Unification of Couplings
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
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. -
Advances in Theoretical & Computational Physics
ISSN: 2639-0108 Research Article Advances in Theoretical & Computational Physics Supreme Theory of Everything Ulaanbaatar Tarzad *Corresponding author Ulaanbaatar Tarzad, Department of Physics, School of Applied Sciences, Department of Physics, School of Applied Sciences, Mongolian Mongolian University of Science and Technology, Ulaanbaatar, Mongolia, University of Science and Technology E-mail: [email protected] Submitted: 27 Mar 2019; Accepted: 24 Apr 2019; Published: 06 June 2019 Abstract Not only universe, but everything has general characters as eternal, infinite, cyclic and wave-particle duality. Everything from elementary particles to celestial bodies, from electromagnetic wave to gravity is in eternal motions, which dissects only to circle. Since everything is described only by trigonometry. Without trigonometry and mathematical circle, the science cannot indicate all the beauty of harmonic universe. Other method may be very good, but it is not perfect. Some part is very nice, another part is problematic. General Theory of Relativity holds that gravity is geometric. Quantum Mechanics describes all particles by wave function of trigonometry. In this paper using trigonometry, particularly mathematics circle, a possible version of the unification of partial theories, evolution history and structure of expanding universe, and the parallel universes are shown. Keywords: HRD, Trigonometry, Projection of Circle, Singularity, The reality of universe describes by geometry, because of that not Celestial Body, Black Hole and Parallel Universes. only gravity is geometrical, but everything is it and nothing is linear. One of the important branches of geometry is trigonometry dealing Introduction with circle and triangle. For this reason, it is easier to describe nature Today scientists describe the universe in terms of two basic partial of universe by mathematics circle. -
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. -
Conceptual Investigations of a Trigger Extension for Muons from Pp Collisions in the CMS Experiment
Conceptual investigations of a trigger extension for muons from pp collisions in the CMS experiment Von der Fakult¨at fur¨ Mathematik, Informatik und Naturwissenschaften der RWTH Aachen University zur Erlangung des akademischen Grades eines Doktors der Naturwissenschaften genehmigte Dissertation vorgelegt von Diplom-Physiker Yusuf Erdogan aus Istanbul Berichter: Universit¨atsprofessor Dr. rer. nat. Achim Stahl Universit¨atsprofessor Dr. rer. nat. Thomas Hebbeker Tag der mundlic¨ hen Prufung¨ : 24. Februar 2015 Diese Dissertation ist auf den Internetseiten der Hochschulbibliothek online verfu¨gbar. Kurzfassung Der Large Hadron Collider wird ab 2023 an seine Experimente fun¨ f bis zehn mal mehr Lu- minosit¨at als der derzeitige Designwert von 1034 cm−2s−1 liefern k¨onnen. Diese Verbes- serung wird die Messung von physikalischen Prozessen mit sehr kleinen Wirkungsquer- schnitten erlauben. Jedoch wird bei diesen hohen Luminosit¨aten, aufgrund von Pile-up Wechselwirkungen, die Belegung des CMS-Detektors sehr hoch sein. Dies wird einer- seits einen systematischen Anstieg von Triggerraten fur¨ einzelne Myonen verursachen, Andererseits werden die Fehlmessungen von Myon-Transversalimpulsen, verst¨arkt durch die begrenzte Impulsaufl¨osung des Myon-Systems, fur¨ hohe Impulswerte dominant sein. In diesem Bereich flacht die Verteilung der Triggerrate ab, was die Beschr¨ankung der Triggerrate durch eine Schwelle der Transversalimpulse erschwert. Außerdem wird die Qualit¨at des Triggers fu¨r einzelne Myonen durch koinzidente Teilchendurchg¨ange ver- ringert, da diese zu Doppeldeutigkeiten in den innersten Myonkammern fuh¨ ren k¨onnen. Im Rahmen der Ver¨offentlichung [2] wurde im Jahr 2007 ein Muon Track fast Tag (MTT) genanntes Konzept vorgestellt, um diese Trigger-Herausforderungen zu adressieren. Die, in dieser Arbeit durchgefuh¨ rten Studien sind in drei Abschitte unterteilt. -
Inside the Perimeter Is Published by Perimeter Institute for Theoretical Physics
the Perimeter fall/winter 2014 Skateboarding Physicist Seeks a Unified Theory of Self The Black Hole that Birthed the Big Bang The Beauty of Truth: A Chat with Savas Dimopoulos Subir Sachdev's Superconductivity Puzzles Editor Natasha Waxman [email protected] Contributing Authors Graphic Design Niayesh Afshordi Gabriela Secara Erin Bow Mike Brown Photographers & Artists Phil Froklage Tibra Ali Colin Hunter Justin Bishop Robert B. Mann Amanda Ferneyhough Razieh Pourhasan Liz Goheen Natasha Waxman Alioscia Hamma Jim McDonnell Copy Editors Gabriela Secara Tenille Bonoguore Tegan Sitler Erin Bow Mike Brown Colin Hunter Inside the Perimeter is published by Perimeter Institute for Theoretical Physics. www.perimeterinstitute.ca To subscribe, email us at [email protected]. 31 Caroline Street North, Waterloo, Ontario, Canada p: 519.569.7600 f: 519.569.7611 02 IN THIS ISSUE 04/ Young at Heart, Neil Turok 06/ Skateboarding Physicist Seeks a Unified Theory of Self,Colin Hunter 10/ Inspired by the Beauty of Math: A Chat with Kevin Costello, Colin Hunter 12/ The Black Hole that Birthed the Big Bang, Niayesh Afshordi, Robert B. Mann, and Razieh Pourhasan 14/ Is the Universe a Bubble?, Colin Hunter 15/ Probing Nature’s Building Blocks, Phil Froklage 16/ The Beauty of Truth: A Chat with Savas Dimopoulos, Colin Hunter 18/ Conference Reports 22/ Back to the Classroom, Erin Bow 24/ Finding the Door, Erin Bow 26/ "Bright Minds in Their Life’s Prime", Colin Hunter 28/ Anthology: The Portraits of Alioscia Hamma, Natasha Waxman 34/ Superconductivity Puzzles, Colin Hunter 36/ Particles 39/ Donor Profile: Amy Doofenbaker, Colin Hunter 40/ From the Black Hole Bistro, Erin Bow 42/ PI Kids are Asking, Erin Bow 03 neil’s notes Young at Heart n the cover of this issue, on the initial singularity from which everything the lip of a halfpipe, teeters emerged. -
Curriculum Vitae
CURRICULUM VITAE Raman Sundrum July 26, 2019 CONTACT INFORMATION Physical Sciences Complex, University of Maryland, College Park, MD 20742 Office - (301) 405-6012 Email: [email protected] CAREER John S. Toll Chair, Director of the Maryland Center for Fundamental Physics, 2012 - present. Distinguished University Professor, University of Maryland, 2011-present. Elkins Chair, Professor of Physics, University of Maryland, 2010-2012. Alumni Centennial Chair, Johns Hopkins University, 2006- 2010. Full Professor at the Department of Physics and Astronomy, The Johns Hopkins University, 2001- 2010. Associate Professor at the Department of Physics and Astronomy, The Johns Hop- kins University, 2000- 2001. Research Associate at the Department of Physics, Stanford University, 1999- 2000. Advisor { Prof. Savas Dimopoulos. 1 Postdoctoral Fellow at the Department of Physics, Boston University. 1996- 1999. Postdoc advisor { Prof. Sekhar Chivukula. Postdoctoral Fellow in Theoretical Physics at Harvard University, 1993-1996. Post- doc advisor { Prof. Howard Georgi. Postdoctoral Fellow in Theoretical Physics at the University of California at Berke- ley, 1990-1993. Postdoc advisor { Prof. Stanley Mandelstam. EDUCATION Yale University, New-Haven, Connecticut Ph.D. in Elementary Particle Theory, May 1990 Thesis Title: `Theoretical and Phenomenological Aspects of Effective Gauge Theo- ries' Thesis advisor: Prof. Lawrence Krauss Brown University, Providence, Rhode Island Participant in the 1988 Theoretical Advanced Summer Institute University of Sydney, Australia B.Sc with First Class Honours in Mathematics and Physics, Dec. 1984 AWARDS, DISTINCTIONS J. J. Sakurai Prize in Theoretical Particle Physics, American Physical Society, 2019. Distinguished Visiting Research Chair, Perimeter Institute, 2012 - present. 2 Moore Fellow, Cal Tech, 2015. American Association for the Advancement of Science, Fellow, 2011. -
The Discovery of Asymptotic Freedom
The Discovery of Asymptotic Freedom The 2004 Nobel Prize in Physics, awarded to David Gross, Frank Wilczek, and David Politzer, recognizes the key discovery that explained how quarks, the elementary constituents of the atomic nucleus, are bound together to form protons and neutrons. In 1973, Gross and Wilczek, working at Princeton, and Politzer, working independently at Harvard, showed that the attraction between quarks grows weaker as the quarks approach one another more closely, and correspondingly that the attraction grows stronger as the quarks are separated. This discovery, known as “asymptotic freedom,” established quantum chromodynamics (QCD) as the correct theory of the strong nuclear force, one of the four fundamental forces in Nature. At the time of the discovery, Wilczek was a 21-year-old graduate student working under Gross’s supervision at Princeton, while Politzer was a 23-year-old graduate student at Harvard. Currently Gross is the Director of the Kavli Institute for Theoretical Physics at the University of California at Santa Barbara, and Wilczek is the Herman Feshbach Professor of Physics at MIT. Politzer is Professor of Theoretical Physics at Caltech; he joined the Caltech faculty in 1976. Of the four fundamental forces --- the others besides the strong nuclear force are electromagnetism, the weak nuclear force (responsible for the decay of radioactive nuclei), and gravitation --- the strong force was by far the most poorly understood in the early 1970s. It had been suggested in 1964 by Caltech physicist Murray Gell-Mann that protons and neutrons contain more elementary objects, which he called quarks. Yet isolated quarks are never seen, indicating that the quarks are permanently bound together by powerful nuclear forces. -
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. -
Standard Model of Particle Physics, Or Beyond?
Standard Model of Particle Physics, or Beyond? Mariano Quir´os High Energy Phys. Inst., BCN (Spain) ICTP-SAIFR, November 13th, 2019 Outline The outline of this colloquium is I Standard Model: reminder I Electroweak interactions I Strong interactions I The Higgs sector I Experimental successes I Theoretical and observational drawbacks I Beyond the Standard Model I Supersymmetry I Large extra dimensions I Warped extra dimensions/composite Higgs I Concluding remarks Disclaimer: I will not discuss any technical details. With my apologies to my theorist (and experimental) colleagues The Standard Model: reminder I The knowledge of the Standard Model of strong and electroweak interactions requires (as any other physical theory) the knowledge of I The elementary particles or fields (the characters of the play) I How particles interact (their behavior) The characters of the play I Quarks: spin-1/2 fermions I Leptons: spin-1/2 fermions I Higgs boson: spin-0 boson I Carriers of the interactions: spin-1 (gauge) bosons I All these particles have already been discovered and their mass, spin, and charge measured \More in detail the characters of the play" - Everybody knows the Periodic Table of the Elements - Compare elementary particles with some (of course composite) very heavy nuclei What are the interactions between the elementary building blocks of the Standard Model? I Interactions are governed by a symmetry principle I The more symmetric the theory the more couplings are related (the less of them they are) and the more predictive it is Strong interactions: -
Symposium Celebrating CERN's Discoveries and Looking Into the Future
CERN–EP–2003–073 CERN–TH–2003–281 December 1st, 2003 Proceedings Symposium celebrating the Anniversary of CERN’s Discoveries and a Look into the Future 111999777333::: NNNeeeuuutttrrraaalll CCCuuurrrrrreeennntttsss 111999888333::: WWW±±± &&& ZZZ000 BBBooosssooonnnsss Tuesday 16 September 2003 CERN, Geneva, Switzerland Editors: Roger Cashmore, Luciano Maiani & Jean-Pierre Revol Table of contents Table of contents 2 Programme of the Symposium 4 Foreword (L. Maiani) 7 Acknowledgements 8 Selected Photographs of the Event 9 Contributions: Welcome (L. Maiani) 13 The Making of the Standard Model (S. Weinberg) 16 CERN’s Contribution to Accelerators and Beams (G. Brianti) 30 The Discovery of Neutral Currents (D. Haidt) 44 The Discovery of the W & Z, a personal recollection (P. Darriulat) 57 W & Z Physics at LEP (P. Zerwas) 70 Physics at the LHC (J. Ellis) 85 Challenges of the LHC: – the accelerator challenge (L. Evans) 96 – the detector challenge (J. Engelen) 103 – the computing challenge (P. Messina) 110 Particle Detectors and Society (G. Charpak) 126 The future for CERN (L. Maiani) 136 – 2 – Table of contents (cont.) Panel discussion on the Future of Particle Physics (chaired by Carlo Rubbia) 145 Participants: Robert Aymar, Georges Charpak, Pierre Darriulat, Luciano Maiani, Simon van der Meer, Lev Okun, Donald Perkins, Carlo Rubbia, Martinus Veltman, and Steven Weinberg. Statements from the floor by: Fabiola Gianotti, Ignatios Antoniadis, S. Glashow, H. Schopper, C. Llewellyn Smith, V. Telegdi, G. Bellettini, and V. Soergel. Additional contributions: Comment on the occasion (S. L. Glashow) 174 Comment on Perturbative QCD in early CERN experiments (D. H. Perkins) 175 Personal remarks on the discovery of Neutral Currents (A. -
Confusions Regarding Quantum Mechanics Gerard ’T Hooft, Reply by Sheldon Lee Glashow
INFERENCE / Vol. 5, No. 3 Confusions Regarding Quantum Mechanics Gerard ’t Hooft, reply by Sheldon Lee Glashow In response to “The Yang–Mills Model” (Vol. 5, No. 2). began to argue about how the equation is supposed to be interpreted. Why is it that positions and velocities of par- ticles at one given moment cannot be calculated, or even To the editors: defined unambiguously? Physicists know very well how to use the equation. Quantum mechanics was one of the most significant and They use it to derive with perplexing accuracy the prop- important discoveries of twentieth-century science. It all erties of atoms, molecules, elementary particles, and the began, I think, in the year 1900 when Max Planck published forces between all of these. The way the equation is used his paper entitled “On the Theory of the Energy Distribu- is nothing to complain about, but what exactly does it say? tion Law of the Normal Spectrum.”1 In it, he describes a The first question one may rightfully ask, and that simple observation: if one attaches an entropy to the radi- has been asked by many researchers and their students, ation field as if its total energy came in packages—now is this: called quanta—then the intensity of the radiation associ- ated to a certain temperature agrees quite well with the What do these wave functions represent? In particular, what observations. Planck had described his hypothesis as “an is represented by the wave functions that are not associ- act of desperation.”2 But it was the only one that worked. -
Steven Weinberg
Obituary Steven Weinberg (1933–2021) Theoretical physicist whose electroweak theory won the Nobel prize. teven Weinberg brought the funda- on to positions at Columbia University, New mental understanding of nature to York; the University of Berkeley, California; new levels of power and completeness. the Massachusetts Institute of Technology in He played a central part in formulating Cambridge; and, in 1973, to Harvard University and establishing theoretical physics’ in Cambridge, where he was Higgins Professor Stwo standard models — the standard model of Physics. In 1982, he moved to the University of fundamental interactions and the standard of Texas at Austin, where he remained, teach- model of cosmology. His greatest achievement ing until earlier this year. was to propose the unified theory of electro- Scientists, no less than composers, have magnetism and weak interactions, which is still styles. Einstein and Richard Feynman were in use. This won him the Nobel Prize in Phys- rebellious, most comfortable when they were ics in 1979, shared with his school classmate ‘thinking different’. Weinberg was not like that. Sheldon Lee Glashow, and with Abdus Salam. His approach was scholarly. Most obviously, he His 1967 Physical Review Letters paper, ‘A was keenly interested in the history of physics in Model of Leptons’, combined disparate ideas the West, about which he wrote several deeply about gauge symmetry, symmetry breaking researched and unashamedly ‘Whiggish’ books, and the classification of particles into an ele- most recently To Explain the World (2015). gant whole. Given the state of knowledge at He paid close attention to other people’s CERN/SPL the time, the breakthrough still calls to mind work.