Technical Activities 1982: Center for Radiation Research
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The Suitability of Smartphone Camera Sensors for Detecting Radiation Yehia H
www.nature.com/scientificreports OPEN The suitability of smartphone camera sensors for detecting radiation Yehia H. Johary1,2, Jamie Trapp2, Ali Aamry3, Hussin Aamri4, N. Tamam5 & A. Sulieman6* The advanced image sensors installed on now-ubiquitous smartphones can be used to detect ionising radiation in addition to visible light. Radiation incidents on a smartphone camera’s Complementary Metal Oxide Semiconductor (CMOS) sensor creates a signal which can be isolated from a visible light signal to turn the smartphone into a radiation detector. This work aims to report a detailed investigation of a well-reviewed smartphone application for radiation dosimetry that is available for popular smartphone devices under a calibration protocol that is typically used for the commercial calibration of radiation detectors. The iPhone 6s smartphone, which has a CMOS camera sensor, was used in this study. Black tape was utilized to block visible light. The Radioactivity counter app developed by Rolf-Dieter Klein and available on Apple’s App Store was installed on the device and tested using a calibrated radioactive source, calibration concrete pads with a range of known concentrations of radioactive elements, and in direct sunlight. The smartphone CMOS sensor is sensitive to radiation doses as low as 10 µGy/h, with a linear dose response and an angular dependence. The RadioactivityCounter app is limited in that it requires 4–10 min to ofer a stable measurement. The precision of the measurement is also afected by heat and a smartphone’s battery level. Although the smartphone is not as accurate as a conventional detector, it is useful enough to detect radiation before the radiation reaches hazardous levels. -
Matters of Gravity, a Newsletter for the Gravity Community
MATTERS OF GRAVITY Number 5 Spring 1995 Table of Contents Editorial and Correspondents ................................................... ..... 2 Gravity news: LISA Recommended to ESA as Possible New Cornerstone Mission, Peter Bender ..... 3 LIGO Project News, Stan Whitcomb ................................................ 5 Research briefs: Some Recent Work in General Relativistic Astrophysics, John Friedman............... 7 Pair Creation of Black Holes, Gary Horowitz ........................................ 10 Conformal Field Equations and Global Properties of Spacetimes, Bernd Schmidt ..... 12 Conference Reports: Aspen Workshop on Numerical Investigations of Singularities in GR, Susan Scott .... 15 Second Annual Penn State Conference: Quantum Geometry, Abhay Ashtekar ....... 17 First Samos Meeting, Spiros Cotsakis and Dieter Brill ............................... 19 Aspen Conference on Gravitational Waves and Their Detection, Syd Meshkov ........ 20 arXiv:gr-qc/9502007v1 2 Feb 1995 Editor: Jorge Pullin Center for Gravitational Physics and Geometry The Pennsylvania State University University Park, PA 16802-6300 Fax: (814)863-9608 Phone (814)863-9597 Internet: [email protected] 1 Editorial Well, I don’t have much to say, just to to remind everyone that suggestions and ideas for contributions are especially welcome. I also wish to thank the editors and contributors who made this issue possible. The next newsletter is due September 1st. If everything goes well this newsletter should be available in the gr-qc Los Alamos bul- letin board under number gr-qc/9502007. To retrieve it send email to [email protected] (or [email protected] in Europe) with Subject: get 9502007 (number 2 is available as 9309003, number 3 as 9402002 and number 4 as 9409004). All issues are available as postscript or TeX files in the WWW http://vishnu.nirvana.phys.psu.edu Or email me. -
The Charm of Theoretical Physics (1958– 1993)?
Eur. Phys. J. H 42, 611{661 (2017) DOI: 10.1140/epjh/e2017-80040-9 THE EUROPEAN PHYSICAL JOURNAL H Oral history interview The Charm of Theoretical Physics (1958{ 1993)? Luciano Maiani1 and Luisa Bonolis2,a 1 Dipartimento di Fisica and INFN, Piazzale A. Moro 5, 00185 Rome, Italy 2 Max Planck Institute for the History of Science, Boltzmannstraße 22, 14195 Berlin, Germany Received 10 July 2017 / Received in final form 7 August 2017 Published online 4 December 2017 c The Author(s) 2017. This article is published with open access at Springerlink.com Abstract. Personal recollections on theoretical particle physics in the years when the Standard Theory was formed. In the background, the remarkable development of Italian theoretical physics in the second part of the last century, with great personalities like Bruno Touschek, Raoul Gatto, Nicola Cabibbo and their schools. 1 Apprenticeship L. B. How did your interest in physics arise? You enrolled in the late 1950s, when the period of post-war reconstruction of physics in Europe was coming to an end, and Italy was entering into a phase of great expansion. Those were very exciting years. It was the beginning of the space era. L. M. The beginning of the space era certainly had a strong influence on many people, absolutely. The landing on the moon in 1969 was for sure unforgettable, but at that time I was already working in Physics and about to get married. My interest in physics started well before. The real beginning was around 1955. Most important for me was astronomy. It is not surprising that astronomy marked for many people the beginning of their interest in science. -
2007 Annual Report APS
American Physical Society APS 2007 Annual Report APS The AMERICAN PHYSICAL SOCIETY strives to: Be the leading voice for physics and an authoritative source of physics information for the advancement of physics and the benefit of humanity; Collaborate with national scientific societies for the advancement of science, science education, and the science community; Cooperate with international physics societies to promote physics, to support physicists worldwide, and to foster international collaboration; Have an active, engaged, and diverse membership, and support the activities of its units and members. Cover photos: Top: Complementary effect in flowing grains that spontaneously separate similar and well-mixed grains into two charged streams of demixed grains (Troy Shinbrot, Keirnan LaMarche and Ben Glass). Middle: Face-on view of a simulation of Weibel turbulence from intense laser-plasma interactions. (T. Haugbolle and C. Hededal, Niels Bohr Institute). Bottom: A scanning microscope image of platinum-lace nanoballs; liposomes aggregate, providing a foamlike template for a platinum sheet to grow (DOE and Sandia National Laboratories, Albuquerque, NM). Text paper is 50% sugar cane bagasse pulp, 50% recycled fiber, including 30% post consumer fiber, elemental chlorine free. Cover paper is 50% recycled, including 15% post consumer fiber, elemental chlorine free. Annual Report Design: Leanne Poteet/APS/2008 Charts: Krystal Ferguson/APS/2008 ast year, 2007, started out as a very good year for both the American Physical Society and American physics. APS’ journals and meetings showed solidly growing impact, sales, and attendance — with a good mixture Lof US and foreign contributions. In US research, especially rapid growth was seen in biophysics, optics, as- trophysics, fundamental quantum physics and several other areas. -
Special Collections of the University of Miami Libraries ASM0466 Kursunoglu, Behram Papers Container List
Special Collections of the University of Miami Libraries ASM0466 Kursunoglu, Behram Papers Container List Box Title or No. Description 1 Papers and Bound Periodicals 1967-1978 2 Videocassettes 3 Videocassettes 4 Videocassettes 5 Videocassettes 6 Videocassettes 7 Videocassettes 8 Audiocassettes 9 Documents pertaining to visiting professors A-E 10 Documents pertaining to visiting professors F-On 11 Documents pertaining to visiting professors Op-Sn 12 Documents pertaining to visiting professors St-Z The following is a list of visiting professors that are represented in the collection: * = Nobel Laureate The numbers after the names signify the number of files. *Nikolai Basov, Russian Academy of Sciences, Lebedev Institute *Hans A. Bethe, Cornell University Gregory Breit, Yale University Nikolai Bogolubov, Soviet Academy of Sciences, Moscow University * Walter H. Brattain, Columbia University Special Collections of the University of Miami Libraries ASM0466 Kursunoglu, Behram Papers Container List Box Title or No. Description Jocelyn Bell Burnell, Cambridge University H.B.G. Casimir, Phillips, Eindhoven, Netherlands Britton Chance, University of Pennsylvania *Leon Cooper, Brown University Jean Couture, Former Sec. of Energy for France *Francis H.C. Crick, Salk Institute Richard Dalitz, Oxford University *Hans G. Dehmelt, University of Washington *Max Delbruck, of California Tech. *P.A.M. Dirac (16), Cambridge University Freeman Dyson (2), Institute For Advanced Studies, Princeton *John C. Eccles, University of Buffalo *Gerald Edelman, Rockefeller University, NY *Manfred Eigen, Max Planck Institute Göttingen *Albert . Einstein (2), Institute For Advance Studies, Princeton *Richard Feynman, of California Tech. *Paul Flory, Stanford University *Murray Gell-Mann, of CaliforniaTech. *Dona1d Glaser, Berkeley, UniversityCa1. Thomas Gold, Cornell University Special Collections of the University of Miami Libraries ASM0466 Kursunoglu, Behram Papers Container List Box Title or No. -
Bernard F. Whiting NATIONALITY
CURRICULUM VITAE NAME: Bernard F. Whiting NATIONALITY: Australian and American ADDRESS: Department of Physics, 2200 New Physics Building, University of Florida, Gainesville, FL 32611-8440, USA DATE OF BIRTH: October 15, 1950 PLACE OF BIRTH: Melbourne, AUSTRALIA EDUCATION: Undergraduate and Postgraduate at the University of Melbourne; Resident in Newman College, 1968-1977. B.Sc. Honors 04/08/1972 University of Melbourne Ph.D. 12/15/1979 University of Melbourne AWARDS AND POSTS 1968-1971 Commonwealth University Grant 1973-1974 Physics (RAAF Academy) Research Support 1975-1977 Melbourne University Post Graduate Research Award 1978-1979 Newman College, Archbishop Mannix Travelling Scholarship. Senior Visiting Scholar to General Relativity Group in DAMTP, Cambridge. 1980-1982 S.R.C. Research Grants at Cambridge University, under award with Professor S. W. Hawking. 2-5/1983 Visiting Research Associate in the Centers for Relativity and Theoretical Physics, Austin, Texas. May 1983 Invited visitor to the Enrico Fermi Institute, Chicago for two weeks of discussion with Professor S. Chandrasekhar. 6-7/1983 Visitor in DAMTP, Cambridge. 8/83-7/84 Chercheur Associ´edu C.N.R.S. au D´epartment d’Astrophysique de l’Observatoire de Meudon. 8/84-12/85 Boursier Joliot-Curie, au DAF de l’Observatoire de Meudon. 1986-1989 Research Associate with Professor James W. York Jr., supported by NSF in the Institute of Field Physics, UNC-Chapel Hill. 1989-1990 Research Associate in the Institute of Fundamental Theory, Department of Physics, University of Florida, Gainesville. 1990-1993 Visiting Assistant Professor in Astrophysics, Department of Physics, University of Florida, Gainesville. 1992-1993 Faculty Exchange Visitor: Instituut voor Theoretische Fysica, Utrecht (under UF-Utrecht Exchange Program). -
As Assessment of the Physics Laboratory, FY 2010
AN ASSESSMENT OF THE NATIONAL INSTITUTE OF STANDARDS AND TECHNOLOGY PHYSICS LABORATORY FISCAL YEAR 2010 Panel on Physics Laboratory Assessments Board Division on Engineering and Physical Sciences THE NATIONAL ACADEMIES PRESS Washington, D.C. www.nap.edu THE NATIONAL ACADEMIES PRESS 500 Fifth Street, N.W. Washington, DC 20001 NOTICE: The project that is the subject of this report was approved by the Governing Board of the National Research Council, whose members are drawn from the councils of the National Academy of Sciences, the National Academy of Engineering, and the Institute of Medicine. The members of the panel responsible for the report were chosen for their special competences and with regard for appropriate balance. This study was supported by Contract No. SB134106Z011, TO#8, between the National Academy of Sciences and the National Institute of Standards and Technology, an agency of the U.S. Department of Commerce. Any opinions, findings, conclusions, or recommendations expressed in this publication are those of the authors and do not necessarily reflect the views of the agency that provided support for the project. International Standard Book Number-13: 978-0-309-16158-9 International Standard Book Number-10: 0-309-16158-4 Copies of this report are available from Laboratory Assessments Board Division on Engineering and Physical Sciences National Research Council 500 Fifth Street, N.W. Washington, DC 20001 Additional copies of this report are available from the National Academies Press, 500 Fifth Street, N.W., Lockbox 285, Washington, DC 20055; (800) 624-6242 or (202) 334-3313 (in the Washington metropolitan area); Internet, http://www.nap.edu. -
Technical Activities 1983: Center for Radiation Research
— a i i lot aboob? NBSIR 84-2848 Technical Activities 1983 Center for Radiation Research U S. DEPARTMENT OF COMMERCE National Bureau of Standards National Measurement Laboratory Center for Radiation Research Washington, DC 20234 February 1984 V o/ w * ^ z \ LxJ ®^EAU 0* U S. DEPARTMENT OF COMMERCE NATIONAL BUREAU OF STANDARDS “QC — 103 . U56 84-2343 1934 NATIONAL F.ITKSA! OF STn.ID.iftDS LIBRARY ^ NBSIR 84-2848 TECHNICAL ACTIVITIES 1983 CENTER FOR RADIATION RESEARCH Randall S. Caswell, Acting Director U S. DEPARTMENT OF COMMERCE National Bureau of Standards National Measurement Laboratory Center for Radiation Research Washington, DC 20234 February 1984 U.S. DEPARTMENT OF COMMERCE, Malcolm Baldrige, Secretary NATIONAL BUREAU OF STANDARDS, Enwit Ambler. Director ABSTRACT This report summarizes research projects, measurement method develop- ment, testing and data evaluation activities, carried out during Fiscal Year 1983 in the NBS Center for Radiation Research. These activities fall in the areas of radiation measurements, atomic and plasma radiation, nuclear radiation, radiation physics, radiometric physics, and radiation sources and instrumentation. Key Words: Atomic radiation; nuclear radiation; plasma radiation; radiation instrumentation; radiation measurements; radiation physics; radiation sources; radiometric physics. i INTRODUCTION This report is a summary of the technical activities of the NBS Center for Radiation Research (CRR) for the period October 1, 1982 to September 30, 1983. The Center is one of five Centers in the National -
Confluence of Cosmology, Massive Neutrinos, Elementary Particles, and Gravitation Confluence of Cosmology, Massive Neutrinos, Elementary Particles, and Gravitation
Confluence of Cosmology, Massive Neutrinos, Elementary Particles, and Gravitation Confluence of Cosmology, Massive Neutrinos, Elementary Particles, and Gravitation Edited by Behram N. Kursunoglu Global Foundation, Inc. Coral Gables, Florida Stephan L. Mintz Florida International University Miami, Florida and Arnold Perlmutter University of Miami Coral Gables, Florida Kluwer Academic Publishers New York, Boston, Dordrecht, London, Moscow eBook ISBN: 0-306-47094-2 Print ISBN: 0-306-46208-7 ©2002 Kluwer Academic Publishers New York, Boston, Dordrecht, London, Moscow All rights reserved No part of this eBook may be reproduced or transmitted in any form or by any means, electronic, mechanical, recording, or otherwise, without written consent from the Publisher Created in the United States of America Visit Kluwer Online at: http://www.kluweronline.com and Kluwer's eBookstore at: http://www.ebooks.kluweronline.com PREFACE Just before the preliminary program of Orbis Scientiae 1998 went to press the news in physics was suddenly dominated by the discovery that neutrinos are, after all, massive particles. This was predicted by some physicists including Dr. Behram Kusunoglu, who had a paper published on this subject in 1976 in the Physical Review. Massive neutrinos do not necessarily simplify the physics of elementary particles but they do give elementary particle physics a new direction. If the dark matter content of the universe turns out to consist of neutrinos, the fact that they are massive should make an impact on cosmology. Some of the papers in this volume have attempted to provide answers to these questions. We have a long way to go before we find the real reasons for nature’s creation of neutrinos. -
The Miami 2019 Physics Conference
Welcome to the Miami 2019 Physics Conference Breakfast, as covered by your registration fees, will be served 8AM-10AM daily, Thurs, Dec.12 thru Tues, Dec.17, in the conference lobby and pre-conference area, as shown in the map below. (Meals in the hotel restaurants are not covered by your registration fees!) Registration materials will be available starting at 9AM, Thurs, Dec.12 (at the location indicated by the red dot). Lectures begin at 3PM, Thurs. Dec.12, in the Lakeview Room. Daily sessions will begin at 10AM on Fri, Dec.13 thru Tues, Dec.17. Afternoon sessions begin at 3PM on Fri, Dec.13 thru Mon, Dec.16 and continue until 7PM with a break at 4:30PM. On Tues, Dec.17, the afternoon session begins at 3PM and ends at 4:30PM with no break. Check the conference website (https://cgc.physics.miami.edu/2019ScheduleDetails.pdf) or the conference registration desk for up-to-date schedule details. All other conference meals will also be served in the conference lobby and pre- conference area, scheduled as follows. Afternoon breaks are available from 4PM-5PM daily. A welcome reception and buffet will be served at 7PM on Thurs, Dec.12. The banquet begins at 7PM on Sun, Dec.15. Companions who have paid and received a name tag are welcome to enjoy these events. We hope you have a pleasant stay and a great conference. 12 December 2019 Dear Participants: It is my pleasure to welcome you to the 16th topical physics conference in the “Miami” series --- a meeting that continues a sixth decade of physics conferences held in south Florida. -
The" Optical Lever" Intracavity Readout Scheme for Gravitational-Wave
The “optical lever” intracavity readout scheme for gravitational-wave antennae F.Ya.Khalili∗ Dept. of Physics, Moscow State University, Moscow 199899, Russia Abstract An improved version of the “optical bar” intracavity readout scheme for gravitational- wave antennae is considered. We propose to call this scheme “optical lever” because it can provide significant gain in the signal displacement of the local mirror similar to the gain which can be obtained using ordinary mechanical lever with unequal arms. In this scheme displacement of the local mirror can be close to the signal displace- ment of the end mirrors of hypothetical gravitational-wave antenna with arm lengths equal to the half-wavelength of the gravitational wave. 1 Introduction All contemporary large-scale gravitational-wave antennae are based on common principle: they convert phase shift of the optical pumping field into the intensity modulation of the arXiv:gr-qc/0203002v1 1 Mar 2002 output light beam being registered by photodetector [1]. This principle allows to obtain sensitivity necessary to detect gravitational waves from astrophysical sources. However, its use in the next generations of gravitational-wave antennae where substantially higher sensitivity is required, encounters serious problems. An excessively high value of optical pumping power which also depends sharply on the required sensitivity, is likely to be the most important one. For example, at the stage II of the LIGO project the light power circulating in the interferometer arms will be increased to about 1 MWatt, in comparison with about 10 KWatt being currently used [2]. In particular, so high values of the optical power can produce undesirable non-linear effects in the large-scale Fabry-Perot cavities [3]. -
A the Proposal to Extend Intensity Frontier of N,Uclear and Particle
.— — .— .---- L/4- dk!”w-3%fJ ‘L*3 c. \ .— .—. —— t LA-UR+4-3982 t-or Reference I I Not to be taken from this room I ..— — ..—. -— I I I 1 1 A PROPOSAL TO EXTEND THE INTENSITY FRONTIER OF N,UCLEAR AND PARTICLE LosAlamos National Laboratory LosAlamos,New Mexico 87545 I . I 1 A PROPOSU TO EXTEND 1 THE INTENSITY FRONTIER OF 1 NUCLEAR AND PARTICLE I PHYSICS TO 45 GeV (WF 11) December 1984 LOS ALAMOS NATIONAL LABORATORY I ! I I I I 1 I I ACKNOWLEDGMENTS 1. EXECUTIVE SUMMARY 2. STRONG INTERACTION PHYSICS I I 3. ELECTROWEAK INTEIViCTIONS I 4. DESIGN OF THE ACCELEWTORS 5. SCOPE OF THE EXPERIMENTAL AREA FACILITIES 6. COST ESTIMATE ANll SCHEDULE I I ACKNOWLEDGMENTS The following committees and individuals made important contributions to this document: SCIENCE POLICY ADVISORY COMMITTEE Barry C. Barish California Institute of Technology Val L. Fitch Princeton University Leonard S. Kisslinger Carnegie-Mellon University Alan D. Krisch University of Michigan Malcolm MacFarlane Indiana University Sydney Meshkov National Bureau of Standards Peter Parker Yale University Frederick Reines University of California, Irvine S. Peter Rosen Los Alamos National Laboratory, P-DO Lee C. Teng Fermi National Accelerator Laboratory Akihiko Yokosawa Argonne National Laboratory John D. Walecka Stanford University SCIENCE POLICY ADVISORY COMMITTEE - NUCLEAR SUBCOMMITTEE Andrew Bather Indiana University Donald Geesaman Argonne National Laboratory William Gibbs Los Alamos National Laboratory Charles Glashausser Rutgers University Jochen Heisenberg University of New Hampshire Leonard Kissinger Carnegie-Mellon University Malcolm MacFarlane Indiana University Gerald Miller University of Washington Christopher Morris Los Alamos National Laboratory LAMPF 11 ACCELERATOR REVIEW COMMITTEE Lee Teng, Chairman Fermi National Accelerator Laboratory Matthew Allen Stanford Linear Accelerator Center Mark Barton Brookhaven National Laboratory Michael Craddock TRIUMF Grahame Rees Rutherford Laboratory Robert Siemann Cornell University Lloyd Smith Lawrence Berkeley Laboratory OTHER PHYSICS COMMUNITY CONTRIBUTORS P.