Problems of Fundamental Physics
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Einstein and Gravitational Waves
Einstein and gravitational waves By Alfonso León Guillén Gómez Independent scientific researcher Bogotá Colombia March 2021 [email protected] In memory of Blanquita Guillén Gómez September 7, 1929 - March 21, 2021 Abstract The author presents the history of gravitational waves according to Einstein, linking it to his biography and his time in order to understand it in his connection with the history of the Semites, the personality of Einstein in the handling of his conflict-generating circumstances in his relationships competition with his colleagues and in the formulation of the so-called general theory of relativity. We will fall back on the vicissitudes that Einstein experienced in the transition from his scientific work to normal science as a pillar of theoretical physics. We will deal with how Einstein introduced the relativistic ether, conferring an "odor of materiality" to his geometric explanation of gravity, where undoubtedly it does not fit, but that he had to give in to the pressure that was justified by his most renowned colleagues, led by Lorentz. Einstein had to do it to stay in the queue that would lead him to the Nobel. It was thus, as developing the relativistic ether thread, in June 1916, he introduced the gravitational waves of which, in an act of personal liberation and scientific honesty, when he could, in 1938, he demonstrated how they could not exist, within the scenario of his relativity, to immediately also put an end to the relativistic ether. Introduction Between December 1969 and February 1970, the author formulated -
E Helsinki Forum and East-West Scientific Exchange
[E HELSINKI FORUM AND EAST-WEST SCIENTIFIC EXCHANGE JOINT HEARING BEFORE THE SUBCOMMITTEE ON SCIENCE, RESEARCH AND TECHNOLOGY OF THE COMMITTEE ON SCIENCE AND TECHNOLOGY AND THE Sul COMMITTEE ON INTERNATIONAL SECURITY AND SCIENTIFIC AFFAIRS OF THE COMMITTEE ON FOREIGN AFFAIRS HOUSE OF REPRESENTATIVES AND THE COMMISSION ON SECURITY AND COOPERATION IN EUROPE NINETY-SIXTH CONGRESS SECOND SESSION JANUARY 31, 1980 [No. 89] (Committee on Science and Technology) ted for the use of the Committee on Science and Technology and the Committee on Foreign Affairs U.S. GOVERNMENT PRINTING OFFICE 421 0 WASHINGTON: 1980 COMMITTEE ON SCIENCE AND TECHNOLOGY DON FUQUA, Florida, Chairman ROBERT A. ROE, New Jersey JOHN W. WYDLER, New York MIKE McCORMACK, Washington LARRY WINN. JR., Kansas GEORGE E. BROWN, JR., California BARRY M. GOLDWATER, JR., California JAMES H. SCHEUER, New York HAMILTON FISH, JS., New York RICHARD L. OTTINGER, New York MANUEL LUJAN, JR., New Mexico TOM HARKIN, Iowa HAROLD C. HOLLENBECK, New Jersey JIM LLOYD, California ROBERT K. DORNAN, California JEROME A. AMBRO, New York ROBERT S. WALKER, Pennsylvania MARILYN LLOYD BOUQUARD, Tennessee EDWIN B. FORSYTHE, NeW Jersey JAMES J. BLANCHARD, Michigan KEN KRAMER, Colorado DOUG WALGREN, Pennsylvania WILLIAM CARNEY, New York RONNIE G. FLIPPO, Alabama ROBERT W. DAVIS, Michigan DAN GLICKMAN, Kansas TOBY ROTH, Wisconsin ALBERT GORE, JR., Tennessee DONALD LAWRENCE RITTER, WES WATKINS, Oklahoma Pennsylvania ROBERT A. YOUNG, Missouri BILL ROYER, California RICHARD C. WHITE, Texas HAROLD L. VOLKMER, Missouri DONALD J. PEASE, Ohio HOWARD WOLPE, Michigan NICHOLAS MAVROULES, Massachusetts BILL NELSON, Florida BERYL ANTHONY, JR., Arkansas STANLEY N. LUNDINE, New York ALLEN E. -
Preliminary Programme.Pdf
Institute for Nuclear Research of the Russian Academy of Sciences Joint Institute for Nuclear Research QUARKS-2018 20th International Seminar on High Energy Physics Valday, Russia, May 27 | June 2, 2018. Preliminary program Moscow, 2018 Sunday, May 27 Afternoon: Registration Plenary Session. 18:00 1. Opening. 2. Sergey Sibiryakov (EPFL, Lausanne & CERN & INR RAS) Ultra-light scalar dark matter: Motivation, Dynamics, Probes. | 30 min. 3. Alexander Zakharov (ITEP, Moscow & BLTP JINR, Dubna) Constraints on alternative theories of gravity with observations of | 30 min. the Galactic Center. 4. Shinji Mukohyama (Yukawa Inst., Kyoto U.) Horava-Lifshitz cosmology revisited. | 30 min. 5. Eugeny Babichev (LPT Orsay) Scalar-tensor theories after GW170817. | 30 min. 1 Monday, May 28 Plenary Session. 10:00 1. Alexander Studenikin (Moscow State U.) Overview on electromagnetic properties of neutrino. | 30 min. 2. Nikolay Krasnikov (INR RAS, Moscow) Search for light dark matter at accelerators. NA64 experiment. | 30 min. 3. Alexander Nozik (INR RAS, Moscow) Status and perspectives of the Troitsk nu-mass experiment. | 30 min. Coffee Break. 11:30 { 11:50 4. Zhan-Arys Dzhilkibaev (INR RAS, Moscow) Baikal-GVD project: current status and prospects. | 30 min. 5. Dmitry Zaborov (CPPM, Marseille) KM3NeT: Neutrino oscillation and astroparticle research in the | 30 min. Mediterranean sea. 6. Rodion Burenin (IKI RAS, Moscow) Current cosmological constraints on linear perturbations ampli- | 30 min. tude, neutrino mass and number of relativistic species . Parallel Section #1 (Hall #1). 15:00 1. Andrei Smilga (Nantes U.) Classical and quantum dynamics of higher-derivative theories. | 30 min. 2. Masahide Yamaguchi (Tokyo Inst. of Technology) Ghost-Free Theory with Third-Order Time Derivatives. -
Immanuel KANT and a New Physics
International Journal of Advanced Research in Physical Science (IJARPS) Volume 7, Issue 9, 2019, PP 13-26 ISSN No. (Online) 2349-7882 www.arcjournals.org Immanuel KANT and a New Physics Stanislav Konstantinov¹*, Stefano Veneroni² 1Department of Physical Electronics, Herzen State Pedagogical University, Saint Petersburg RSC”Energy”, Russia 2Department of Italian Studies, University of Eastern Piedmont, Vercelli, Italy *Corresponding Author: Stanislav Konstantinov, Department of Physical Electronics, Herzen State Pedagogical University, Saint Petersburg RSC”Energy”, Russia Abstract: A new Physics is born at the time of the crisis of theoretical physics and the entire scientific paradigm. The article proposes to come back to Immanuel Kant's philosophical heritage and, in particular, to his monograph “Critique of pure reason”, in order to better understand the concept of quantum vacuum (dark matter) in “New Physics” and its participation in all interactions in an open Universe. Keywords: quantum vacuum, dark matter, electromagnetism, gravity, nuclear forces PACS Number: 01.10.Fv, 04.50.-h, 12.10.Kt, 95.36.+x, 98.80.-k 1. INTRODUCTION Nowadays, in the scientific community, there is no unambiguous definition for the concept of “New Physics”. So Academician of the Russian Academy of Sciences, chief researcher at the Institute for Nuclear Research Valery Rubakov, who received Hamburg Prize in Theoretical Physics 2020 believes that despite all efforts, no experimental indications of a “new Physics” have yet been received. In his article “Higgs Boson”, he writes: “This is actually already starting to cause concern: is it right we all understand, it‟s quite possible, however, that we still haven‟t reached the “new physics” in terms of energy and in the amount of data collected. -
Valery Rubakov Chief Scientist Institute for Nuclear Research Russian Academy of Sciences, Moscow
INDIAN INSTITUTE OF SCIENCE EDUCATION AND RESEARCH (IISER) PUNE DR. HOMI BHABHA ROAD, PASHAN, PUNE-411008 INDIA The First Annual Homi Bhabha Distinguished Public Lecture in Physics The Universe Before the Hot Big Bang November 18, 2014, 5:30 PM ABSTRACT C.V. Raman Auditorium, It is known for long time that the Universe went through IISER Pune the hot Big Bang stage, with extraordinarily high temperatures of matter and extremely rapid expansion of space. It is less known that existing observational data strongly suggest that the hot Big Bang stage was ABOUT THE SPEAKER not the first one, but was preceded by yet another epoch with completely different – and unusual – Academician Prof. Rubakov is a leading properties. cosmologist and quantum field theorist renowned for his work on the physics of the The best guess for that early epoch is cosmic inflation, early universe, dark energy, dark matter and but alternative theories are not yet ruled out. It is extra dimensions. reassuring that future cosmological observations will R.Dupke most likely be capable of unveiling the nature of the Prof. Rubakov received a Ph.D. in physics / earliest epoch and physics that governed the Universe and mathematics from the Institute for Nuclear at that time. Research, Russian Academy of Sciences in STScI 1981. He then began his career as a junior research fellow at the Institute for Nuclear Research, Russian Academy of Sciences, becoming vice-director of research in 1987 Image Credit: NASA/ and chief scientist in 1994. He is also a professor of physics at Moscow State University. He has authored more than 150 research papers on particle physics, gravitation and cosmology, many of which have been very influential in the field. -
CERN Courier Is Distributed to Member State Governments, Institutes and Laboratories Affiliated with CERN, and to Their Personnel
Contents Covering current developments in high- energy physics and related fields worldwide CERN Courier is distributed to Member State governments, institutes and laboratories affiliated with CERN, and to their personnel. It is published monthly except January and August, in English and French editions. The views expressed are not CERN necessarily those of the CERN management. Editor: Gordon Fraser CERN, 1211 Geneva 23, Switzerland E-mail [email protected] Fax +41 (22) 782 1906 Web http://www.cerncourier.com COURIER Advisory Board VOLUME 39 NUMBER 1 FEBRUARY 1999 R Landua (Chairman), F Close, E Lillest0l, H Hoffmann, C Johnson, K Potter, PS'phicas Laboratory correspondents Argonne National Laboratory (USA): D Ayres Brookhaven, National Laboratory (USA): PYamin Cornell University (USA): D G Cassel DESY Laboratory (Germany): Ilka Flegel, PWaloschek Fermi National Accelerator Laboratory (USA): Judy Jackson GSI Darmstadt (Germany): G Siegert INFN(ltaly):APascolini IHEP, Beijing (China): Qi Nading Jefferson Laboratory (USA): S Corneliussen JINR Dubna (Russia): BStarchenko KEK National Laboratory (Japan): A Maki Lawrence Berkeley Laboratory (USA): B Feinberg Cosmic rays p26 LHC construction pll End of line for Am PS pl8 Los Alamos National Laboratory (USA): C Hoffmann NIKHEF Laboratory (Netherlands): Margriet van der Heijden Novosibirsk Institute (Russia): S Eidelman Orsay Laboratory (France): Anne-Marie Lutz News PSI Laboratory (Switzerland): P-R Kettle New Director for SLAC. The case of the missing neutron stars. Rutherford Appleton Laboratory (UK): Jacky Hutchinson Saclay Laboratory (France): Elisabeth Locci Are neutrinos seasonal? IHEP, Serpukhov (Russia): Yu Ryabov Stanford Linear Accelerator Center (USA): M Riordan TRIUMF Laboratory (Canada): M K Craddock Astrowatch Produced for CERN by Institute of Physics Publishing Ltd Features I0P Publishing Ltd, Dirac House, Temple Back, A cold start for LHC 11 Bristol BS16BE, UK Tel. -
Faces & Places
CERN Courier September 2018 Faces & Places Discover these and more – download the first chapter of every title for free. A WARDS iopscience.org/books IOP award winners for 2018 announced J Thomas, KCL, S Bates, M Alexander, R Hahn/Fermilab, J Ramage Each year, the UK Institute of Physics (IOP) Expanding PhysicsTM recognises outstanding and exceptional contributions to physics. 2018 sees five IOP Expanding Physics IOP Expanding Physics IOP Expanding Physics IOP Expanding Physics awards go to those working in high-energy Key Nuclear Reaction An Introduction to A Short Course Nuclear and physics and related fields. Experiments Elementary Particle on Relativistic Particle Physics Jenny Thomas from University College Discoveries and consequences Phenomenology Heavy Ion Collisions Claude Amsler London received the Michael Faraday Medal Hans Paetz gen. Schieck Philip G Ratcliffe Asis Kumar Chaudhuri and Prize “for her outstanding investigations into the physics of neutrino oscillations, in particular her leadership of the MINOS/ MINOS+ long-baseline neutrino-oscillation experiment”. MINOS was one of the seminal oscillation experiments, confirming that accelerator neutrinos change type as they travel. Thomas was one of a handful of people who orchestrated the formation of the collaboration, becoming co-spokesperson in 2010 and leading the proposal of a new phase Prize winners (clockwise from top left): Jenny Thomas, Bobby Acharya, Michael Begg, of the MINOS experiment, MINOS+. Hiranya Peiris, Stefan Söldner-Rembold and James Ramage. IOP Expanding Physics IOP Expanding Physics IOP Expanding Physics IOP Expanding Physics Bobby Acharya from the International Centre for Theoretical Physics in Italy and Ltd from a manufacturer of conventional Fermilab from 2009 to 2011. -
D Working Paper
S SUMMER SCHOOLS EXPERT COMMENTARIES S GUEST LECTURES CENARIOS T S S TABLE NTERNATIONAL RELATIONS C I S NALYSIS AND FORECASTING FOREIGN POLICY ISCUSSIONS A T D C REFERENCE BOOKS DIALOGUE ETWORK SCIENCE WORKING PAPERS DUCATION N PROJE OUND E REPORTS NALYSIS AND FORECASTING URITY R A S ATION C C PROJE E ORGANIZATION OMPETITIONS C NTERNATIONAL ACTIVITY CONFERENCES DU I E S S S FOREIGN POLICY TALENT POOL CS S EDUCATION POOL POLITI EPORTS OUND TABLES ION R R ENARIO GLOBAL POLITICS ETWORK C NTERNATIONAL I N IVIL OCIETY INTERNATIONAL ORGANIZATIONS S C S LOBAL RELATION G TALENT SS EFERENCE BOOKS NTERNATIONAL Y R I RUSSIANY RUSSIAN Y S C S ORGANIZATIONS DUCATION C E E INTERNATIONAL U SECURITY C RELATION SUMMER C AFFAIRS COUNCIL POLI SCHOOLS IALOGUE IETY D TING ONAL OUND I R GUEST LECTURES C SC O S TABLES I TY IGRATION EPORTS I R S A V ARTNERSHIP OREIGN P I NTERNATIONAL IBRARY OADMAPS XPERT R F E I S ONFEREN IPLOMA D M C L URITY GLOBAL NTERNAT MIGRATION COMMENTARIES IVIL C I ACT S ILATERAL NTHOLOGIE C POOL D SCIENCE C REPORTS I BOOK E ISCUSSIONS INTERNSHIPS B A D IPLOMA E WEBSITE PARTNERSHIP INTERNSHIPS S S Y C TALENT C DIALOGUE GLOBAL NTHOLOGIESGLOBAL Y A C S D POLI FORE SCIENCE CONFERENCES POLI Y S C ITE EFEREN S S NALYSISSCIENCE IGRATION A IBRARY OADMAP EB ENARIO OREIGN R IPLOMA C F R L M OREIGN D S W NALY AND FORECASTING F S DIALOGUE INTERNATIONAL ORGANIZATIONS A AND S NETWORK INTERNATIONAL RELATIONS E CLUB MEETINGS DIALOGUE DIPLOMACY PROJECTS HOOL S S C IALOGUE S T D C URITY UMMER ITE E S HIP C S OMMENTARIE TURE IVIL OCIETY C S C S EBSITE -
Rubakov and Shaposhnikov Win INR Prize for Fundamental Physics
PEOPLE AWARDS Rubakov and Shaposhnikov win INR prize for fundamental physics Valery Rubakov, from the Institute for Nuclear Research (INR) of the Russian Academy of Sciences in Moscow, and Mikhail Shaposhnikov, from the Swiss Federal Institute of Technology in Lausanne (EPFL), have been awarded the Markov Prize for 2005. INR established the prize in 2002 in memory of Moisey Alexandrovich Markov, a strong proponent of research in underground and deep-underwater neutrino physics, and one of the founders of INR. Rubakov and Shaposhnikov received the prize for their outstanding contributions to studies of the cosmological effects of gauge interactions and for the development of novel ideas of space-time and gravity. One of their best-known papers concerns electroweak non- conservation of baryon and lepton numbers at high temperatures (written with Vadim Kuzmin), a cornerstone of the modern theory of the early universe. In 1983 Rubakov and Shaposhnikov also conjectured that we live on a four- dimensional brane embedded in a multidimensional space-time, and suggested a Left to right: Mikhail Shaposhnikov, Albert Tavkhelidze (chairman of the expert committee mechanism for matter localization on the brane. of the Markov Prize), Valery Rubakov and Victor Matveev (director of the INR). proponent of its successor, NA48. and pointing out the importance of the effect EPS physics prizes Mathieu de Naurois of the Laboratoire de of gravitational lensing by local matter on the Physique Nucleaire et de Hautes Energies, CMB background. awarded in Lisbon IN2P3/CNRS, received the EPS-HEPP Young There were two recipients of the 2005 Physicist Prize for "his new ideas and decisive Outreach Prize - Dave Barney of CERN and The 2005 prizes of the High Energy and Particle contributions" in the cosmic gamma-ray Peter Kalmus of Queen Mary, University of Physics (HEPP) Division of the European experiments, CELESTE and HESS. -
Institute for Theoretical and Mathematical Physics
Lomonosov Moscow State University Institute for Theoretical and Mathematical Physics itmp.msu.ru December 2020 About ITMP ❑ ITMP is a division of MSU. It is the advanced research centre in the field of fundamental theoretical and mathematical physics. ❑ ITMP was founded in December 2018. The Institute is supported by the Theoretical Physics and Mathematics Advancement Foundation «BASIS». ❑ Our main goal is to become a research centre of international level. We aim at growing into a platform for cooperation between national and foreign researchers, students and PhD students. Presently, the activity of the Institute is focused on the following areas: ❏ string theory and quantum gravity, ❏ conformal field theories andAdS/CFT correspondence, ❏ integrable systems, ❏ quantum field theory and mathematical methods ❏ modified gravitation theory and cosmology. Scientific Council: VALERY RUBAKOV Institute for Nuclear Research RAS, Faculty of Physics MSU, a chairman ARKADY TSEYTLIN ITMP MSU, Lebedev Physical Institute RAS, Imperial College London (UK) The Scientific Council includes GLEB ARUTYUNOV Hamburg University (Germany) outstanding researchers, scientific VLADIMIR BELOKUROV members and ITMP employees, and Faculty of Physics MSU decides on the development strategy, MIKHAIL VASIL Lebedev Physical Institute RAS principles of working ideas and key MAXIM GRIGORIEV personnel decisions. ITMP MSU & Lebedev Physical Institute RAS SERGEY KOZYREV Steklov Mathematical Institute RAS DMITRY LEVKOV ITMP MSU & Institute for Nuclear Research RAS ALEXEY SEMIKHATOV Lebedev Physical Institute RAS Our Team Director Prof. Arkady Tseytlin Deputies Director Research interests of Arkady Tseytlin include quantum field theory and quantum gravity, superstring theory, conformal theories and Maxim Grigoriev Candidate of Physical and Mathematical AdS/CFT correspondence. He obtained Sciences several key results in superstring theory and field theory. -
Radiochemical Solar Neutrino Experiments
Radiochemical solar neutrino experiments V N Gavrin1 and B T Cleveland2,3 1 Institute for Nuclear Research of the Russian Academy of Sciences, Moscow 117312, Russia 2 Department of Physics, University of Washington, Seattle Washington 98195, USA E-mail: 1 [email protected], 2 [email protected] Abstract. Radiochemical experiments have been crucial to solar neutrino research. Even today, they provide + the only direct measurement of the rate of the proton-proton fusion reaction, p + p → d + e + νe, which generates most of the Sun’s energy. We first give a little history of radiochemical solar neutrino experiments with emphasis on the gallium experiment SAGE – the only currently operating detector of this type. The combined result of all data from the Ga experiments is a capture rate of 67.6 ± 3.7 SNU. For comparison to theory, we use the calculated flux at the Sun from a standard solar model, take into account neutrino propagation from the Sun to the Earth and the results of neutrino source experiments with Ga, and obtain +3.9 67.3−3.5 SNU. Using the data from all solar neutrino experiments we calculate an electron neutrino pp flux ♁ +0.76 10 2 of φpp = (3.41−0.77) × 10 /(cm -s), which agrees well with the prediction from a detailed solar model ♁ +0.13 10 2 of φpp = (3.30−0.14) × 10 /(cm -s). Four tests of the Ga experiments have been carried out with very intense reactor-produced neutrino sources and the ratio of observed to calculated rates is 0.88 ± 0.05. -
Celebrating a Century of Progress Physics Uspekhi Was Set up 100 Years Ago to Support the Fledgling Physics Community in the Soviet Union
News & Analysis physicsworld.com Celebrating a century of progress Physics Uspekhi was set up 100 years ago to support the fledgling physics community in the Soviet Union. A century later, the journal’s current editor-in-chief Valery Rubakov talks to Matin Durrani about the future of Russian physics How did your interest in physics began to pick up and the country has begin? been spending about 1% of its gross I studied physics at Moscow State domestic product on research and University, graduating in 1978 and Rubakov Valery development. Do you think this then was awarded a PhD at the is enough? Institute for Nuclear Research of If I compare today’s situation with the Russian Academy of Sciences the 1990s then we are a lot better off in 1981. I have been affiliated to now. However, doing fundamental both institutions ever since, work- science is still difficult. I have no ing in areas such as quantum field idea of the share of fundamental sci- theory, elementary particle physics ence in overall research and develop- and cosmology. ment spending, but I definitely feel that fundamental science is either What has been your most notable underfunded or funded improperly, achievement? or, most likely, both. Hard to say, but what I am probably best known for is the idea of baryon In 2014 Russian president Vladimir number non-conservation in the Putin called for all state research early universe within the Standard funding to be distributed via a Model of particle physics and its competitive grants system. What extensions. This result, obtained happened to this plan? together with Vadim Kuzmin and Serving the starts contracting, then stops before I think it is impossible to distrib- Mikhail Shaposhnikov, was initially community a hot expansion begins.