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Magnetic Monopole Searches See the Related Review(S): Magnetic Monopoles
Citation: P.A. Zyla et al. (Particle Data Group), Prog. Theor. Exp. Phys. 2020, 083C01 (2020) Magnetic Monopole Searches See the related review(s): Magnetic Monopoles Monopole Production Cross Section — Accelerator Searches X-SECT MASS CHG ENERGY (cm2) (GeV) (g) (GeV) BEAM DOCUMENT ID TECN <2.5E−37 200–6000 1 13000 pp 1 ACHARYA 17 INDU <2E−37 200–6000 2 13000 pp 1 ACHARYA 17 INDU <4E−37 200–5000 3 13000 pp 1 ACHARYA 17 INDU <1.5E−36 400–4000 4 13000 pp 1 ACHARYA 17 INDU <7E−36 1000–3000 5 13000 pp 1 ACHARYA 17 INDU <5E−40 200–2500 0.5–2.0 8000 pp 2 AAD 16AB ATLS <2E−37 100–3500 1 8000 pp 3 ACHARYA 16 INDU <2E−37 100–3500 2 8000 pp 3 ACHARYA 16 INDU <6E−37 500–3000 3 8000 pp 3 ACHARYA 16 INDU <7E−36 1000–2000 4 8000 pp 3 ACHARYA 16 INDU <1.6E−38 200–1200 1 7000 pp 4 AAD 12CS ATLS <5E−38 45–102 1 206 e+ e− 5 ABBIENDI 08 OPAL <0.2E−36 200–700 1 1960 p p 6 ABULENCIA 06K CNTR < 2.E−36 1 300 e+ p 7,8 AKTAS 05A INDU < 0.2 E−36 2 300 e+ p 7,8 AKTAS 05A INDU < 0.09E−36 3 300 e+ p 7,8 AKTAS 05A INDU < 0.05E−36 ≥ 6 300 e+ p 7,8 AKTAS 05A INDU < 2.E−36 1 300 e+ p 7,9 AKTAS 05A INDU < 0.2E−36 2 300 e+ p 7,9 AKTAS 05A INDU < 0.07E−36 3 300 e+ p 7,9 AKTAS 05A INDU < 0.06E−36 ≥ 6 300 e+ p 7,9 AKTAS 05A INDU < 0.6E−36 >265 1 1800 p p 10 KALBFLEISCH 04 INDU < 0.2E−36 >355 2 1800 p p 10 KALBFLEISCH 04 INDU < 0.07E−36 >410 3 1800 p p 10 KALBFLEISCH 04 INDU < 0.2E−36 >375 6 1800 p p 10 KALBFLEISCH 04 INDU < 0.7E−36 >295 1 1800 p p 11,12 KALBFLEISCH 00 INDU < 7.8E−36 >260 2 1800 p p 11,12 KALBFLEISCH 00 INDU < 2.3E−36 >325 3 1800 p p 11,13 KALBFLEISCH 00 INDU < 0.11E−36 >420 6 1800 p p 11,13 KALBFLEISCH 00 INDU <0.65E−33 <3.3 ≥ 2 11A 197Au 14,15 HE 97 <1.90E−33 <8.1 ≥ 2 160A 208Pb 14,15 HE 97 <3.E−37 <45.0 1.0 88–94 e+ e− PINFOLD 93 PLAS <3.E−37 <41.6 2.0 88–94 e+ e− PINFOLD 93 PLAS <7.E−35 <44.9 0.2–1.0 89–93 e+ e− KINOSHITA 92 PLAS <2.E−34 <850 ≥ 0.5 1800 p p BERTANI 90 PLAS <1.2E−33 <800 ≥ 1 1800 p p PRICE 90 PLAS <1.E−37 <29 1 50–61 e+ e− KINOSHITA 89 PLAS <1.E−37 <18 2 50–61 e+ e− KINOSHITA 89 PLAS <1.E−38 <17 <1 35 e+ e− BRAUNSCH.. -
The Moedal Experiment at the LHC. Searching Beyond the Standard
126 EPJ Web of Conferences , 02024 (2016) DOI: 10.1051/epjconf/201612602024 ICNFP 2015 The MoEDAL experiment at the LHC Searching beyond the standard model James L. Pinfold (for the MoEDAL Collaboration)1,a 1 University of Alberta, Physics Department, Edmonton, Alberta T6G 0V1, Canada Abstract. MoEDAL is a pioneering experiment designed to search for highly ionizing avatars of new physics such as magnetic monopoles or massive (pseudo-)stable charged particles. Its groundbreaking physics program defines a number of scenarios that yield potentially revolutionary insights into such foundational questions as: are there extra dimensions or new symmetries; what is the mechanism for the generation of mass; does magnetic charge exist; what is the nature of dark matter; and, how did the big-bang develop. MoEDAL’s purpose is to meet such far-reaching challenges at the frontier of the field. The innovative MoEDAL detector employs unconventional methodologies tuned to the prospect of discovery physics. The largely passive MoEDAL detector, deployed at Point 8 on the LHC ring, has a dual nature. First, it acts like a giant camera, comprised of nuclear track detectors - analyzed offline by ultra fast scanning microscopes - sensitive only to new physics. Second, it is uniquely able to trap the particle messengers of physics beyond the Standard Model for further study. MoEDAL’s radiation environment is monitored by a state-of-the-art real-time TimePix pixel detector array. A new MoEDAL sub-detector to extend MoEDAL’s reach to millicharged, minimally ionizing, particles (MMIPs) is under study Finally we shall describe the next step for MoEDAL called Cosmic MoEDAL, where we define a very large high altitude array to take the search for highly ionizing avatars of new physics to higher masses that are available from the cosmos. -
Accelerator Search of the Magnetic Monopo
Accelerator Based Magnetic Monopole Search Experiments (Overview) Vasily Dzhordzhadze, Praveen Chaudhari∗, Peter Cameron, Nicholas D’Imperio, Veljko Radeka, Pavel Rehak, Margareta Rehak, Sergio Rescia, Yannis Semertzidis, John Sondericker, and Peter Thieberger. Brookhaven National Laboratory ABSTRACT We present an overview of accelerator-based searches for magnetic monopoles and we show why such searches are important for modern particle physics. Possible properties of monopoles are reviewed as well as experimental methods used in the search for them at accelerators. Two types of experimental methods, direct and indirect are discussed. Finally, we describe proposed magnetic monopole search experiments at RHIC and LHC. Content 1. Magnetic Monopole characteristics 2. Experimental techniques 3. Monopole Search experiments 4. Magnetic Monopoles in virtual processes 5. Future experiments 6. Summary 1. Magnetic Monopole characteristics The magnetic monopole puzzle remains one of the fundamental and unsolved problems in physics. This problem has a along history. The military engineer Pierre de Maricourt [1] in1269 was breaking magnets, trying to separate their poles. P. Curie assumed the existence of single magnetic poles [2]. A real breakthrough happened after P. Dirac’s approach to the solution of the electron charge quantization problem [3]. Before Dirac, J. Maxwell postulated his fundamental laws of electrodynamics [4], which represent a complete description of all known classical electromagnetic phenomena. Together with the Lorenz force law and the Newton equations of motion, they describe all the classical dynamics of interacting charged particles and electromagnetic fields. In analogy to electrostatics one can add a magnetic charge, by introducing a magnetic charge density, thus magnetic fields are no longer due solely to the motion of an electric charge and in Maxwell equation a magnetic current will appear in analogy to the electric current. -
Lectures on D-Branes
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server CPHT/CL-615-0698 hep-th/9806199 Lectures on D-branes Constantin P. Bachas1 Centre de Physique Th´eorique, Ecole Polytechnique 91128 Palaiseau, FRANCE [email protected] ABSTRACT This is an introduction to the physics of D-branes. Topics cov- ered include Polchinski’s original calculation, a critical assessment of some duality checks, D-brane scattering, and effective worldvol- ume actions. Based on lectures given in 1997 at the Isaac Newton Institute, Cambridge, at the Trieste Spring School on String The- ory, and at the 31rst International Symposium Ahrenshoop in Buckow. June 1998 1Address after Sept. 1: Laboratoire de Physique Th´eorique, Ecole Normale Sup´erieure, 24 rue Lhomond, 75231 Paris, FRANCE, email : [email protected] Lectures on D-branes Constantin Bachas 1 Foreword Referring in his ‘Republic’ to stereography – the study of solid forms – Plato was saying : ... for even now, neglected and curtailed as it is, not only by the many but even by professed students, who can suggest no use for it, never- theless in the face of all these obstacles it makes progress on account of its elegance, and it would not be astonishing if it were unravelled. 2 Two and a half millenia later, much of this could have been said for string theory. The subject has progressed over the years by leaps and bounds, despite periods of neglect and (understandable) criticism for lack of direct experimental in- put. To be sure, the construction and key ingredients of the theory – gravity, gauge invariance, chirality – have a firm empirical basis, yet what has often catalyzed progress is the power and elegance of the underlying ideas, which look (at least a posteriori) inevitable. -
Magnetic Monopoles
Magnetic Monopoles Since Maxwell discovered the unified theory, Maxwell equations, of electric and magnetic forces, people have studied its implications. Maxwell conjectured the electromagnetic wave in his equations to be the light, based on the speed of electromagnetic wave being close to the speed of light. Since Herz and Heaviside, independently, have written the current form of Maxwell’s equations, 1905 Poincare and Einstein independently found the Lorentz transformation which is the property of Maxwell equation. The study of cathode ray has led to the discovery of electrons. The electron orbits are bending around when a magnet was brought near it. By imagining the motion of electron near a tip of a very long solenoid, Poincare introduced a magnetic monopole around which the magnetic field comes out radially. B = gr/r3 1. Consider the motion of a charged particle with equation of motion, m d2r/dt2 = e v x B Find the conserved energy E and the explicit form of the conserved angular momentum J=mr x dr/dt+.… 2. Find the orbit of the charged particle. 3. Consider the motion of two magnetic monopoles appearing in the 4-dim field theory. Magnetic monopoles are characterized by their positions and internal phase angle. The Lagrangian for the relative position r and phase ψ is given as below. where ψ ~ ψ+2π and ∇xw(r)= -r/r3 , and r0 and a are constant positive parameters.. µ r r 1 1 a2 L = 1+ 0 r˙ 2 + r2 1+ 0 − (ψ˙ + w(r) r˙)2 + 0 2 r0 2 r r · 2µr0 1+ r Calling the conserved charge q under the shift symmetry of ψ and the conjugate momentum π of the coordinate r, find the expression for the conserved energy and angular momentum J. -
117. Magnetic Monopoles
1 117. Magnetic Monopoles 117. Magnetic Monopoles Revised August 2019 by D. Milstead (Stockholm U.) and E.J. Weinberg (Columbia U.). 117.1 Theory of magnetic monopoles The symmetry between electric and magnetic fields in the source-free Maxwell’s equations naturally suggests that electric charges might have magnetic counterparts, known as magnetic monopoles. Although the greatest interest has been in the supermassive monopoles that are a firm prediction of all grand unified theories, one cannot exclude the possibility of lighter monopoles. In either case, the magnetic charge is constrained by a quantization condition first found by Dirac [1]. Consider a monopole with magnetic charge QM and a Coulomb magnetic field Q ˆr B = M . (117.1) 4π r2 Any vector potential A whose curl is equal to B must be singular along some line running from the origin to spatial infinity. This Dirac string singularity could potentially be detected through the extra phase that the wavefunction of a particle with electric charge QE would acquire if it moved along a loop encircling the string. For the string to be unobservable, this phase must be a multiple of 2π. Requiring that this be the case for any pair of electric and magnetic charges gives min min the condition that all charges be integer multiples of minimum charges QE and QM obeying min min QE QM = 2π . (117.2) (For monopoles which also carry an electric charge, called dyons [2], the quantization conditions on their electric charges can be modified. However, the constraints on magnetic charges, as well as those on all purely electric particles, will be unchanged.) Another way to understand this result is to note that the conserved orbital angular momentum of a point electric charge moving in the field of a magnetic monopole has an additional component, with L = mr × v − 4πQEQM ˆr (117.3) Requiring the radial component of L to be quantized in half-integer units yields Eq. -
Continuous Gravitational Waves and Magnetic Monopole Signatures from Single Neutron Stars
PHYSICAL REVIEW D 101, 075028 (2020) Continuous gravitational waves and magnetic monopole signatures from single neutron stars † ‡ P. V. S. Pavan Chandra,1,* Mrunal Korwar,2, and Arun M. Thalapillil 1, 1Indian Institute of Science Education and Research, Homi Bhabha Road, Pashan, Pune 411008, India 2Department of Physics, University of Wisconsin-Madison, Madison, Wisconsin 53706, USA (Received 2 December 2019; accepted 1 April 2020; published 15 April 2020) Future observations of continuous gravitational waves from single neutron stars, apart from their monumental astrophysical significance, could also shed light on fundamental physics and exotic particle states. One such avenue is based on the fact that magnetic fields cause deformations of a neutron star, which results in a magnetic-field-induced quadrupole ellipticity. If the magnetic and rotation axes are different, this quadrupole ellipticity may generate continuous gravitational waves which may last decades, and may be observable in current or future detectors. Light, milli-magnetic monopoles, if they exist, could be pair-produced nonperturbatively in the extreme magnetic fields of neutron stars, such as magnetars. This nonperturbative production furnishes a new, direct dissipative mechanism for the neutron star magnetic fields. Through their consequent effect on the magnetic-field-induced quadrupole ellipticity, they may then potentially leave imprints in the early stage continuous gravitational wave emissions. We speculate on this possibility in the present study, by considering some of the relevant physics and taking a very simplified toy model of a magnetar as the prototypical system. Preliminary indications are that new- born millisecond magnetars could be promising candidates to look for such imprints. -
Measurement of Neutrino's Magnetic Monopole Charge, Vacuum Energy and Cause of Quantum Mechanical Uncertainty
Measurement of Neutrino's Magnetic Monopole Charge, Vacuum Energy and Cause of Quantum Mechanical Uncertainty Eue Jin Jeong ( [email protected] ) Tachyonics Research Institute Dennis Edmondson Columbia College, Marysville, Washington Research Article Keywords: fundamental physics, elementary particle physics, electricity and magnetism, experimental physics Posted Date: October 9th, 2020 DOI: https://doi.org/10.21203/rs.3.rs-88897/v1 License: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License Measurement of Neutrino's Magnetic Monopole Charge, Vacuum Energy and Cause of Quantum Mechanical Uncertainty Abstract Charge conservation in the theory of elementary particle physics is one of the best- established principles in physics. As such, if there are magnetic monopoles in the universe, the magnetic charge will most likely be a conserved quantity like electric charges. If neutrinos are magnetic monopoles, as physicists have speculated the possibility, then neutrons must also have a magnetic monopole charge, and the Earth should show signs of having a magnetic monopole charge on a macroscopic scale. To test this hypothesis, experiments were performed to detect the magnetic monopole's effect near the equator by measuring the Earth's radial magnetic force using two balanced high strength neodymium rods magnets that successfully identified the magnetic monopole charge. From this observation, we conclude that at least the electron neutrino which is a byproduct of weak decay of the neutron must be magnetic monopole. We present mathematical expressions for the vacuum electric field based on the findings and discuss various physical consequences related to the symmetry in Maxwell's equations, the origin of quantum mechanical uncertainty, the medium for electromagnetic wave propagation in space, and the logistic distribution of the massive number of magnetic monopoles in the universe. -
Particle & Nuclear Physics Quantum Field Theory
Particle & Nuclear Physics Quantum Field Theory NOW AVAILABLE New Books & Highlights in 2019-2020 ON WORLDSCINET World Scientific Lecture Notes in Physics - Vol 83 Lectures of Sidney Coleman on Quantum Field Field Theory Theory A Path Integral Approach Foreword by David Kaiser 3rd Edition edited by Bryan Gin-ge Chen (Leiden University, Netherlands), David by Ashok Das (University of Rochester, USA & Institute of Physics, Derbes (University of Chicago, USA), David Griffiths (Reed College, Bhubaneswar, India) USA), Brian Hill (Saint Mary’s College of California, USA), Richard Sohn (Kronos, Inc., Lowell, USA) & Yuan-Sen Ting (Harvard University, “This book is well-written and very readable. The book is a self-consistent USA) introduction to the path integral formalism and no prior knowledge of it is required, although the reader should be familiar with quantum “Sidney Coleman was the master teacher of quantum field theory. All of mechanics. This book is an excellent guide for the reader who wants a us who knew him became his students and disciples. Sidney’s legendary good and detailed introduction to the path integral and most of its important course remains fresh and bracing, because he chose his topics with a sure application in physics. I especially recommend it for graduate students in feel for the essential, and treated them with elegant economy.” theoretical physics and for researchers who want to be introduced to the Frank Wilczek powerful path integral methods.” Nobel Laureate in Physics 2004 Mathematical Reviews 1196pp Dec 2018 -
Lectures on D-Branes
CPHT/CL-615-0698 hep-th/9806199 Lectures on D-branes Constantin P. Bachas1 Centre de Physique Th´eorique, Ecole Polytechnique 91128 Palaiseau, FRANCE [email protected] ABSTRACT This is an introduction to the physics of D-branes. Topics cov- ered include Polchinski’s original calculation, a critical assessment of some duality checks, D-brane scattering, and effective worldvol- ume actions. Based on lectures given in 1997 at the Isaac Newton Institute, Cambridge, at the Trieste Spring School on String The- ory, and at the 31rst International Symposium Ahrenshoop in Buckow. arXiv:hep-th/9806199v2 17 Jan 1999 June 1998 1Address after Sept. 1: Laboratoire de Physique Th´eorique, Ecole Normale Sup´erieure, 24 rue Lhomond, 75231 Paris, FRANCE, email : [email protected] Lectures on D-branes Constantin Bachas 1 Foreword Referring in his ‘Republic’ to stereography – the study of solid forms – Plato was saying : ... for even now, neglected and curtailed as it is, not only by the many but even by professed students, who can suggest no use for it, never- theless in the face of all these obstacles it makes progress on account of its elegance, and it would not be astonishing if it were unravelled. 2 Two and a half millenia later, much of this could have been said for string theory. The subject has progressed over the years by leaps and bounds, despite periods of neglect and (understandable) criticism for lack of direct experimental in- put. To be sure, the construction and key ingredients of the theory – gravity, gauge invariance, chirality – have a firm empirical basis, yet what has often catalyzed progress is the power and elegance of the underlying ideas, which look (at least a posteriori) inevitable. -
Scientific Report for the Year 2000
The Erwin Schr¨odinger International Boltzmanngasse 9 ESI Institute for Mathematical Physics A-1090 Wien, Austria Scientific Report for the Year 2000 Vienna, ESI-Report 2000 March 1, 2001 Supported by Federal Ministry of Education, Science, and Culture, Austria ESI–Report 2000 ERWIN SCHRODINGER¨ INTERNATIONAL INSTITUTE OF MATHEMATICAL PHYSICS, SCIENTIFIC REPORT FOR THE YEAR 2000 ESI, Boltzmanngasse 9, A-1090 Wien, Austria March 1, 2001 Honorary President: Walter Thirring, Tel. +43-1-4277-51516. President: Jakob Yngvason: +43-1-4277-51506. [email protected] Director: Peter W. Michor: +43-1-3172047-16. [email protected] Director: Klaus Schmidt: +43-1-3172047-14. [email protected] Administration: Ulrike Fischer, Eva Kissler, Ursula Sagmeister: +43-1-3172047-12, [email protected] Computer group: Andreas Cap, Gerald Teschl, Hermann Schichl. International Scientific Advisory board: Jean-Pierre Bourguignon (IHES), Giovanni Gallavotti (Roma), Krzysztof Gawedzki (IHES), Vaughan F.R. Jones (Berkeley), Viktor Kac (MIT), Elliott Lieb (Princeton), Harald Grosse (Vienna), Harald Niederreiter (Vienna), ESI preprints are available via ‘anonymous ftp’ or ‘gopher’: FTP.ESI.AC.AT and via the URL: http://www.esi.ac.at. Table of contents General remarks . 2 Winter School in Geometry and Physics . 2 Wolfgang Pauli und die Physik des 20. Jahrhunderts . 3 Summer Session Seminar Sophus Lie . 3 PROGRAMS IN 2000 . 4 Duality, String Theory, and M-theory . 4 Confinement . 5 Representation theory . 7 Algebraic Groups, Invariant Theory, and Applications . 7 Quantum Measurement and Information . 9 CONTINUATION OF PROGRAMS FROM 1999 and earlier . 10 List of Preprints in 2000 . 13 List of seminars and colloquia outside of conferences . -
David Olive: His Life and Work
David Olive his life and work Edward Corrigan Department of Mathematics, University of York, YO10 5DD, UK Peter Goddard Institute for Advanced Study, Princeton, NJ 08540, USA St John's College, Cambridge, CB2 1TP, UK Abstract David Olive, who died in Barton, Cambridgeshire, on 7 November 2012, aged 75, was a theoretical physicist who made seminal contributions to the development of string theory and to our understanding of the structure of quantum field theory. In early work on S-matrix theory, he helped to provide the conceptual framework within which string theory was initially formulated. His work, with Gliozzi and Scherk, on supersymmetry in string theory made possible the whole idea of superstrings, now understood as the natural framework for string theory. Olive's pioneering insights about the duality between electric and magnetic objects in gauge theories were way ahead of their time; it took two decades before his bold and courageous duality conjectures began to be understood. Although somewhat quiet and reserved, he took delight in the company of others, generously sharing his emerging understanding of new ideas with students and colleagues. He was widely influential, not only through the depth and vision of his original work, but also because the clarity, simplicity and elegance of his expositions of new and difficult ideas and theories provided routes into emerging areas of research, both for students and for the theoretical physics community more generally. arXiv:2009.05849v1 [physics.hist-ph] 12 Sep 2020 [A version of section I Biography is to be published in the Biographical Memoirs of Fellows of the Royal Society.] I Biography Childhood David Olive was born on 16 April, 1937, somewhat prematurely, in a nursing home in Staines, near the family home in Scotts Avenue, Sunbury-on-Thames, Surrey.