Physicists Find Elusive Higgs Boson Seen As Key to Universe
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Spin and Parity of the Λ(1405) Baryon
Spin and Parity of the (1405) Baryon here [1], precisely because of the difficulty in producing it, and in particular because it must be produced spin polarized for a measurement to be made. We used photoproduction data from the CLAS detector at Jefferson Lab. The reaction + p K+ + (1405) was analyzed in the decay channel (1405) + + , where the decay distribution to + and the variation of the + polarization with respect to the (1405) polarization direction determined the spin and parity. The (1405) was produced in the c.m. energy range K 2.55 < W < 2.85 GeV and for 0.6 coscm.. 0.9 . The decay angular distribution of the (1405) in its rest Every subatomic particle has a set of properties that frame was found to be isotropic, which means the define its identity. Beyond mass, charge, and magnetic particle is consistent with spin J = ½. The first figure moment, each particle has discrete quantum numbers illustrates how the polarization P of a parent particle that include its spin angular momentum J and its with spin ½, in this case the (1405), transfers intrinsic parity P. The spin comes in integer steps of + starting from ½ for 3-quark objects (baryons). The polarization Q to the daughter baryon, in this case the , depending on whether the decay is in a spatial S wave parity is either positive (“+”) or negative (“”) (L=0) or P wave (L=1). This distinction is what depending on the inversion symmetry of its spatial wave determines the parity of the final state, and hence of the function. For example, the familiar proton and neutron parent. -
The Subatomic Particle Mass Spectrum
The Subatomic Particle Mass Spectrum Robert L. Oldershaw 12 Emily Lane Amherst, MA 01002 USA [email protected] Key Words: Subatomic Particles; Particle Mass Spectrum; General Relativity; Kerr Metric; Discrete Self-Similarity; Discrete Scale Relativity 1 Abstract: Representative members of the subatomic particle mass spectrum in the 100 MeV to 7,000 MeV range are retrodicted to a first approximation using the Kerr solution of General Relativity. The particle masses appear to form a restricted set of quantized values of a Kerr- based angular momentum-mass relation: M = n1/2 M, where values of n are a set of discrete integers and M is a revised Planck mass. A fractal paradigm manifesting global discrete self- similarity is critical to a proper determination of M, which differs from the conventional Planck mass by a factor of roughly 1019. This exceedingly simple and generic mass equation retrodicts the masses of a representative set of 27 well-known particles with an average relative error of 1.6%. A more rigorous mass formula, which includes the total spin angular momentum rule of Quantum Mechanics, the canonical spin values of the particles, and the dimensionless rotational parameter of the Kerr angular momentum-mass relation, is able to retrodict the masses of the 8 dominant baryons in the 900 MeV to 1700 MeV range at the < 99.7% > level. 2 “There remains one especially unsatisfactory feature [of the Standard Model of particle physics]: the observed masses of the particles, m. There is no theory that adequately explains these numbers. We use the numbers in all our theories, but we do not understand them – what they are, or where they come from. -
FUNDAMENTAL PARTICLES Year 14 Physics Erin Hannigan
FUNDAMENTAL PARTICLES Year 14 Physics Erin Hannigan 1 Key Word List ■ Natural Philosophy – the science of matter and energy and their interactions. ■ Hadron – any elementary particle that interacts strongly with other particles. ■ Lepton – an elementary particle that participates in weak interactions. ■ Subatomic Particle – a body having finite mass and internal structure but negligible dimensions. ■ Quark – any of a number f subatomic particles carrying a fractional electric charge, postulated as building blocks of the hadrons. Quarks have not been directly observed but theoretical predictions based on their existence have been confirmed experimentally. ■ Atom – the smallest component of an element having the chemical properties of the element. 2 Fundamental Particles ■ Fundamental particles (also called elementary particles) are the smallest building blocks of the universe. The key characteristic of fundamental particles is that they have no internal structure. ■ There are two type of fundamental particles: – Particles that make up all matter, called fermions – Particles that carry force, called bosons ■ The four fundamental forces include: – Gravity – The weak force – Electromagnetism – The strong force 3 The Four Fundamental Forces ■ The four fundamental forces of nature govern everything that happens in the universe. ■ Gravity – The attraction between two objects that have mass or energy ■ The weak force – Responsible for particle decay – Physicists describe this interaction through the exchange of force-carrying particles called -
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). -
Introduction to Subatomic- Particle Spectrometers∗
IIT-CAPP-15/2 Introduction to Subatomic- Particle Spectrometers∗ Daniel M. Kaplan Illinois Institute of Technology Chicago, IL 60616 Charles E. Lane Drexel University Philadelphia, PA 19104 Kenneth S. Nelsony University of Virginia Charlottesville, VA 22901 Abstract An introductory review, suitable for the beginning student of high-energy physics or professionals from other fields who may desire familiarity with subatomic-particle detection techniques. Subatomic-particle fundamentals and the basics of particle in- teractions with matter are summarized, after which we review particle detectors. We conclude with three examples that illustrate the variety of subatomic-particle spectrom- eters and exemplify the combined use of several detection techniques to characterize interaction events more-or-less completely. arXiv:physics/9805026v3 [physics.ins-det] 17 Jul 2015 ∗To appear in the Wiley Encyclopedia of Electrical and Electronics Engineering. yNow at Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723. 1 Contents 1 Introduction 5 2 Overview of Subatomic Particles 5 2.1 Leptons, Hadrons, Gauge and Higgs Bosons . 5 2.2 Neutrinos . 6 2.3 Quarks . 8 3 Overview of Particle Detection 9 3.1 Position Measurement: Hodoscopes and Telescopes . 9 3.2 Momentum and Energy Measurement . 9 3.2.1 Magnetic Spectrometry . 9 3.2.2 Calorimeters . 10 3.3 Particle Identification . 10 3.3.1 Calorimetric Electron (and Photon) Identification . 10 3.3.2 Muon Identification . 11 3.3.3 Time of Flight and Ionization . 11 3.3.4 Cherenkov Detectors . 11 3.3.5 Transition-Radiation Detectors . 12 3.4 Neutrino Detection . 12 3.4.1 Reactor Neutrinos . 12 3.4.2 Detection of High Energy Neutrinos . -
A Young Physicist's Guide to the Higgs Boson
A Young Physicist’s Guide to the Higgs Boson Tel Aviv University Future Scientists – CERN Tour Presented by Stephen Sekula Associate Professor of Experimental Particle Physics SMU, Dallas, TX Programme ● You have a problem in your theory: (why do you need the Higgs Particle?) ● How to Make a Higgs Particle (One-at-a-Time) ● How to See a Higgs Particle (Without fooling yourself too much) ● A View from the Shadows: What are the New Questions? (An Epilogue) Stephen J. Sekula - SMU 2/44 You Have a Problem in Your Theory Credit for the ideas/example in this section goes to Prof. Daniel Stolarski (Carleton University) The Usual Explanation Usual Statement: “You need the Higgs Particle to explain mass.” 2 F=ma F=G m1 m2 /r Most of the mass of matter lies in the nucleus of the atom, and most of the mass of the nucleus arises from “binding energy” - the strength of the force that holds particles together to form nuclei imparts mass-energy to the nucleus (ala E = mc2). Corrected Statement: “You need the Higgs Particle to explain fundamental mass.” (e.g. the electron’s mass) E2=m2 c4+ p2 c2→( p=0)→ E=mc2 Stephen J. Sekula - SMU 4/44 Yes, the Higgs is important for mass, but let’s try this... ● No doubt, the Higgs particle plays a role in fundamental mass (I will come back to this point) ● But, as students who’ve been exposed to introductory physics (mechanics, electricity and magnetism) and some modern physics topics (quantum mechanics and special relativity) you are more familiar with.. -
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. -
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. -
Going Massive Have Frequently Been One of Them
excitement — then gives an accurate primer on the standard model of particle physics. He enumerates the forces and particles, and discusses the role of quantum fields and symmetries, as well as the accelerators and detectors that provide the evidence to keep C. MARCELLONI/CERN the crazy concepts rooted in reality. Towards the end of the book, Carroll touches on the discovery’s impact. I could have done without the Winnie the Pooh-style subtitles to each chapter, such as “In which we suggest that everything in the universe is made out of fields”. But this is a minor flaw and, elsewhere, he discusses the issues and events with passion and clarity. An example is the moment, nine days after the LHC was switched on in 2008, when one-eighth of it suffered a catastrophic leak of liquid helium. Or, as Carroll accurately puts it, “it exploded”. The disappointment, the challenges of explaining the event to the public and of dealing with the alleged risks of turning on the machine — ‘Black holes will eat you!’ — are beautifully done. Josef Kristofoletti’s massive mural of the ATLAS particle detector adorns a building at CERN. Carroll gives a sense of the intensity (and the international nature) of the effort of PARTICLE PHYSICS building and running the LHC. I was not surprised by his report that 1 in 16 of the passengers passing through Geneva airport are in some way associated with CERN. I Going massive have frequently been one of them. And that is just the tip of an iceberg of teleconferences, Jonathan Butterworth enjoys the latest chronicle e-mails, night shifts and a general shortage of the hunt for the ‘most wanted’ particle. -
Language and Materiality Ethnographic and Theoretical Explorations
Language and Materiality Ethnographic and Theoretical Explorations Edited by Jillian R. Cavanaugh CUNY, New York Shalini Shankar Northwestern University University Printing House, Cambridge CB2 8BS, United Kingdom One Liberty Plaza, 20th Floor, New York, NY 10006, USA 477 Williamstown Road, Port Melbourne, VIC 3207, Australia 4843/24, 2nd Floor, Ansari Road, Daryaganj, Delhi - 110002, India 79 Anson Road, #06-04/06, Singapore 079906 Cambridge University Press is part of the University of Cambridge. It furthers the University’s mission by disseminating knowledge in the pursuit of education, learning, and research at the highest international levels of excellence. www.cambridge.org Information on this title: www.cambridge.org/9781107180949 DOI: 10.1017/9781316848418 C Cambridge University Press 2017 This publication is in copyright. Subject to statutory exception and to the provisions of relevant collective licensing agreements, no reproduction of any part may take place without the written permission of Cambridge University Press. First published 2017 Printed in <country> by <printer> A catalogue record for this publication is available from the British Library. Library of Congress Cataloging-in-Publication Data ISBN 978-1-107-18094-9 Hardback Cambridge University Press has no responsibility for the persistence or accuracy of URLs for external or third-party internet websites referred to in this publication and does not guarantee that any content on such websites is, or will remain, accurate or appropriate. 4 Fontroversy! Or, How to Care about the Shape of Language Keith M. Murphy Introduction On July 4, 2012, standing in the well of a packed lecture hall on the cam- pus of the European Organization for Nuclear Research (CERN), just outside Geneva, particle physicist Joseph Incandela looked up at the hall’s projection screen and, with only a hint of nerves in his voice, uttered the following pro- nouncement: “If we combine the ZZ and gamma-gamma, this is what we get. -
Prhep Hep2001
International Europhysics Conference on HEP PROCEEDINGS Searches for new particles at Colliders Fabiola Gianotti∗ CERN, EP Division, 1211 Gen`eve 23, Switzerland E-mail: [email protected] Abstract: Most recent results from the searches for new particles at LEP, Tevatron and PrHEP hep2001 HERA, presented at the 2001 Summer Conferences, are reviewed. Prospects at future machines (LHC and Linear Colliders) are also discussed. The emphasis is put on the quest for Higgs bosons, Supersymmetry, Extra-dimensions and Flavour-Changing Neu- tral Current processes. In each case, the phenomenological framework, the experimental strategies, and the analysis methods are described, and the sensitivity and reach of the various machines are compared. 1. Introduction The search for new particles is one of the most exciting, rapidly-evolving and prolific fields in today’s high-energy experimental physics, motivated also by a rich spectrum of theoretical scenarios and predictions. Over the last years, the three operational high-energy Colliders, LEP, Tevatron and HERA, have explored the few hundred GeV energy range and set stringent bounds on various models. In addition, recently LEP has reported an exciting 2σ hint in the search for a Standard Model (SM) Higgs boson of mass about 115 GeV, and the H1 experiment at HERA has observed an excess of W ’s produced in association with a high transverse momentum hadronic system. Since 1996, i.e. since the beginning of its phase two, LEP has delivered an integrated 1 luminosity of about 700 pb− per experiment at a centre-of-mass energy above the W -pair production threshold. The machine performance in terms of both energy and luminosity went beyond any optimistic expectation. -
Université Joseph Fourier Les Houches Session LXXXVII 2007
houches87cov.tex; 12/05/2008; 18:25 p. 1 1 Université Joseph Fourier 1 2 2 3 Les Houches 3 4 4 5 Session LXXXVII 5 6 6 7 2007 7 8 8 9 9 10 10 11 11 12 12 13 13 14 14 15 String Theory and the Real World: 15 16 16 17 From Particle Physics to Astrophysics 17 18 18 19 19 20 20 21 21 22 22 23 23 24 24 25 25 26 26 27 27 28 28 29 29 30 30 31 31 32 32 33 33 34 34 35 35 36 36 37 37 38 38 39 39 40 40 41 41 42 42 houches87cov.tex; 12/05/2008; 18:25 p. 2 1 Lecturers who contributed to this volume 1 2 2 3 3 4 4 I. Antoniadis 5 5 J.L.F. Barbón 6 6 Marcus K. Benna 7 7 Thibault Damour 8 8 Frederik Denef 9 9 F. Gianotti 10 10 G.F. Giudice 11 11 Kenneth Intriligator 12 12 Elias Kiritsis 13 13 Igor R. Klebanov 14 14 Marc Lilley 15 15 Juan M. Maldacena 16 16 Eliezer Rabinovici 17 17 Nathan Seiberg 18 18 Angel M. Uranga 19 19 Pierre Vanhove 20 20 21 21 22 22 23 23 24 24 25 25 26 26 27 27 28 28 29 29 30 30 31 31 32 32 33 33 34 34 35 35 36 36 37 37 38 38 39 39 40 40 41 41 42 42 houches87cov.tex; 12/05/2008; 18:25 p. 3 1 ÉCOLE D’ÉTÉ DE PHYSIQUE DES HOUCHES 1 2 2 3 SESSION LXXXVII, 2 JULY–27 JULY 2007 3 4 4 5 5 6 6 COLE THÉMATIQUE DU 7 É CNRS 7 8 8 9 9 10 10 11 11 12 12 13 13 14 14 15 STRING THEORY AND THE REAL WORLD: 15 16 16 17 FROM PARTICLE PHYSICS TO ASTROPHYSICS 17 18 18 19 19 20 20 21 21 Edited by 22 22 23 C.