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Summer 2018 Astron 9 Week 2 FINAL
ORDER OF MAGNITUDE PHYSICS RICHARD ANANTUA, JEFFREY FUNG AND JING LUAN WEEK 2: FUNDAMENTAL INTERACTIONS, NUCLEAR AND ATOMIC PHYSICS REVIEW OF BASICS • Units • Systems include SI and cgs • Dimensional analysis must confirm units on both sides of an equation match • BUCKINGHAM’S PI THEOREM - For a physical equation involving N variables, if there are R independent dimensions, then there are N-R independent dimensionless groups, denoted Π", …, Π%&'. UNITS REVIEW – BASE UNITS • Physical quantities may be expressed using several choices of units • Unit systems express physical quantities in terms of base units or combinations thereof Quantity SI (mks) Gaussian (cgs) Imperial Length Meter (m) Centimeter (cm) Foot (ft) Mass Kilogram (kg) Gram (g) Pound (lb) Time Second (s) Second (s) Second (s) Temperature Kelvin (K) Kelvin (K)* Farenheit (ºF) Luminous intensity Candela (cd) Candela (cd)* Amount Mole (mol) Mole (mol)* Current Ampere (A) * Sometimes not considered a base cgs unit REVIEW – DERIVED UNITS • Units may be derived from others Quantity SI cgs Momentum kg m s-1 g cm s-1 Force Newton N=kg m s-2 dyne dyn=g cm s-2 Energy Joule J=kg m2 s-2 erg=g cm2 s-2 Power Watt J=kg m2 s-3 erg/s=g cm2 s-3 Pressure Pascal Pa=kg m-1 s-2 barye Ba=g cm-1 s-2 • Some unit systems differ in which units are considered fundamental Electrostatic Units SI (mks) Gaussian cgs Charge A s (cm3 g s-2)1/2 Current A (cm3 g s-4)1/2 REVIEW – UNITS • The cgs system for electrostatics is based on the assumptions kE=1, kM =2kE/c2 • EXERCISE: Given the Gaussian cgs unit of force is g cm s-2, what is the electrostatic unit of charge? # 2 ! = ⟹ # = ! & 2 )/+ = g cm/ s1+ )/+ [&]2 REVIEW – BUCKINGHAM’S PI THEOREM • BUCKINGHAM’S PI THEOREM - For a physical equation involving N variables, if there are R independent dimensions, then there are N-R independent dimensionless groups, denoted Π", …, Π%&'. -
PHOTONICS and PLASMONICS SEMINAR – SPRING 2011 Unit Value: 1 Instructor: Prof
EE298‐5 PHOTONICS AND PLASMONICS SEMINAR – SPRING 2011 unit value: 1 instructor: Prof. Ivan Kaminow, [email protected] coordinator: Lea Barker, [email protected] class time: FRIDAYS, 11:00AM ‐ 12:30, 521 CORY HALL pre‐requisite: An interest in Photonics and/or Plasmonics. May be taken for credit and/or fun. website: http://inst.eecs.berkeley.edu/~ee298‐5/sp11/ plasmonics list: [email protected] This course is intended to give students at the advanced undergraduate or graduate level, and researchers, insight into current research based on a series of invited talks. SCHEDULE: 1/21 ‐ Prof. REUVEN GORDON, U. Victoria, Canada, “Challenging the Limits of Diffraction” Abstract: This talk will show ways of challenging three limits of optical diffraction. First, it will be shown how to focus light below the Abbe diffraction limit [1]. Next it will be shown how to squeeze light through small holes in a metal screen, allowing for 100% transmission in some cases, in contrast to Betheʹs aperture theory as found in textbooks [2,3]. This has interesting applications for biosensors. Finally, it will be shown how to optically trap nanoparticles with powers orders of magnitude smaller than required by conventional by Rayleigh scattering formulations [4], which has interesting applications for manipulating viruses and quantum dots. Theoretical and experimental results will be presented. (1) R. Gordon, ʺProposal for superfocusing at visible wavelengths using radiationless interference of a plasmonic array,ʺ Physical Review Letters, 102, 207402 (2009). (2) R. Gordon, A. G. Brolo, A. McKinnon, A. Rajora, B. Leathem, and K. L. Kavanagh, ʺStrong polarization in the optical transmission through elliptical nanohole arraysʺ Physical Review Letters, 92, 037401, (2004). -
Physical Review Journals Catalog 2021
2021 PHYSICAL REVIEW JOURNALS CATALOG PUBLISHED BY THE AMERICAN PHYSICAL SOCIETY Physical Review Journals 2021 1 © 2020 American Physical Society 2 Physical Review Journals 2021 Table of Contents Founded in 1899, the American Physical Society (APS) strives to advance and diffuse the knowledge of physics. In support of this objective, APS publishes primary research and review journals, five of which are open access. Physical Review Letters..............................................................................................................2 Physical Review X .......................................................................................................................3 PRX Quantum .............................................................................................................................4 Reviews of Modern Physics ......................................................................................................5 Physical Review A .......................................................................................................................6 Physical Review B ......................................................................................................................7 Physical Review C.......................................................................................................................8 Physical Review D ......................................................................................................................9 Physical Review E ................................................................................................................... -
Radiation Forces on Small Particles in the Solar System T
1CARUS 40, 1-48 (1979) Radiation Forces on Small Particles in the Solar System t JOSEPH A. BURNS Cornell University, 2 Ithaca, New York 14853 and NASA-Ames Research Center PHILIPPE L. LAMY CNRS-LAS, Marseille, France 13012 AND STEVEN SOTER Cornell University, Ithaca, New York 14853 Received May 12, 1978; revised May 2, 1979 We present a new and more accurate expression for the radiation pressure and Poynting- Robertson drag forces; it is more complete than previous ones, which considered only perfectly absorbing particles or artificial scattering laws. Using a simple heuristic derivation, the equation of motion for a particle of mass m and geometrical cross section A, moving with velocity v through a radiation field of energy flux density S, is found to be (to terms of order v/c) mi, = (SA/c)Qpr[(1 - i'/c)S - v/c], where S is a unit vector in the direction of the incident radiation,/" is the particle's radial velocity, and c is the speed of light; the radiation pressure efficiency factor Qpr ~ Qabs + Q~a(l - (cos a)), where Qabs and Q~c~ are the efficiency factors for absorption and scattering, and (cos a) accounts for the asymmetry of the scattered radiation. This result is confirmed by a new formal derivation applying special relativistic transformations for the incoming and outgoing energy and momentum as seen in the particle and solar frames of reference. Qpr is evaluated from Mie theory for small spherical particles with measured optical properties, irradiated by the actual solar spectrum. Of the eight materials studied, only for iron, magnetite, and graphite grains does the radiation pressure force exceed gravity and then just for sizes around 0. -
Introduction to Copyright and Licensing in an Open Access Environment
IOP publications Frequently asked questions Glossary Frequently asked questions Creative Commons Moral rights Creative Commons Assignment Open access Dealing with copyright works Introduction to copyright copyright.iop.org Introduction to Introduction open access environment access open copyright and licensing in an in licensing and copyright Introduction to copyright to Introduction works copyright with Dealing access Open Assignment Commons Creative Commons Creative questions asked Frequently Glossary questions asked Frequently publications IOP Moral rights rights Moral What is copyright? As soon as an idea is expressed in a physical medium, such as writing a paper, it qualifies for copyright protection. Copyright is a legal right that gives the copyright holder exclusive rights over how others use their work. The level and type of protection offered by copyright varies between countries. A form of intellectual property, copyright can be dealt with like other types of property – it can be acquired, disposed of or licensed. Copyright is time-limited. The period of protection varies, but in most countries a journal article created at the present time will be protected for between 50 and 70 years from the death of the last surviving author. By means of a number of local and international laws and conventions, copyright which arises in one country is recognised and protected in many others. Treatment of copyright in the digital environment is evolving at an unprecedented rate. Copyright exists to protect the rights of an owner of an original piece of work by imposing restrictions on reuse but it does not always fit well with how we use and share information in the digital sphere. -
Architecture and Literature in Victorian Britain by Benjamin Zenas Cannon Doctor of Philosophy in English University of California, Berkeley Prof
Disappearing Walls: Architecture and Literature in Victorian Britain By Benjamin Zenas Cannon A dissertation submitted in partial satisfaction of the requirements for the degree of Doctor of Philosophy in English in the Graduate Division of the University of California, Berkeley Committee in Charge: Professor Ian Duncan, Chair Professor Kent Puckett Professor Andrew Shanken Spring 2014 Disappearing Walls: Literature and Architecture in Victorian Britain © 2014 By Benjamin Zenas Cannon Abstract Disappearing Walls: Architecture and Literature in Victorian Britain By Benjamin Zenas Cannon Doctor of Philosophy in English University of California, Berkeley Prof. Ian Duncan, Chair From Discipline and Punish and The Madwoman in the Attic to recent work on urbanism, display, and material culture, criticism has regularly cast nineteenth-century architecture not as a set of buildings but as an ideological metastructure. Seen primarily in terms of prisons, museums, and the newly gendered private home, this “grid of intelligibility” polices the boundaries not only of physical interaction but also of cultural values and modes of knowing. As my project argues, however, architecture in fact offered nineteenth-century theorists unique opportunities to broaden radically the parameters of aesthetic agency. A building is generally not built by a single person; it is almost always a corporate effort. At the same time, a building will often exist for long enough that it will decay or be repurposed. Long before literature asked “what is an author?” Victorian architecture theory asked: “who can be said to have made this?” Figures like John Ruskin, Owen Jones, and James Fergusson radicalize this question into what I call a redistribution of intention, an ethically charged recognition of the value of other makers. -
Electric Units and Standards
DEPARTMENT OF COMMERCE OF THE Bureau of Standards S. W. STRATTON, Director No. 60 ELECTRIC UNITS AND STANDARDS list Edition 1 Issued September 25. 1916 WASHINGTON GOVERNMENT PRINTING OFFICE DEPARTMENT OF COMMERCE Circular OF THE Bureau of Standards S. W. STRATTON, Director No. 60 ELECTRIC UNITS AND STANDARDS [1st Edition] Issued September 25, 1916 WASHINGTON GOVERNMENT PRINTING OFFICE 1916 ADDITIONAL COPIES OF THIS PUBLICATION MAY BE PROCURED FROM THE SUPERINTENDENT OF DOCUMENTS GOVERNMENT PRINTING OFFICE WASHINGTON, D. C. AT 15 CENTS PER COPY A complete list of the Bureau’s publications may be obtained free of charge on application to the Bureau of Standards, Washington, D. C. ELECTRIC UNITS AND STANDARDS CONTENTS Page I. The systems of units 4 1. Units and standards in general 4 2. The electrostatic and electromagnetic systems 8 () The numerically different systems of units 12 () Gaussian systems, and ratios of the units 13 “ ’ (c) Practical ’ electromagnetic units 15 3. The international electric units 16 II. Evolution of present system of concrete standards 18 1. Early electric standards 18 2. Basis of present laws 22 3. Progress since 1893 24 III. Units and standards of the principal electric quantities 29 1. Resistance 29 () International ohm 29 Definition 29 Mercury standards 30 Secondary standards 31 () Resistance standards in practice 31 (c) Absolute ohm 32 2. Current 33 (a) International ampere 33 Definition 34 The silver voltameter 35 ( b ) Resistance standards used in current measurement 36 (c) Absolute ampere 37 3. Electromotive force 38 (a) International volt 38 Definition 39 Weston normal cell 39 (b) Portable Weston cells 41 (c) Absolute and semiabsolute volt 42 4. -
Planetary Defence Activities Beyond NASA and ESA
Planetary Defence Activities Beyond NASA and ESA Brent W. Barbee 1. Introduction The collision of a significant asteroid or comet with Earth represents a singular natural disaster for a myriad of reasons, including: its extraterrestrial origin; the fact that it is perhaps the only natural disaster that is preventable in many cases, given sufficient preparation and warning; its scope, which ranges from damaging a city to an extinction-level event; and the duality of asteroids and comets themselves---they are grave potential threats, but are also tantalising scientific clues to our ancient past and resources with which we may one day build a prosperous spacefaring future. Accordingly, the problems of developing the means to interact with asteroids and comets for purposes of defence, scientific study, exploration, and resource utilisation have grown in importance over the past several decades. Since the 1980s, more and more asteroids and comets (especially the former) have been discovered, radically changing our picture of the solar system. At the beginning of the year 1980, approximately 9,000 asteroids were known to exist. By the beginning of 2001, that number had risen to approximately 125,000 thanks to the Earth-based telescopic survey efforts of the era, particularly the emergence of modern automated telescopic search systems, pioneered by the Massachusetts Institute of Technology’s (MIT’s) LINEAR system in the mid-to-late 1990s.1 Today, in late 2019, about 840,000 asteroids have been discovered,2 with more and more being found every week, month, and year. Of those, approximately 21,400 are categorised as near-Earth asteroids (NEAs), 2,000 of which are categorised as Potentially Hazardous Asteroids (PHAs)3 and 2,749 of which are categorised as potentially accessible.4 The hazards posed to us by asteroids affect people everywhere around the world. -
From Big Data to Econophysics and Its Use to Explain Complex Phenomena
Journal of Risk and Financial Management Review From Big Data to Econophysics and Its Use to Explain Complex Phenomena Paulo Ferreira 1,2,3,* , Éder J.A.L. Pereira 4,5 and Hernane B.B. Pereira 4,6 1 VALORIZA—Research Center for Endogenous Resource Valorization, 7300-555 Portalegre, Portugal 2 Department of Economic Sciences and Organizations, Instituto Politécnico de Portalegre, 7300-555 Portalegre, Portugal 3 Centro de Estudos e Formação Avançada em Gestão e Economia, Instituto de Investigação e Formação Avançada, Universidade de Évora, Largo dos Colegiais 2, 7000 Évora, Portugal 4 Programa de Modelagem Computacional, SENAI Cimatec, Av. Orlando Gomes 1845, 41 650-010 Salvador, BA, Brazil; [email protected] (É.J.A.L.P.); [email protected] (H.B.B.P.) 5 Instituto Federal do Maranhão, 65075-441 São Luís-MA, Brazil 6 Universidade do Estado da Bahia, 41 150-000 Salvador, BA, Brazil * Correspondence: [email protected] Received: 5 June 2020; Accepted: 10 July 2020; Published: 13 July 2020 Abstract: Big data has become a very frequent research topic, due to the increase in data availability. In this introductory paper, we make the linkage between the use of big data and Econophysics, a research field which uses a large amount of data and deals with complex systems. Different approaches such as power laws and complex networks are discussed, as possible frameworks to analyze complex phenomena that could be studied using Econophysics and resorting to big data. Keywords: big data; complexity; networks; stock markets; power laws 1. Introduction Big data has become a very popular expression in recent years, related to the advance of technology which allows, on the one hand, the recovery of a great amount of data, and on the other hand, the analysis of that data, benefiting from the increasing computational capacity of devices. -
Machine Learning for Condensed Matter Physics
Review Article Machine Learning for Condensed Matter Physics Edwin A. Bedolla-Montiel1, Luis Carlos Padierna1 and Ram´on Casta~neda-Priego1 1 Divisi´onde Ciencias e Ingenier´ıas,Universidad de Guanajuato, Loma del Bosque 103, 37150 Le´on,Mexico E-mail: [email protected] Abstract. Condensed Matter Physics (CMP) seeks to understand the microscopic interactions of matter at the quantum and atomistic levels, and describes how these interactions result in both mesoscopic and macroscopic properties. CMP overlaps with many other important branches of science, such as Chemistry, Materials Science, Statistical Physics, and High-Performance Computing. With the advancements in modern Machine Learning (ML) technology, a keen interest in applying these algorithms to further CMP research has created a compelling new area of research at the intersection of both fields. In this review, we aim to explore the main areas within CMP, which have successfully applied ML techniques to further research, such as the description and use of ML schemes for potential energy surfaces, the characterization of topological phases of matter in lattice systems, the prediction of phase transitions in off-lattice and atomistic simulations, the interpretation of ML theories with physics- inspired frameworks and the enhancement of simulation methods with ML algorithms. We also discuss in detial the main challenges and drawbacks of using ML methods on CMP problems, as well as some perspectives for future developments. Keywords: machine learning, condensed matter physics Submitted -
Guide for the Use of the International System of Units (SI)
Guide for the Use of the International System of Units (SI) m kg s cd SI mol K A NIST Special Publication 811 2008 Edition Ambler Thompson and Barry N. Taylor NIST Special Publication 811 2008 Edition Guide for the Use of the International System of Units (SI) Ambler Thompson Technology Services and Barry N. Taylor Physics Laboratory National Institute of Standards and Technology Gaithersburg, MD 20899 (Supersedes NIST Special Publication 811, 1995 Edition, April 1995) March 2008 U.S. Department of Commerce Carlos M. Gutierrez, Secretary National Institute of Standards and Technology James M. Turner, Acting Director National Institute of Standards and Technology Special Publication 811, 2008 Edition (Supersedes NIST Special Publication 811, April 1995 Edition) Natl. Inst. Stand. Technol. Spec. Publ. 811, 2008 Ed., 85 pages (March 2008; 2nd printing November 2008) CODEN: NSPUE3 Note on 2nd printing: This 2nd printing dated November 2008 of NIST SP811 corrects a number of minor typographical errors present in the 1st printing dated March 2008. Guide for the Use of the International System of Units (SI) Preface The International System of Units, universally abbreviated SI (from the French Le Système International d’Unités), is the modern metric system of measurement. Long the dominant measurement system used in science, the SI is becoming the dominant measurement system used in international commerce. The Omnibus Trade and Competitiveness Act of August 1988 [Public Law (PL) 100-418] changed the name of the National Bureau of Standards (NBS) to the National Institute of Standards and Technology (NIST) and gave to NIST the added task of helping U.S. -
Disappearing Walls: Architecture and Literature in Victorian Britain by Benjamin Zenas Cannon a Dissertation Submitted in Partia
Disappearing Walls: Architecture and Literature in Victorian Britain By Benjamin Zenas Cannon A dissertation submitted in partial satisfaction of the requirements for the degree of Doctor of Philosophy in English in the Graduate Division of the University of California, Berkeley Committee in Charge: Professor Ian Duncan, Chair Professor Kent Puckett Professor Andrew Shanken Spring 2014 Disappearing Walls: Literature and Architecture in Victorian Britain © 2014 By Benjamin Zenas Cannon Abstract Disappearing Walls: Architecture and Literature in Victorian Britain By Benjamin Zenas Cannon Doctor of Philosophy in English University of California, Berkeley Prof. Ian Duncan, Chair From Discipline and Punish and The Madwoman in the Attic to recent work on urbanism, display, and material culture, criticism has regularly cast nineteenth-century architecture not as a set of buildings but as an ideological metastructure. Seen primarily in terms of prisons, museums, and the newly gendered private home, this “grid of intelligibility” polices the boundaries not only of physical interaction but also of cultural values and modes of knowing. As my project argues, however, architecture in fact offered nineteenth-century theorists unique opportunities to broaden radically the parameters of aesthetic agency. A building is generally not built by a single person; it is almost always a corporate effort. At the same time, a building will often exist for long enough that it will decay or be repurposed. Long before literature asked “what is an author?” Victorian architecture theory asked: “who can be said to have made this?” Figures like John Ruskin, Owen Jones, and James Fergusson radicalize this question into what I call a redistribution of intention, an ethically charged recognition of the value of other makers.