Heavy-Quark Physics and Cp Violation
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The Btev Experiment: Physics and Detector
The BTeV Experiment: Physics and Detector FPCP 2003 K. Honscheid Ohio State University FPCP 2003 K. Honscheid Ohio State B Physics Today CKM Picture okay Vud Vus Vub VCKM = Vcd Vcs Vcb Vtd Vts Vtb CP Violation observed sin(2b) = 0.734 +/- 0.054 >1011 b hadrons No conflict with SM (including Bs) FPCP 2003 K. Honscheid Ohio State B Physics at Hadron Colliders Tevatron LHC Energy 2 TeV 14 TeV b cross section ~100 mb ~500 mb c cross section ~1000 mb ~3500 mb b fraction 2x10-3 6x10-3 Inst. Luminosity 2x1032 >2x1032 Bunch spacing 132 ns (396 ns) 25 ns Int./crossing <2> (<6>) <1> Luminous region 30 cm 5.3 cm Large cross sections Triggering is an issue All b-hadrons produced (B, Bs, Bc, b-baryons) FPCP 2003 K. Honscheid Ohio State Detector Requirements •Trigger, trigger, trigger •Vertex, decay distance •Momentum •PID FPCP 2003 K. Honscheid 0 Ohio State •Neutrals (g, p ) From F. Teubert Forward vs. Central Geometry Multi-purpose experiments require large solid angle coverage. Central Geometry (CDF, D0, Atlas, CMS) 100mb Dedicated B experiments can take 230mb advantage of Forward geometry (BTeV, LHCb) bg b production angle FPCP 2003 K. Honscheid b production angle Ohio State The BTeV Detector Beam Line FPCP 2003 K. Honscheid Ohio State Pixel Vertex Detector Reasons for Pixel Detector: • Superior signal to noise • Excellent spatial resolution -- 5-10 microns depending on angle, etc • Very Low occupancy • Very fast • Radiation hard Special features: • It is used directly in the L1 trigger • Pulse height is measured on every channel with a 3 bit FADC • It is inside a dipole and gives a crude standalone momentum Doublet FPCP 2003 K. -
Reconstruction of Semileptonic K0 Decays at Babar
Reconstruction of Semileptonic K0 Decays at BaBar Henry Hinnefeld 2010 NSF/REU Program Physics Department, University of Notre Dame Advisor: Dr. John LoSecco Abstract The oscillations observed in a pion composed of a superposition of energy states can provide a valuable tool with which to examine recoiling particles produced along with the pion in a two body decay. By characterizing these oscillation in the D+ ! π+ K0 decay we develop a technique that can be applied to other similar decays. The neutral kaons produced in the D+ ! π+ K0 decay are generated in flavor eigenstates due to their production via the weak force. Kaon flavor eigenstates differ from kaon mass eigenstates so the K0 can be equally represented as a superposition of mass 0 0 eigenstates, labelled KS and KL. Conservation of energy and momentum require that the recoiling π also be in an entangled superposition of energy states. The K0 flavor can be determined by 0 measuring the lepton charge in a KL ! π l ν decay. A central difficulty with this method is the 0 accurate reconstruction of KLs in experimental data without the missing information carried off by the (undetected) neutrino. Using data generated at the Stanford Linear Accelerator (SLAC) and software created as part of the BaBar experiment I developed a set of kinematic, geometric, 0 and statistical filters that extract lists of KL candidates from experimental data. The cuts were first developed by examining simulated Monte Carlo data, and were later refined by examining 0 + − 0 trends in data from the KL ! π π π decay. -
Minutes of the High Energy Physics Advisory Panel Meeting February 14-15, 2008 Palomar Hotel, Washington, D.C
Minutes of the High Energy Physics Advisory Panel Meeting February 14-15, 2008 Palomar Hotel, Washington, D.C. HEPAP members present: Jonathan A. Bagger, Vice Chair Lisa Randall Daniela Bortoletto Tor Raubenheimer James E. Brau Kate Scholberg Patricia Burchat Melvyn J. Shochet, Chair Robert N. Cahn Sally Seidel Priscilla Cushman (Thursday only) Henry Sobel Larry D. Gladney Maury Tigner Robert Kephart William Trischuk William R. Molzon Herman White Angela V. Olinto Guy Wormser (Thursday only) Saul Perlmutter HEPAP members absent: Hiroaki Aihara Joseph Lykken Alice Bean Stephen L. Olsen Sarah Eno Also participating: Charles Baltay, Department of Physics, Yale University Barry Barish, Director, Global Design Effort, International Linear Collider William Carithers, Physics Division, Lawrence Berkeley National Laboratory Tony Chan, Assistant Director for Mathematics and Physical Sciences, National Science Foundation Glen Crawford, Program Manager, Office of High Energy Physics, Office of Science, Department of Energy Joseph Dehmer, Director, Division of Physics, National Science Foundation Persis Drell, Director, Stanford Linear Accelerator Center Thomas Ferbel, Department of Physics and Astronomy, University of Rochester Marvin Goldberg, Program Director, Division of Physics, National Science Foundation Paul Grannis, Department of Physics and Astronomy, State University of New York Michael Harrison, Physics Department, Brookhaven National Laboratory Abolhassan Jawahery, BaBar Collaboration Spokesman, Stanford Linear Accelerator Center Steve -
Study of Exclusive Charmless Semileptonic Decays of the B Meson
SLAC-R-743 Study of Exclusive Charmless Semileptonic Decays of the B Meson Amanda Jacqueline Weinstein SLAC-Report-743 December 2004 Prepared for the Department of Energy under contract number DE-AC02-76SF00515 This document, and the material and data contained therein, was developed under sponsorship of the United States Government. Neither the United States nor the Department of Energy, nor the Leland Stanford Junior University, nor their employees, nor their respective contractors, subcontractors, or their employees, makes an warranty, express or implied, or assumes any liability of responsibility for accuracy, completeness or useful- ness of any information, apparatus, product or process disclosed, or represents that its use will not infringe privately owned rights. Mention of any product, its manufacturer, or suppliers shall not, nor is it intended to, imply approval, disapproval, or fitness of any particular use. A royalty-free, nonexclusive right to use and dis- seminate same for any purpose whatsoever, is expressly reserved to the United States and the University. STUDY OF EXCLUSIVE CHARMLESS SEMILEPTONIC DECAYS OF THE B MESON a dissertation submitted to the department of physics and the committee on graduate studies of stanford university in partial fulfillment of the requirements for the degree of doctor of philosophy Amanda Jacqueline Weinstein December 2004 c Copyright by Amanda Jacqueline Weinstein 2005 All Rights Reserved ii I certify that I have read this dissertation and that, in my opinion, it is fully adequate in scope and quality as a dissertation for the degree of Doctor of Philosophy. Jonathan Dorfan (Principal Adviser) I certify that I have read this dissertation and that, in my opinion, it is fully adequate in scope and quality as a dissertation for the degree of Doctor of Philosophy. -
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 -
ANTIMATTER a Review of Its Role in the Universe and Its Applications
A review of its role in the ANTIMATTER universe and its applications THE DISCOVERY OF NATURE’S SYMMETRIES ntimatter plays an intrinsic role in our Aunderstanding of the subatomic world THE UNIVERSE THROUGH THE LOOKING-GLASS C.D. Anderson, Anderson, Emilio VisualSegrè Archives C.D. The beginning of the 20th century or vice versa, it absorbed or emitted saw a cascade of brilliant insights into quanta of electromagnetic radiation the nature of matter and energy. The of definite energy, giving rise to a first was Max Planck’s realisation that characteristic spectrum of bright or energy (in the form of electromagnetic dark lines at specific wavelengths. radiation i.e. light) had discrete values The Austrian physicist, Erwin – it was quantised. The second was Schrödinger laid down a more precise that energy and mass were equivalent, mathematical formulation of this as described by Einstein’s special behaviour based on wave theory and theory of relativity and his iconic probability – quantum mechanics. The first image of a positron track found in cosmic rays equation, E = mc2, where c is the The Schrödinger wave equation could speed of light in a vacuum; the theory predict the spectrum of the simplest or positron; when an electron also predicted that objects behave atom, hydrogen, which consists of met a positron, they would annihilate somewhat differently when moving a single electron orbiting a positive according to Einstein’s equation, proton. However, the spectrum generating two gamma rays in the featured additional lines that were not process. The concept of antimatter explained. In 1928, the British physicist was born. -
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. -
Report on HEPAP Activities
Report on HEPAP activities Mel Shochet University of Chicago 6/4/09 Fermilab Users Meeting 1 What is HEPAP? High Energy Physics Advisory Panel • Advises the DOE & NSF on the particle physics program. • Federal Advisory Committee Act rules – Public meetings – US members are Special Government Employees on meeting days. • Subject to federal conflict-of-interest rules • “Special” ⇒ paycheck = $0.00 – Appointed by DOE Under-Secretary for Science & NSF Director – Reports to Assoc. Dir. for OHEP & Asst. Dir. Math & Phys. Sciences – Broad membership: subfield, univ & labs, demographics (geography,…) • Members don’t serve as representatives of constituencies; advise on the health of the entire field. • Foreign members provide information on programs in Europe & Asia 6/4/09 Fermilab Users Meeting 2 Current Membership • Hiroaki Aihara, Tokyo • Daniel Marlow, Princeton • Marina Artuso, Syracuse • Ann Nelson, Washington • Alice Bean, Kansas • Stephen Olsen, Hawaii • Patricia Burchat, Stanford • Lisa Randall, Harvard • Priscilla Cushman, Minn. • Kate Scholberg, Duke • Lance Dixon, SLAC • Sally Seidel, New Mexico • Sarah Eno, Maryland • Melvyn Shochet, Chicago • Graciela Gelmini, UCLA • Henry Sobel, Irvine • Larry Gladney, Penn • Paris Sphicas, CERN • Boris Kayser, FNAL (DPF) • Maury Tigner, Cornell • Robert Kephart, FNAL • William Trischuk, Toronto • Steve Kettell, BNL • Herman White, FNAL • Wim Leemans, LBNL 6/4/09 Fermilab Users Meeting 3 Meetings • 3 meetings per year • Agenda – reports from the funding agencies on budgets & their impact, recent events, successes and problems – reports from specialized subpanels that need HEPAP approval to become official government documents (ex. P5) – reports from other committees that impact HEP (ex. EPP2010) – informational reports on issues that might arise in the future (ex. -
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. -
Phenomenology of Gev-Scale Heavy Neutral Leptons Arxiv:1805.08567
Prepared for submission to JHEP INR-TH-2018-014 Phenomenology of GeV-scale Heavy Neutral Leptons Kyrylo Bondarenko,1 Alexey Boyarsky,1 Dmitry Gorbunov,2;3 Oleg Ruchayskiy4 1Intituut-Lorentz, Leiden University, Niels Bohrweg 2, 2333 CA Leiden, The Netherlands 2Institute for Nuclear Research of the Russian Academy of Sciences, Moscow 117312, Russia 3Moscow Institute of Physics and Technology, Dolgoprudny 141700, Russia 4Discovery Center, Niels Bohr Institute, Copenhagen University, Blegdamsvej 17, DK- 2100 Copenhagen, Denmark E-mail: [email protected], [email protected], [email protected], [email protected] Abstract: We review and revise phenomenology of the GeV-scale heavy neutral leptons (HNLs). We extend the previous analyses by including more channels of HNLs production and decay and provide with more refined treatment, including QCD corrections for the HNLs of masses (1) GeV. We summarize the relevance O of individual production and decay channels for different masses, resolving a few discrepancies in the literature. Our final results are directly suitable for sensitivity studies of particle physics experiments (ranging from proton beam-dump to the LHC) aiming at searches for heavy neutral leptons. arXiv:1805.08567v3 [hep-ph] 9 Nov 2018 ArXiv ePrint: 1805.08567 Contents 1 Introduction: heavy neutral leptons1 1.1 General introduction to heavy neutral leptons2 2 HNL production in proton fixed target experiments3 2.1 Production from hadrons3 2.1.1 Production from light unflavored and strange mesons5 2.1.2 -
Minutes High Energy Physics Advisory Panel October 22–23, 2009 Hilton Embassy Row Washington, D.C
Draft Minutes High Energy Physics Advisory Panel October 22–23, 2009 Hilton Embassy Row Washington, D.C. HEPAP members present: Hiroaki Aihara Wim Leemans Marina Artuso Daniel Marlow Alice Bean Ann Nelson Patricia Burchat Paris Sphicas Lance Dixon Kate Scholberg Graciela Gelmini Melvyn J. Shochet, Chair Larry Gladney Henry Sobel Boris Kayser Maury Tigner Robert Kephart William Trischuk Steven Kettell Herman White HEPAP members absent: Priscilla Cushman Lisa Randall Sarah Eno Sally Seidel Stephen Olson Also participating: Barry Barish, Director, Global Design Effort, International Linear Collider Frederick Bernthal, President, Universities Research Association Glen Crawford, HEPAP Designated Federal Officer, Office of High Energy Physics, Office of Science, Department of Energy Joseph Dehmer, Director, Division of Physics, National Science Foundation Cristinel Diaconu, Directeur de Recherche, IN2P3/CNRS, France Robert Diebold, Diebold Consulting Marvin Goldberg, Program Director, Division of Physics, National Science Foundation Judith Jackson, Director, Office of Communication, Fermi National Accelerator Laboratory Young-Kee Kim, Deputy Director, Fermi National Accelerator Laboratory John Kogut, HEPAP Executive Secretary, Office of High Energy Physics, Office of Science, Department of Energy Dennis Kovar, Associate Director, Office of High Energy Physics, Office of Science, Department of Energy Kevin Lesko, Nuclear Science Division, Lawrence Berkeley National Laboratory Marsha Marsden, Office of High Energy Physics, Office of Science,