Low Energy Tests of the Standard Model
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The Lamb Shift Experiment in Muonic Hydrogen
The Lamb Shift Experiment in Muonic Hydrogen Dissertation submitted to the Physics Faculty of the Ludwig{Maximilians{University Munich by Aldo Sady Antognini from Bellinzona, Switzerland Munich, November 2005 1st Referee : Prof. Dr. Theodor W. H¨ansch 2nd Referee : Prof. Dr. Dietrich Habs Date of the Oral Examination : December 21, 2005 Even if I don't think, I am. Itsuo Tsuda Je suis ou` je ne pense pas, je pense ou` je ne suis pas. Jacques Lacan A mia mamma e mio papa` con tanto amore Abstract The subject of this thesis is the muonic hydrogen (µ−p) Lamb shift experiment being performed at the Paul Scherrer Institute, Switzerland. Its goal is to measure the 2S 2P − energy difference in µp atoms by laser spectroscopy and to deduce the proton root{mean{ −3 square (rms) charge radius rp with 10 precision, an order of magnitude better than presently known. This would make it possible to test bound{state quantum electrody- namics (QED) in hydrogen at the relative accuracy level of 10−7, and will lead to an improvement in the determination of the Rydberg constant by more than a factor of seven. Moreover it will represent a benchmark for QCD theories. The experiment is based on the measurement of the energy difference between the F=1 F=2 2S1=2 and 2P3=2 levels in µp atoms to a precision of 30 ppm, using a pulsed laser tunable at wavelengths around 6 µm. Negative muons from a unique low{energy muon beam are −1 stopped at a rate of 70 s in 0.6 hPa of H2 gas. -
Baryon Resonances and Pentaquarks on the Lattice ✩
Nuclear Physics A 754 (2005) 248c–260c Baryon resonances and pentaquarks on the lattice ✩ F.X. Lee a,b,∗, C. Bennhold a a Center for Nuclear Studies, George Washington University, Washington, DC 20052, USA b Jefferson Lab, 12000 Jefferson Avenue, Newport News, VA 23606, USA Received 17 December 2004; accepted 22 December 2004 Available online 21 January 2005 Abstract We review recent progress in computing excited baryons and pentaquarks in lattice QCD. 2004 Elsevier B.V. All rights reserved. 1. QCD primer Quantum Chromodynamics (QCD) is widely accepted as the fundamental theory of the strong interaction. The QCD Lagrangian density can be written down simply in one line (in Euclidean space) 1 L = Tr F F µν +¯q γ µD + m q, (1) QCD 2 µν µ q where Fµν = ∂Aµ − ∂Aν + g[Aµ,Aν] is the gluon field strength tensor and Dµ = ∂µ + gAµ is the covariant derivative which provides the interaction between the gluon and quark terms. The action of QCD is the integral of the Lagrangian density over space– 4 time: SQCD = LQCD d x. QCD is a highly non-linear relativistic quantum field theory. It is well known that the theory has chiral symmetry in the mq = 0 limit and the symmetry is spontaneously broken in the vacuum. At high energies, it exhibits asymptotic freedom, ✩ Based on plenary talk by F.X. Lee at HYP2003, JLab. * Corresponding author. E-mail address: [email protected] (F.X. Lee). 0375-9474/$ – see front matter 2004 Elsevier B.V. All rights reserved. doi:10.1016/j.nuclphysa.2004.12.072 F.X. -
Casimir Effect Mechanism of Pairing Between Fermions in the Vicinity of A
Casimir effect mechanism of pairing between fermions in the vicinity of a magnetic quantum critical point Yaroslav A. Kharkov1 and Oleg P. Sushkov1 1School of Physics, University of New South Wales, Sydney 2052, Australia We consider two immobile spin 1/2 fermions in a two-dimensional magnetic system that is close to the O(3) magnetic quantum critical point (QCP) which separates magnetically ordered and disordered phases. Focusing on the disordered phase in the vicinity of the QCP, we demonstrate that the criticality results in a strong long range attraction between the fermions, with potential V (r) 1/rν , ν 0.75, where r is separation between the fermions. The mechanism of the enhanced∝ − attraction≈ is similar to Casimir effect and corresponds to multi-magnon exchange processes between the fermions. While we consider a model system, the problem is originally motivated by recent establishment of magnetic QCP in hole doped cuprates under the superconducting dome at doping of about 10%. We suggest the mechanism of magnetic critical enhancement of pairing in cuprates. PACS numbers: 74.40.Kb, 75.50.Ee, 74.20.Mn I. INTRODUCTION in the frame of normal Fermi liquid picture (large Fermi surface). Within this approach electrons interact via ex- change of an antiferromagnetic (AF) fluctuation (param- In the present paper we study interaction between 11 fermions mediated by magnetic fluctuations in a vicin- agnon). The lightly doped AF Mott insulator approach, ity of magnetic quantum critical point. To address this instead, necessarily implies small Fermi surface. In this case holes interact/pair via exchange of the Goldstone generic problem we consider a specific model of two holes 12 injected into the bilayer antiferromagnet. -
Ghost-Free Scalar-Fermion Interactions
PHYSICAL REVIEW D 98, 044043 (2018) Ghost-free scalar-fermion interactions † ‡ Rampei Kimura,1,2,* Yuki Sakakihara,3, and Masahide Yamaguchi2, 1Waseda Institute for Advanced Study, Waseda University, 1-6-1 Nishi-Waseda, Shinjuku, Tokyo 169-8050, Japan 2Department of Physics, Tokyo Institute of Technology, Tokyo 152-8551, Japan 3Department of Physics, Kwansei Gakuin University, Sanda, Hyogo 669-1337, Japan (Received 15 June 2018; published 28 August 2018) We discuss a covariant extension of interactions between scalar fields and fermions in a flat space-time. We show, in a covariant theory, how to evade fermionic ghosts appearing because of the extra degrees of freedom behind a fermionic nature even in the Lagrangian with first derivatives. We will give a concrete example of a quadratic theory with up to the first derivative of multiple scalar fields and a Weyl fermion. We examine not only the maximally degenerate condition, which makes the number of degrees of freedom correct, but also a supplementary condition guaranteeing that the time evolution takes place properly. We also show that proposed derivative interaction terms between scalar fields and a Weyl fermion cannot be removed by field redefinitions. DOI: 10.1103/PhysRevD.98.044043 I. INTRODUCTION scalar-tensor theories [4–6,13–20], vector-tensor theories [21–29], and form fields [30–32]. Construction of general theory without ghost degrees of On the other hand, generic theory with fermionic d.o.f. freedom (d.o.f.) has been discussed for a long time. has not yet been investigated well. If we could find such According to Ostrogradsky’s theorem, a ghost always appears in a higher (time) derivative theory as long as it fermionic theories which have not been explored, some is nondegenerate [1] (see also Ref. -
The Ghost Particle 1 Ask Students If They Can Think of Some Things They Cannot Directly See but They Know Exist
Original broadcast: February 21, 2006 BEFORE WATCHING The Ghost Particle 1 Ask students if they can think of some things they cannot directly see but they know exist. Have them provide examples and reasoning for PROGRAM OVERVIEW how they know these things exist. NOVA explores the 70–year struggle so (Some examples and evidence of their existence include: [bacteria and virus- far to understand the most elusive of all es—illnesses], [energy—heat from the elementary particles, the neutrino. sun], [magnetism—effect on a com- pass], and [gravity—objects falling The program: towards Earth].) How do scientists • relates how the neutrino first came to be theorized by physicist observe and measure things that cannot be seen with the naked eye? Wolfgang Pauli in 1930. (They use instruments such as • notes the challenge of studying a particle with no electric charge. microscopes and telescopes, and • describes the first experiment that confirmed the existence of the they look at how unseen things neutrino in 1956. affect other objects.) • recounts how scientists came to believe that neutrinos—which are 2 Review the structure of an atom, produced during radioactive decay—would also be involved in including protons, neutrons, and nuclear fusion, a process suspected as the fuel source for the sun. electrons. Ask students what they know about subatomic particles, • tells how theoretician John Bahcall and chemist Ray Davis began i.e., any of the various units of mat- studying neutrinos to better understand how stars shine—Bahcall ter below the size of an atom. To created the first mathematical model predicting the sun’s solar help students better understand the neutrino production and Davis designed an experiment to measure size of some subatomic particles, solar neutrinos. -
Arxiv:1908.02416V2 [Hep-Th] 21 Aug 2019
ACFI-T19-08 Unitarity, stability and loops of unstable ghosts John F. Donoghue∗ Department of Physics, University of Massachusetts Amherst, MA 01003, USA Gabriel Menezesy Department of Physics, University of Massachusetts Amherst, MA 01003, USA and Departamento de F´ısica, Universidade Federal Rural do Rio de Janeiro, 23897-000, Serop´edica, RJ, Brazil We present a new understanding of the unstable ghost-like resonance which appears in theories such as quadratic gravity and Lee-Wick type theories. Quantum corrections make this resonance unstable, such that it does not appear in the asymptotic spectrum. We prove that these theories are unitary to all orders. Unitarity is satisfied by the inclusion of only cuts from stable states in the unitarity sum. This removes the need to consider this as a ghost state in the unitarity sum. However, we often use a narrow-width approximation where we do include cuts through unstable states, and ignore cuts through the stable decay products. If we do this with the unstable ghost resonance at one loop, we get the correct answer only by using a contour which was originally defined by Lee and Wick. The quantum effects also provide damping in both the Feynman and the retarded propagators, leading to stability under perturbations. 1. INTRODUCTION Theories such as quadratic gravity [1{19] and Lee-Wick theories [20{28] have propagators which contain both quadratic and quartic momentum dependence. In addition to the pole at q2 = 0, this combination will produce a high mass pole, via 1 1 1 = − : (1) 2 q4 q2 q2 − µ2 q − µ2 The negative sign for the second term implies that this pole is ghost-like, i.e. -
QCD Lagrangian Gauge Invariance Colour Algebra Feynman Rules 2.Tree Level Amplitudes Application of Feynman Rules Polarisation Sums 3
QCD and precision calculations Lecture 1: basics Gudrun Heinrich Max Planck Institute for Physics, Munich [email protected] PREFIT School, March 2, 2020 1 Outline 1. Basics of QCD QCD Lagrangian Gauge invariance Colour algebra Feynman rules 2.Tree level amplitudes Application of Feynman rules Polarisation sums 3. NLO calculations (details see lectures 2-4) 4. Beyond NLO 2 Some literature 3 QCD QCD is a very rich field! asymptotic freedom confinement strong CP-problem QCD at finite temperature quark-gluon-plasma flavour puzzles spectroscopy lattice gauge theory disclaimer: I am not doing justice to it by just considering perturbative QCD, and even that only at fixed order However, as the focus will be on precision calculations, I will make a (highly biased) choice 4 Motivation • at hadron colliders, QCD is everywhere • without QCD corrections, (most of) the data are not well described , Grazzini, Kallweit, Rathlev ‘17 GH, Jahn, Jones, Kerner, Pires ‘17 5 QCD corrections perturbation theory in the strong coupling next-to-next-to-leading order leading order next-to-leading order NLO corrections typically NNLO corrections typically a few % but there are prominent exceptions (e.g. Higgs production, NLO corr. ~100%) Why can we do such an expansion at all? important concepts: • asymptotic freedom • factorisation 6 Factorisation parton distribution functions partonic cross power-suppressed non-perturbative (PDFs) section corrections factorisation scale (separate short- and long-distance dynamics) renormalisation scale (UV divergences from loops, -
How to Modify LAMMPS: from the Prospective of a Particle Method Researcher
chemengineering Article How to Modify LAMMPS: From the Prospective of a Particle Method Researcher Andrea Albano 1,* , Eve le Guillou 2, Antoine Danzé 2, Irene Moulitsas 2 , Iwan H. Sahputra 1,3, Amin Rahmat 1, Carlos Alberto Duque-Daza 1,4, Xiaocheng Shang 5 , Khai Ching Ng 6, Mostapha Ariane 7 and Alessio Alexiadis 1,* 1 School of Chemical Engineering, University of Birmingham, Birmingham B15 2TT, UK; [email protected] (I.H.S.); [email protected] (A.R.); [email protected] (C.A.D.-D.) 2 Centre for Computational Engineering Sciences, Cranfield University, Bedford MK43 0AL, UK; Eve.M.Le-Guillou@cranfield.ac.uk (E.l.G.); A.Danze@cranfield.ac.uk (A.D.); i.moulitsas@cranfield.ac.uk (I.M.) 3 Industrial Engineering Department, Petra Christian University, Surabaya 60236, Indonesia 4 Department of Mechanical and Mechatronic Engineering, Universidad Nacional de Colombia, Bogotá 111321, Colombia 5 School of Mathematics, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK; [email protected] 6 Department of Mechanical, Materials and Manufacturing Engineering, University of Nottingham Malaysia, Jalan Broga, Semenyih 43500, Malaysia; [email protected] 7 Department of Materials and Engineering, Sayens-University of Burgundy, 21000 Dijon, France; [email protected] * Correspondence: [email protected] or [email protected] (A.A.); [email protected] (A.A.) Citation: Albano, A.; le Guillou, E.; Danzé, A.; Moulitsas, I.; Sahputra, Abstract: LAMMPS is a powerful simulator originally developed for molecular dynamics that, today, I.H.; Rahmat, A.; Duque-Daza, C.A.; also accounts for other particle-based algorithms such as DEM, SPH, or Peridynamics. -
Exploring Hyperons and Hypernuclei with Lattice
UNH-03-01 LBNL-53972 NT@UW-03-031 Exploring Hyperons and Hypernuclei with Lattice QCD S.R. Beane,1, 2 P.F. Bedaque,3 A. Parre˜no,4 and M.J. Savage5 1Department of Physics, University of New Hampshire, Durham, NH 03824-3568. 2Jefferson Laboratory, 12000 Jefferson Avenue, Newport News, VA 23606. 3Lawrence-Berkeley Laboratory, Berkeley, CA 94720. 4Dept. ECM, Facultat de F´ısica, Universitat de Barcelona, E-08028, Barcelona, Spain. 5Department of Physics, University of Washington, Seattle, WA 98195-1560. Abstract In this work we outline a program for lattice QCD that would provide a first step toward under- standing the strong and weak interactions of strange baryons. The study of hypernuclear physics has provided a significant amount of information regarding the structure and weak decays of light nuclei containing one or two Λ’s, and Σ’s. From a theoretical standpoint, little is known about the hyperon-nucleon interaction, which is required input for systematic calculations of hypernuclear structure. Furthermore, the long-standing discrepancies in the P wave amplitudes for nonleptonic − hyperon decays remain to be understood, and their resolution is central to a better understanding of the weak decays of hypernuclei. We present a framework that utilizes L¨uscher’s finite-volume techniques in lattice QCD to extract the scattering length and effective range for ΛN scattering in both QCD and partially-quenched QCD. The effective theory describing the nonleptonic decays of hyperons using isospin symmetry alone, appropriate for lattice calculations, is constructed. arXiv:nucl-th/0311027v1 7 Nov 2003 1 I. INTRODUCTION Nuclear physics is a fascinating field that remains poorly understood at a fundamental level. -
Proton Polarisability Contribution to the Lamb Shift in Muonic Hydrogen
Proton polarisability contribution to the Lamb shift in muonic hydrogen Mike Birse University of Manchester Work done in collaboration with Judith McGovern Eur. Phys. J. A 48 (2012) 120 Mike Birse Proton polarisability contribution to the Lamb shift Mainz, June 2014 The Lamb shift in muonic hydrogen Much larger than in electronic hydrogen: DEL = E(2p1) − E(2s1) ' +0:2 eV 2 2 Dominated by vacuum polarisation Much more sensitive to proton structure, in particular, its charge radius th 2 DEL = 206:0668(25) − 5:2275(10)hrEi meV Results of many years of effort by Borie, Pachucki, Indelicato, Jentschura and others; collated in Antognini et al, Ann Phys 331 (2013) 127 Mike Birse Proton polarisability contribution to the Lamb shift Mainz, June 2014 The Lamb shift in muonic hydrogen Much larger than in electronic hydrogen: DEL = E(2p1) − E(2s1) ' +0:2 eV 2 2 Dominated by vacuum polarisation Much more sensitive to proton structure, in particular, its charge radius th 2 DEL = 206:0668(25) − 5:2275(10)hrEi meV Results of many years of effort by Borie, Pachucki, Indelicato, Jentschura and others; collated in Antognini et al, Ann Phys 331 (2013) 127 Includes contribution from two-photon exchange DE2g = 33:2 ± 2:0 µeV Sensitive to polarisabilities of proton by virtual photons Mike Birse Proton polarisability contribution to the Lamb shift Mainz, June 2014 Two-photon exchange Integral over T µn(n;q2) – doubly-virtual Compton amplitude for proton Spin-averaged, forward scattering ! two independent tensor structures Common choice: qµqn 1 p · q p · q -
Hyperon-Nucleon Force from Lattice
UTCCS-P-43, TKYNT-08-07, UTHEP-564 Hyperon-Nucleon Force from Lattice QCD a, ,1 b c,d e Hidekatsu Nemura ∗ , Noriyoshi Ishii , Sinya Aoki , and Tetsuo Hatsuda aAdvanced Meson Science Laboratory, Nishina Center for Accelerator-Based Science, RIKEN,Wako 351-0198, Japan bCenter for Computational Sciences, University of Tsukuba, Tsukuba 305-8571, Japan cGraduate School of Pure and Applied Sciences, University of Tsukuba, Tsukuba 305-8571, Japan dRiken BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973, USA eDepartment of Physics, The University of Tokyo, Tokyo 113-0033, Japan Abstract We calculate potentials between a proton and a Ξ0 (hyperon with strangeness −2) through the equal-time Bethe- Salpeter wave function, employing quenched lattice QCD simulations with the plaquette gauge action and the Wilson quark action on (4.5 fm)4 lattice at the lattice spacing a ≃ 0.14 fm. The ud quark mass in our study corresponds to 0 mπ ≃ 0.37 and 0.51 GeV, while the s quark mass corresponds to the physical value of mK . The central pΞ potential 1 3 has a strong (weak) repulsive core in the S0 ( S1) channel for r ∼< 0.6 fm, while the potential has attractive well at 0 medium and long distances (0.6 fm ∼< r ∼< 1.2 fm) in both channels. The sign of the pΞ scattering length and its quark mass dependence indicate a net attraction in both channels at low energies. Key words: Lattice QCD, Hyperon-nucleon interaction, Nuclear forces, Hypernuclei PACS: 12.38.Gc, 13.75.Ev, 21.30.-x, 21.80.+a 1. -
The Concept of the Photon—Revisited
The concept of the photon—revisited Ashok Muthukrishnan,1 Marlan O. Scully,1,2 and M. Suhail Zubairy1,3 1Institute for Quantum Studies and Department of Physics, Texas A&M University, College Station, TX 77843 2Departments of Chemistry and Aerospace and Mechanical Engineering, Princeton University, Princeton, NJ 08544 3Department of Electronics, Quaid-i-Azam University, Islamabad, Pakistan The photon concept is one of the most debated issues in the history of physical science. Some thirty years ago, we published an article in Physics Today entitled “The Concept of the Photon,”1 in which we described the “photon” as a classical electromagnetic field plus the fluctuations associated with the vacuum. However, subsequent developments required us to envision the photon as an intrinsically quantum mechanical entity, whose basic physics is much deeper than can be explained by the simple ‘classical wave plus vacuum fluctuations’ picture. These ideas and the extensions of our conceptual understanding are discussed in detail in our recent quantum optics book.2 In this article we revisit the photon concept based on examples from these sources and more. © 2003 Optical Society of America OCIS codes: 270.0270, 260.0260. he “photon” is a quintessentially twentieth-century con- on are vacuum fluctuations (as in our earlier article1), and as- Tcept, intimately tied to the birth of quantum mechanics pects of many-particle correlations (as in our recent book2). and quantum electrodynamics. However, the root of the idea Examples of the first are spontaneous emission, Lamb shift, may be said to be much older, as old as the historical debate and the scattering of atoms off the vacuum field at the en- on the nature of light itself – whether it is a wave or a particle trance to a micromaser.