentalist supported by the NSF; he collaborated with the late Prof. -
Astronomers Win Big in Science Mega-Awards US$36 Million in Breakthrough Prizes Awarded to Researchers in Physics, Life Sciences and Mathematics
NATURE | NEWS Astronomers win big in science mega-awards US$36 million in Breakthrough prizes awarded to researchers in physics, life sciences and mathematics. Mark Zastrow 10 November 2014 Steve Jennings/Getty Astrophysicists Brian Schmidt, Adam Riess and Saul Perlmutter accept their US$3-million Breakthrough Prizes in Physics on 9 November. The astronomers who discovered dark energy and the developers of the gene-editing technique known as CRISPR have won Breakthrough prizes. At US$3 million per winner, the awards are science’s most lucrative prize. Winners were announced on 9 November at a gala in the iconic Hangar One at NASA’s Ames Research Center in Mountain View, California. The first Breakthrough prizes were given in 2012 as a series of physics awards given by Russian Internet entrepreneur Yuri Milner. He soon recruited other online magnates, including Mark Zuckerberg of Facebook, Sergey Brin of Google and Jack Ma of Alibaba Group, to fund awards in life sciences and mathematics. The prizes, which attempt to elevate scientists to pop-culture heroes, have drawn both praise and criticism from the research community. This year’s Breakthrough Prize in Fundamental Physics was given to two teams of astrophysicists who raced to find exploding white dwarfs in distant galaxies. One group was led by Saul Perlmutter of the University of California (UC) in Berkeley, and the other by Adam Riess of Johns Hopkins University in Baltimore, Maryland, and Brian Schmidt of the Australian National University in Weston Creek. Their work led to the discovery, in 1998, that the expansion of the Universe was speeding up, leaving cosmologists struggling to explain the apparent ‘dark energy’ that is driving the phenomenon. -
Research in Physics 2008-2013
Research in Physics 2008-2013 Theoretical Physics .................................................................................................................................. 1 Condensed Matter, Materials and Soft Matter Physics ....................................................................... 38 Nanoscale Physics Cluster ........................................................................................................... 38 Magnetic Resonance Cluster ...................................................................................................... 96 Materials Physics Cluster .......................................................................................................... 121 Astronomy and Astrophysics (A&A) .................................................................................................... 172 Elementary Particle Physics (EPP) ....................................................................................................... 204 Centre for Fusion Space and Astrophysics (CFSA) .............................................................................. 247 Theoretical Physics Theoretical Physics 10 Staff; 10 PDRAs; 22 PhDs; 219 articles; 2472 citations; £2.9 M grant awards; £1.1 M in-kind; 20 PhDs awarded The main themes of research in Theoretical Physics are: Molecular & Materials Modelling; Complexity & Biological Physics; Quantum Condensed Matter. The Theory Group has a breadth of expertise in materials modelling, esp. in molecular dynamics and electronic structure calculations.