National Institute for Subatomic Physics
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Hendrik Antoon Lorentz's Struggle with Quantum Theory A. J
Hendrik Antoon Lorentz’s struggle with quantum theory A. J. Kox Archive for History of Exact Sciences ISSN 0003-9519 Volume 67 Number 2 Arch. Hist. Exact Sci. (2013) 67:149-170 DOI 10.1007/s00407-012-0107-8 1 23 Your article is published under the Creative Commons Attribution license which allows users to read, copy, distribute and make derivative works, as long as the author of the original work is cited. You may self- archive this article on your own website, an institutional repository or funder’s repository and make it publicly available immediately. 1 23 Arch. Hist. Exact Sci. (2013) 67:149–170 DOI 10.1007/s00407-012-0107-8 Hendrik Antoon Lorentz’s struggle with quantum theory A. J. Kox Received: 15 June 2012 / Published online: 24 July 2012 © The Author(s) 2012. This article is published with open access at Springerlink.com Abstract A historical overview is given of the contributions of Hendrik Antoon Lorentz in quantum theory. Although especially his early work is valuable, the main importance of Lorentz’s work lies in the conceptual clarifications he provided and in his critique of the foundations of quantum theory. 1 Introduction The Dutch physicist Hendrik Antoon Lorentz (1853–1928) is generally viewed as an icon of classical, nineteenth-century physics—indeed, as one of the last masters of that era. Thus, it may come as a bit of a surprise that he also made important contribu- tions to quantum theory, the quintessential non-classical twentieth-century develop- ment in physics. The importance of Lorentz’s work lies not so much in his concrete contributions to the actual physics—although some of his early work was ground- breaking—but rather in the conceptual clarifications he provided and his critique of the foundations and interpretations of the new ideas. -
Einstein's Mistakes
Einstein’s Mistakes Einstein was the greatest genius of the Twentieth Century, but his discoveries were blighted with mistakes. The Human Failing of Genius. 1 PART 1 An evaluation of the man Here, Einstein grows up, his thinking evolves, and many quotations from him are listed. Albert Einstein (1879-1955) Einstein at 14 Einstein at 26 Einstein at 42 3 Albert Einstein (1879-1955) Einstein at age 61 (1940) 4 Albert Einstein (1879-1955) Born in Ulm, Swabian region of Southern Germany. From a Jewish merchant family. Had a sister Maja. Family rejected Jewish customs. Did not inherit any mathematical talent. Inherited stubbornness, Inherited a roguish sense of humor, An inclination to mysticism, And a habit of grüblen or protracted, agonizing “brooding” over whatever was on its mind. Leading to the thought experiment. 5 Portrait in 1947 – age 68, and his habit of agonizing brooding over whatever was on its mind. He was in Princeton, NJ, USA. 6 Einstein the mystic •“Everyone who is seriously involved in pursuit of science becomes convinced that a spirit is manifest in the laws of the universe, one that is vastly superior to that of man..” •“When I assess a theory, I ask myself, if I was God, would I have arranged the universe that way?” •His roguish sense of humor was always there. •When asked what will be his reactions to observational evidence against the bending of light predicted by his general theory of relativity, he said: •”Then I would feel sorry for the Good Lord. The theory is correct anyway.” 7 Einstein: Mathematics •More quotations from Einstein: •“How it is possible that mathematics, a product of human thought that is independent of experience, fits so excellently the objects of physical reality?” •Questions asked by many people and Einstein: •“Is God a mathematician?” •His conclusion: •“ The Lord is cunning, but not malicious.” 8 Einstein the Stubborn Mystic “What interests me is whether God had any choice in the creation of the world” Some broadcasters expunged the comment from the soundtrack because they thought it was blasphemous. -
Physical and Chemical Sciences 2010-2015 Utrecht University
RESEARCH REVIEW PHYSICAL AND CHEMICAL SCIENCES 2010-2015 UTRECHT UNIVERSITY Quality Assurance Netherlands Universities (QANU) Catharijnesingel 56 PO Box 8035 3503 RA Utrecht The Netherlands Phone: +31 (0) 30 230 3100 E-mail: [email protected] Internet: www.qanu.nl Project number: 0630 © 2017 QANU Text and numerical material from this publication may be reproduced in print, by photocopying or by any other means with the permission of QANU if the source is mentioned. 2 QANU / Research Review Physical and Chemical Sciences, Utrecht University REPORT ON THE RESEARCH REVIEW OF PHYSICAL AND CHEMICAL SCIENCES OF UTRECHT UNIVERSITY CONTENT 1. Foreword committee chair 5 2. The review committee and the procedures 7 2.1 Scope of the review 7 2.2 Composition of the committee 7 2.3 Independence 7 2.4 Data provided to the committee 7 2.5 Procedures followed by the committee 8 3. Quantitative and qualitative assessment of Physical and Chemical Sciences 9 3.1 Broader context 9 3.2 Research quality 10 3.3 Relevance to Society 11 3.4 Viability 13 3.5 PhD programmes 15 3.6 Research integrity policy 17 3.7 Diversity 18 3.8 Conclusion 19 3.9 Quantitative assessment of Physical and Chemical Sciences 20 4. Quantitative and qualitative assessment of the separate research institutes 21 4.1 Debye Institute for Nanomaterial Science 21 4.2 Institute for Marine and Atmospheric research 24 4.3 Institute for Theoretical Physics 27 4.4 Institute for Sub-Atomic Physics 30 5. Recommendations 33 Appendices 35 Appendix 1: Explanation of the SEP criteria and categories 37 Appendix 2: Curricula Vitae of the committee members 39 Appendix 3: Programme of the site visit 41 Appendix 4: Quantitative Data 47 QANU / Research Review Physical and Chemical Sciences, Utrecht University 3 4 QANU / Research Review Physical and Chemical Sciences, Utrecht University 1. -
Seismic Characterization of the Euregio Meuse-Rhine in View of Einstein Telescope
SEISMIC CHARACTERIZATION OF THE EUREGIO MEUSE-RHINE IN VIEW OF EINSTEIN TELESCOPE 13 September 2019 First results of seismic studies of the Belgian-Dutch-German site for Einstein Telescope Soumen Koley1, Maria Bader1, Alessandro Bertolini1, Jo van den Brand1,2, Henk Jan Bulten1,3, Stefan Hild1,2, Frank Linde1,4, Bas Swinkels1, Bjorn Vink5 1. Nikhef, National Institute for Subatomic Physics, Amsterdam, The Netherlands 2. Maastricht University, Maastricht, The Netherlands 3. VU University Amsterdam, Amsterdam, The Netherlands 4. University of Amsterdam, Amsterdam, The Netherlands 5. Antea Group, Maastricht, The Netherlands CONFIDENTIAL Figure 1: Artist impression of the Einstein Telescope gravitational wave observatory situated at a depth of 200-300 meters in the Euregio Meuse-Rhine landscape. The triangular topology with 10 kilometers long arms allows for the installation of multiple so-called laser interferometers. Each of which can detect ripples in the fabric of space-time – the unique signature of a gravitational wave – as minute relative movements of the mirrors hanging at the bottom of the red and white towers indicated in the illustration at the corners of the triangle. 1 SEISMIC CHARACTERIZATION OF THE EUREGIO MEUSE-RHINE IN VIEW OF EINSTEIN TELESCOPE Figure 2: Drill rig for the 2018-2019 campaign used for the completion of the 260 meters deep borehole near Terziet on the Dutch-Belgian border in South Limburg. Two broadband seismic sensors were installed: one at a depth of 250 meters and one just below the surface. Both sensors are accessible via the KNMI portal: http://rdsa.knmi.nl/dataportal/. 2 SEISMIC CHARACTERIZATION OF THE EUREGIO MEUSE-RHINE IN VIEW OF EINSTEIN TELESCOPE Executive summary The European 2011 Conceptual Design Report for Einstein Telescope identified the Euregio Meuse-Rhine and in particular the South Limburg border region as one of the prospective sites for this next generation gravitational wave observatory. -
De Nobelprijzen Komen Eraan!
De Nobelprijzen komen eraan! De Nobelprijzen komen eraan! In de loop van volgende week worden de Nobelprijswinnaars van dit jaar aangekondigd. Daarna weten we wie in december deze felbegeerde prijzen in ontvangst mogen gaan nemen. De Nobelprijzen zijn wellicht de meest prestigieuze en bekende academische onderscheidingen ter wereld, maar waarom eigenlijk? Hoe zijn de prijzen ontstaan, en wie was hun grondlegger, Alfred Nobel? Afbeelding 1. Alfred Nobel.Alfred Nobel (1833-1896) was de grondlegger van de Nobelprijzen. Volgende week is de jaarlijkse aankondiging van de prijswinnaard. Alfred Nobel Alfred Nobel was een belangrijke negentiende-eeuwse Zweedse scheikundige en uitvinder. Hij werd geboren in Stockholm in 1833 in een gezin met acht kinderen. Zijn vader, Immanuel Nobel, was een werktuigkundige en uitvinder die succesvol was met het maken van wapens en stoommotoren. Immanuel wou dat zijn zonen zijn bedrijf zouden overnemen en stuurde Alfred daarom op een twee jaar durende reis naar onder andere Duitsland, Frankrijk en de Verenigde Staten, om te leren over chemische werktuigbouwkunde. In Parijs ontmoette bron: https://www.quantumuniverse.nl/de-nobelprijzen-komen-eraan Pagina 1 van 5 De Nobelprijzen komen eraan! Alfred de Italiaanse scheikundige Ascanio Sobrero, die drie jaar eerder het explosief nitroglycerine had ontdekt. Nitroglycerine had een veel grotere explosieve kracht dan het buskruit, maar was ook veel gevaarlijker om te gebruiken omdat het instabiel is. Alfred raakte geinteresseerd in nitroglycerine en hoe het gebruikt kon worden voor commerciele doeleinden, en ging daarom werken aan de stabiliteit en veiligheid van de stof. Een makkelijk project was dit niet, en meerdere malen ging het flink mis. -
Kamerlingh Onnes Laboratory and Lorentz Institute
europhysicsnews 2015 • Volume 46 • number 2 Europhysics news is the magazine of the European physics community. It is owned by the European Physical Society and produced in cooperation with EDP Sciences. The staff of EDP Sciences are involved in the production of the magazine and are not responsible for editorial content. Most contributors to Europhysics news are volunteers and their work is greatly appreciated EPS HISTORIC SITES by the Editor and the Editorial Advisory Board. Europhysics news is also available online at: www.europhysicsnews.org General instructions to authors can be found at: www.eps.org/?page=publications Kamerlingh Onnes Laboratory Editor: Victor R. Velasco (SP) Email: [email protected] and Lorentz Institute Science Editor: Jo Hermans (NL) Email: [email protected] Leiden, The Netherlands Executive Editor: David Lee Email: [email protected] Graphic designer: Xavier de Araujo ‘The coldest place on earth’ Email: [email protected] Director of Publication: Jean-Marc Quilbé Editorial Advisory Board: Gonçalo Figueira (PT), Guillaume Fiquet (FR), On 9 February 2015, the site of the former Physics Zsolt Fülöp (Hu), Adelbert Goede (NL), Agnès Henri (FR), Martin Huber (CH), Robert Klanner (DE), Laboratory of Leiden University was officially Peter Liljeroth (FI), Stephen Price (UK), recognised as one of the ‘EPS Historic Sites’ Laurence Ramos (FR), Chris Rossel (CH), Claude Sébenne (FR), Marc Türler (CH) of the European Physical Society. On that day © European Physical Society and EDP Sciences EPS president-elect Christophe Rossel unveiled EPS Secretariat the commemorative plaque near the present-day Address: EPS • 6 rue des Frères Lumière 68200 Mulhouse • France entrance to the complex (since 2004 the location Tel: +33 389 32 94 40 • fax: +33 389 32 94 49 of Leiden University’s Law Faculty). -
Scientific References for Nobel Physics Prizes
1 Scientific References for Nobel Physics Prizes © Dr. John Andraos, 2004 Department of Chemistry, York University 4700 Keele Street, Toronto, ONTARIO M3J 1P3, CANADA For suggestions, corrections, additional information, and comments please send e-mails to [email protected] http://www.chem.yorku.ca/NAMED/ 1901 - Wilhelm Conrad Roentgen "in recognition of the extraordinary services he has rendered by the discovery of the remarkable rays subsequently named after him." Roentgen X-ray Roentgen, W.C. Ann. Physik 1898, 64 , 1 Stanton, A. Science 1896, 3 , 227; 726 (translation) 1902 - Hendrik Antoon Lorentz and Pieter Zeeman "in recognition of the extraordinary service they rendered by their researches into the influence of magnetism upon radiation phenomena." Zeeman effect Zeeman, P., Verhandlungen der Physikalischen Gesellschaft zu Berlin 1896, 7 , 128 Zeeman, P., Nature 1897, 55 , 347 (translation by A. Stanton) 1903 - Antoine Henri Becquerel "in recognition of the extraordinary service he has rendered by his discovery of spontaneous radioactivity." Becquerel, A.H. Compt. Rend. 1896, 122 , 420; 501; 559; 689; 1086 Becquerel, A.H. Compt. Rend. 1896, 123 , 855 Becquerel, A.H. Compt. Rend. 1897, 124 , 444; 800 Becquerel, A.H. Compt. Rend. 1899, 129 , 996; 1205 Becquerel, A.H. Compt. Rend. 1900, 130 , 327; 809; 1583 Becquerel, A.H. Compt. Rend. 1900, 131 , 137 Becquerel, A.H. Compt. Rend. 1901, 133 , 977 1903 - Pierre Curie and Marie Curie, nee Sklodowska "in recognition of the extraordinary services they have rendered by their joint researches on the radiation phenomena discovered by Professor Henri Becquerel." Curie unit of radiation Curie, P; Desains, P., Compt. Rend. -
Spectroscopy & the Nobel
Newsroom 1971 CHEMISTRY NOBEL OSA Honorary Member Gerhard Herzberg “for his contributions to the knowledge of electronic structure and geometry of molecules, particularly free radicals” 1907 PHYSICS NOBEL 1930 PHYSICS NOBEL 1966 CHEMISTRY NOBEL OSA Honorary Member Albert OSA Honorary Member Sir Robert S. Mulliken “for Abraham Michelson “for his Chandrasekhara Venkata his fundamental work optical precision instruments Raman “for his work on the concerning chemical bonds and the spectroscopic and scattering of light and for and the electronic structure metrological investigations the discovery of the effect of molecules by the carried out with their aid” named after him” molecular orbital method” 1902 PHYSICS NOBEL 1919 PHYSICS NOBEL Hendrik Antoon Lorentz and Johannes Stark “for his Pieter Zeeman “for their discovery of the Doppler researches into the influence effect in canal rays and of magnetism upon radiation the splitting of spectral phenomena” lines in electric fields” 1955 PHYSICS NOBEL OSA Honorary Member Willis Eugene Lamb “for his discoveries concerning the fine structure of the hydrogen Spectroscopy spectrum” & the Nobel ctober is when scientists around the world await the results from Stockholm. O Since the Nobel Prize was established in 1895, a surprising number of the awards have gone to advances related to or enabled by spectroscopy—from the spectral splitting of the Zeeman and Stark effects to cutting-edge advances enabled by laser frequency combs. We offer a small (and far from complete) sample here; to explore further, visit www.nobelprize.org. 16 OPTICS & PHOTONICS NEWS OCTOBER 2018 1996 CHEMISTRY NOBEL OSA Fellow Robert F. Curl Jr., Richard Smalley and Harold 1999 CHEMISTRY NOBEL Kroto (not pictured) “for their Ahmed H. -
Liste Der Nobelpreisträger
Physiologie Wirtschafts- Jahr Physik Chemie oder Literatur Frieden wissenschaften Medizin Wilhelm Henry Dunant Jacobus H. Emil von Sully 1901 Conrad — van ’t Hoff Behring Prudhomme Röntgen Frédéric Passy Hendrik Antoon Theodor Élie Ducommun 1902 Emil Fischer Ronald Ross — Lorentz Mommsen Pieter Zeeman Albert Gobat Henri Becquerel Svante Niels Ryberg Bjørnstjerne 1903 William Randal Cremer — Pierre Curie Arrhenius Finsen Bjørnson Marie Curie Frédéric John William William Mistral 1904 Iwan Pawlow Institut de Droit international — Strutt Ramsay José Echegaray Adolf von Henryk 1905 Philipp Lenard Robert Koch Bertha von Suttner — Baeyer Sienkiewicz Camillo Golgi Joseph John Giosuè 1906 Henri Moissan Theodore Roosevelt — Thomson Santiago Carducci Ramón y Cajal Albert A. Alphonse Rudyard \Ernesto Teodoro Moneta 1907 Eduard Buchner — Michelson Laveran Kipling Louis Renault Ilja Gabriel Ernest Rudolf Klas Pontus Arnoldson 1908 Metschnikow — Lippmann Rutherford Eucken Paul Ehrlich Fredrik Bajer Theodor Auguste Beernaert Guglielmo Wilhelm Kocher Selma 1909 — Marconi Ostwald Ferdinand Lagerlöf Paul Henri d’Estournelles de Braun Constant Johannes Albrecht Ständiges Internationales 1910 Diderik van Otto Wallach Paul Heyse — Kossel Friedensbüro der Waals Allvar Maurice Tobias Asser 1911 Wilhelm Wien Marie Curie — Gullstrand Maeterlinck Alfred Fried Victor Grignard Gerhart 1912 Gustaf Dalén Alexis Carrel Elihu Root — Paul Sabatier Hauptmann Heike Charles Rabindranath 1913 Kamerlingh Alfred Werner Henri La Fontaine — Robert Richet Tagore Onnes Theodore -
Sun – Part 20 – Solar Magnetic Field 2 – Zeeman Effect
Sun – Part 20 - Solar magnetic field 2 – Zeeman effect The Zeeman effect The effect in a solar spectral line Pieter Zeeman This is a means of measuring a magnetic field from a distance, one that is particularly useful in astronomy where such measurements for stars have to be made indirectly. Use of the Zeeman effect is particularly important in relation to the Sun's magnetic field because of the central role played by the solar magnetic field in solar activity eg solar flares, coronal mass ejections, which can, potentially, pose a serious hazard to many aspects of human life. The Zeeman effect is the splitting of a spectral line into several components due to the presence of a static magnetic field. Normally, atoms in a star’s atmosphere will absorb a certain frequency of energy in the electromagnetic spectrum. However, when the atoms are within a magnetic field, these lines become split into multiple, closely spaced lines. For example, under normal conditions, an atomic spectral line of 400nm would be single. However, in a strong magnetic field, because of the Zeeman effect, the line would be split to yield a more energetic line and a less energetic line, in addition to the original line. The distance between the splits is a function of the magnetic field, so this effect can be used to measure the magnetic fields of the Sun and other stars. The energy also becomes polarised, with an orientation depending on the orientation of the magnetic field. Thus, strength and direction of a star’s magnetic field can be determined by study of Zeeman effect lines. -
Hendrik Antoon Lorentz 1853 - 1928 Awarded the Nobel Prize for Physics in 1902
Hendrik Antoon Lorentz 1853 - 1928 Awarded the Nobel Prize for Physics in 1902 In the early 1890s electrons had not yet been discovered. The famous Dutch physicist Hendrik Lorentz postulated the existence of tiny charged particles to explain a number of physical phenomena. Lorentz argued that electromagnetic radiation is produced by the vibration of these charged particles. Soon, the English physicist J.J. Thomson discovered these particles ('electrons') experimentally. You may know that the spectral lines are an optical phenomenon, and they appear when the light from a gas flame is split into different colors. An important consequence of Lorentz's electron theory was the prediction that spectral lines would split if the source of light from which they come is placed within a strong magnetic field. Lorentz supposed that the presence of a magnetic field would alter the motion of the charged particles in the light source which produced the spectral lines, causing them to shift their position. In 1902 Lorentz and his countryman Pieter Zeeman were awarded the Nobel Prize for Physics for the discovery and explanation of the splitting of spectral lines. He explained mathematically the length contraction of an object Hendrik Antoon Lorentz was born in Arnhem in the Netherlands, on July 18th, 1853. His father was the owner of a nursery, his mother died when Hendrik was only four years old, and his father moving at relativistic speed married for a second time. The stepmother seemed to have taken good care of him and his younger brother. In 1870 Lorentz entered the University of Leiden, where he studied physics and mathematics. -
Letter of Interest Fundamental Physics with Gravitational Wave Detectors
Snowmass2021 - Letter of Interest Fundamental physics with gravitational wave detectors Thematic Areas: (check all that apply /) (CF1) Dark Matter: Particle Like (CF2) Dark Matter: Wavelike (CF3) Dark Matter: Cosmic Probes (CF4) Dark Energy and Cosmic Acceleration: The Modern Universe (CF5) Dark Energy and Cosmic Acceleration: Cosmic Dawn and Before (CF6) Dark Energy and Cosmic Acceleration: Complementarity of Probes and New Facilities (CF7) Cosmic Probes of Fundamental Physics (TF09) Cosmology Theory (TF10) Quantum Information Science Theory Contact Information: Emanuele Berti (Johns Hopkins University) [[email protected]], Vitor Cardoso (Instituto Superior Tecnico,´ Lisbon) [[email protected]], Bangalore Sathyaprakash (Pennsylvania State University & Cardiff University) [[email protected]], Nicolas´ Yunes (University of Illinois at Urbana-Champaign) [[email protected]] Authors: (see long author lists after the text) Abstract: (maximum 200 words) Gravitational wave detectors are formidable tools to explore black holes and neutron stars. These com- pact objects are extraordinarily efficient at producing electromagnetic and gravitational radiation. As such, they are ideal laboratories for fundamental physics and they have an immense discovery potential. The detection of merging black holes by third-generation Earth-based detectors and space-based detectors will provide exquisite tests of general relativity. Loud “golden” events and extreme mass-ratio inspirals can strengthen the observational evidence for horizons by mapping the exterior spacetime geometry, inform us on possible near-horizon modifications, and perhaps reveal a breakdown of Einstein’s gravity. Measure- ments of the black-hole spin distribution and continuous gravitational-wave searches can turn black holes into efficient detectors of ultralight bosons across ten or more orders of magnitude in mass.