Main Attributes of Nuclides Presented in This Book
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Igor Tamm 1895 - 1971 Awarded the Nobel Prize for Physics in 1958
Igor Tamm 1895 - 1971 Awarded the Nobel Prize for Physics in 1958 The famous Russian physicist Igor Evgenievich Tamm is best known for his theoretical explanation of the origin of the Cherenkov radiation. But really his works covered various fields of physics: nuclear physics, elementary particles, solid-state physics and so on. In about 1935, he and his colleague, Ilya Frank, concluded that although objects can’t travel faster than light in a vacuum, they can do so in other media. Cherenkov radiation is emitted if charged particles pass the media faster than the speed of light ! For this research Tamm together with his Russian colleagues was awarded the 1958 Nobel Prize in Physics. Igor Tamm was born in 1895 in Vladivostok when Russia was still ruled by the Tsar. His father was a civil engineer who worked on the electricity and sewage systems. When Tamm was six years old his family moved to Elizavetgrad, in the Ukraine. Tamm led an expedition to He graduated from the local Gymnasium in 1913. Young Tamm dreamed of becoming a revolutionary, but his father disapproved . However only his mother was able to convince him to search for treasure in the Pamirs change his plans. She told him that his father’s weak heart could not take it if something happened to him. In 1923 Tamm was offered a teaching post at the Second Moscow University and later he was And so, in 1913, Tamm decided to leave Russia for a year and continue his studies in Edinburgh. awarded a professorship at Moscow State University. -
Measurements of Elastic Electron-Proton Scattering at Large Momentum Transfer*
SLAC-PUB-4395 Rev. January 1993 m Measurements of Elastic Electron-Proton Scattering at Large Momentum Transfer* A. F. SILL,(~) R. G. ARNOLD,P. E. BOSTED,~. C. CHANG,@) J. GoMEz,(~)A. T. KATRAMATOU,C. J. MARTOFF, G. G. PETRATOS,(~)A. A. RAHBAR,S. E. ROCK,AND Z. M. SZALATA Department of Physics The American University, Washington DC 20016 D.J. SHERDEN Stanford Linear Accelerator Center , Stanford University, Stanford, California 94309 J. M. LAMBERT Department of Physics Georgetown University, Washington DC 20057 and R. M. LOMBARD-NELSEN De’partemente de Physique Nucle’aire CEN Saclay, Gif-sur- Yvette, 91191 Cedex, France Submitted to Physical Review D *Work supported by US Department of Energy contract DE-AC03-76SF00515 (SLAC), and National Science Foundation Grants PHY83-40337 and PHY85-10549 (American University). R. M. Lombard-Nelsen was supported by C. N. R. S. (French National Center for Scientific Research). Javier Gomez was partially supported by CONICIT, Venezuela. (‘)Present address: Department of Physics and Astronomy, University of Rochester, NY 14627. (*)Permanent address: Department of Physics and Astronomy, University of Maryland, College Park, MD 20742. (C)Present address: Continuous Electron Beam Accelerator Facility, Newport News, VA 23606. (d)Present address: Temple University, Philadelphia, PA 19122. (c)Present address: Stanford Linear Accelerator Center, Stanford CA 94309. ABSTRACT Measurements of the forward-angle differential cross section for elastic electron-proton scattering were made in the range of momentum transfer from Q2 = 2.9 to 31.3 (GeV/c)2 using an electron beam at the Stanford Linear Accel- erator Center. The data span six orders of magnitude in cross section. -
Gas-Phase Electrochemistry: Measuring Absolute Potentials and Investigating Ion and Electron Hydration*
Pure Appl. Chem., Vol. 83, No. 12, pp. 2129–2151, 2011. doi:10.1351/PAC-CON-11-08-15 © 2011 IUPAC, Publication date (Web): 7 October 2011 Gas-phase electrochemistry: Measuring absolute potentials and investigating ion and electron hydration* William A. Donald1,‡ and Evan R. Williams2 1School of Chemistry, Bio21 Institute of Molecular Science and Biotechnology, and ARC Centre of Excellence for Free Radical Chemistry and Biotechnology, University of Melbourne, Melbourne, Victoria, Australia; 2Department of Chemistry, University of California, Berkeley, CA, USA Abstract: In solution, half-cell potentials and ion solvation energies (or enthalpies) are meas- ured relative to other values, thus establishing ladders of thermochemical values that are ref- erenced to the potential of the standard hydrogen electrode (SHE) and the proton hydration energy (or enthalpy), respectively, which are both arbitrarily assigned a value of 0. In this focused review article, we describe three routes for obtaining absolute solution-phase half- cell potentials using ion nanocalorimetry, in which the energy resulting from electron capture (EC) by large hydrated ions in the gas phase are obtained from the number of water mole- cules lost from the reduced precursor cluster, which was developed by the Williams group at the University of California, Berkeley. Recent ion nanocalorimetry methods for investigating ion and electron hydration and for obtaining the absolute hydration enthalpy of the electron are discussed. From these methods, an absolute electrochemical scale and ion solvation scale can be established from experimental measurements without any models. Keywords: absolute potentials; clusters; electrochemistry; electron capture dissociation; elec- tron transfer; gaseous state; hydrated ions; hydration; ion nanocalorimetry; solvation; thermo chemistry. -
Glossary Glossary
Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts. -
Department of Physics and Astronomy 1
Department of Physics and Astronomy 1 PHSX 216 and PHSX 236, provide a calculus-based foundation in Department of Physics physics for students in physical science, engineering, and mathematics. PHSX 313 and the laboratory course, PHSX 316, provide an introduction and Astronomy to modern physics for majors in physics and some engineering and physical science programs. Why study physics and astronomy? Students in biological sciences, health sciences, physical sciences, mathematics, engineering, and prospective elementary and secondary Our goal is to understand the physical universe. The questions teachers should see appropriate sections of this catalog and major addressed by our department’s research and education missions range advisors for guidance about required physics course work. Chemistry from the applied, such as an improved understanding of the materials that majors should note that PHSX 211 and PHSX 212 are prerequisites to can be used for solar cell energy production, to foundational questions advanced work in chemistry. about the nature of mass and space and how the Universe was formed and subsequently evolved, and how astrophysical phenomena affected For programs in engineering physics (http://catalog.ku.edu/engineering/ the Earth and its evolution. We study the properties of systems ranging engineering-physics/), see the School of Engineering section of the online in size from smaller than an atom to larger than a galaxy on timescales catalog. ranging from billionths of a second to the age of the universe. Our courses and laboratory/research experiences help students hone their Graduate Programs problem solving and analytical skills and thereby become broadly trained critical thinkers. While about half of our majors move on to graduate The department offers two primary graduate programs: (i) an M.S. -
DOCUMENT Mute
DOCUMENT mute ED 124 18 . 88 SE 019 612 TITLEN: Radioactivity .and Man iinicourse, Career Oriented Pre-Technical Physics* , INSTITUTI N Dallas Independent School District, Tex. SPONS AGE CY Bureauvof Ele*entary and Secondary tducat4.0n (D5 HEN/OE),-WashingtOn, D.C. -RUB DATE 7 For rilated 0, NOTE - 78p.; Drawings may not reproduce wel documens, see SE 018 322-333 and SE 019 605-616 , . 4 EDRS PRICE MF-$0.83 HC-$4.67 Plus Postag4. DESCRIPTOR Instructional Materialsi Physics; *Program Guides; *Radiation Effects; *Science Activities; Science .41 Careers; Science Education; *Science Materials; Secondary Zdution;.*Secondary School Science; Technical Educe ion IDENTIFIrRS Elementary Seco dart' VIAlcation ACt Title III; ESEA Title' III 07. 1 ABSTRACT .1j This instructional guide, intended for student use, develops the subject of radioactivity and can through a series. of sequential activities.. `A technical development of the subject is pursued with examples stressing practical aspects'of the concepts. Included in the minicourse are:, (1) the rationale,(2) terminal behavioral objectives, (3) enabling behavioral objectives,(4) activities,(5) resource ,packages, and (6) evaluation materials. The' * benefits as well as the dangers of radiometivity to Ian are considered.,This unit is one of twelve intended for use in.the second year of tv9 year vocationally oriented .physics. program. (CP) j t I J ***********************************************************************. * . Documents acquired by ERIC include many inforgal unpublished * materials not a40.1able.from other sources. ERIC makes every effort * * to obtiit the best copy available. Nevertheless,items of.marginel * *.reproducibility are often encountered and this-affects the quality * - *`of the microfiche and hardcopy reproductions ERIC makes available * *. -
Neutron Scattering
Neutron Scattering Basic properties of neutron and electron neutron electron −27 −31 mass mkn =×1.675 10 g mke =×9.109 10 g charge 0 e spin s = ½ s = ½ −e= −e= magnetic dipole moment µnn= gs with gn = 3.826 µee= gs with ge = 2.0 2mn 2me =22k 2π =22k Ek== E = 2m λ 2m energy n e 81.81 150.26 Em[]eV = 2 Ee[]V = 2 λ ⎣⎡Å⎦⎤ λ ⎣⎦⎡⎤Å interaction with matter: Coulomb interaction — 9 strong-force interaction 9 — magnetic dipole-dipole 9 9 interaction Several salient features are apparent from this table: – electrons are charged and experience strong, long-range Coulomb interactions in a solid. They therefore typically only penetrate a few atomic layers into the solid. Electron scattering is therefore a surface-sensitive probe. Neutrons are uncharged and do not experience Coulomb interaction. The strong-force interaction is naturally strong but very short-range, and the magnetic interaction is long-range but weak. Neutrons therefore penetrate deeply into most materials, so that neutron scattering is a bulk probe. – Electrons with wavelengths comparable to interatomic distances (λ ~2Å ) have energies of several tens of electron volts, comparable to energies of plasmons and interband transitions in solids. Electron scattering is therefore well suited as a probe of these high-energy excitations. Neutrons with λ ~2Å have energies of several tens of meV , comparable to the thermal energies kTB at room temperature. These so-called “thermal neutrons” are excellent probes of low-energy excitations such as lattice vibrations and spin waves with energies in the meV range. -
Inspec Archive - List of Journals Covered Between 1898 and 1968
February 2006 www.iee.org/inspec Inspec Archive - List of Journals Covered between 1898 and 1968 Abhandlungen der Berlin Akademie Acta Universitatis Lundensis. Sectio II. Medica, Abhandlungen der Braunschweigischen Mathematica, Scientiae Rerum Naturalium Wissenschaftlichen Gesellschaft Acta Universitatis Tamperensis Abhandlungen der Deutschen Akademie der Acustica Wissenschaften zu Berlin, Klasse fur Advanced Energy Conversion Mathematik, Physik und Technik Advances in Atomic and Molecular Physics Abhandlungen der Konigliches Preussisches Advances in Electronics Meteorologies Institut Advances in Physics Abhandlungen der Preussischen Akademieder Advances in Theoretical Physics Wissenschaften Advances of Science Accademia delle Scienze, Medico e Naturali, AEG Mitteilungen Ferrara AEG Progress ACEC Journal AEG Zeitung ACEC Review AEI Engineering Acero y Energia AEI Engineering Review Acta Academiae Aboensis, Mathematical AEI Journal of Telecommunications Physics AEI Research Laboratory Reports Acta and Commentationes Universitatis Aerial Age Tartuensis (Dorpatensis) Aerial Age Weekly Acta Automatica Sinica Aeronautical Engineering Review Acta Bolyaiana Aeronautical Journal Acta Chemica Scandinavica Aeronautical Research Council Current Papers Acta Crystallographica Aeronautical Research Council Reports and Acta Electronica Memoranda Acta Electronica Sinica Aeronautics Acta Geophysica Sinica Aeroplane Acta Mathematica Aerospace Engineering Acta Mathematica Sinica Agricultural and Horticultural Engineering Acta Mechanica Abstracts Acta Medica -
DMAAC – February 1973
LUNAR TOPOGRAPHIC ORTHOPHOTOMAP (LTO) AND LUNAR ORTHOPHOTMAP (LO) SERIES (Published by DMATC) Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Scale: 1:250,000 Projection: Transverse Mercator Sheet Size: 25.5”x 26.5” The Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Series are the first comprehensive and continuous mapping to be accomplished from Apollo Mission 15-17 mapping photographs. This series is also the first major effort to apply recent advances in orthophotography to lunar mapping. Presently developed maps of this series were designed to support initial lunar scientific investigations primarily employing results of Apollo Mission 15-17 data. Individual maps of this series cover 4 degrees of lunar latitude and 5 degrees of lunar longitude consisting of 1/16 of the area of a 1:1,000,000 scale Lunar Astronautical Chart (LAC) (Section 4.2.1). Their apha-numeric identification (example – LTO38B1) consists of the designator LTO for topographic orthophoto editions or LO for orthophoto editions followed by the LAC number in which they fall, followed by an A, B, C or D designator defining the pertinent LAC quadrant and a 1, 2, 3, or 4 designator defining the specific sub-quadrant actually covered. The following designation (250) identifies the sheets as being at 1:250,000 scale. The LTO editions display 100-meter contours, 50-meter supplemental contours and spot elevations in a red overprint to the base, which is lithographed in black and white. LO editions are identical except that all relief information is omitted and selenographic graticule is restricted to border ticks, presenting an umencumbered view of lunar features imaged by the photographic base. -
August 2017 Posidonius P & Luther
A PUBLICATION OF THE LUNAR SECTION OF THE A.L.P.O. EDITED BY: Wayne Bailey [email protected] 17 Autumn Lane, Sewell, NJ 08080 RECENT BACK ISSUES: http://moon.scopesandscapes.com/tlo_back.html FEATURE OF THE MONTH – AUGUST 2017 POSIDONIUS P & LUTHER Sketch and text by Robert H. Hays, Jr. - Worth, Illinois, USA March 5, 2017 01:28-01:48; UT, 15 cm refl, 170x, seeing 7-8/10. I drew these craters on the evening of March 4/5, 2017 while the moon was hiding some Hyades stars. This area is in northeast Mare Serenitatis west of Posidonius itself. Posidonius P is the largest crater on this sketch. The smaller crater south of P is Posidonius F and Posidonius G is the tiny pit to the north. There is a halo around Posidonius G, but this crater is noticeably north of the halo's center. A very low round swelling is northeast of Posidonius G. Luther is the crater well to the west of Posidonius P. All four of these craters are crisp, symmetric features, differing only in size. There are an assortment of elevations near Luther. The peak Luther alpha is well to the west of Luther, and showed dark shadowing at this time. All of the other features near Luther are more subtle than Luther alpha. One mound is between Luther and Luther alpha. Two more mounds are north of Luther, and a low ridge is just east of this crater. A pair of very low mounds are south of Luther. These are the vaguest features depicted here, and may be too conspicuous on the sketch. -
Appendix E Nobel Prizes in Nuclear Science
Nuclear Science—A Guide to the Nuclear Science Wall Chart ©2018 Contemporary Physics Education Project (CPEP) Appendix E Nobel Prizes in Nuclear Science Many Nobel Prizes have been awarded for nuclear research and instrumentation. The field has spun off: particle physics, nuclear astrophysics, nuclear power reactors, nuclear medicine, and nuclear weapons. Understanding how the nucleus works and applying that knowledge to technology has been one of the most significant accomplishments of twentieth century scientific research. Each prize was awarded for physics unless otherwise noted. Name(s) Discovery Year Henri Becquerel, Pierre Discovered spontaneous radioactivity 1903 Curie, and Marie Curie Ernest Rutherford Work on the disintegration of the elements and 1908 chemistry of radioactive elements (chem) Marie Curie Discovery of radium and polonium 1911 (chem) Frederick Soddy Work on chemistry of radioactive substances 1921 including the origin and nature of radioactive (chem) isotopes Francis Aston Discovery of isotopes in many non-radioactive 1922 elements, also enunciated the whole-number rule of (chem) atomic masses Charles Wilson Development of the cloud chamber for detecting 1927 charged particles Harold Urey Discovery of heavy hydrogen (deuterium) 1934 (chem) Frederic Joliot and Synthesis of several new radioactive elements 1935 Irene Joliot-Curie (chem) James Chadwick Discovery of the neutron 1935 Carl David Anderson Discovery of the positron 1936 Enrico Fermi New radioactive elements produced by neutron 1938 irradiation Ernest Lawrence -
Supplementvolum-E18 Nu-Mber-41989 .__L,___Society
ISSN 0739-4934 NEWSLETTER I IISTORY OF SCIENCE SUPPLEMENTVOLUM-E18 NU-MBER-41989 .__L,___SOCIETY - WELCOME TO GAINESVILLE HSS EXECUTIVE BY FREDERICK GREGORY COMMITTEE "A SOPI-llSTICATED SLICE of small-town south": so wrote Jonathan Lerner PRESIDENT about Gainesville for Washington Post readers this past spring. Like the majority MARY JO NYE, University of Oklahoma of visitors to Gainesville, Lerner was impressed with the topography of the city, VICE-PRESIDENT which forms a hammock-a dry area, relatively higher than its surroundings, STEPHEN G. BRUSH, University of Maryland that can support hardwood trees. Residents of Gainesville are enormously proud of the extensive canopy that covers 46 percent of their town, the highest per EXECUTIVE SECRETARY MICHAEL M. SOKAL, Worcester centage of any Florida city. In addition to the majestic live oaks, the southern Polytechnic Institute pine, and a variety of palm trees, dogwoods and magnolias are also plentiful. TREASURER Unfortunately the HSS Annual Meeting is held at a time of year that misses the MARY LOUISE GLEASON, New York City blossoms of our giant azaleas, some older ones of which are as high as roof tops. EDITOR f obvious interest to historians of science is nearby Paynes Prairie, an 18,000- RONALD L. NUMBERS, University of acre wildlife preserve whose zoological and botanical life was described in vivid Wisconsin-Madison detail by William Bartram after his travels through the region in 1774. Meeting sessions will be held on the campus of the University of Florida, which, at least in this part of the country, is never to be mixed up with Florida State University in Tallahassee.