Moments with Yakov Borisovich Zeldovich
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The Morphology of the X-Ray Afterglows and of the Jetted Gev Emission in Long Grbs
MNRAS 000,1– ?? (2020) Preprint 17 March 2021 Compiled using MNRAS LATEX style file v3.0 The morphology of the X-ray afterglows and of the jetted GeV emission in long GRBs R. Ruffini,1;2;5;7;14 R. Moradi,1;2;15? J. A. Rueda,1;2;4;8;16 L. Li,1;2;15 N. Sahakyan,1;6 Y.-C. Chen,1;2 Y. Wang,1;2;15 Y. Aimuratov,1;2;9 L. Becerra,1;2;17 C. L. Bianco,1;2;16 C. Cherubini,1;3;11 S. Filippi,1;3;10 M. Karlica,1;2 G. J. Mathews,1;12 M. Muccino,13 G. B. Pisani,1;2 and S. S. Xue1;2 1 ICRANet, Piazza della Repubblica 10, I-65122 Pescara, Italy 2 ICRA, Dipartimento di Fisica, Università di Roma “La Sapienza”, Piazzale Aldo Moro 5, I-00185 Roma, Italy 3 ICRA, University Campus Bio-Medico of Rome, Via Alvaro del Portillo 21, I-00128 Rome, Italy 4 ICRANet-Ferrara, Dipartimento di Fisica e Scienze della Terra, Università degli Studi di Ferrara, Via Saragat 1, I–44122 Ferrara, Italy 5 ICRANet-Rio, Centro Brasileiro de Pesquisas Físicas, Rua Dr. Xavier Sigaud 150, 22290–180 Rio de Janeiro, Brazil 6 ICRANet-Armenia, Marshall Baghramian Avenue 24a, Yerevan 0019, Republic of Armenia 7 Université de Nice Sophia-Antipolis, Grand Château Parc Valrose, Nice, CEDEX 2, France 8 Dipartimento di Fisica e Scienze della Terra, Università degli Studi di Ferrara, Via Saragat 1, I–44122 Ferrara, Italy 9 Fesenkov Astrophysical Institute, Observatory 23, 050020 Almaty, Kazakhstan 10 Department of Engineering, University Campus Bio-Medico of Rome, Nonlinear Physics and Mathematical Modeling Lab, Via Alvaro del Portillo 21, 00128 Rome, Italy 11 Department of Science and Technology for Humans and the Environment and Nonlinear Physics and Mathematical Modeling Lab, University Campus Bio-Medico of Rome, Via Alvaro del Portillo 21, 00128 Rome, Italy 12 Center for Astrophysics, Department of Physics, University of Notre Dame, Notre Dame, IN, 46556, USA 13 Instituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Frascati, I-00044 Frascati, Italy 14 INAF, Viale del Parco Mellini 84, 00136 Rome, Italy 15 INAF – Osservatorio Astronomico d’Abruzzo,Via M. -
What Is Gravity Probe B? a Quest for Experimental Truth the GP-B Flight
What is Gravity Probe B? than Gravity Probe B. It’s just a star, a telescope, and a spinning sphere.” However, it took the exceptional collaboration of Stanford, Gravity Probe B (GP-B) is a NASA physics mission to experimentally MSFC, Lockheed Martin and a host of others more than four decades investigate Einstein’s 1916 general theory of relativity—his theory of gravity. to develop the ultra-precise gyroscopes and the other cutting- GP-B uses four spherical gyroscopes and a telescope, housed in a satellite edge technologies necessary to carry out this “simple” experiment. orbiting 642 km (400 mi) above the Earth, to measure, with unprecedented accuracy, two extraordinary effects predicted by the general theory of rela- The GP-B Flight Mission & Data Analysis tivity: 1) the geodetic effect—the amount by which the Earth warps the local spacetime in which it resides; and 2) the frame-dragging effect—the amount On April 20, 2004 at 9:57:24 AM PDT, a crowd of over 2,000 current and by which the rotating Earth drags its local spacetime around with it. GP-B former GP-B team members and supporters watched and cheered as the tests these two effects by precisely measuring the precession (displacement) GP-B spacecraft lifted off from Vandenberg Air Force Base. That emotionally angles of the spin axes of the four gyros over the course of a year and com- overwhelming day, culminating with the extraordinary live video of paring these experimental results with predictions from Einstein’s theory. the spacecraft separating from the second stage booster meant, as GP-B Program Manager Gaylord Green put it, “that 10,000 things went right.” A Quest for Experimental Truth Once in orbit, the spacecraft first underwent a four-month Initialization The idea of testing general relativity with orbiting gyroscopes was sug- and Orbit Checkout (IOC), in which all systems and instruments were gested independently by two physicists, George Pugh and Leonard Schiff, initialized, tested, and optimized for the data collection to follow. -
Cosmic Background Explorer (COBE) and Beyond
From the Big Bang to the Nobel Prize: Cosmic Background Explorer (COBE) and Beyond Goddard Space Flight Center Lecture John Mather Nov. 21, 2006 Astronomical Search For Origins First Galaxies Big Bang Life Galaxies Evolve Planets Stars Looking Back in Time Measuring Distance This technique enables measurement of enormous distances Astronomer's Toolbox #2: Doppler Shift - Light Atoms emit light at discrete wavelengths that can be seen with a spectroscope This “line spectrum” identifies the atom and its velocity Galaxies attract each other, so the expansion should be slowing down -- Right?? To tell, we need to compare the velocity we measure on nearby galaxies to ones at very high redshift. In other words, we need to extend Hubble’s velocity vs distance plot to much greater distances. Nobel Prize Press Release The Royal Swedish Academy of Sciences has decided to award the Nobel Prize in Physics for 2006 jointly to John C. Mather, NASA Goddard Space Flight Center, Greenbelt, MD, USA, and George F. Smoot, University of California, Berkeley, CA, USA "for their discovery of the blackbody form and anisotropy of the cosmic microwave background radiation". The Power of Thought Georges Lemaitre & Albert Einstein George Gamow Robert Herman & Ralph Alpher Rashid Sunyaev Jim Peebles Power of Hardware - CMB Spectrum Paul Richards Mike Werner David Woody Frank Low Herb Gush Rai Weiss Brief COBE History • 1965, CMB announced - Penzias & Wilson; Dicke, Peebles, Roll, & Wilkinson • 1974, NASA AO for Explorers: ~ 150 proposals, including: – JPL anisotropy proposal (Gulkis, Janssen…) – Berkeley anisotropy proposal (Alvarez, Smoot…) – Goddard/MIT/Princeton COBE proposal (Hauser, Mather, Muehlner, Silverberg, Thaddeus, Weiss, Wilkinson) COBE History (2) • 1976, Mission Definition Science Team selected by HQ (Nancy Boggess, Program Scientist); PI’s chosen • ~ 1979, decision to build COBE in-house at GSFC • 1982, approval to construct for flight • 1986, Challenger explosion, start COBE redesign for Delta launch • 1989, Nov. -
Tests of General Relativity - Wikipedia
12/2/2018 Tests of general relativity - Wikipedia Tests of general relativity T ests of general relativity serve to establish observational evidence for the theory of general relativity. The first three tests, proposed by Einstein in 1915, concerned the "anomalous" precession of the perihelion of Mercury, the bending of light in gravitational fields, and the gravitational redshift. The precession of Mercury was already known; experiments showing light bending in line with the predictions of general relativity was found in 1919, with increasing precision measurements done in subsequent tests, and astrophysical measurement of the gravitational redshift was claimed to be measured in 1925, although measurements sensitive enough to actually confirm the theory were not done until 1954. A program of more accurate tests starting in 1959 tested the various predictions of general relativity with a further degree of accuracy in the weak gravitational field limit, severely limiting possible deviations from the theory. In the 197 0s, additional tests began to be made, starting with Irwin Shapiro's measurement of the relativistic time delay in radar signal travel time near the sun. Beginning in 197 4, Hulse, Taylor and others have studied the behaviour of binary pulsars experiencing much stronger gravitational fields than those found in the Solar System. Both in the weak field limit (as in the Solar System) and with the stronger fields present in systems of binary pulsars the predictions of general relativity have been extremely well tested locally. In February 2016, the Advanced LIGO team announced that they had directly detected gravitational waves from a black hole merger.[1] This discovery, along with additional detections announced in June 2016 and June 2017 ,[2] tested general relativity in the very strong field limit, observing to date no deviations from theory. -
Vatican Observatory N E W S L E T T
vatican observatory NEWSLETTER Spring 2012 embracing, encouraging and promoting scientific study VOF Honors Benefactors at Circles of Giving Awards Dinner DID YOU KNOW? German Jesuit Christoph Cla- vius’s viewing of the total solar eclipse of 1560 made him de- cide that astronomy would be his life's work? He went on to write numerous textbooks and Rich Friedrich and Peter Moore was the senior mathematician on Fr. DiUlio and Marianne Augustine of the Pacific Western Foundation the commission for the reform of On February 24, 2012, the Vatican Observatory Foundation honored friends and benefactors who have so the calendar in 1582. The Vatican generously supported the work of the Vatican Observatory over time. Each year as donors reach a certain Observatory Foundation rec- lifetime giving level, they achieve a Circle of Giving designation and are recognized and thanked publicly ognizes his contribution to the by the President and Board of Directors as well as their fellow benefactors and friends. Each Circle of Giv- field by welcoming benefactors of ing is named in honor of one of the exceptional individuals connected with astronomy, the Society of Jesus $10,000 to the Christoph Clavius and the Vatican Observatory. At this year’s dinner four honorees were present to receive awards from Circle of Giving. Foundation President Fr. Albert J. DiUlio, S.J., and Board Chairman, Richard J. Friedrich. They included Christoph Clavius Bill Ahmanson of The Ahmanson Foundation; Marianne Augustine; Peter Moore of the Pacific Western Foundation; and Dan Cracchiolo of The Steele Foundation, whose award was accepted by his sister, Rose Collins. -
Icranet Activities with Brazil
ICRANet activities with Brazil ICRANet-IRAP PhD Fellowships to Brazilian Students pp. 1-17 Part 1 CAPES-ICRANet Program I cycle – 2013-2016 Part 2 p. 19 2. a – IRAP Ph. D. Program pp. 21-27 2. b – Postdoctoral Program in Europe/Asia pp. 29-42 2. c – Postdoctoral Program in Brazil pp. 43-54 2. d – Senior Visitors in Brazil pp. 55-66 2. e – Senior Visitors in Europe/Asia pp. 67-78 0 1. ICRANet-IRAP PhD Fellowships to Brazilian Students index - de Barros, Gustavo 3 - Pereira, Jonas Pedro 7 - Sversut Arsioli, Bruno 11 - Gomes de Oliveira, Fernanda 15 - Maiolino, Tais 17 1 2 de Barros, Gustavo Position: IRAP PhD – Fifth Cycle, 2006-09 Current position: Professor Adjunto Centro Universitário da Zona Oeste – OEZO Publications: -) Patricelli, B.; Bernardini, M. G.; Bianco, C. L.; Caito, L.; de Barros, G.; Izzo, L.; Ruffini, R.; Vereshchagin, G. V.; “Analysis of GRB 080319B and GRB 050904 within the Fireshell Model: Evidence for a Broader Spectral Energy Distribution”; The Astrophysical Journal, 756 (2012), id. 16; DOI: 10.1088/0004- 637X/756/1/16 -) Bianco, C. L.; Amati, L.; Bernardini, M. G.; Caito, L.; De Barros, G.; Izzo, L.; Patricelli, B.; Ruffini, R.; “The class of ``disguised'' short GRBs and its implications for the Amati relation”; Memorie della Società Astronomica Italiana Supplement, 21 (2012), 139. -) Patricelli, B.; Bernardini, M. G.; Bianco, C. L.; Caito, L.; de Barros, G.; Izzo, L.; Ruffini, R.; Vereshchagin, G.; “High Energetic Gamma Ray Bursts and Their Spectral Properties Within the Fireshell Model”; International Journal of Modern Physics: Conference Series, 12 (2012), pp. -
The Russian-A(Merican) Bomb: the Role of Espionage in the Soviet Atomic Bomb Project
J. Undergrad. Sci. 3: 103-108 (Summer 1996) History of Science The Russian-A(merican) Bomb: The Role of Espionage in the Soviet Atomic Bomb Project MICHAEL I. SCHWARTZ physicists and project coordinators ought to be analyzed so as to achieve an understanding of the project itself, and given the circumstances and problems of the project, just how Introduction successful those scientists could have been. Third and fi- nally, the role that espionage played will be analyzed, in- There was no “Russian” atomic bomb. There only vestigating the various pieces of information handed over was an American one, masterfully discovered by by Soviet spies and its overall usefulness and contribution Soviet spies.”1 to the bomb project. This claim echoes a new theme in Russia regarding Soviet Nuclear Physics—Pre-World War II the Soviet atomic bomb project that has arisen since the democratic revolution of the 1990s. The release of the KGB As aforementioned, Paul Josephson believes that by (Commissariat for State Security) documents regarding the the eve of the Nazi invasion of the Soviet Union, Soviet sci- role that espionage played in the Soviet atomic bomb project entists had the technical capability to embark upon an atom- has raised new questions about one of the most remark- ics weapons program. He cites the significant contributions able and rapid scientific developments in history. Despite made by Soviet physicists to the growing international study both the advanced state of Soviet nuclear physics in the of the nucleus, including the 1932 splitting of the lithium atom years leading up to World War II and reported scientific by proton bombardment,7 Igor Kurchatov’s 1935 discovery achievements of the actual Soviet atomic bomb project, of the isomerism of artificially radioactive atoms, and the strong evidence will be provided that suggests that the So- fact that L. -
The Specola Vaticana: Astronomy at the Vatican
Organizations, People and Strategies in Astronomy 2 (OPSA 2), 217-230 Ed. A. Heck, © 2013 Venngeist. THE SPECOLA VATICANA: ASTRONOMY AT THE VATICAN GUY CONSOLMAGNO AND CHRISTOPHER CORBALLY Specola Vaticana V-00120, Vatican City State [email protected] [email protected] Abstract. The Vatican is an independent nation, with its own national astronomical observatory, the Specola Vaticana (Vatican Observatory). As- tronomy has been supported at the Vatican since the 1582 reform of the calendar; the present-day Observatory has been in operation since 1891. The work of the observatory is divided between two sites, one in the pa- pal summer gardens south of Rome, Italy, and the other affiliated with the Steward Observatory at the University of Arizona, in Tucson, Arizona, USA. Research undertaken by current staff members ranges from cosmol- ogy and the study of galactic evolution to meteoritics and meteors. Given the stable funding provided by the Vatican, the Observatory has specialized in long-term mapping and cataloguing projects that would be difficult to mount under a traditional three-year funding cycle. These have included participation in the Carte du Ciel photographic map of the sky; the at- lases of spectra produced by its Spectrochemical Laboratory; surveys of star clusters and peculiar stars; and the cataloguing of meteorite physical properties. 1. Astronomy in the Holy See Before 1891 To the Christian church, the study of creation has long been supported as an act of worshipping the Creator. Astronomy was one of the seven subjects that made up the curriculum of the medieval universities, which were themselves founded by the Church. -
Aleksei A. Abrikosov 1928–2017
Aleksei A. Abrikosov 1928–2017 A Biographical Memoir by M. R. Norman ©2018 National Academy of Sciences. Any opinions expressed in this memoir are those of the author and do not necessarily reflect the views of the National Academy of Sciences. ALEKSEI ALEKSEEVICH ABRIKOSOV June 25, 1928–March 29, 2017 Elected to the NAS, 2000 Shortly after the 2003 announcement that Aleksei Abrikosov had won the Nobel Prize in Physics, a number of colleagues took Alex to lunch at a nearby Italian restau- rant. During lunch, one of the Russian visitors exclaimed that Alex should get a second Nobel Prize, this time in Literature for his famous “AGD” book with Lev Gor’kov and Igor Dzyaloshinskii (Methods of Quantum Field Theory in Statistical Physics.) Somewhat taken aback, I looked closely at this individual and realized that he was deadly serious. Although I could imagine the reaction of the Nobel Literature committee to such a book (for a lay person, perhaps analogous to trying to read Finnegan’s Wake), I had to admit that my own copy of this book is quite dog-eared, having been put to good use over the By M. R. Norman years. In fact, you know you have made it in physics when your book gets a Dover edition. One of the most charming pictures I ever saw was a rare drawing in color that Alexei Tsvelik did (commissioned by Andrei Varlamov for Alex’s 50th birthday) that was proudly displayed in Alex’s home in Lemont, IL. It showed Alex with his fingers raised in a curled fashion as in the habit of medieval Popes. -
Global Program
PROGRAM Monday morning, July 13th La Sapienza Roma - Aula Magna 09:00 - 10:00 Inaugural Session Chairperson: Paolo de Bernardis Welcoming addresses Remo Ruffini (ICRANet), Yvonne Choquet-Bruhat (French Académie des Sciences), Jose’ Funes (Vatican City), Ricardo Neiva Tavares (Ambassador of Brazil), Sargis Ghazaryan (Ambassador of Armenia), Francis Everitt (Stanford University) and Chris Fryer (University of Arizona) Marcel Grossmann Awards Yakov Sinai, Martin Rees, Sachiko Tsuruta, Ken’Ichi Nomoto, ESA (acceptance speech by Johann-Dietrich Woerner, ESA Director General) Lectiones Magistrales Yakov Sinai (Princeton University) 10:00 - 10:35 Deterministic chaos Martin Rees (University of Cambridge) 10:35 - 11:10 How our understanding of cosmology and black holes has been revolutionised since the 1960s 11:10 - 11:35 Group Picture - Coffee Break Gerard 't Hooft (University of Utrecht) 11:35 - 12:10 Local Conformal Symmetry in Black Holes, Standard Model, and Quantum Gravity Plenary Session: Mathematics and GR Katarzyna Rejzner (University of York) 12:10 - 12:40 Effective quantum gravity observables and locally covariant QFT Zvi Bern (UCLA Physics & Astronomy) 12:40 - 13:10 Ultraviolet surprises in quantum gravity 14:30 - 18:00 Parallel Session 18:45 - 20:00 Stephen Hawking (teleconference) (University of Cambridge) Public Lecture Fire in the Equations Monday afternoon, July 13th Code Classroom Title Chairperson AC2 ChN1 MHD processes near compact objects Sergej Moiseenko FF Extended Theories of Gravity and Quantum Salvatore Capozziello, Gabriele AT1 A Cabibbo Cosmology Gionti AT3 A FF3 Wormholes, Energy Conditions and Time Machines Francisco Lobo Localized selfgravitating field systems in the AT4 FF6 Dmitry Galtsov, Michael Volkov Einstein and alternatives theories of gravity BH1:Binary Black Holes as Sources of Pablo Laguna, Anatoly M. -
Lev Davidovich Landau Born: 12 January, 1908, Baku, Russian Empire Died: 1 April, 1968, Moscow, Soviet Union
Symmetry XIII (2019) 1 Dedicated to Lev Davidovich Landau Born: 12 January, 1908, Baku, Russian Empire Died: 1 April, 1968, Moscow, Soviet Union Symmetry XIII (2019) 2 Volume XIII, 2019 Editorial Symmetry This issue of symmetry is dedicated to the great physicists Lev Devidovich Landau. An annual Publication of CDP, TU Landau Soviet theoretical physicist, one of the founders of quantum theory of (Covid-19 Issue) condensed matter whose pioneering research in this field was recognized with the Patron 1962 Nobel Prize for Physics. In the year 1941, he successfully applied quantum Prof. Dr. Binil Aryal theory to the movement of superfluid liquid helium. Landau argued for the need of yet another radical conceptual revolution in physics in order to resolve the Advisory Board mounting difficulties in relativistic quantum theory. The collective work of Prof. Dr. Om Prakash Niraula Landau’s group embraced practically every branch of theoretical physics. In 1946 Prof. Dr. Raju Khanal he described the phenomenon of Landau damping of electromagnetic waves in Prof. Dr. Narayan Prasad Adhikari plasma. Together with Vitaly L. Ginzburg, in 1950 Landau obtained the correct Prof. Dr. Ram Prasad Regmi equations of the macroscopic theory of superconductivity. During the 1950s he and Prof. Dr. Ishwar Koirala collaborators discovered that even in renormalized quantum electrodynamics, a Dr. Hari Prasad Lamichhane new divergence difficulty appears (the Landau pole). The phenomenon of the Dr. Bal Ram Ghimire coupling constant becoming infinite or vanishing at some energy is an important Dr. Ajay Kumar Jha feature of modern quantum field theories. In this volume, there are 7 articles Dr. -
The Evolution Debate George V
Guest Editorial The Evolution Debate George V. Coyne, S.J. Vatican Observatory ow did we humans come to be in the expanding, which result in H evolving universe known through astrophysics stepwise changes and cosmology? It is quite clear that we do not know in the products everything about this process. But it would be scientifi- carried out by cally untenable to deny that the human brain is a result natural selection of a natural process of the development of ever more in the environ- complex chemistry in an evolving universe that is 13.7 ment in which billion years old and contains about 100 billion galaxies, the products each of which contains on the average about 200 billion come to exist. stars of an immense variety. After the universe became Those products rich in certain basic chemicals through the death of stars survive that can of various masses, those chemicals got together in suc- best adapt to cessive steps to make ever more complex molecules. their environ- Finally, in some extraordinary series of chemical process- ment. There is, es, the human brain came to be the most complicated therefore, an George V. Coyne machine that we know. apparent destiny Did this happen by chance or by necessity? The first toward more perfect beings, i.e., beings better able to thing to be said is that the problem is not formulated adapt in this process; but the apparent destiny can be correctly. It is not just a question of chance or necessity explained by the natural process itself. This apparent because, first of all, it is both.