US Particle Physics: Scientific Opportunities a Strategic Plan for the Next Ten Years
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Μ → Eγ and Matching at Mw
Eur. Phys. J. C (2016) 76:370 DOI 10.1140/epjc/s10052-016-4207-5 Regular Article - Theoretical Physics μ → eγ and matching at mW Sacha Davidson1,2,3,a 1 IPNL, CNRS/IN2P3, 4 rue E. Fermi, 69622 Villeurbanne Cedex, France 2 Université Lyon 1, Villeurbanne, France 3 Université de Lyon, 69622 Lyon, France Received: 18 March 2016 / Accepted: 14 June 2016 / Published online: 4 July 2016 © The Author(s) 2016. This article is published with open access at Springerlink.com Abstract Several experiments search for μ ↔ e flavour attempt to reconstruct the fundamental Lagrangian of New change, for instance in μ → e conversion, μ → eγ and Physics from the operator coefficients. This is probably not μ → eee¯ . This paper studies how to translate these experi- feasible, but could give interesting perspectives. A first step mental constraints from low energy to a New Physics scale in this “bottom-up” approach, explored in this paper, is to M mW . A basis of QCD × QED-invariant operators (as use Effective Field Theory (EFT) [31] to translate the exper- appropriate below mW ) is reviewed, then run to mW with imental bounds to the coefficients of effective operators at one-loop Renormalisation Group Equations (RGEs) of QCD the New Physics scale M > mW . and QED. At mW , these operators are matched onto SU(2)- The goal would be to start from experimental constraints invariant dimension-six operators, which can continue to run on μ–e flavour change, and obtain at M the best bound up with electroweak RGEs. As an example, the μ → eγ on each coefficient from each observable. -
Planck Mass Rotons As Cold Dark Matter and Quintessence* F
Planck Mass Rotons as Cold Dark Matter and Quintessence* F. Winterberg Department of Physics, University of Nevada, Reno, USA Reprint requests to Prof. F. W.; Fax: (775) 784-1398 Z. Naturforsch. 57a, 202–204 (2002); received January 3, 2002 According to the Planck aether hypothesis, the vacuum of space is a superfluid made up of Planck mass particles, with the particles of the standard model explained as quasiparticle – excitations of this superfluid. Astrophysical data suggests that ≈70% of the vacuum energy, called quintessence, is a neg- ative pressure medium, with ≈26% cold dark matter and the remaining ≈4% baryonic matter and radi- ation. This division in parts is about the same as for rotons in superfluid helium, in terms of the Debye energy with a ≈70% energy gap and ≈25% kinetic energy. Having the structure of small vortices, the rotons act like a caviton fluid with a negative pressure. Replacing the Debye energy with the Planck en- ergy, it is conjectured that cold dark matter and quintessence are Planck mass rotons with an energy be- low the Planck energy. Key words: Analog Models of General Relativity. 1. Introduction The analogies between Yang Mills theories and vor- tex dynamics [3], and the analogies between general With greatly improved observational techniques a relativity and condensed matter physics [4 –10] sug- number of important facts about the physical content gest that string theory should perhaps be replaced by and large scale structure of our universe have emerged. some kind of vortex dynamics at the Planck scale. The They are: successful replacement of the bosonic string theory in 1. -
1 Standard Model: Successes and Problems
Searching for new particles at the Large Hadron Collider James Hirschauer (Fermi National Accelerator Laboratory) Sambamurti Memorial Lecture : August 7, 2017 Our current theory of the most fundamental laws of physics, known as the standard model (SM), works very well to explain many aspects of nature. Most recently, the Higgs boson, predicted to exist in the late 1960s, was discovered by the CMS and ATLAS collaborations at the Large Hadron Collider at CERN in 2012 [1] marking the first observation of the full spectrum of predicted SM particles. Despite the great success of this theory, there are several aspects of nature for which the SM description is completely lacking or unsatisfactory, including the identity of the astronomically observed dark matter and the mass of newly discovered Higgs boson. These and other apparent limitations of the SM motivate the search for new phenomena beyond the SM either directly at the LHC or indirectly with lower energy, high precision experiments. In these proceedings, the successes and some of the shortcomings of the SM are described, followed by a description of the methods and status of the search for new phenomena at the LHC, with some focus on supersymmetry (SUSY) [2], a specific theory of physics beyond the standard model (BSM). 1 Standard model: successes and problems The standard model of particle physics describes the interactions of fundamental matter particles (quarks and leptons) via the fundamental forces (mediated by the force carrying particles: the photon, gluon, and weak bosons). The Higgs boson, also a fundamental SM particle, plays a central role in the mechanism that determines the masses of the photon and weak bosons, as well as the rest of the standard model particles. -
Study of Anisotropic Compact Stars with Quintessence Field And
Eur. Phys. J. C (2019) 79:919 https://doi.org/10.1140/epjc/s10052-019-7427-7 Regular Article - Theoretical Physics Study of anisotropic compact stars with quintessence field and modified chaplygin gas in f (T) gravity Pameli Sahaa, Ujjal Debnathb Department of Mathematics, Indian Institute of Engineering Science and Technology, Shibpur, Howrah 711 103, India Received: 18 May 2019 / Accepted: 25 October 2019 / Published online: 12 November 2019 © The Author(s) 2019 Abstract In this work, we get an idea of the existence of 1 Introduction compact stars in the background of f (T ) modified grav- ity where T is a scalar torsion. We acquire the equations Recently, compact stars, the most elemental objects of the of motion using anisotropic property within the spherically galaxies, acquire much attention to the researchers to study compact star with electromagnetic field, quintessence field their ages, structures and evolutions in cosmology as well as and modified Chaplygin gas in the framework of modi- astrophysics. After the stellar death, the residue portion is fied f (T ) gravity. Then by matching condition, we derive formed as compact stars which can be classified into white the unknown constants of our model to obtain many phys- dwarfs, neutron stars, strange stars and black holes. Com- ical quantities to give a sketch of its nature and also study pact star is very densed object i.e., posses massive mass and anisotropic behavior, energy conditions and stability. Finally, smaller radius as compared to the ordinary star. In astro- we estimate the numerical values of mass, surface redshift physics, the study of neutron star and the strange star moti- etc from our model to compare with the observational data vates the researchers to explore their features and structures for different types of compact stars. -
7. Gamma and X-Ray Interactions in Matter
Photon interactions in matter Gamma- and X-Ray • Compton effect • Photoelectric effect Interactions in Matter • Pair production • Rayleigh (coherent) scattering Chapter 7 • Photonuclear interactions F.A. Attix, Introduction to Radiological Kinematics Physics and Radiation Dosimetry Interaction cross sections Energy-transfer cross sections Mass attenuation coefficients 1 2 Compton interaction A.H. Compton • Inelastic photon scattering by an electron • Arthur Holly Compton (September 10, 1892 – March 15, 1962) • Main assumption: the electron struck by the • Received Nobel prize in physics 1927 for incoming photon is unbound and stationary his discovery of the Compton effect – The largest contribution from binding is under • Was a key figure in the Manhattan Project, condition of high Z, low energy and creation of first nuclear reactor, which went critical in December 1942 – Under these conditions photoelectric effect is dominant Born and buried in • Consider two aspects: kinematics and cross Wooster, OH http://en.wikipedia.org/wiki/Arthur_Compton sections http://www.findagrave.com/cgi-bin/fg.cgi?page=gr&GRid=22551 3 4 Compton interaction: Kinematics Compton interaction: Kinematics • An earlier theory of -ray scattering by Thomson, based on observations only at low energies, predicted that the scattered photon should always have the same energy as the incident one, regardless of h or • The failure of the Thomson theory to describe high-energy photon scattering necessitated the • Inelastic collision • After the collision the electron departs -
Fabiola Gianotti
Fabiola Gianotti Date of Birth 29 October 1960 Place Rome, Italy Nomination 18 August 2020 Field Physics Title Director-General of the European Laboratory for Particle Physics, CERN, Geneva Most important awards, prizes and academies Honorary Professor, University of Edinburgh; Corresponding or foreign associate member of the Italian Academy of Sciences (Lincei), the National Academy of Sciences of the United States, the French Academy of Sciences, the Royal Society London, the Royal Academy of Sciences and Arts of Barcelona, the Royal Irish Academy and the Russian Academy of Sciences. Honorary doctoral degrees from: University of Uppsala (2012); Ecole Polytechnique Federale de Lausanne (2013); McGill University, Montreal (2014); University of Oslo (2014); University of Edinburgh (2015); University of Roma Tor Vergata (2017); University of Chicago (2018); University Federico II, Naples (2018); Université de Paris Sud, Orsay (2018); Université Savoie Mont Blanc, Annecy (2018); Weizmann Institute, Israel (2018); Imperial College, London (2019). National honours: Cavaliere di Gran Croce dell'Ordine al Merito della Repubblica, awarded by the Italian President Giorgio Napolitano (2014). Special Breakthrough Prize in Fundamental Physics (shared, 2013); Enrico Fermi Prize of the Italian Physical Society (shared, 2013); Medal of Honour of the Niels Bohr Institute, Copenhagen (2013); Wilhelm Exner Medal, Vienna (2017); Tate Medal of the American Institute of Physics for International Leadership (2019). Summary of scientific research Fabiola Gianotti is a particle physicist working at high-energy accelerators. In her scientific career, she has made significant contributions to several experiments at CERN, including UA2 at the proton-antiproton collider (SpbarpS), ALEPH at the Large Electron-Positron collider (LEP) and ATLAS at the Large Hadron Collider (LHC). -
Calorimetry for Particle Physics
REVIEWS OF MODERN PHYSICS, VOLUME 75, OCTOBER 2003 Calorimetry for particle physics Christian W. Fabjan and Fabiola Gianotti CERN, 1211 Geneva 23, Switzerland (Published 15 October 2003) Calorimetry has become a well-understood, powerful, and versatile measurement method. Besides perfecting this technique to match increasingly demanding operation at high-energy particle accelerators, physicists are developing low-temperature calorimeters to extend detection down to ever lower energies, and atmospheric and deep-sea calorimeters to scrutinize the universe up to the highest energies. The authors summarize the state of the art, with emphasis on the physics of the detectors and innovative technologies. CONTENTS VI. Citius, Altius, Fortius 1280 A. Introduction 1280 B. Atmospheric calorimeters 1280 I. Introduction 1243 1. Setting the energy scale 1283 II. Electromagnetic Calorimetry 1244 2. Energy resolution 1283 A. Physics of the electromagnetic cascade 1244 C. Deep-water calorimeters 1283 B. Energy resolution of electromagnetic VII. Conclusions 1284 calorimeters 1246 Acknowledgments 1284 1. Stochastic term 1247 References 1284 2. Noise term 1247 3. Constant term 1247 4. Additional contributions 1248 C. Main techniques and examples of facilities 1249 I. INTRODUCTION 1. Homogeneous calorimeters 1249 a. Semiconductor calorimeters 1249 Calorimetry is an ubiquitous detection principle in b. Cherenkov calorimeters 1250 particle physics. Originally invented for the study of c. Scintillation calorimeters 1251 cosmic-ray phenomena, this method was developed and d. Noble-liquid calorimeters 1254 perfected for accelerator-based particle physics experi- 2. Sampling calorimeters 1256 mentation primarily in order to measure the energy of a. Scintillation sampling calorimeters 1257 electrons, photons, and hadrons. Calorimeters are b. Gas sampling calorimeters 1257 blocks of instrumented material in which particles to be c. -
Glossary of Scientific Terms in the Mystery of Matter
GLOSSARY OF SCIENTIFIC TERMS IN THE MYSTERY OF MATTER Term Definition Section acid A substance that has a pH of less than 7 and that can react with 1 metals and other substances. air The mixture of oxygen, nitrogen, and other gasses that is consistently 1 present around us. alchemist A person who practices a form of chemistry from the Middle Ages 1 that was concerned with transforming various metals into gold. Alchemy A type of science and philosophy from the Middle Ages that 1 attempted to perform unusual experiments, taking something ordinary and turning it into something extraordinary. alkali metals Any of a group of soft metallic elements that form alkali solutions 3 when they combine with water. They include lithium, sodium, potassium, rubidium, cesium, and francium. alkaline earth Any of a group of metallic elements that includes beryllium, 3 metals magnesium, calcium, strontium, barium, and radium. alpha particle A positively charged particle, indistinguishable from a helium atom 5, 6 nucleus and consisting of two protons and two neutrons. alpha decay A type of radioactive decay in which a nucleus emits 6 an alpha particle. aplastic anemia A disorder of the bone marrow that results in too few blood cells. 4 apothecary The person in a pharmacy who distributes medicine. 1 atom The smallest component of an element that shares the chemical 1, 2, 3, 4, 5, 6 properties of the element and contains a nucleus with neutrons, protons, and electrons. atomic bomb A bomb whose explosive force comes from a chain reaction based on 6 nuclear fission. atomic number The number of protons in the nucleus of an atom. -
New Physics, Dark Matter and Cosmology in the Light of Large Hadron Collider Ahmad Tarhini
New physics, Dark matter and cosmology in the light of Large Hadron Collider Ahmad Tarhini To cite this version: Ahmad Tarhini. New physics, Dark matter and cosmology in the light of Large Hadron Collider. High Energy Physics - Theory [hep-th]. Université Claude Bernard - Lyon I, 2013. English. tel-00847781 HAL Id: tel-00847781 https://tel.archives-ouvertes.fr/tel-00847781 Submitted on 24 Jul 2013 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. No d’ordre 108-2013 LYCEN – T 2013-08 Thèse présentée devant l’Université Claude Bernard Lyon 1 École Doctorale de Physique et d’Astrophysique pour l’obtention du DIPLÔME de DOCTORAT Spécialité : Physique Théorique / Physique des Particules (arrêté du 7 août 2006) par Ahmad TARHINI Nouvelle physique, Matière noire et cosmologie à l’aurore du Large Hadron Collider Soutenue le 5 Juillet 2013 devant la Commission d’Examen Jury : M. D. Tsimpis Président du jury M. U. Ellwanger Rapporteur M. G. Moreau Rapporteur Mme F. Mahmoudi Examinatrice M. G. Moultaka Examinateur M. A.S. Cornell Examinateur M. A. Deandrea Directeur de thèse M. A. Arbey Co-Directeur de thèse ii Order N ◦: 108-2013 Year 2013 PHD THESIS of the UNIVERSITY of LYON Delivered by the UNIVERSITY CLAUDE BERNARD LYON 1 Subject: Theoretical Physics / Particles Physics submitted by Mr. -
Lab Tests of Dark Energy Robert Caldwell Dartmouth College Dark Energy Accelerates the Universe
Lab Tests of Dark Energy Robert Caldwell Dartmouth College Dark Energy Accelerates the Universe Collaboration with Mike Romalis (Princeton), Deanne Dorak & Leo Motta (Dartmouth) “Possible laboratory search for a quintessence field,” MR+RC, arxiv:1302.1579 Dark Energy vs. The Higgs Higgs: Let there be mass m(φ)=gφ a/a¨ > 0 Quintessence: Accelerate It! Dynamical Field Clustering of Galaxies in SDSS-III / BOSS: Cosmological Implications, Sanchez et al 2012 Dynamical Field Planck 2013 Cosmological Parameters XVI Dark Energy Cosmic Scalar Field 1 = (∂φ)2 V (φ)+ + L −2 − Lsm Lint V (φ)=µ4(1 + cos(φ/f)) Cosmic PNGBs, Frieman, Hill and Watkins, PRD 46, 1226 (1992) “Quintessence and the rest of the world,” Carroll, PRL 81, 3067 (1998) Dark Energy Couplings to the Standard Model 1 = (∂φ)2 V (φ)+ + L −2 − Lsm Lint φ µν Photon-Quintessence = F F Lint −4M µν φ = E" B" ! M · “dark” interaction: quintessence does not see EM radiation Dark Energy Coupling to Electromagnetism Varying φ creates an anomalous charge density or current 1 ! E! ρ/# = ! φ B! ∇ · − 0 −Mc∇ · ∂E! 1 ! B! µ " µ J! = (φ˙B! + ! φ E! ) ∇× − 0 0 ∂t − 0 Mc3 ∇ × Magnetized bodies create an anomalous electric field Charged bodies create an anomalous magnetic field EM waves see novel permittivity / permeability Dark Energy Coupling to Electromagnetism Cosmic Solution: φ˙/Mc2 H ∼ φ/Mc2 Hv/c2 ∇ ∼ 42 !H 10− GeV ∼ • source terms are very weak • must be clever to see effect Dark Energy Coupling to Electromagnetism Cosmic Birefringence: 2 ˙ ∂ 2 φ wave equation µ ! B# B# = # B# 0 0 ∂t2 −∇ Mc∇× ˙ -
On the Exotic Higgs Decays in Effective Field Theory
Eur. Phys. J. C (2016) 76:514 DOI 10.1140/epjc/s10052-016-4362-8 Regular Article - Theoretical Physics On the exotic Higgs decays in effective field theory Hermès Bélusca-Maïtoa, Adam Falkowskib Laboratoire de Physique Théorique, Université Paris-Sud, Bat. 210, 91405 Orsay, France Received: 22 April 2016 / Accepted: 9 September 2016 / Published online: 22 September 2016 © The Author(s) 2016. This article is published with open access at Springerlink.com Abstract We discuss exotic Higgs decays in an effec- in powers of 1/. The leading effects are expected from tive field theory where the Standard Model is extended by operators of dimension 6, as their coefficients are suppressed dimension-6 operators. We review and update the status of by 1/2. The first classification of dimension-6 operators two-body lepton- and quark-flavor-violating decays involv- was performed in Ref. [1]. For one generation of fermions, ing the Higgs boson. We also comment on the possibility of a complete non-redundant set (henceforth referred to as a observing three-body flavor-violating Higgs decays in this basis) was identified and explicitly written down in Ref. [2]. context. Reference [3] extended this to three generations of fermions, in which case a basis is characterized by 2499 independent parameters. Contents In this paper we are interested in the subset of these operators that lead to exotic decays of the 125 GeV Higgs 1 Introduction ..................... 1 boson. By “exotic” we mean decays that are forbidden in 2 Exotic Higgs couplings from dimension-6 Lagrangian 2 the SM or predicted to occur with an extremely suppressed 3 Two-body Higgs decays .............. -
Dark Energy Theory Overview
Dark Energy Theory Overview Ed Copeland -- Nottingham University 1. Issues with pure Lambda 2. Models of Dark Energy 3. Modified Gravity approaches 4. Testing for and parameterising Dark Energy Dark Side of the Universe - Bergen - July 26th 2016 1 M. Betoule et al.: Joint cosmological analysis of the SNLS and SDSS SNe Ia. 46 The Universe is sample σcoh low-z 0.12 HST accelerating and C 44 SDSS-II 0.11 β yet we still really SNLS 0.08 − have little idea 1 42 HST 0.11 X what is causing ↵ SNLS σ Table 9. Values of coh used in the cosmological fits. Those val- + 40 this acceleration. ues correspond to the weighted mean per survey of the values ) G ( SDSS shown in Figure 7, except for HST sample for which we use the 38 Is it a average value of all samples. They do not depend on a specific M − cosmological B choice of cosmological model (see the discussion in §5.5). ? 36 m constant, an Low-z = 34 evolving scalar µ 0.2 field, evidence of modifications of 0.4 . General CDM 0 2 ⇤ 0.0 0.15 µ Relativity on . − 0 2 − large scales or µ 0.4 − 2 1 0 something yet to 10− 10− 10 coh 0.1 z be dreamt up ? σ Betoule et al 2014 2 Fig. 8. Top: Hubble diagram of the combined sample. The dis- tance modulus redshift relation of the best-fit ⇤CDM cosmol- 0.05 1 1 ogy for a fixed H0 = 70 km s− Mpc− is shown as the black line.