Fundamental Interactions
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Searches for Electroweak Production of Supersymmetric Gauginos and Sleptons and R-Parity Violating and Long-Lived Signatures with the ATLAS Detector
Searches for electroweak production of supersymmetric gauginos and sleptons and R-parity violating and long-lived signatures with the ATLAS detector Ruo yu Shang University of Illinois at Urbana-Champaign (for the ATLAS collaboration) Supersymmetry (SUSY) • Standard model does not answer: What is dark matter? Why is the mass of Higgs not at Planck scale? • SUSY states the existence of the super partners whose spin differing by 1/2. • A solution to cancel the quantum corrections and restore the Higgs mass. • Also provides a potential candidate to dark matter with a stable WIMP! 2 Search for SUSY at LHC squark gluino 1. Gluino, stop, higgsino are the most important ones to the problem of Higgs mass. 2. Standard search for gluino/squark (top- right plots) usually includes • large jet multiplicity • missing energy ɆT carried away by lightest SUSY particle (LSP) • See next talk by Dr. Vakhtang TSISKARIDZE. 3. Dozens of analyses have extensively excluded gluino mass up to ~2 TeV. Still no sign of SUSY. 4. What are we missing? 3 This talk • Alternative searches to probe supersymmetry. 1. Search for electroweak SUSY 2. Search for R-parity violating SUSY. 3. Search for long-lived particles. 4 Search for electroweak SUSY Look for strong interaction 1. Perhaps gluino mass is beyond LHC energy scale. gluino ↓ 2. Let’s try to find gauginos! multi-jets 3. For electroweak productions we look for Look for electroweak interaction • leptons (e/μ/τ) from chargino/neutralino decay. EW gaugino • ɆT carried away by LSP. ↓ multi-leptons 5 https://cds.cern.ch/record/2267406 Neutralino/chargino via WZ decay 2� 3� 2� SR ɆT [GeV] • Models assume gauginos decay to W/Z + LSP. -
The Nobel Prize in Physics 1999
The Nobel Prize in Physics 1999 The last Nobel Prize of the Millenium in Physics has been awarded jointly to Professor Gerardus ’t Hooft of the University of Utrecht in Holland and his thesis advisor Professor Emeritus Martinus J.G. Veltman of Holland. According to the Academy’s citation, the Nobel Prize has been awarded for ’elucidating the quantum structure of electroweak interaction in Physics’. It further goes on to say that they have placed particle physics theory on a firmer mathematical foundation. In this short note, we will try to understand both these aspects of the award. The work for which they have been awarded the Nobel Prize was done in 1971. However, the precise predictions of properties of particles that were made possible as a result of their work, were tested to a very high degree of accuracy only in this last decade. To understand the full significance of this Nobel Prize, we will have to summarise briefly the developement of our current theoretical framework about the basic constituents of matter and the forces which hold them together. In fact the path can be partially traced in a chain of Nobel prizes starting from one in 1965 to S. Tomonaga, J. Schwinger and R. Feynman, to the one to S.L. Glashow, A. Salam and S. Weinberg in 1979, and then to C. Rubia and Simon van der Meer in 1984 ending with the current one. In the article on ‘Search for a final theory of matter’ in this issue, Prof. Ashoke Sen has described the ‘Standard Model (SM)’ of particle physics, wherein he has listed all the elementary particles according to the SM. -
Structure of Matter
STRUCTURE OF MATTER Discoveries and Mysteries Part 2 Rolf Landua CERN Particles Fields Electromagnetic Weak Strong 1895 - e Brownian Radio- 190 Photon motion activity 1 1905 0 Atom 191 Special relativity 0 Nucleus Quantum mechanics 192 p+ Wave / particle 0 Fermions / Bosons 193 Spin + n Fermi Beta- e Yukawa Antimatter Decay 0 π 194 μ - exchange 0 π 195 P, C, CP τ- QED violation p- 0 Particle zoo 196 νe W bosons Higgs 2 0 u d s EW unification νμ 197 GUT QCD c Colour 1975 0 τ- STANDARD MODEL SUSY 198 b ντ Superstrings g 0 W Z 199 3 generations 0 t 2000 ν mass 201 0 WEAK INTERACTION p n Electron (“Beta”) Z Z+1 Henri Becquerel (1900): Beta-radiation = electrons Two-body reaction? But electron energy/momentum is continuous: two-body two-body momentum energy W. Pauli (1930) postulate: - there is a third particle involved + + - neutral - very small or zero mass p n e 휈 - “Neutrino” (Fermi) FERMI THEORY (1934) p n Point-like interaction e 휈 Enrico Fermi W = Overlap of the four wave functions x Universal constant G -5 2 G ~ 10 / M p = “Fermi constant” FERMI: PREDICTION ABOUT NEUTRINO INTERACTIONS p n E = 1 MeV: σ = 10-43 cm2 휈 e (Range: 1020 cm ~ 100 l.yr) time Reines, Cowan (1956): Neutrino ‘beam’ from reactor Reactions prove existence of neutrinos and then ….. THE PREDICTION FAILED !! σ ‘Unitarity limit’ > 100 % probability E2 ~ 300 GeV GLASGOW REFORMULATES FERMI THEORY (1958) p n S. Glashow W(eak) boson Very short range interaction e 휈 If mass of W boson ~ 100 GeV : theory o.k. -
SHELDON LEE GLASHOW Lyman Laboratory of Physics Harvard University Cambridge, Mass., USA
TOWARDS A UNIFIED THEORY - THREADS IN A TAPESTRY Nobel Lecture, 8 December, 1979 by SHELDON LEE GLASHOW Lyman Laboratory of Physics Harvard University Cambridge, Mass., USA INTRODUCTION In 1956, when I began doing theoretical physics, the study of elementary particles was like a patchwork quilt. Electrodynamics, weak interactions, and strong interactions were clearly separate disciplines, separately taught and separately studied. There was no coherent theory that described them all. Developments such as the observation of parity violation, the successes of quantum electrodynamics, the discovery of hadron resonances and the appearance of strangeness were well-defined parts of the picture, but they could not be easily fitted together. Things have changed. Today we have what has been called a “standard theory” of elementary particle physics in which strong, weak, and electro- magnetic interactions all arise from a local symmetry principle. It is, in a sense, a complete and apparently correct theory, offering a qualitative description of all particle phenomena and precise quantitative predictions in many instances. There is no experimental data that contradicts the theory. In principle, if not yet in practice, all experimental data can be expressed in terms of a small number of “fundamental” masses and cou- pling constants. The theory we now have is an integral work of art: the patchwork quilt has become a tapestry. Tapestries are made by many artisans working together. The contribu- tions of separate workers cannot be discerned in the completed work, and the loose and false threads have been covered over. So it is in our picture of particle physics. Part of the picture is the unification of weak and electromagnetic interactions and the prediction of neutral currents, now being celebrated by the award of the Nobel Prize. -
Nobel Pris Og NBI
Hvilke forskere, både danske og udenlandske, med tilknytning til NBI har gennem tiden modtaget en nobelpris? M I Nobelpristagere med tilknytning til NBI Der er en lang række Nobelpristagere, som har været ansat i en eller anden form på NBI (Niels Bohr Institutet). Der er desuden en del, der har opholdt sig og arbejdet på institutet i en periode, men ikke har været ansat. De har så været lønnet af deres hjemmeuniversitet og brugt tiden til et samarbejde med en eller flere forskere på NBI, som oftest med en videnskabelig artikel som resultat. Endeligt har der i ”utallige” år været en skik, at fysik nobelpristagere blev inviteret til at komme til København, give en forelæsning, og efter eget ønske blive lidt tid umiddelbart efter modtagelsen af Nobelprisen (hvor de jo alligevel var i Stockholm). I den form har en meget stor del af nobelpristagerne efter institutets oprettelse, været på besøg.. Jeg husker selv fra et af mine første studieår en strålende forelæsning af: Donald Arthur Glaser f: 1926 i USA nobelpris i 1960, med en efterfølgende animeret fest med nobelpristageren i fysik- matematik- og kemi- studerendes forening (som hed parentesen). Der har især i Bohrs tid men været en lang række konferencer og møder, hvor stort set hele den videnskabelige verdens store, har været tilstede f.eks.: Max Karl Ernst Ludwig Planck f: D 1858 d: 1947 nobelpris 1916, Albert Einstein f: D 1879 d: 1955 nobelrpis 1921, Douglas D. Osheroff f: USA 1945 nobelpris 1996 og mange, mange andre. I den nedenstående liste er udvalgt de, der dokumenterbart har haft en eller anden form for regulær ansættelse på NBI. -
The Man Behind an Identity in Quantum Electrodynamics by F
The man behind an identity in quantum electrodynamics by F. J. Duarte Introduction The 6th of May, 2010, marks the 10th anniversary of the passing of John Clive Ward a quiet genius of physics whose ideas and contributions helped shape the post-war quantum era. Since John was an Australian citizen it is only appropriate to remember him in the pages of this journal. First, as a manner of introduction, I will outline John’s most salient contributions. Then, I will attempt a description of the physicists, teacher, and friend that I was privileged to know. Physics theoreticians thus producing a series of brilliant papers on: In an approximated chronological order the contributions of the Ising Model (Kac and Ward, 1952), quantum solid-state John Ward began with a paper published (with Maurice L. physics (Ward and Wilks, 1952), quantum statistics (Montroll H. Pryce) in Nature as part of his doctoral research at Oxford and Ward, 1958), and Fermion theory (Luttinger and Ward, (Pryce and Ward, 1947). This was a solution to a problem, 1960). His last paper was on the Dirac equation and higher that according to John was posed by Dirac, and that J. A. symmetries (Ward, 1978). Wheeler had tried to solve (Ward, 2004). The suggestion to tackle this problem was made by Pryce (a former student of In a piece written in an Oxford publication it was once stated R. H. Fowler and John’s supervisor). This had to do with that Ward “has contributed deeply to an astonishingly broad the decay of γ particles and the emission of two correlated range of theoretical physics: statistical mechanics, plasma photons in opposite directions. -
Some Aspects of the Theory of Heavy Ion Collisions
Some Aspects of the Theory of Heavy Ion Collisions Franc¸ois Gelis Institut de Physique Th´eorique CEA/Saclay, Universit´eParis-Saclay 91191, Gif sur Yvette, France June 16, 2021 Abstract We review the theoretical aspects relevant in the description of high energy heavy ion collisions, with an emphasis on the learnings about the underlying QCD phenomena that have emerged from these collisions. 1 Introduction to heavy ion collisions Elementary forces in Nature The interactions among the elementary constituents of matter are divided into four fundamental forces: gravitation, electromagnetism, weak nuclear forces and strong nuclear forces. All these interactions except gravity have a well tested a microscopic quantum description in terms of local gauge theories, in which the elementary matter fields are spin-1=2 fermions, interacting via the exchange of spin-1 bosons. In this framework, a special role is played by the Higgs spin-0 boson (the only fundamental scalar particle in the Standard Model), whose non-zero vacuum expectation value gives to all the other fields a mass proportional to their coupling to the Higgs. The discovery of the Higgs boson at the Large Hadron Collider in 2012 has so far confirmed all the Standard Model expectations. In this picture, gravity has remained a bit of an outlier: even though the classical field theory of gravitation (general relativity) has been verified experimentally with a high degree of precision (the latest of these verifications being the observation of gravitational waves emitted during the merger of massive compact objects - black holes or arXiv:2102.07604v3 [hep-ph] 15 Jun 2021 neutron stars), the quest for a theory of quantum gravity has been inconclusive until now (and possible experimental probes are far out of reach for the foreseeable future). -
Electro-Weak Interactions
Electro-weak interactions Marcello Fanti Physics Dept. | University of Milan M. Fanti (Physics Dep., UniMi) Fundamental Interactions 1 / 36 The ElectroWeak model M. Fanti (Physics Dep., UniMi) Fundamental Interactions 2 / 36 Electromagnetic vs weak interaction Electromagnetic interactions mediated by a photon, treat left/right fermions in the same way g M = [¯u (eγµ)u ] − µν [¯u (eγν)u ] 3 1 q2 4 2 1 − γ5 Weak charged interactions only apply to left-handed component: = L 2 Fermi theory (effective low-energy theory): GF µ 5 ν 5 M = p u¯3γ (1 − γ )u1 gµν u¯4γ (1 − γ )u2 2 Complete theory with a vector boson W mediator: g 1 − γ5 g g 1 − γ5 p µ µν p ν M = u¯3 γ u1 − 2 2 u¯4 γ u2 2 2 q − MW 2 2 2 g µ 5 ν 5 −−−! u¯3γ (1 − γ )u1 gµν u¯4γ (1 − γ )u2 2 2 low q 8 MW p 2 2 g −5 −2 ) GF = | and from weak decays GF = (1:1663787 ± 0:0000006) · 10 GeV 8 MW M. Fanti (Physics Dep., UniMi) Fundamental Interactions 3 / 36 Experimental facts e e Electromagnetic interactions γ Conserves charge along fermion lines ¡ Perfectly left/right symmetric e e Long-range interaction electromagnetic µ ) neutral mass-less mediator field A (the photon, γ) currents eL νL Weak charged current interactions Produces charge variation in the fermions, ∆Q = ±1 W ± Acts only on left-handed component, !! ¡ L u Short-range interaction L dL ) charged massive mediator field (W ±)µ weak charged − − − currents E.g. -
ELECTROWEAK PHYSICS Theory for the Experimentalist
ELECTROWEAK PHYSICS Theory for the experimentalist Chris Hays Oxford University CONTENTS Introduction vii 1 The geometry of forces 1 1.1 The fiber bundle of the universe 2 1.2 Spacetime metric 3 1.3 Connections 5 1.4 Curvature 6 1.5 Principle of least action 7 1.6 Conservation laws 9 2 Path integrals and fields 11 2.1 Non-relativistic path integral 12 2.2 Perturbation theory 13 2.2.1 Green’s functions 14 2.3 Path integral of a scalar field 15 2.3.1 Free-field transition amplitude 16 2.3.2 Interacting-field transition amplitude 17 2.4 Path integral of a fermion field 18 2.5 Path integral of a gauge field 19 2.5.1 Free-field generating functional 21 3 The Higgs mechanism 23 iii iv CONTENTS 3.1 Self-interacting scalar field theory 23 3.1.1 Real scalar field 23 3.1.2 Complex scalar field 24 3.2 Gauged scalar field theory 25 3.2.1 U(1)-charged scalar field 25 3.2.2 SU(2)-charged scalar field 26 3.2.3 Propagators after symmetry breaking 27 4 The Electroweak theory 29 4.1 The Electroweak Lagrangian 29 4.2 Electroweak symmetry breaking 30 4.2.1 Scalar field Lagrangian 31 4.2.2 Fermion field Lagrangian 33 4.3 Electroweak propagators 34 5 Cross sections and Feynman diagrams 37 5.1 Scattering matrix 37 5.2 Cross sections and lifetimes 38 5.3 Feynman rules 40 6 Scalar renormalization 47 6.1 Renormalized Lagrangian 47 6.2 Regularization 49 6.2.1 Propagator loop corrections 49 6.2.2 Vertex loop correction 50 6.3 The renormalization group 51 7 QED renormalization 55 7.1 QED divergences 55 7.2 Fermion self energy 56 7.3 Vacuum polarization 57 7.4 Vertex correction 61 -
New Heavy Resonances: from the Electroweak to the Planck Scale
New heavy resonances : from the electroweak to the planck scale Florian Lyonnet To cite this version: Florian Lyonnet. New heavy resonances : from the electroweak to the planck scale. High Energy Physics - Phenomenology [hep-ph]. Université de Grenoble, 2014. English. NNT : 2014GRENY035. tel-01110759v2 HAL Id: tel-01110759 https://tel.archives-ouvertes.fr/tel-01110759v2 Submitted on 10 Apr 2017 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. THÈSE Pour obtenirle grade de DOCTEUR DE L’UNIVERSITÉ DE GRENOBLE Spécialité:Physique Subatomiqueet Astroparticules Arrêtéministériel:7août2006 Présentéepar FlorianLyonnet ThèsedirigéeparIngoSchienbein préparéeau sein Laboratoirede Physique Subatomiqueet de Cosmolo- gie et de Ecoledoctoralede physique de Grenoble New heavy resonances: from the Electroweak to thePlanck scale ThèsesoutenuepubliquementOH VHSWHPEUH , devant le jurycomposéde : Mr. Aldo,Deandrea Prof., UniversitéClaudeBernardLyon 1, Rapporteur Mr. Jean-Loïc,Kneur DR,LaboratoireCharlesCoulombMontpellier,Rapporteur Mr. Roberto Bonciani Dr., UniversitàdegliStudidi Roma”LaSapienza”,Examinateur Mr. MichaelKlasen Prof., UniversitätMünster,Examinateur Mr. FrançoisMontanet Prof.,UniversitéJosephFourierde Grenoble,3UpVLGHQW Mr. JeanOrloff Prof., UniversitéBlaisePascal de Clermont-Ferrand,Examinateur Mr. IngoSchienbein MCF., UniversitéJosephFourier, Directeurde thèse ACKNOWLEDMENGTS My years at the LPSC have been exciting, intense, and I would like to express my sincere gratitude to all the people that contributed to it on the professional as well as personal level. -
The Charm of Theoretical Physics (1958– 1993)?
Eur. Phys. J. H 42, 611{661 (2017) DOI: 10.1140/epjh/e2017-80040-9 THE EUROPEAN PHYSICAL JOURNAL H Oral history interview The Charm of Theoretical Physics (1958{ 1993)? Luciano Maiani1 and Luisa Bonolis2,a 1 Dipartimento di Fisica and INFN, Piazzale A. Moro 5, 00185 Rome, Italy 2 Max Planck Institute for the History of Science, Boltzmannstraße 22, 14195 Berlin, Germany Received 10 July 2017 / Received in final form 7 August 2017 Published online 4 December 2017 c The Author(s) 2017. This article is published with open access at Springerlink.com Abstract. Personal recollections on theoretical particle physics in the years when the Standard Theory was formed. In the background, the remarkable development of Italian theoretical physics in the second part of the last century, with great personalities like Bruno Touschek, Raoul Gatto, Nicola Cabibbo and their schools. 1 Apprenticeship L. B. How did your interest in physics arise? You enrolled in the late 1950s, when the period of post-war reconstruction of physics in Europe was coming to an end, and Italy was entering into a phase of great expansion. Those were very exciting years. It was the beginning of the space era. L. M. The beginning of the space era certainly had a strong influence on many people, absolutely. The landing on the moon in 1969 was for sure unforgettable, but at that time I was already working in Physics and about to get married. My interest in physics started well before. The real beginning was around 1955. Most important for me was astronomy. It is not surprising that astronomy marked for many people the beginning of their interest in science. -
Communications-Mathematics and Applied Mathematics/Download/8110
A Mathematician's Journey to the Edge of the Universe "The only true wisdom is in knowing you know nothing." ― Socrates Manjunath.R #16/1, 8th Main Road, Shivanagar, Rajajinagar, Bangalore560010, Karnataka, India *Corresponding Author Email: [email protected] *Website: http://www.myw3schools.com/ A Mathematician's Journey to the Edge of the Universe What’s the Ultimate Question? Since the dawn of the history of science from Copernicus (who took the details of Ptolemy, and found a way to look at the same construction from a slightly different perspective and discover that the Earth is not the center of the universe) and Galileo to the present, we (a hoard of talking monkeys who's consciousness is from a collection of connected neurons − hammering away on typewriters and by pure chance eventually ranging the values for the (fundamental) numbers that would allow the development of any form of intelligent life) have gazed at the stars and attempted to chart the heavens and still discovering the fundamental laws of nature often get asked: What is Dark Matter? ... What is Dark Energy? ... What Came Before the Big Bang? ... What's Inside a Black Hole? ... Will the universe continue expanding? Will it just stop or even begin to contract? Are We Alone? Beginning at Stonehenge and ending with the current crisis in String Theory, the story of this eternal question to uncover the mysteries of the universe describes a narrative that includes some of the greatest discoveries of all time and leading personalities, including Aristotle, Johannes Kepler, and Isaac Newton, and the rise to the modern era of Einstein, Eddington, and Hawking.