APS News April 2019, Vol. 28, No. 4
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Women in Physics, 2000 Highlights
By Rachel Ivie AIP Publication Number R-430 June, 2000 Katie Stowe Women in Physics, 2000 Highlights • An increasingly large number of girls have some exposure to physics by taking it in high school. By 1997, almost one-half of high school physics students were girls (Figure 1) . About 400,000 girls take high school physics each year. • Women’s participation in physics decreases with each step up the academic ladder. For example, more than two-fifths of high school physics students in 1993 were girls, but women earned less than one-fifth of bachelor’s degrees in physics five years later (Figures 1 and 3) . • Although women now earn more than one half of all bachelor’s degrees in the U.S., physics is not attracting women as quickly as other fields, including life sciences, chemistry, and engineering (Figures 4 and 5) . Compared to other fields, women are sorely underrepresented in physics at both the bachelor’s and PhD levels (Figures 4, 5, 6, 7, and Table 1) . • Twenty U.S. physics departments (excluding women’s colleges) had more than 40% female bachelor’s degree recipients during the five academic years 1994-98. This report lists these departments as well as women’s colleges that grant bachelor’s degrees in physics (Tables 2 and 3) . • The proportion of women teaching physics decreases as academic rank and level of the department increases (Table 4) . However, the percentage of women faculty members at each rank is at least as high as the percentage of women earning PhDs at various points in the past. -
Parallel Sessions
Identification of Dark Matter July 23-27, 2012 9th International Conference Chicago, IL http://kicp-workshops.uchicago.edu/IDM2012/ PARALLEL SESSIONS http://kicp.uchicago.edu/ http://www.nsf.gov/ http://www.uchicago.edu/ http://www.fnal.gov/ International Advisory Committee Daniel Akerib Elena Aprile Rita Bernabei Case Western Reserve University, Columbia University, USA Universita degli Studi di Roma, Italy Cleveland, USA Gianfranco Bertone Joakim Edsjo Katherine Freese University of Amsterdam Oskar Klein Centre / Stockholm University of Michigan, USA University Richard Gaitskell Gilles Gerbier Anne Green Brown University, USA IRFU/ CEA Saclay, France University of Nottingham, UK Karsten Jedamzik Xiangdong Ji Lawrence Krauss Universite de Montpellier, France University of Maryland, USA Arizona State University, USA Vitaly Kudryavtsev Reina Maruyama Leszek Roszkowski University of Sheffield University of Wisconsin-Madison University of Sheffield, UK Bernard Sadoulet Pierre Salati Daniel Santos University of California, Berkeley, USA University of California, Berkeley, USA LPSC/UJF/CNRS Pierre Sikivie Daniel Snowden-Ifft Neil Spooner University of Florida, USA Occidental College University of Sheffield, UK Max Tegmark Karl van Bibber Kavli Institute for Astrophysics & Space Naval Postgraduate School Monterey, Research at MIT, USA USA Local Organizing Committee Daniel Bauer Matthew Buckley Juan Collar Fermi National Accelerator Laboratory Fermi National Accelerator Laboratory Kavli Institute for Cosmological Physics Scott Dodelson Aimee -
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 ................................................................................................................... -
Development of a Liquid Xenon Time Projection Chamber for the XENON Dark Matter Search
Development of a Liquid Xenon Time Projection Chamber for the XENON Dark Matter Search Kaixuan Ni Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in the Graduate School of Arts and Sciences COLUMBIA UNIVERSITY 2006 c 2006 Kaixuan Ni All rights reserved Development of a Liquid Xenon Time Projection Chamber for the XENON Dark Matter Search Kaixuan Ni Advisor: Professor Elena Aprile Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in the Graduate School of Arts and Sciences COLUMBIA UNIVERSITY 2006 c 2006 Kaixuan Ni All rights reserved ABSTRACT Development of a Liquid Xenon Time Projection Chamber for the XENON Dark Matter Search Kaixuan Ni This thesis describes the research conducted for the XENON dark matter direct detection experiment. The tiny energy and small cross-section, from the interaction of dark matter particle on the target, requires a low threshold and sufficient background rejection capability of the detector. The XENON experiment uses dual phase technology to detect scintillation and ionization simultaneously from an event in liquid xenon (LXe). The distinct ratio, be- tween scintillation and ionization, for nuclear recoil and electron recoil events provides excellent background rejection potential. The XENON detector is designed to have 3D position sensitivity down to mm scale, which provides additional event information for background rejection. Started in 2002, the XENON project made steady progress in the R&D phase during the past few years. Those include developing sensitive photon detectors in LXe, improving the energy resolution and LXe purity for detect- ing very low energy events. -
Physics in Your Future Introduces Physics and Careers in Physics to Young People, Their Parents, Teachers and Advisors
TM American Physical Society • Committee on the Status of Women in Physics Chiara La Tessa of Brookhaven National Laboratory is inside the target room of the NASA Space Radiation Laboratory at Brookhaven. She is aligning a detector called EGG counter in the center of a beam – something that’s done before each experiment. Physics helps us understand the world around us, the world inside us, and the world beyond us. Physics is the most basic and fundamental science; it deals with how and why matter and energy act as they do. The laws of physics apply to force and motion, gravity, electricity, magnetism, sound, light and heat. They help us understand the physical world and develop products that people need. Mastering physics is fun and challenging. It involves working with others, as well as alone. You learn how to solve problems, observe things carefully, make measurements and keep accurate records. You can use these valuable skills for the rest of your life. They open doors to many good jobs. Physicists ask questions about the physical world and try to find exact answers. They are creative and persistent. Some do basic research. Their goal is to increase our knowledge of the universe. Others do applied research. They use basic knowledge to solve world problems such as food and energy supply, environmental protection, transportation, communication and defense. Physicists work in industry, educational institutions, government, and medical centers today. Most are active scientists and engineers. They do research and development, administration, and teaching. Others use their physics background in fields like publishing, sales, law, accounting and medicine. -
Modeling Popularity and Reliability of Sources in Multilingual Wikipedia
information Article Modeling Popularity and Reliability of Sources in Multilingual Wikipedia Włodzimierz Lewoniewski * , Krzysztof W˛ecel and Witold Abramowicz Department of Information Systems, Pozna´nUniversity of Economics and Business, 61-875 Pozna´n,Poland; [email protected] (K.W.); [email protected] (W.A.) * Correspondence: [email protected] Received: 31 March 2020; Accepted: 7 May 2020; Published: 13 May 2020 Abstract: One of the most important factors impacting quality of content in Wikipedia is presence of reliable sources. By following references, readers can verify facts or find more details about described topic. A Wikipedia article can be edited independently in any of over 300 languages, even by anonymous users, therefore information about the same topic may be inconsistent. This also applies to use of references in different language versions of a particular article, so the same statement can have different sources. In this paper we analyzed over 40 million articles from the 55 most developed language versions of Wikipedia to extract information about over 200 million references and find the most popular and reliable sources. We presented 10 models for the assessment of the popularity and reliability of the sources based on analysis of meta information about the references in Wikipedia articles, page views and authors of the articles. Using DBpedia and Wikidata we automatically identified the alignment of the sources to a specific domain. Additionally, we analyzed the changes of popularity and reliability in time and identified growth leaders in each of the considered months. The results can be used for quality improvements of the content in different languages versions of Wikipedia. -
Meeting of the Executive Committee of the DPF
Meeting of the Executive Committee of the DPF December 19, 1997 Present: Bagger, Beier, Burchat, Devlin, Frisch, Georgi, Gordon, Grannis, Kinoshita, Naples, Newman-Holmes, Rutherfoord, Schellman Guests: B. Barnett, T. McIlrath, R. Peccei, J. Sandweiss Agenda: 1. Report of the Chair 2. Report of the Secretary-Treasurer 3. Report of the APS Treasurer 4. Congressional Reception 5. Report on OSTP and OMB Visit 6. APS Council Report 7. Physical Review Letters 8. DPF 99 9. DPF 2000/2001 10. April Meeting 11. Education and Outreach 12. Tanaka Prize 13. APS Centennial 14. Prize for Technical Contributions 15. Phenomenology in the U.S. 16. FNAL Director Search 17. DPF Committees For more on these items, see the DPF home page, http://www.aps.org/units/dpf/. Report of the Chair Paul Grannis introduced the new members of the Executive Committee and thanked the people who are retiring. He announced that Bruce Barnett of Johns Hopkins will begin a three-year term as organizer of the DPF Congressional Reception, and that Bob Cahn of LBNL will take over as Public Information Coordinator. Grannis also reminded the Executive Committee that Gene Beier will replace Frank Sciulli as the DPF representative on ICFA. Report of the Secretary-Treasurer As of November 1, 1997, the DPF account balance stood at $86,274. The prize account balances stood as follows: Panofsky, $64,103; Sakurai, $174,053; Wilson, $107,697. The Panofsky Prize Fund remains significantly underendowed. Howard Georgi will take over the fund raising effort. Howard Gordon and Pat Burchat have volunteered to help. Report of the APS Treasurer Tom McIlrath presented a positive report on APS finances. -
Citation Statistics from 110 Years of Physical Review
Citation Statistics from 110 Years of Physical Review Publicly available data reveal long-term systematic features about citation statistics and how papers are referenced. The data also tell fascinating citation histories of individual articles. Sidney Redner he first article published in the Physical Review was Treceived in 1893; the journal’s first volume included 6 issues and 24 articles. In the 20th century, the Phys- ical Review branched into topical sections and spawned new journals (see figure 1). Today, all arti- cles in the Physical Review family of journals (PR) are available online and, as a useful byproduct, all cita- tions in PR articles are electronically available. The citation data provide a treasure trove of quantitative information. As individuals who write sci- entific papers, most of us are keenly interested in how often our own work is cited. As dispassionate observers, we Figure 1. The Physical Review can use the citation data to identify influential research, was the first member of a family new trends in research, unanticipated connections across of journals that now includes two series of Physical fields, and downturns in subfields that are exhausted. A Review, the topical journals Physical Review A–E, certain pleasure can also be gleaned from the data when Physical Review Letters (PRL), Reviews of Modern Physics, they reveal the idiosyncratic features in the citation his- and Physical Review Special Topics: Accelerators and tories of individual articles. Beams. The first issue of Physical Review bears a publica- The investigation of citation statistics has a long his- tion date a year later than the receipt of its first article. -
Dark Matter Working Group Executive Summary (Ness '02)
Dark Matter Working Group Executive Summary (NeSS ’02) Working Group Leaders: Rick Gaitskell, Brown; and Dick Arnowitt, Texas A&M. (Document Version 020925v21) Working Group Members: Craig Aalseth, PNL; Dan Akerib, CWRU; Elena Aprile, Columbia; Priscilla Cushman, U. Minnesota; John Ellis, CERN; Jonathan Feng, UC Irvine; Gilles Gerbier, Saclay; Alexander Kusenko, UCLA; Kirk McDonald, Princeton; Jeff Martoff, Temple; Richard Schnee, CWRU; and Nigel Smith, RAL. Introduction No currently observed particle is a suitable candidate for cold dark matter. The solution to the non baryonic dark matter problem, both in the universe as a whole, and in our own galaxy, may be resolved by physics found at the intersection of astronomy, high energy particle physics, and cosmology. The main candidates for this dark matter are relic particles generated, in great abundance, shortly after the Big Bang. Currently, there are 20 operating experiments designed to perform the direct detection of these particles being conducted at all the underground physics laboratories worldwide (bar one). One of them is sited at a US underground laboratory, although US sourced funding is made to six experiments. Existing results have put significant constraints on the allowed particle theories of dark matter, with one experiment claiming a positive observation, yet to be confirmed by other experiments. The planned dark matter experiments that were discussed at this workshop would be able to cover most of the parameter space of major theoretical proposals. The new physics required for particle dark matter is also expected to be discovered in the next round of high energy accelerator experiments (LHC, NLC). Theoretically and experimentally there is great complementarity between direct detection and accelerator programs. -
Testing the Purity Monitor for the XENON Dark Matter Search
Testing the Purity Monitor for the XENON Dark Matter Search Alison Andrews Laboratori Nazionali del Gran Sasso Columbia University REU August 4, 2006 1 Introduction Evidence for dark matter is found in many observed features of the universe. New- q GM(r) tonian gravitation predicts the rotational velocities of galaxies by v(r) = r , where mass is described by M(r) = 4π R ρ(r)r2dr. Actual measurements of the rota- tional velocities of galaxies, however, describe a distribution of mass where M(r) ∝ r. Fritz Zwicky studied this inconsistency in the Coma galaxy cluster in 1933, and he proposed the existence of a non-luminous dark matter. Over thirty years later, Vera Rubin supported Zwickys work with additional observations of galaxy rotational 1 curves. Their studies imply the existence of a halo of dark matter with ρ(r) ∝ r2 . Further evidence of dark matter is gravitational lensing. The General Theory of Relativity predicts the bending of light through areas of gravitational potential. Observations of this phenomenon show that the amount of bending around galaxy clusters corresponds to a greater amount of mass than is visible. Dark matter also helps to explain the formation and temperature distribution of the universe. A favored candidate for cold non-baryonic dark matter is the Weakly Interac- tive Massive Particle (or WIMP). Direct detection of WIMPs in experiments like XENON aim to detect the energy released from the elastic scattering of a WIMP off a terrestrial nucleus. 1 2 The XENON Dark Matter Search The XENON experiment aims to detect dark matter particles by measuring the scintillation and ionization of the nuclear recoils which result from the elastic collision of WIMPs with Xe nuclei using a dual phase (liquid/gas) xenon time projection chamber. -
Writing Physics Papers
Physics 2151W Lab Manual | Page 45 WID Handbook for Intermediate Laboratory - Physics 2151W Writing Physics Papers Dr. Igor Strakovsky Department of Physics, GWU Publish or Perish - Presentation of Scientific Results Intermediate Laboratory – Physics 2151W is focused on significantly improving the students' writing skills with respect to producing scientific papers, to do peer reviews, and presentations at the Physics Department Mini-Workshop. Third Edition, 2013 Physics 2151W Lab Manual | Page 46 OUTLINE Why are we Writing Papers? What Physics Journals are there? Structure of a Physics Article. Style of Technical Papers. Hints for Effective Writing. Submit and Fight. Why are We Writing Papers? To communicate our original, interesting, and useful research. To let others know what we are working on (and that we are working at all.) To organize our thoughts. To formulate our research in a comprehensible way. To secure further funding. To further our careers. To make our publication lists look more impressive. To make our Citation Index very impressive. To have fun? Because we believe someone is going to read it!!! Physics 2151W Lab Manual | Page 47 What Physics Journals are there? Hard Science Journals Physical Review Series: Physical Review A Physical Review E http://pra.aps.org/ http://pre.aps.org/ Atomic, Molecular, and Optical physics. Stat, Non-Linear, & Soft Material Phys. Physical Review B Physical Review Letters http://prb.aps.org/ http://prl.aps.org/ Condensed matter and Materials physics. Moving physics forward. Physical Review C Review of Modern Physics http://prc.aps.org/ http://rmp.aps.org/ Nuclear physics. Reviews in all areas. Physical Review D http://prd.aps.org/ Particles, Fields, Gravitation, and Cosmology. -
Elena Aprile Columbia University
XENON1T: First Results (arXiv:1705.06655) Elena Aprile Columbia University Patras Axion-Wimp 2017 May 15-19 Thessaloniki, Greece 1 XENON World ~130 scientists from 22 institutions Laboratori Nazionali del Gran Sasso (LNGS), Italy XENON1T Elena Aprile (Columbia) XENON1T: First Results @ Patras Axion-WIMP 2017 2 Phases of the XENON program XENON10 XENON100 XENON1T / XENONnT 2005-2007 2008-2016 2013-2018 / 2019-2023 15 cm drift TPC – 25 kg 30 cm drift TPC – 161 kg 100 cm / 144 cm drift TPC - 3200 kg / ~8000 kg Achieved (2007) Achieved (2016) Projected (2018) / Projected (2023) σ -44 2 σ -45 2 σ -47 2 σ -48 2 SI = 8.8 x 10 cm SI = 1.1 x 10 cm SI = 1.6 x 10 cm / SI = 1.6 x 10 cm Elena Aprile (Columbia) XENON1T: First Results @ Patras Axion-WIMP 2017 3 The XENON1T Experiment Elena Aprile (Columbia) XENON1T: First Results @ Patras Axion-WIMP 2017 4 The XENON1T Experiment Elena Aprile (Columbia) XENON1T: First Results @ Patras Axion-WIMP 2017 4 July 2013 Uwe Oberlack LNGS SC Meeting - 29-Oct-2013 17 Aug. 2014 XENON1T Cryostat 7 XENON1T Cryostat 7 XENON1T Cryostat 7 XENON1T Cryostat 7 XENON1T Cryostat 7 Time Projection Chamber Eur. Phys. J. C 75, no. 11, 546 (2015) Elena Aprile (Columbia) XENON1T: First Results @ Patras Axion-WIMP 2017 8 Cryostat in the Water Tank Elena Aprile (Columbia) XENON1T: First Results @ Patras Axion-WIMP 2017 9 Cherenkov Muon Veto • Active shield against muons • 84 high-QE 8'' Hamamatsu R5912 PMTs • Trigger efficiency > 99.5% for neutrons with muons in water tank • Can suppress cosmogenic background to < 0.01 events/ton/year