Heavy-Quark Physics and Cp Violation

Total Page:16

File Type:pdf, Size:1020Kb

Heavy-Quark Physics and Cp Violation COURSE HEAVYQUARK PHYSICS AND CP VIOLATION Jerey D Richman University of California y Santa Barbara California USA y Email richmancharmphysicsucsbedu c Elsevier Science BV Al l rights reserved Photograph of Lecturer Contents Intro duction Roadmap and Overview of Bottom and Charm Physics Intro duction to the Cabibb oKobayashiMaskawa Matrix and a First Lo ok at CP Violation Exp erimental Challenges and Approaches in HeavyQuark Physics Historical Persp ective Bumps in the Road and Lessons in Data Analysis Avery short history of heavyquark physics Bumps in the road case studies Some rules for data analysis Leptonic Decays Intro duction to leptonic decays Measurements of leptonic decays Lattice calculations of leptonic decay constants Semileptonic Decays Intro duction to semileptonic decays Dynamics of semileptonic decay Heavy quark eective theory and semileptonic decays Inclusive semileptonic decay and jV j cb Leptonendp oint region in semileptonic B deca y and jV j ub Form factors and kinematic distributions for exclusive semileptonic decay HQET predictions and the IsgurWise function Exclusive semileptonic decay jV j and jV j cb ub Hadronic Decays Lifetimes and Rare Decays Hadronic Decays Lifetimes Rare decays CP Violation and Oscillations Intro duction to CP violation CP violation and cosmology CP violation in decay direct CP violation CP violation in mixing indirect CP violation Phenomenology of mixing CP violation due to interference b etween mixing and decay Acknowledgements App endix Remarks on Hadronic Currents Form Factors and Decay Constants App endix Remarks on CP Conjugate Amplitudes References Intro duction I am delighted to present these lectures on the physics of charm and b ottom hadrons to this enthusiastic group of graduate students and p ostdo cs here in Les Houches Whyisheavyquark physics interesting I hop e to show you that we can now address an extraordinarily broad range of issues ranging from the mysteries of the Cabibb oKobayashi Maskawa CKM quark mixing matrix to the dynamics of the strong and weak interactions to fascinating rare pro cesses that are sensitive to physics beyond the standard mo del In the near future several new and ongoing exp eriments will address the driving question of this eld what is the origin of CP violation So far CP violation has b een observed only as a tiny partinathousand eect in kaon decays There is as yet very little empirical evidence to establish that physics within the framework of the standard mo delnamely the phase structure of the CKM matrixis resp onsible If the CKM matrix is indeed the source then we will observe large CP violating asymmetries in b oth B and B meson decays If the exp ected pattern of CP violation is s not observed then these investigations will provide a windowinto new physics beyond the standard mo del I was more than a little surprised to discov er that nearly all of the memb ers of this audience are theorists This fact is b oth intriguing and a little daunting I have the opp ortunity to explain the challenges and excitement of building exp eriments and p erforming new measurements At the same time there is a risk that I will bore you with to o many exp erimental details or fail to motivate them suciently For some of you learning how measurements are p erformed may b e something like learning how your sausages are madeyou would rather not know I hop e that by the end of these lectures you will at least conclude that the sausages we make are kosher between theory and exp eriment in heavyquark The interaction physics has been extremely pro ductive and I will devote a signi cant part of these lectures to a review of theoretical progress from the perspective of an exp erimentalist I will discuss theory at a fairly simple level mainly to obtain insights into the key physical ideas and J D Richman to help explain the phenomenology that app ears in exp erimental mea surements For discussions of the more technical theoretical issues I refer you to the lectures of other sp eakers at this scho ol for example Buras Manohar Martinelli and Wise Exp erimentalists need to know ab out theory for several reasons First in planning an incisive and coherent set of measurements it helps greatly to understand the theoretical issues It is also imp ortant to have a sense of how reliable the predictions are and to know the key assumptions that are really being tested In p erforming a mea surement one m ust understand all of the kinematic distributions that describ e the pro cesses under study since both the detection eciency and the ability to reject backgrounds dep end on knowledge of such distributions Similarly theorists should have some knowledge of the strengths and weaknesses of dierent exp eriments as well as a sense of which kinds of measurements are practical and which are not It is also imp ortantfor theorists to b e aware of assumptions that exp erimentalists make and to understand the dep endence of the measurements on these assumptions A measured branching fraction for example may well dep end either on a mo del for the decay distributions for the signal or on a mo del de scribing the background comp osition For phenomenologists esp ecially it is imp ortant to b e able to communicate with exp erimentalists since predictions that are not clearly stated may simply b e ignored These lectures are unashamedly p edagogical so I will not aim for the level of impartiality that is customary in a review talk or article I hav e made some recent attempts at such reviews My own work in heavyquark physics has b een mainly on the CLEO exp eriment al though more recently I have b een involved in the construction of the BaBar detector Many of my examples are from CLEO analyses b oth b ecause I am most familiar with them and b ecause CLEO results are often as good as those from other exp eriments When other measure ments are b etter than those of CLEO however I will fo cus on them esp ecially to show the advantages of dierent metho ds My goal then is to present a balanced and coheren t picture of b oth exp eriment and theory The p edagogical approachgives me more free dom to be selective to sp end more time than usual on simple physics arguments and to present some of myown opinions ab out the strengths and weaknesses of various measurements In the pro cess I hop e b oth to giveyou a picture of howheavyavor physics is done and to convey my enthusiasm for this eld I am happy to say that these lectures are destined to become out HeavyQuark Physics and CP Violation ofdate in the relatively near future as exp eriments provide us with a vast amount of new data We can therefore exp ect ma jor advances in nearly all areas of bottom and charm quark physics and we need young p eople likeyou to help explore this new territory Roadmap and Overview of Bottom and Charm Physics The physics of b ottom and charm hadrons is a broad sub ject and it is useful to begin with a roadmap of the main topics and physics issues Here is an outline of the lectures Intro duction to the CKM matrix Exp erimental c hallenges of b and c physics Historical p ersp ective bumps in the road and lessons in data anal ysis Leptonic decays of pseudoscalar mesons Semileptonic decays and measurements of CKM elements Hadronic decays lifetimes and rare decays CP violation and oscillations All of the physical pro cesses that I discuss involve underlying weak pro cesses mediated by the W b oson but strong and even electromag netic interactions play a crucial role as well The thread that runs through these lectures ties all of these sub jects to the quest to under stand CP violation Although this list is rather long it is far from complete For exam ple I will say very little ab out baryons apart from lifetime measure ments or ab out sp ectroscopy The physics of heavyquark pro duction including Z bb and other related electroweak phenomena such as the b forwardbackward asymmetry is entirely absent these topics could easily b e the sub ject of another series of lectures I b egin in Section with a short intro duction to the CKM matrix and a review of its present status Because m m the b quark must b t decay into quarks outside its own generation As a consequence even b c decay mo des are suppressed by jV j the dominant cb resulting in the long lifetimes of b hadrons of order ps In some exp eriments these long lifetimes have made distinguishing b hadrons from backgrounds much easier since separated decay vertices are ev ident if the b hadron is moving rapidly B decays provide various ern the strengths of b c ways to measure jV j and jV j which gov cb ub and b u transitions Furthermore the app earance of the t quark in virtual intermediate states of B and B mixing and p enguin decay s J D Richman pro cesses allows one to extract jV j and jV j We will also see that td ts phases of the CKM elements not just their magnitudes are exp eri mentally accessible and are asso ciated with CP violating asymmetries For reasons that I will discuss the determination of CKM elements is less imp ortant in charm physics Although jV j and jV j can be de cs cd termined from charm semileptonic decays the main fo cus has been to infer these quantities from unitarity of the CKM matrix and then to use measured branching fractions to test theoretical predictions for the absolute scale of the decay rates Section describ es the main challenges confronting exp eriments that study b ottom and charmquark physics I compare the strengths and weaknesses
Recommended publications
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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
    [Show full text]
  • 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.
    [Show full text]
  • 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
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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
    [Show full text]
  • 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,
    [Show full text]