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Fotonica Ed Elettronica Quantistica
Fotonica ed elettronica quantistica http://www.dsf.unica.it/~fotonica/teaching/fotonica.html Fotonica ed elettronica quantistica Quantum optics - Quantization of electromagnetic field - Statistics of light, photon counting and noise; - HBT and correlation; g1 e g2 coherence; antibunching; single photons - Squeezing - Quantum cryptography - Quantum computer, entanglement and teleportation Light-matter Interaction - Two-level atom - Laser physics - Spectroscopy - Electronics and photonics at the nanometer scale - Cold atoms - Photodetectors - Solar cells http://www.dsf.unica.it/~fotonica/teaching/fotonica.html Energy Temperature LHC at CERN, Higgs, SUSY, ??? TeV 15 q q particle accelerators 10 K q GeV proton rest mass - quarks 1012K MeV electron rest mass / gamma rays 109K keV Nuclear Fusion, x rays, Sun center 106K Atoms ionize - visible light eV Sun surface fundamental components components fundamental room temperature 103K meV Liquid He, superconductors, space 1K dilution refrigerators, quantum Hall µeV laser-cooled atoms 10-3K neV Bose-Einstein condensates 10-6K peV low T record 480 picokelvin 10-9K -12 complexity, organization organization complexity, 10 K Nobel Prizes in Physics 2010 - Andre Geims, Konstantin Novoselov 2009 - Charles K. Kao, Willard S. Boyle, George E. Smith 2007 - Albert Fert, Peter Gruenberg 2005 - Roy J. Glauber, John L. Hall, Theodor W. Hänsch 2001 - Eric A. Cornell, Wolfgang Ketterle, Carl E. Wieman 1997 - Steven Chu, Claude Cohen-Tannoudji, William D. Phillips 1989 - Norman F. Ramsey, Hans G. Dehmelt, Wolfgang Paul 1981 - Nicolaas Bloembergen, Arthur L. Schawlow, Kai M. Siegbahn 1966 - Alfred Kastler 1964 - Charles H. Townes, Nicolay G. Basov, Aleksandr M. Prokhorov 1944 - Isidor Isaac Rabi 1930 - Venkata Raman 1921 - Albert Einstein 1907 - Albert A. -
Frontiers of Quantum and Mesoscopic Thermodynamics 29 July - 3 August 2013, Prague, Czech Republic
Frontiers of Quantum and Mesoscopic Thermodynamics 29 July - 3 August 2013, Prague, Czech Republic Under the auspicies of Ing. Milosˇ Zeman President of the Czech Republic Milan Stˇ echˇ President of the Senate of the Parliament of the Czech Republic Prof. Ing. Jirˇ´ı Drahos,ˇ DrSc., dr. h. c. President of the Academy of Sciences of the Czech Republic Dominik Cardinal Duka OP Archbishop of Prague Supported by • Committee on Education, Science, Culture, Human Rights and Petitions of the Senate of the Parliament of the Czech Republic • Institute of Physics, the Academy of Sciences of the Czech Republic • Institute for Theoretical Physics, University of Amsterdam, The Netherlands • Department of Physics, Texas A&M University, USA • Institut de Physique Theorique,´ CEA/CNRS Saclay, France Topics • Foundations of quantum physics • Non-equilibrium statistical physics • Quantum thermodynamics • Quantum measurement, entanglement and coherence • Dissipation, dephasing, noise and decoherence • Quantum optics • Macroscopic quantum behavior, e.g., cold atoms, Bose-Einstein condensates • Physics of quantum computing and quantum information • Mesoscopic, nano-electromechanical and nano-optical systems • Biological systems, molecular motors • Cosmology, gravitation and astrophysics Scientific Committee Chair: Theo M. Nieuwenhuizen (University of Amsterdam) Co-Chair: Vaclav´ Spiˇ ckaˇ (Institute of Physics, Acad. Sci. CR, Prague) Raymond Dean Astumian (University of Maine, Orono) Roger Balian (IPhT, Saclay) Gordon Baym (University of Illinois at Urbana -
Laboratoire Kastler Brossel, LKB, ENS PARIS, Sorbonne Université, COLL DE FRANCE, CNRS, Mr Antoine HEIDMANN
Research evaluation REPORT ON THE RESEARCH UNIT: Kastler Brossel Laboratory LKB UNDER THE SUPERVISION OF THE FOLLOWING INSTITUTIONS AND RESEARCH BODIES: École Normale Supérieure Sorbonne Université Collège de France Centre National de la Recherche Scientifique - CNRS EVALUATION CAMPAIGN 2017-2018 GROUP D In the name of Hcéres1 : In the name of the expert committee2 : Michel Cosnard, President Vahid Sandoghdar, Chairman of the committee Under the decree No.2014-1365 dated 14 November 2014, 1 The president of HCERES "countersigns the evaluation reports set up by the expert committees and signed by their chairman." (Article 8, paragraph 5); 2 The evaluation reports "are signed by the chairman of the expert committee". (Article 11, paragraph 2). Laboratoire Kastler Brossel, LKB, ENS PARIS, Sorbonne Université, COLL DE FRANCE, CNRS, Mr Antoine HEIDMANN This report is the sole result of the unit’s evaluation by the expert committee, the composition of which is specified below. The assessments contained herein are the expression of an independent and collegial reviewing by the committee. UNIT PRESENTATION Unit name: Laboratoire Kastler-Brossel Unit acronym: LKB Requested label: UMR Application type: Renewal Current number: UMR 8552 Head of the unit Mr Antoine HEIDMANN (2017-2018): Project leader Mr Antoine HEIDMANN (2019-2023): Number of teams: 12 COMMITTEE MEMBERS Chair: Mr Vahid SANDOGHDAR, Max Planck Institute, Germany Experts: Mr Jean-Claude BERNARD, CNRS (supporting personnel) Mr Benoît BOULANGER, Université Grenoble Alpes (representative -
Booklet 2008-09.Indd
The Shaw Prize The Shaw Prize is an international award to honour individuals who are currently active in their respective fields and who have achieved distinguished and significant advances, who have made outstanding contributions in culture and the arts, or who in other domains have achieved excellence. The award is dedicated to furthering societal progress, enhancing quality of life, and enriching humanity’s spiritual civilization. Preference will be given to individuals whose significant work was recently achieved. Founder's Biographical Note The Shaw Prize was established under the auspices of Mr Run Run Shaw. Mr Shaw, born in China in 1907, is a native of Ningbo County, Zhejiang Province. He joined his brother’s film company in China in the 1920s. In the 1950s he founded the film company Shaw Brothers (Hong Kong) Limited in Hong Kong. He has been Executive Chairman of Television Broadcasts Limited in Hong Kong since the 1970s. Mr Shaw has also founded two charities, The Sir Run Run Shaw Charitable Trust and The Shaw Foundation Hong Kong, both dedicated to the promotion of education, scientific and technological research, medical and welfare services, and culture and the arts. ~ 1 ~ Message from the Chief Executive I am delighted to congratulate the six distinguished scientists who receive this year’s Shaw Prize. Their accomplishments enrich human knowledge and have a profound impact on the advancement of science. This year, the Shaw Prize recognises remarkable achievements in the areas of astronomy, life science and medicine, and mathematical sciences. The exemplary work and dedication of this year’s recipients vividly demonstrate that constant drive for excellence will eventually bear fruit. -
Luis Alvarez: the Ideas Man
CERN Courier March 2012 Commemoration Luis Alvarez: the ideas man The years from the early 1950s to the late 1980s came alive again during a symposium to commemorate the birth of one of the great scientists and inventors of the 20th century. Luis Alvarez – one of the greatest experimental physicists of the 20th century – combined the interests of a scientist, an inventor, a detective and an explorer. He left his mark on areas that ranged from radar through to cosmic rays, nuclear physics, particle accel- erators, detectors and large-scale data analysis, as well as particles and astrophysics. On 19 November, some 200 people gathered at Berkeley to commemorate the 100th anniversary of his birth. Alumni of the Alvarez group – among them physicists, engineers, programmers and bubble-chamber film scanners – were joined by his collaborators, family, present-day students and admirers, as well as scientists whose professional lineage traces back to him. Hosted by the Lawrence Berkeley National Laboratory (LBNL) and the University of California at Berkeley, the symposium reviewed his long career and lasting legacy. A recurring theme of the symposium was, as one speaker put it, a “Shakespeare-type dilemma”: how could one person have accom- plished all of that in one lifetime? Beyond his own initiatives, Alvarez created a culture around him that inspired others to, as George Smoot put it, “think big,” as well as to “think broadly and then deep” and to take risks. Combined with Alvarez’s strong scientific standards and great care in execut- ing them, these principles led directly to the awarding of two Nobel Luis Alvarez celebrating the announcement of his 1968 Nobel prizes in physics to scientists at Berkeley – George Smoot in 2006 prize. -
I. I. Rabi Papers [Finding Aid]. Library of Congress. [PDF Rendered Tue Apr
I. I. Rabi Papers A Finding Aid to the Collection in the Library of Congress Manuscript Division, Library of Congress Washington, D.C. 1992 Revised 2010 March Contact information: http://hdl.loc.gov/loc.mss/mss.contact Additional search options available at: http://hdl.loc.gov/loc.mss/eadmss.ms998009 LC Online Catalog record: http://lccn.loc.gov/mm89076467 Prepared by Joseph Sullivan with the assistance of Kathleen A. Kelly and John R. Monagle Collection Summary Title: I. I. Rabi Papers Span Dates: 1899-1989 Bulk Dates: (bulk 1945-1968) ID No.: MSS76467 Creator: Rabi, I. I. (Isador Isaac), 1898- Extent: 41,500 items ; 105 cartons plus 1 oversize plus 4 classified ; 42 linear feet Language: Collection material in English Location: Manuscript Division, Library of Congress, Washington, D.C. Summary: Physicist and educator. The collection documents Rabi's research in physics, particularly in the fields of radar and nuclear energy, leading to the development of lasers, atomic clocks, and magnetic resonance imaging (MRI) and to his 1944 Nobel Prize in physics; his work as a consultant to the atomic bomb project at Los Alamos Scientific Laboratory and as an advisor on science policy to the United States government, the United Nations, and the North Atlantic Treaty Organization during and after World War II; and his studies, research, and professorships in physics chiefly at Columbia University and also at Massachusetts Institute of Technology. Selected Search Terms The following terms have been used to index the description of this collection in the Library's online catalog. They are grouped by name of person or organization, by subject or location, and by occupation and listed alphabetically therein. -
Laser Spectroscopy to Resolve Hyperfine Structure of Rubidium
Laser spectroscopy to resolve hyperfine structure of rubidium Hannah Saddler, Adam Egbert, and Will Weigand (Dated: 12 November 2015) This experiment had two main goals: to create an absorption spectrum for rubidium using the technique of absorption spectroscopy and to resolve the hyperfine structures for the two rubidium isotopes using saturation absorption spectroscopy. The absorption spectrum was used to determine the frequency difference between the ground state and first excited state for both isotopes. The calculated frequency difference was 6950 MHz ± 90 MHz for rubidium 87 and 3060 MHz ± 60 MHz for rubidium 85. Both values agree with the literature values. The hyperfine structure for rubidium 87 was able to be resolved using this experimental setup. The energy differences were determined to be 260 MHz ± 10 MHz and 150 MHz ± 10 Mhz MHz. The hyperfine structure for rubidium 85 was unable to be resolved using this experimental setup. Additionally the theory of doppler broadening was used to make measurements of the full width half maximum. These values were used to calculate a temperature of 310K ± 40 K which makes sense because the experiments were performed at room temperature. I. INTRODUCTION in the theory section and how they were manipulated and used to derive the results from the recorded data. Addi- tionally there is an explanation of experimental error and The era of modern spectroscopy began with the in- uncertainty associated the results. Section V is a conclu- vention of the laser. The word laser was originally an sion that ties the results of the experiment we performed acronym that stood for light amplification by stimulated to the usefulness of the technique of laser spectroscopy. -
Enrico Fermi
Fermi, Enrico Inventors and Inventions Enrico Fermi Italian American physicist Fermi helped develop Fermi-Dirac statistics, which liceo (secondary school) and, on the advice of Amidei, elucidate the group behavior of elementary particles. joined the Scuola Normale Superiore at Pisa. This elite He also developed the theory of beta decay and college, attached to the University of Pisa, admitted only discovered neutron-induced artificial radioactivity. forty of Italy’s top students, who were given free board Finally, he succeeded in producing the first sustained and lodging. Fermi performed exceedingly well in the nuclear chain reaction, which led to the discovery highly competitive entrance exam. He completed his of nuclear energy and the development of the university education after only four years of research and atomic bomb. studies, receiving his Ph.D. in physics from the Univer- sity of Pisa and his undergraduate diploma from the Born: September 29, 1901; Rome, Italy Scuola Normale Superiore in July, 1922. He became Died: November 28, 1954; Chicago, Illinois an expert theoretical physicist and a talented exper- Primary field: Physics imentalist. This rare combination provided a solid foun- Primary inventions: Controlled nuclear chain dation for all his subsequent inventions. reaction; Fermi-Dirac statistics; theory of beta decay Life’s Work After postdoctoral work at the University of Göttingen, Early Life in Germany (1922-1923), and the University of Leiden, Enrico Fermi (ehn-REE-koh FUR-mee) was the third in the Netherlands (fall, 1924), Fermi took an interim po- child of Alberto Fermi and Ida de Gattis. Enrico was very sition at the University of Florence in December, 1924. -
Science & ROGER PENROSE
Science & ROGER PENROSE Live Webinar - hosted by the Center for Consciousness Studies August 3 – 6, 2021 9:00 am – 12:30 pm (MST-Arizona) each day 4 Online Live Sessions DAY 1 Tuesday August 3, 2021 9:00 am to 12:30 pm MST-Arizona Overview / Black Holes SIR ROGER PENROSE (Nobel Laureate) Oxford University, UK Tuesday August 3, 2021 9:00 am – 10:30 am MST-Arizona Roger Penrose was born, August 8, 1931 in Colchester Essex UK. He earned a 1st class mathematics degree at University College London; a PhD at Cambridge UK, and became assistant lecturer, Bedford College London, Research Fellow St John’s College, Cambridge (now Honorary Fellow), a post-doc at King’s College London, NATO Fellow at Princeton, Syracuse, and Cornell Universities, USA. He also served a 1-year appointment at University of Texas, became a Reader then full Professor at Birkbeck College, London, and Rouse Ball Professor of Mathematics, Oxford University (during which he served several 1/2-year periods as Mathematics Professor at Rice University, Houston, Texas). He is now Emeritus Rouse Ball Professor, Fellow, Wadham College, Oxford (now Emeritus Fellow). He has received many awards and honorary degrees, including knighthood, Fellow of the Royal Society and of the US National Academy of Sciences, the De Morgan Medal of London Mathematical Society, the Copley Medal of the Royal Society, the Wolf Prize in mathematics (shared with Stephen Hawking), the Pomeranchuk Prize (Moscow), and one half of the 2020 Nobel Prize in Physics, the other half shared by Reinhard Genzel and Andrea Ghez. -
Nobel 2012: Trapped Ions and Photons
FEATURES Nobel 2012: Trapped ions and photons l Michel Brune1, Jean-Michel Raimond1, Claude Cohen-Tannoudji 1,2 - DOI: 10.1051/epn/2012601 l 1 Laboratoire Kastler Brossel, ENS, CNRS, UMPC Paris 6, 24 rue Lhomond, 75005 Paris, France l 2 Collège de France, 11 place Marcelin Berthelot, 75005 Paris, France m This colorized The 2012 Nobel prize in physics has been awarded jointly to Serge Haroche image shows the fluorescence from three (Collège de France and Ecole Normale Supérieure) and David Wineland (National trapped beryllium ions illuminated with Institute for Standards and Technology, USA) “for ground-breaking experimental an ultraviolet laser methods that enable measuring and manipulation of individual quantum systems”. beam. Black and blue areas indicate lower intensity, and red and white higher intensity. hat are these methods, why are they For instance, Einstein and Bohr once imagined weighing NIST physicists used jointly recognized? a photon trapped forever in a box, covered by perfect three beryllium ions to demonstrate a crucial The key endeavour in the last century mirrors. These gedankenexperiments and their “ridicu- step in a procedure that of quantum physics has been the explo- lous consequences”, as Schrödinger once stated, played could enable future ration of the coupling between matter and electromag- a considerable role in the genesis of quantum physics quantum computers W to break today's netic radiation. For a long time, the available experimental interpretation. The technical progress made these most commonly used techniques were limited to a large number of atoms and experiments possible. One can now realize some of the encryption codes. -
Shs-17-2018-14.Pdf
Science beyond borders Nobukata Nagasawa ORCID 0000-0002-9658-7680 Emeritus Professor of University of Tokyo [email protected] On social and psychological aspects of a negligible reception of Natanson’s article of 1911 in the early history of quantum statistics Abstract Possible reasons are studied why Ladislas (Władysław) Natanson’s paper on the statistical theory of radiation, published in 1911 both in English and in the German translation, was not cited properly in the early history of quantum statistics by outstanding scientists, such as Arnold Sommerfeld, Paul Ehrenfest, Satyendra Nath Bose and Albert Einstein. The social and psychological aspects are discussed as back- ground to many so far discussions on the academic evaluation of his theory. In order to avoid in the future such Natansonian cases of very limited reception of valuable scientific works, it is pro- posed to introduce a digital tag in which all the information of PUBLICATION e-ISSN 2543-702X INFO ISSN 2451-3202 DIAMOND OPEN ACCESS CITATION Nagasawa, Nobukata 2018: On social and psychological aspects of a negligible reception of Natanson’s article of 1911 in the early history of quantum statistics. Studia Historiae Scientiarum 17, pp. 391–419. Available online: https://doi.org/10.4467/2543702XSHS.18.014.9334. ARCHIVE RECEIVED: 13.06.2017 LICENSE POLICY ACCEPTED: 12.09.2018 Green SHERPA / PUBLISHED ONLINE: 12.12.2018 RoMEO Colour WWW http://www.ejournals.eu/sj/index.php/SHS/; http://pau.krakow.pl/Studia-Historiae-Scientiarum/ Nobukata Nagasawa On social and psychological aspects of a negligible reception... relevant papers published so far should be automatically accu- mulated and updated. -
The Galactic Center: a Laboratory for Fundamental Astrophysics And
The Galactic Center: A Laboratory for Fundamental Astrophysics and Galactic Nuclei An Astro2010 Science White Paper Authors: Andrea Ghez (UCLA; [email protected]), Mark Morris (UCLA), Jessica Lu (Caltech), Nevin Weinberg (UCB), Keith Matthews (Caltech), Tal Alexander (Weizmann Inst.), Phil Armitage (U. of Colorado), Eric Becklin (Ames/UCLA), Warren Brown (CfA), Randy Campbell (Keck) Tuan Do (UCLA), Andrea Eckart (U. of Cologne), Reinhard Genzel (MPE/UCB), Andy Gould (Ohio State), Brad Hansen (UCLA), Luis Ho (Carnegie), Fred Lo (NRAO), Avi Loeb (Harvard), Fulvio Melia (U. of Arizona), David Merritt (RIT), Milos Milosavljevic (U. of Texas), Hagai Perets (Weizmann Inst.), Fred Rasio (Northwestern), Mark Reid (CfA), Samir Salim (NOAO), Rainer Sch¨odel (IAA), Sylvana Yelda (UCLA) Submitted to Science Frontier Panels on (1) The Galactic Neighborhood (GAN) arXiv:0903.0383v1 [astro-ph.GA] 2 Mar 2009 (2) Cosmology and Fundamental Physics (CFP) Supplemental Animations: http://www.astro.ucla.edu/∼ghezgroup/gc/pictures/Future GCorbits.shtml Galactic Center Stellar Dynamics Astro2010 White Paper 1 Abstract As the closest example of a galactic nucleus, the Galactic center presents an exquisite lab- oratory for learning about supermassive black holes (SMBH) and their environs. In this document, we describe how detailed studies of stellar dynamics deep in the potential well of a galaxy offer several exciting directions in the coming decade. First, it will be possible to obtain precision measurements of the Galaxy’s central potential, providing both a unique test of General Relativity (GR) and a detection of the extended dark matter distribution that is predicted to exist around the SMBH. Tests of gravity have not previously been pos- sible on scales larger than our solar system, or in regimes where the gravitational energy of a body is >∼1% of its rest mass energy.