Letter of Intent: Antimatter Gravity Experiment (AGE) at Fermilab
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Active Galactic Nuclei: a Brief Introduction
Active Galactic Nuclei: a brief introduction Manel Errando Washington University in St. Louis The discovery of quasars 3C 273: The first AGN z=0.158 2 <latexit sha1_base64="4D0JDPO4VKf1BWj0/SwyHGTHSAM=">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</latexit> <latexit sha1_base64="H7Rv+ZHksM7/70841dw/vasasCQ=">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</latexit> The power source of quasars • The luminosity (L) of quasars, i.e. how bright they are, can be as high as Lquasar ~ 1012 Lsun ~ 1040 W. • The energy source of quasars is accretion power: - Nuclear fusion: 2 11 1 ∆E =0.007 mc =6 10 W s g− -
The Cherenkov Telescope Array Observatory Comes of Age
The Organisation DOI: 10.18727/0722-6691/5194 The Cherenkov Telescope Array Observatory Comes of Age Federico Ferrini 1 Conceived around a decade ago by a the detection of a clear signal from Wolfgang Wild 1, 2 group of scientists, we are now on the the Crab nebula above 1 TeV with the cusp of constructing the largest observa- Whipple 10-m imaging atmospheric tory to study the gamma-ray Universe. Cherenkov telescope (IACT). Since then, 1 CTAO, Heidelberg (DE) and Bologna (IT) Here we present a short look back at the the instrumentation for, and techniques 2 ESO evolution and recent matu ration of the of, astronomy with IACTs have evolved CTA project, as well as an outline of our to the extent that a flourishing new scien- expectations for the near future. A com- tific discipline has been established, with The Cherenkov Telescope Array (CTA) is prehensive introduction to CTA, including the detection of more than 150 sources the next-generation ground-based the detection technique, its history, the and a major impact in astrophysics — observatory for gamma-ray astronomy extraordinary improvements with respect and, more widely, in physics. The current at very high energies. With up to 120 to previous experimental facilities, and the major arrays of IACTs (the High Energy telescopes on two sites, CTA will be the scientific objectives has been provided by Stereoscopic System [H.E.S.S.], the world’s largest and most sensitive Werner Hofmann, Spokesperson of the Major Atmospheric Gamma Imaging high-energy gamma-ray observatory CTA Consortium (Hofmann, 2017). Cherenkov Telescope [MAGIC], and the covering the entire sky. -
4. Particle Generators/Accelerators
Joint innovative training and teaching/ learning program in enhancing development and transfer knowledge of application of ionizing radiation in materials processing 4. Particle Generators/Accelerators Diana Adlienė Department of Physics Kaunas University of Technolog y Joint innovative training and teaching/ learning program in enhancing development and transfer knowledge of application of ionizing radiation in materials processing This project has been funded with support from the European Commission. This publication reflects the views only of the author. Polish National Agency and the Commission cannot be held responsible for any use which may be made of the information contained therein. Date: Oct. 2017 DISCLAIMER This presentation contains some information addapted from open access education and training materials provided by IAEA TABLE OF CONTENTS 1. Introduction 2. X-ray machines 3. Particle generators/accelerators 4. Types of industrial irradiators The best accelerator in the universe… INTRODUCTION • Naturally occurring radioactive sources: – Up to 5 MeV Alpha’s (helium nuclei) – Up to 3 MeV Beta particles (electrons) • Natural sources are difficult to maintain, their applications are limited: – Chemical processing: purity, messy, and expensive; – Low intensity; – Poor geometry; – Uncontrolled energies, usually very broad Artificial sources (beams) are requested! INTRODUCTION • Beams of accelerated particles can be used to produce beams of secondary particles: Photons (x-rays, gamma-rays, visible light) are generated from beams -
MAGIC Observations of the Diffuse Γ-Ray Emission in the Vicinity of the Galactic Center? MAGIC Collaboration: V
A&A 642, A190 (2020) Astronomy https://doi.org/10.1051/0004-6361/201936896 & c MAGIC Collaboration 2020 Astrophysics MAGIC observations of the diffuse γ-ray emission in the vicinity of the Galactic center? MAGIC Collaboration: V. A. Acciari1,2, S. Ansoldi3,24, L. A. Antonelli4, A. Arbet Engels5, D. Baack6, A. Babic´7, B. Banerjee8, U. Barres de Almeida9, J. A. Barrio10, J. Becerra González1,2, W. Bednarek11, L. Bellizzi12, E. Bernardini13,17, A. Berti14, J. Besenrieder15, W. Bhattacharyya13, C. Bigongiari4, A. Biland5, O. Blanch16, G. Bonnoli12, Ž. Bošnjak7, G. Busetto17, R. Carosi18, G. Ceribella15, Y. Chai15, A. Chilingaryan19, S. Cikota7, S. M. Colak16, U. Colin15, E. Colombo1,2, J. L. Contreras10, J. Cortina20, S. Covino4, V. D’Elia4, P. Da Vela18, F. Dazzi4, A. De Angelis17, B. De Lotto3, M. Delfino16,27, J. Delgado16,27, D. Depaoli14, F. Di Pierro14, L. Di Venere14, E. Do Souto Espiñeira16, D. Dominis Prester7, A. Donini3, D. Dorner21, M. Doro17, D. Elsaesser6, V. Fallah Ramazani22, A. Fattorini6, A. Fernández-Barral17, G. Ferrara4, D. Fidalgo10, L. Foffano17, M. V. Fonseca10, L. Font23, C. Fruck15;??, S. Fukami24, R. J. García López1,2, M. Garczarczyk13, S. Gasparyan19, M. Gaug23, N. Giglietto14, F. Giordano14, N. Godinovic´7, D. Green15, D. Guberman16, D. Hadasch24, A. Hahn15, J. Herrera1,2, J. Hoang10, D. Hrupec7, M. Hütten15, T. Inada24, S. Inoue24, K. Ishio15, Y. Iwamura24;??, L. Jouvin16, D. Kerszberg16, H. Kubo24, J. Kushida24, A. Lamastra4, D. Lelas7, F. Leone4, E. Lindfors22, S. Lombardi4, F. Longo3,28, M. López10, R. López-Coto17, A. López-Oramas1,2, S. Loporchio14, B. Machado de Oliveira Fraga9, C. -
Guide to Understanding Condensation
Guide to Understanding Condensation The complete Andersen® Owner-To-Owner™ limited warranty is available at: www.andersenwindows.com. “Andersen” is a registered trademark of Andersen Corporation. All other marks where denoted are marks of Andersen Corporation. © 2007 Andersen Corporation. All rights reserved. 7/07 INTRODUCTION 2 The moisture that suddenly appears in cold weather on the interior We have created this brochure to answer questions you may have or exterior of window and patio door glass can block the view, drip about condensation, indoor humidity and exterior condensation. on the floor or freeze on the glass. It can be an annoying problem. We’ll start with the basics and offer solutions and alternatives While it may seem natural to blame the windows or doors, interior along the way. condensation is really an indication of excess humidity in the home. Exterior condensation, on the other hand, is a form of dew — the Should you run into problems or situations not covered in the glass simply provides a surface on which the moisture can condense. following pages, please contact your Andersen retailer. The important thing to realize is that if excessive humidity is Visit the Andersen website: www.andersenwindows.com causing window condensation, it may also be causing problems elsewhere in your home. Here are some other signs of excess The Andersen customer service toll-free number: 1-888-888-7020. humidity: • A “damp feeling” in the home. • Staining or discoloration of interior surfaces. • Mold or mildew on surfaces or a “musty smell.” • Warped wooden surfaces. • Cracking, peeling or blistering interior or exterior paint. -
Antimatter Gravity and the Universe Dragan Hajdukovic
Antimatter gravity and the Universe Dragan Hajdukovic To cite this version: Dragan Hajdukovic. Antimatter gravity and the Universe. Modern Physics Letters A, World Scientific Publishing, 2019, 10.1142/S0217732320300013. hal-02106808v3 HAL Id: hal-02106808 https://hal.archives-ouvertes.fr/hal-02106808v3 Submitted on 21 Nov 2019 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. 1 Brief Review Antimatter gravity and the Universe Dragan Slavkov Hajdukovic Institute of Physics, Astrophysics and Cosmology Crnogorskih junaka 172, Cetinje, Montenegro [email protected] Abstract: The aim of this brief review is twofold. First, we give an overview of the unprecedented experimental efforts to measure the gravitational acceleration of antimatter; with antihydrogen, in three competing experiments at CERN (AEGIS, ALPHA and GBAR), and with muonium and positronium in other laboratories in the world. Second, we present the 21st Century’s attempts to develop a new model of the Universe with the assumed gravitational repulsion between matter and antimatter; so far, three radically different and incompatible theoretical paradigms have been proposed. Two of these 3 models, Dirac-Milne Cosmology (that incorporates CPT violation) and the Lattice Universe (based on CPT symmetry), assume a symmetric Universe composed of equal amounts of matter and antimatter, with antimatter somehow “hidden” in cosmic voids; this hypothesis produced encouraging preliminary results. -
Installation of the Cyclotron Based Clinical Neutron Therapy System in Seattle
Proceedings of the Tenth International Conference on Cyclotrons and their Applications, East Lansing, Michigan, USA INSTALLATION OF THE CYCLOTRON BASED CLINICAL NEUTRON THERAPY SYSTEM IN SEATTLE R. Risler, J. Eenmaa, J. Jacky, I. Kalet, and P. Wootton Medical Radiation Physics RC-08, University of Washington, Seattle ~ 98195, USA S. Lindbaeck Instrument AB Scanditronix, Uppsala, Sweden Sumnary radiation areas is via sliding shielding doors rather than a maze, mai nl y to save space. For the same reason A cyclotron facility has been built for cancer a single door is used to alternately close one or the treatment with fast neutrons. 50.5 MeV protons from a other therapy room. All power supplies and the control conventional, positive ion cyclotron are used to b0m computer are located on the second floor, above the bard a semi-thick Beryllium target located 150 am from maintenance area. The cooler room contains a heat the treatment site. Two treatment rooms are available, exchanger and other refrigeration equipment. Not shown one with a fixed horizontal beam and one with an iso in the diagram is the cooling tower located in another centric gantry capable of 360 degree rotation. In part of the building. Also not shown is the hot lab addition 33 51 MeV protons and 16.5 - 25.5 MeV now under construction an an area adjacent to the deuterons are generated for isotope production inside cyclotron vault. It will be used to process radio the cyclotron vault. The control computer is also used isotopes produced at a target station in the vault. to record and verify treatment parameters for indi vidual patients and to set up and monitor the actual radiation treatment. -
Chapter 3 Bose-Einstein Condensation of an Ideal
Chapter 3 Bose-Einstein Condensation of An Ideal Gas An ideal gas consisting of non-interacting Bose particles is a ¯ctitious system since every realistic Bose gas shows some level of particle-particle interaction. Nevertheless, such a mathematical model provides the simplest example for the realization of Bose-Einstein condensation. This simple model, ¯rst studied by A. Einstein [1], correctly describes important basic properties of actual non-ideal (interacting) Bose gas. In particular, such basic concepts as BEC critical temperature Tc (or critical particle density nc), condensate fraction N0=N and the dimensionality issue will be obtained. 3.1 The ideal Bose gas in the canonical and grand canonical ensemble Suppose an ideal gas of non-interacting particles with ¯xed particle number N is trapped in a box with a volume V and at equilibrium temperature T . We assume a particle system somehow establishes an equilibrium temperature in spite of the absence of interaction. Such a system can be characterized by the thermodynamic partition function of canonical ensemble X Z = e¡¯ER ; (3.1) R where R stands for a macroscopic state of the gas and is uniquely speci¯ed by the occupa- tion number ni of each single particle state i: fn0; n1; ¢ ¢ ¢ ¢ ¢ ¢g. ¯ = 1=kBT is a temperature parameter. Then, the total energy of a macroscopic state R is given by only the kinetic energy: X ER = "ini; (3.2) i where "i is the eigen-energy of the single particle state i and the occupation number ni satis¯es the normalization condition X N = ni: (3.3) i 1 The probability -
22 Thesis Cyclotron Design and Construction Design and Construction of a Cyclotron Capable of Accelerating Protons
22 Thesis Cyclotron Design and Construction Design and Construction of a Cyclotron Capable of Accelerating Protons to 2 MeV by Leslie Dewan Submitted to the Department of Nuclear Science and Engineering in Partial Fulfillment of the Requirements for the Degree of Bachelor of Science in Nuclear Science and Engineering at the Massachusetts Institute of Technology June 2007 © 2007 Leslie Dewan All rights reserved The author hereby grants to MIT permission to reproduce and to distribute publicly paper and electronic copies of this thesis document in whole or in part in any medium now known or hereafter created. Signature of Author: Leslie Dewan Department of Nuclear Science and Engineering May 16, 2007 Certified by: David G. Cory Professor of Nuclear Science and Engineering Thesis Supervisor Accepted by: David G. Cory Professor of Nuclear Science and Engineering Chairman, NSE Committee for Undergraduate Students Leslie Dewan 1 of 23 5/16/07 22 Thesis Cyclotron Design and Construction Design and Construction of a Cyclotron Capable of Accelerating Protons to 2 MeV by Leslie Dewan Submitted to the Department of Nuclear Science and Engineering on May 16, 2007 in Partial Fulfillment of the Requirements for the Degree of Bachelor of Science in Nuclear Science and Engineering ABSTRACT This thesis describes the design and construction of a cyclotron capable of accelerating protons to 2 MeV. A cyclotron is a charged particle accelerator that uses a magnetic field to confine particles to a spiral flight path in a vacuum chamber. An applied electrical field accelerates these particles to high energies, typically on the order of mega-electron volts. -
It's Just a Phase!
BASIS Lesson Plan Lesson Name: It’s Just a Phase! Grade Level Connection(s) NGSS Standards: Grade 2, Physical Science FOSS CA Edition: Grade 3 Physical Science: Matter and Energy Module *Note to teachers: Detailed standards connections can be found at the end of this lesson plan. Teaser/Overview Properties of matter are illustrated through a series of demonstrations and hands-on explorations. Students will learn to identify solids, liquids, and gases. Water will be used to demonstrate the three phases. Students will learn about sublimation through a fun experiment with dry ice (solid CO2). Next, they will compare the propensity of several liquids to evaporate. Finally, they will learn about freezing and melting while making ice cream. Lesson Objectives ● Students will be able to identify the three states of matter (solid, liquid, gas) based on the relative properties of those states. ● Students will understand how to describe the transition from one phase to another (melting, freezing, evaporation, condensation, sublimation) ● Students will learn that matter can change phase when heat/energy is added or removed Vocabulary Words ● Solid: A phase of matter that is characterized by a resistance to change in shape and volume. ● Liquid: A phase of matter that is characterized by a resistance to change in volume; a liquid takes the shape of its container ● Gas: A phase of matter that can change shape and volume ● Phase change: Transformation from one phase of matter to another ● Melting: Transformation from a solid to a liquid ● Freezing: Transformation -
Cyclotrons: Old but Still New
Cyclotrons: Old but Still New The history of accelerators is a history of inventions William A. Barletta Director, US Particle Accelerator School Dept. of Physics, MIT Economics Faculty, University of Ljubljana US Particle Accelerator School ~ 650 cyclotrons operating round the world Radioisotope production >$600M annually Proton beam radiation therapy ~30 machines Nuclear physics research Nuclear structure, unstable isotopes,etc High-energy physics research? DAEδALUS Cyclotrons are big business US Particle Accelerator School Cyclotrons start with the ion linac (Wiederoe) Vrf Vrf Phase shift between tubes is 180o As the ions increase their velocity, drift tubes must get longer 1 v 1 "c 1 Ldrift = = = "# rf 2 f rf 2 f rf 2 Etot = Ngap•Vrf ==> High energy implies large size US Particle Accelerator School ! To make it smaller, Let’s curl up the Wiederoe linac… Bend the drift tubes Connect equipotentials Eliminate excess Cu Supply magnetic field to bend beam 1 2# mc $ 2# mc " rev = = % = const. frf eZion B eZion B Orbits are isochronous, independent of energy ! US Particle Accelerator School … and we have Lawrence’s* cyclotron The electrodes are excited at a fixed frequency (rf-voltage source) Particles remain in resonance throughout acceleration A new bunch can be accelerated on every rf-voltage peak: ===> “continuous-wave (cw) operation” Lawrence, E.O. and Sloan, D.: Proc. Nat. Ac. Sc., 17, 64 (1931) Lawrence, E.O. & Livingstone M.S.: Phys. Rev 37, 1707 (1931). * The first cyclotron patent (German) was filed in 1929 by Leó Szilard but never published in a journal US Particle Accelerator School Synchronism only requires that τrev = N/frf “Isochronous” particles take the same revolution time for each turn. -
Capillary Condensation of Colloid–Polymer Mixtures Confined
INSTITUTE OF PHYSICS PUBLISHING JOURNAL OF PHYSICS: CONDENSED MATTER J. Phys.: Condens. Matter 15 (2003) S3411–S3420 PII: S0953-8984(03)66420-9 Capillary condensation of colloid–polymer mixtures confined between parallel plates Matthias Schmidt1,Andrea Fortini and Marjolein Dijkstra Soft Condensed Matter, Debye Institute, Utrecht University, Princetonplein 5, 3584 CC Utrecht, The Netherlands Received 21 July 2003 Published 20 November 2003 Onlineatstacks.iop.org/JPhysCM/15/S3411 Abstract We investigate the fluid–fluid demixing phase transition of the Asakura–Oosawa model colloid–polymer mixture confined between two smooth parallel hard walls using density functional theory and computer simulations. Comparing fluid density profiles for statepoints away from colloidal gas–liquid coexistence yields good agreement of the theoretical results with simulation data. Theoretical and simulation results predict consistently a shift of the demixing binodal and the critical point towards higher polymer reservoir packing fraction and towards higher colloid fugacities upon decreasing the plate separation distance. This implies capillary condensation of the colloid liquid phase, which should be experimentally observable inside slitlike micropores in contact with abulkcolloidal gas. 1. Introduction Capillary condensation denotes the phenomenon that spatial confinement can stabilize a liquid phase coexisting with its vapour in bulk [1, 2]. In order for this to happen the attractive interaction between the confining walls and the fluid particles needs to be sufficiently strong. Although the main body of work on this subject has been done in the context of confined simple liquids, one might expect that capillary condensation is particularly well suited to be studied with colloidal dispersions. In these complex fluids length scales are on the micron rather than on the ångstrom¨ scale which is typical for atomicsubstances.