A Route Towards Ghost Imaging with Inelastically Scattered Electrons
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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. -
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. -
Multi-Wavelength Compressive Computational Ghost Imaging
Multi-wavelength compressive computational ghost imaging Stephen S. Welsha , Matthew P. Edgara, Phillip Jonathanb , Baoqing Suna , Miles. J. Padgetta aUniversity of Glasgow, Kelvin Building University Avenue G12 8QQ, Glasgow, UK; bDepartment of Mathematics and Statistics, Lancaster University, Lancaster, LA1 4YF, UK; ABSTRACT The field of ghost imaging encompasses systems which can retrieve the spatial information of an object through correlated measurements of a projected light field, having spatial resolution, and the associated reflected or trans- mitted light intensity measured by a photodetector. By employing a digital light projector in a computational ghost imaging system with multiple spectrally filtered photodetectors we obtain high-quality multi-wavelength reconstructions of real macroscopic objects. We compare different reconstruction algorithms and reveal the use of compressive sensing techniques for achieving sub-Nyquist performance. Furthermore, we demonstrate the use of this technology in non-visible and fluorescence imaging applications. Keywords: Ghost Imaging, Single Pixel Detectors, DLP Technologies, Multi-wavelength Imaging, Non-visible Imaging, Fluorescence Imaging 1. INTRODUCTION Ghost imaging (GI) has been an active research area for nearly two decades. First demonstrated utilizing spatially entangled photons,1 it was later shown possible using classical correlations of pseudo-thermal light sources.2{5 Early demonstrations of so called `classical GI' used a laser beam propagated through a ground glass diffuser in order to produce a pseudo-thermal speckle field. A beam splitter was used to produce two identical copies of the field which were subsequently propagated along two different paths: the test path and the reference path. The test path contained a partially transmissive or reflective object (typically planar) and a single-pixel photodetector (SPD) with no spatial resolution, whereas the reference path contained a detector with spatial resolution, typically a charged coupled device (CCD). -
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. -
Lensless Imaging with Compressive Ultrafast Sensing Guy Satat, Matthew Tancik and Ramesh Raskar
1 Lensless Imaging with Compressive Ultrafast Sensing Guy Satat, Matthew Tancik and Ramesh Raskar Abstract—Lensless imaging is an important and challenging time: the physics-based approach is done in one shot (i.e. all problem. One notable solution to lensless imaging is a single the sensing is done in parallel). The single pixel camera and pixel camera which benefits from ideas central to compressive its variants require hundreds of consecutive acquisitions, which sampling. However, traditional single pixel cameras require many illumination patterns which result in a long acquisition process. translates into a substantially longer overall acquisition time. Here we present a method for lensless imaging based on compres- Recently, time-resolved sensors enabled new imaging ca- sive ultrafast sensing. Each sensor acquisition is encoded with a pabilities. Here we consider a time-resolved system with different illumination pattern and produces a time series where pulsed active illumination combined with a sensor with a time is a function of the photon’s origin in the scene. Currently time resolution on the order of picoseconds. Picosecond time available hardware with picosecond time resolution enables time tagging photons as they arrive to an omnidirectional sensor. resolution allows distinguishing between photons that arrive This allows lensless imaging with significantly fewer patterns from different parts of the target with mm resolution. The compared to regular single pixel imaging. To that end, we develop sensor provides more information per acquisition (compared a framework for designing lensless imaging systems that use to regular pixel), and so fewer masks are needed. Moreover, the ultrafast detectors. We provide an algorithm for ideal sensor time-resolved sensor is characterized by a measurement matrix placement and an algorithm for optimized active illumination patterns. -
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. -
Fast First-Photon Ghost Imaging
www.nature.com/scientificreports OPEN Fast frst-photon ghost imaging Xialin Liu, Jianhong Shi, Xiaoyan Wu & Guihua Zeng Conventional imaging at low light levels requires hundreds of detected photons per pixel to suppress the Poisson noise for accurate refectivity inference. We propose a high-efciency photon-limited imaging technique, called fast frst-photon ghost imaging, which recovers the image by conditional Received: 11 December 2017 averaging of the reference patterns selected by the frst-photon detection signal. Our technique merges the physics of low-fux measurements with the framework of computational ghost imaging. Accepted: 9 March 2018 Experimental results demonstrate that it can reconstruct an image from less than 0.1 detected photon Published: xx xx xxxx per pixel, which is three orders of magnitude less than conventional imaging techniques. A signal- to-noise ratio model of the system is established for noise analysis. With less data manipulation and shorter time requirements, our technique has potential applications in many felds, ranging from biological microscopy to remote sensing. Photon-limited imaging has attracted great interest on account of its important applications under extreme envi- ronments, such as night vision1, biological imaging2, remote sensing3, and so forth, when of-the-shelf methods fail due to photon-limited data. Conventionally, the transverse spatial image is recovered by either a spatially resolving detector array with foodlight illumination or a single detector with raster-scanned point-by-point illumination. In this way, even with time-resolved single-photon detectors, hundreds of photons per pixel are necessary to suppress the Poisson noise that is inherent in photon counting to obtain accurate intensity values. -
Three-Point Vertex Functions in Yang-Mills Theory and QCD in Landau Gauge
EPJ Web of Conferences 137, 03001 (2017) DOI: 10.1051/ epjconf/201713703001 XIIth Quark Confinement & the Hadron Spectrum Three-point vertex functions in Yang-Mills Theory and QCD in Landau gauge Adrian L. Blum1;a, Reinhard Alkofer1;b, Markus Q. Huber1;c, and Andreas Windisch2;d 1Institute of Physics, University of Graz, NAWI Graz, Universitätsplatz 5, 8010 Graz, Austria 2Department of Physics, Washington University, St. Louis, MO, 63130, USA Abstract. Solutions for the three-gluon and quark-gluon vertices from Dyson-Schwinger equations and the three-particle irreducible formalism are discussed. Dynamical quarks (“unquenching”) change the three-gluon vertex via the quark-triangle diagrams which themselves include fully dressed quark-gluon vertex functions. On the other hand, the quark-swordfish diagram is, at least with the model used for the two-quark-two-gluon vertex employed here, of minor importance. For the leading tensor structure of the three- gluon vertex the “unquenching” effect can be summarized for the nonperturbative part as a shift of the related dressing function towards the infrared. 1 Introduction All the information about a quantum field theory is contained in its n-point functions. E.g., once the n-point functions of quantum chromodynamics (QCD) are computed, they can be used in a next step to calculate hadron properties. On the level of three-point functions, especially the three-gluon and quark-gluon vertices are of interest and they have thus been the objectives of many non-perturbative studies in recent years. For instance, in the Landau gauge they have been studied using lattice [1–9] and continuum methods [10–37].