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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. -
2019 in the Academic Ranking of World Universities (ARWU)
THE UNIVERSITY OF MANCHESTER FACTS AND FIGURES 2020 2 The University 4 World ranking 6 Academic pedigree 8 World-class research CONTENTS 10 Students 12 Making a difference 14 Global challenges, Manchester solutions 16 Stellify 18 Graduate careers 20 Staff 22 Faculties and Schools 24 Alumni 26 Innovation 28 Widening participation UNIVERSITY OF MANCHESTER 30 Cultural institutions UNIVERSITY OF MANCHESTER 32 Income 34 Campus investment 36 At a glance 1 THE UNIVERSITY OF MANCHESTER Our vision is to be recognised globally for the excellence of our people, research, learning and innovation, and for the benefits we bring to society and the environment. Our core goals and strategic themes Research and discovery Teaching and learning Social responsibility Our people, our values Innovation Civic engagement Global influence 2 3 WORLD RANKING The quality of our teaching and the impact of our research are the cornerstones of our success. We have risen from 78th in 2004* to 33rd – our highest ever place – in 2019 in the Academic Ranking of World Universities (ARWU). League table World ranking European ranking UK ranking 33 8 6 ARWU 33 8 6 WORLD EUROPE UK QS 27 8 6 Times Higher Education 55 16 8 *2004 ranking refers to the Victoria University of Manchester prior to the merger with UMIST. 4 5 ACADEMIC PEDIGREE 1906 1908 1915 1922 1922 We attract the highest-calibre researchers and teachers, with 25 Nobel Prize winners among J Thomson Ernest Rutherford William Archibald V Hill Niels Bohr Physics Chemistry Larence Bragg Physiology or Medicine Physics our current and former staff and students. -
Conference on the History of Quantum Physics Max-Planck-Institut Für Wissenschaftsgeschichte Berlin, 2–6 July 2007 Abstract
Conference on the history of quantum physics Max-Planck-Institut für Wissenschaftsgeschichte Berlin, 2–6 July 2007 Abstract Title: Walther Nernst, Albert Einstein, Otto Stern, Adriaan Fokker, and the rotational specific heat of hydrogen Author: Clayton A. Gearhart (St. John’s University, Minnesota, USA) In 1911, the German physical chemist Walther Nernst argued that the new quantum theory promised to clear up long-standing puzzles in kinetic theory, particularly in understanding the discrepancies between the predictions of the equipartition theorem and the measured specific heats of gases. Nernst noted that hydrogen gas would be a good test case. The first measurements were published by his assistant Arnold Euken in 1912, and showed a sharp drop in the specific heat at low temperatures, corresponding to rotational degrees of freedom “freezing out.” In his 1911 paper, Nernst also developed a theory for a quantum rotator (a tiny rotating dumbbell representing a diatomic gas). Remarkably, he did not quantize rotational energies. Instead, the specific heat fell off because the gas reached equilibrium by exchanging harmonic oscillator quanta with quantized Planck resonators. Nernst’s theory was flawed. But Einstein adopted a corrected version at the 1911 Solvay Conference, and in 1913, he and Otto Stern published a detailed treatment. Following Nernst, Einstein and Stern did not quantize the rotators. But they did explore the new zero- point energy that Max Planck had introduced in his “second quantum theory” in 1911. Einstein and Stern calculated the specific heat of hydrogen for two cases, one that assumed a zero-point energy for a rotator and one that did not. -
Dr. Julie Brown, CTO of UDC, Awarded Prestigious 2020 Karl Ferdinand Braun Prize from the Society of Information Display
8/3/2020 Dr. Julie Brown, CTO of UDC, Awarded Prestigious 2020 Karl Ferdinand Braun Prize from the Society of Information Display Dr. Mike Weaver, VP of UDC, Honored with 2020 SID Fellow Award EWING, N.J.--(BUSINESS WIRE)-- Universal Display Corporation (Nasdaq: OLED), enabling energy-efficient displays and lighting with its UniversalPHOLED® technology and materials, today announced that Dr. Julie Brown, Senior Vice President and Chief Technical Officer, was awarded the 2020 Karl Ferdinand Braun Prize by the Society of Information Display (SID). Additionally, Dr. Mike Weaver, Vice President of PHOLED R&D, was named a 2020 SID Fellow. The Karl Ferdinand Braun Prize was awarded to Dr. Brown for her outstanding technical achievements and contributions to the development and commercialization of phosphorescent OLED materials and display technology. The Society for Information Display created this prize in 1987 in honor of the German physicist and Nobel Laureate Karl Ferdinand Braun who invented the cathode-ray tube (CRT). Dr. Brown has been a leading innovator in the discovery and development of state-of-the-art OLED technologies and materials for display and lighting applications for over two decades, and is the first woman to be awarded this prestigious prize. Joining Universal Display (UDC) in 1998, Dr. Brown leads a global team of unique chemists, physicists and engineers and spearheads the R&D vision of UDC, from its start-up years to its successful commercial present, and continues to create and shape the Company’s innovation strategy for its future growth. The distinction of Fellow honors an SID member of outstanding qualifications and experience as a scientist or engineer in the field of information display. -
Von Richthofen, Einstein and the AGA Estimating Achievement from Fame
Von Richthofen, Einstein and the AGA Estimating achievement from fame Every schoolboy has heard of Einstein; fewer have heard of Antoine Becquerel; almost nobody has heard of Nils Dalén. Yet they all won Nobel Prizes for Physics. Can we gauge a scientist’s achievements by his or her fame? If so, how? And how do fighter pilots help? Mikhail Simkin and Vwani Roychowdhury look for the linkages. “It was a famous victory.” We instinctively rank the had published. However, in 2001–2002 popular French achievements of great men and women by how famous TV presenters Igor and Grichka Bogdanoff published they are. But is instinct enough? And how exactly does a great man’s fame relate to the greatness of his achieve- ment? Some achievements are easy to quantify. Such is the case with fighter pilots of the First World War. Their achievements can be easily measured and ranked, in terms of their victories – the number of enemy planes they shot down. These aces achieved varying degrees of fame, which have lasted down to the internet age. A few years ago we compared1 the fame of First World War fighter pilot aces (measured in Google hits) with their achievement (measured in victories); and we found that We can estimate fame grows exponentially with achievement. fame from Google; Is the same true in other areas of excellence? Bagrow et al. have studied the relationship between can this tell us 2 achievement and fame for physicists . The relationship Manfred von Richthofen (in cockpit) with members of his so- about actual they found was linear. -
The Physical Tourist Physics and New York City
Phys. perspect. 5 (2003) 87–121 © Birkha¨user Verlag, Basel, 2003 1422–6944/05/010087–35 The Physical Tourist Physics and New York City Benjamin Bederson* I discuss the contributions of physicists who have lived and worked in New York City within the context of the high schools, colleges, universities, and other institutions with which they were and are associated. I close with a walking tour of major sites of interest in Manhattan. Key words: Thomas A. Edison; Nikola Tesla; Michael I. Pupin; Hall of Fame for GreatAmericans;AlbertEinstein;OttoStern;HenryGoldman;J.RobertOppenheimer; Richard P. Feynman; Julian Schwinger; Isidor I. Rabi; Bronx High School of Science; StuyvesantHighSchool;TownsendHarrisHighSchool;NewYorkAcademyofSciences; Andrei Sakharov; Fordham University; Victor F. Hess; Cooper Union; Peter Cooper; City University of New York; City College; Brooklyn College; Melba Phillips; Hunter College; Rosalyn Yalow; Queens College; Lehman College; New York University; Courant Institute of Mathematical Sciences; Samuel F.B. Morse; John W. Draper; Columbia University; Polytechnic University; Manhattan Project; American Museum of Natural History; Rockefeller University; New York Public Library. Introduction When I was approached by the editors of Physics in Perspecti6e to prepare an article on New York City for The Physical Tourist section, I was happy to do so. I have been a New Yorker all my life, except for short-term stays elsewhere on sabbatical leaves and other visits. My professional life developed in New York, and I married and raised my family in New York and its environs. Accordingly, writing such an article seemed a natural thing to do. About halfway through its preparation, however, the attack on the World Trade Center took place. -
A Brief History of Nuclear Astrophysics
A BRIEF HISTORY OF NUCLEAR ASTROPHYSICS PART I THE ENERGY OF THE SUN AND STARS Nikos Prantzos Institut d’Astrophysique de Paris Stellar Origin of Energy the Elements Nuclear Astrophysics Astronomy Nuclear Physics Thermodynamics: the energy of the Sun and the age of the Earth 1847 : Robert Julius von Mayer Sun heated by fall of meteors 1854 : Hermann von Helmholtz Gravitational energy of Kant’s contracting protosolar nebula of gas and dust turns into kinetic energy Timescale ~ EGrav/LSun ~ 30 My 1850s : William Thompson (Lord Kelvin) Sun heated at formation from meteorite fall, now « an incadescent liquid mass » cooling Age 10 – 100 My 1859: Charles Darwin Origin of species : Rate of erosion of the Weald valley is 1 inch/century or 22 miles wild (X 1100 feet high) in 300 My Such large Earth ages also required by geologists, like Charles Lyell A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. Homer Lane ; 1880s :August Ritter : Sun gaseous Compressible As it shrinks, it releases gravitational energy AND it gets hotter Earth Mayer – Kelvin - Helmholtz Helmholtz - Ritter A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. Homer Lane ; 1880s :August Ritter : Sun gaseous Compressible As it shrinks, it releases gravitational energy AND it gets hotter Earth Mayer – Kelvin - Helmholtz Helmholtz - Ritter A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. -
Nobel Prizes Social Network
Nobel prizes social network Marie Skłodowska Curie (Phys.1903, Chem.1911) Nobel prizes social network Henri Becquerel (Phys.1903) Pierre Curie (Phys.1903) = Marie Skłodowska Curie (Phys.1903, Chem.1911) Nobel prizes social network Henri Becquerel (Phys.1903) Pierre Curie (Phys.1903) = Marie Skłodowska Curie (Phys.1903, Chem.1911) Irène Joliot-Curie (Chem.1935) Nobel prizes social network Henri Becquerel (Phys.1903) Pierre Curie (Phys.1903) = Marie Skłodowska Curie (Phys.1903, Chem.1911) Irène Joliot-Curie (Chem.1935) = Frédéric Joliot-Curie (Chem.1935) Nobel prizes social network Henri Becquerel (Phys.1903) Pierre Curie (Phys.1903) = Marie Skłodowska Curie (Phys.1903, Chem.1911) Paul Langevin Irène Joliot-Curie (Chem.1935) = Frédéric Joliot-Curie (Chem.1935) Nobel prizes social network Henri Becquerel (Phys.1903) Pierre Curie (Phys.1903) = Marie Skłodowska Curie (Phys.1903, Chem.1911) Paul Langevin Maurice de Broglie Louis de Broglie (Phys.1929) Irène Joliot-Curie (Chem.1935) = Frédéric Joliot-Curie (Chem.1935) Nobel prizes social network Sir J. J. Thomson (Phys.1906) Henri Becquerel (Phys.1903) Pierre Curie (Phys.1903) = Marie Skłodowska Curie (Phys.1903, Chem.1911) Paul Langevin Maurice de Broglie Louis de Broglie (Phys.1929) Irène Joliot-Curie (Chem.1935) = Frédéric Joliot-Curie (Chem.1935) Nobel prizes social network (more) Sir J. J. Thomson (Phys.1906) Nobel prizes social network (more) Sir J. J. Thomson (Phys.1906) Owen Richardson (Phys.1928) Nobel prizes social network (more) Sir J. J. Thomson (Phys.1906) Owen Richardson (Phys.1928) Clinton Davisson (Phys.1937) Nobel prizes social network (more) Sir J. J. Thomson (Phys.1906) Owen Richardson (Phys.1928) Charlotte Richardson = Clinton Davisson (Phys.1937) Nobel prizes social network (more) Sir J. -
50 31-01-2018 Time: 60 Min
8thAHMED BIN ABOOD MEMORIAL State Level Physics-Maths Knowledge Test-2018 Organized by Department of Physics Department of Mathematics Milliya Arts, Science and Management Science College, BEED Max. Marks: 50 31-01-2018 Time: 60 min Instructions:- All the questions carry equal marks. Mobile and Calculators are not allowed. Student must write his/her names, college name and allotted seat number on the response sheet provided. Student must stick the answer in the prescribed response sheet by completely blacken the oval with black/blue pen only. Incorrect Method Correct Method Section A 1) If the earth completely loses its gravity, then for any body……… (a) both mass and weight becomes zero (b) neither mass nor weight becomes zero (c) weight becomes zero but not the mass (d) mass becomes zero but not the weight 2) The angular speed of a flywheel is 3π rad/s. It is rotating at…….. (a) 3 rpm (b) 6 rpm (c) 90 rpm (d) 60 rpm 3) Resonance occurs when …. (a) a body vibrates at a frequency lower than its normal frequency. (b) a body vibrates at a frequency higher than its normal frequency. (c) a body is set into vibrations with its natural frequency of another body vibrating with the same frequency. (d) a body is made of the same material as the sound source. 4) The SI unit of magnetic flux density is…… (a) tesla (b) henry (c) volt (d) volt-second 5) Ampere’s circuital law is integral form of….. (a) Lenz’s law (b) Faraday’s law (c) Biot-Savart’s law (d) Coulomb’s law 1 6) The energy band gap is highest in the case of ……. -
Einstein and the Early Theory of Superconductivity, 1919–1922
Einstein and the Early Theory of Superconductivity, 1919–1922 Tilman Sauer Einstein Papers Project California Institute of Technology 20-7 Pasadena, CA 91125, USA [email protected] Abstract Einstein’s early thoughts about superconductivity are discussed as a case study of how theoretical physics reacts to experimental find- ings that are incompatible with established theoretical notions. One such notion that is discussed is the model of electric conductivity implied by Drude’s electron theory of metals, and the derivation of the Wiedemann-Franz law within this framework. After summarizing the experimental knowledge on superconductivity around 1920, the topic is then discussed both on a phenomenological level in terms of implications of Maxwell’s equations for the case of infinite conduc- tivity, and on a microscopic level in terms of suggested models for superconductive charge transport. Analyzing Einstein’s manuscripts and correspondence as well as his own 1922 paper on the subject, it is shown that Einstein had a sustained interest in superconductivity and was well informed about the phenomenon. It is argued that his appointment as special professor in Leiden in 1920 was motivated to a considerable extent by his perception as a leading theoretician of quantum theory and condensed matter physics and the hope that he would contribute to the theoretical direction of the experiments done at Kamerlingh Onnes’ cryogenic laboratory. Einstein tried to live up to these expectations by proposing at least three experiments on the arXiv:physics/0612159v1 [physics.hist-ph] 15 Dec 2006 phenomenon, one of which was carried out twice in Leiden. Com- pared to other theoretical proposals at the time, the prominent role of quantum concepts was characteristic of Einstein’s understanding of the phenomenon. -
William Lawrence Bragg
W ILLIAM L AWRENCE B R A G G The diffraction of X-rays by crystals Nobel Lecture, September 6, 1922* It is with the very greatest pleasure that I take this opportunity of expressing my gratitude to you for the great honour which you bestowed upon me, when you awarded my father and myself the Nobel Prize for Physics in the year 1915. In other years scientists have come here to express their thanks to you, who have received this great distinction for the work of an illustrious career devoted to research. That you should have given me, at the very out- set of my scientific career, even the most humble place amongst their ranks, is an honour of which I cannot but be very proud. You invited me here two years ago, after the end of the war, but a series of unfortunate circumstances made it impossible for me to accept your invi- tation. I have always profoundly regretted this, and it was therefore with the very greatest satisfaction that I received the invitation of Prof. Arrhenius a few months ago, and arranged for this visit. I am at last able to tell you how deeply grateful I am to you, and to give you my thanks in person. You have already honoured with the Nobel Prize Prof. von Laue, to whom we owe the great discovery which has made possible all progress in a new realm of science, the study of the structure of matter by the diffraction of X-rays. Prof von Laue, in his Nobel Lecture, has described to you how he was led to make his epochal discovery. -
Photon Mapping Superluminal Particles
EUROGRAPHICS 2020/ F. Banterle and A. Wilkie Short Paper Photon Mapping Superluminal Particles G. Waldemarson1;2 and M. Doggett2 1Arm Ltd, Sweden 2 Lund University, Sweden Abstract One type of light source that remains largely unexplored in the field of light transport rendering is the light generated by superluminal particles, a phenomenon more commonly known as Cherenkov radiation [C37ˇ ]. By re-purposing the Frank-Tamm equation [FT91] for rendering, the energy output of these particles can be estimated and consequently mapped to photons, making it possible to visualize the brilliant blue light characteristic of the effect. In this paper we extend a stochastic progressive photon mapper and simulate the emission of superluminal particles from a source object close to a medium with a high index of refraction. In practice, the source is treated as a new kind of light source, allowing us to efficiently reuse existing photon mapping methods. CCS Concepts • Computing methodologies ! Ray tracing; 1. Introduction in the direction of the particle but will not otherwise cross one an- other, as depicted in figure 1. However, if the particle travels faster In the late 19th and early 20th century, the phenomenon today than these spheres the waves will constructively interfere, generat- known as Cherenkov radiation were predicted and observed a num- ing coherent photons at an angle proportional to the velocity of the ber of times [Wat11] but it was first properly investigated in 1934 particle, similar to the propagation of a sonic boom from supersonic by Pavel Cherenkov under the supervision of Sergey Vavilov at the aircraft. Formally, this occurs when the criterion c0 = c < v < c Lebedev Institute [C37ˇ ].