Report 2018/2019 ETH Institute for Theoretical Studies

Total Page:16

File Type:pdf, Size:1020Kb

Report 2018/2019 ETH Institute for Theoretical Studies Report 2018/2019 ETH Institute for Theoretical Studies ETH-ITS Table of Contents Foreword 5 The ETH Institute for Theoretical Studies 6 History and aims 6 Fellows at the ITS 6 Collaborations 7 Activities 8 Meetings, talks, minicourses 8 The ITS Science Colloquium 10 Programme 2018–2019 11 Fellows’ seminar 12 Programme 2018–2019 12 Awards 13 Fellows’ report 14 Outlook 22 People at the ETH-ITS 24 Director 24 Coordinator 24 Board of Patrons 24 Advisory Committee 24 2013–2017 2017–2019 Fellows 2014–2019 25 Senior Fellows Junior Fellows (with current affiliation of former Junior Fellows) Contact 27 Clausiusstrasse 47, the address of the ETH Institute for Theoretical Studies. 4 Foreword The academic year 2018/2019 was in several ways special for the Institute for Theoretical Studies. Firstly, it experimen- ted a new way of functioning, dedicating a semester to the interdisciplinary subject of «modular forms, periods and scattering amplitudes», hosting over forty physicists and mathematicians, with a school, a workshop and other events involving several young scientists and putting into contact participants with scientists of ETH. Secondly, the Institute was evaluated by an international committee, who was very positively impressed by the achievements of the Institute and gave interesting suggestions for improvement. Thirdly, on a more personal note, this was my last year as the director of the ETH-ITS; the last six years were an intense period in which I had the unique opportunity to meet scientists in a variety of subjects who are shaping their respective disciplines. I thank the donors for making this possible, the Fellows of the Institute for their excellent scientific contributions, the school board of ETH Zurich for their continuous support, the Advisory Committee for its commitment and advice, and Christina Buchmann, who is retiring this year as coordinator, for her invaluable help and competence in running the Institute. The new director Rahul Pandharipande, professor of mathematics at ETH Zurich, took office on 1 June 2019. Livia Kürsteiner is the new coordinator. I wish the new team a successful start. Giovanni Felder, Institute’s director The ETH Institute for Theoretical Studies is supported by Dr. Max Rössler, the Walter Haefner Foundation and the ETH Foundation. 5 Ruth Britto lecturing at the school on Modular forms, periods and scattering amplitudes, organized in collaboration with SwissMAP. The ETH Institute for Theoretical Studies History and aims The ETH Institute for Theoretical Studies (ETH-ITS) is an interdisciplinary Institute dedicated to research in mathematics, theoretical computer science and theoretical natural sciences. It was founded on 1 June 2013 on the initiative of former ETH president Ralph Eichler, with a generous donation of Dr. Max Rössler and the Walter Haefner Foundation. The aim of the Institute is to enable top theoretical scientists to be active for an extended period of time at ETH, interact with local researchers, and establish lasting scientific collaborations in an interdisciplinary context. Fellows at the ITS The Institute hosts up to six Senior Fellows and up to twelve Junior Fellows. Junior Fellows are talented young independent postdocs spending up to three years at ETH Zurich to work on research subjects of their choice. They are supported by a mentor, who is an ETH professor. The Junior Fellows are selected by the director, with the assistance of the scientific Advisory Committee, by a nomination procedure: candidates are selected from a group of young researchers that are nominated by faculty members and senior researchers of universities and research institutions and are invited to apply. 6 Schedule for the selection of Junior Fellows Mid-September Target date for nominations, eligible candidates are invited to apply Mid-October Deadline for application of nominated candidates November Interviews with ETH members of the Advisory Committee December Offers are made Senior Fellows are leading international researchers in mathematics, theoretical computer science and theoretical natural sciences, spending up to a year at the Institute on a sabbatical leave from their home institutions. They dedicate their time to research and participate in the activities of the Institute and of ETH Zurich, for example by giving a course on research topics. They are invited by the Vice-President for Research and Corporate Relations of ETH Zurich on the recommendation of the Advisory Committee. Candidates are often suggested by members of the Advisory Committee or ETH faculty, but they can also apply directly. www.ethz.ch/eth-its/fellows → Collaborations The ETH Institute for Theoretical Studies collaborates with the Departments of ETH and their visitor programmes, such as the Forschungsinstitut für Mathematik (FIM) at the Department of mathematics and the Pauli Centre at the Department of physics. It also nurtures the relationship with other Swiss research institutions through its Fellows and by contributing to scientific activities. This year it organized a school within the thematic programme on «Modular forms, periods and scat- tering amplitudes» together with the National Competence Centre in Research SwissMAP – The Mathematics of Physics and contributed to the programme goMATH – Women in Mathematics of the Department of Mathematics of ETH Zurich. 7 Participants at the workshop on Modular forms, periods and scattering amplitudes. Activities Meetings, talks, minicourses In the spring semester 2019 a thematic programme on «Modular forms, periods and scattering amplitudes» took place at the ETH-ITS. It was organized by Babis Anastasiou (ETH Zurich), Claude Duhr (CERN), Giovanni Felder (ETH Zurich) and Eric Panzer (University of Oxford). Over the last few years, the calculations of scattering amplitudes in particle physics and string theory led to the development of sophisticated mathematical methods and brought new questions in the classical area of mathematics of modular forms. The aim of the programme was to bring together experts on these integrals and related objects, both in physics and in mathematics, with the grand goal of advancing the field via a cross-fertilisation between disciplines. The programme started with a school with minicourses by Ruth Britto (Dublin), Claude Duhr (CERN), Javier Fresán (Ecole Polytechnique) and Nils Matthes (Oxford), with talks accessible to both mathematicians and physicists and ended with a workshop. There were a number of visitors and further activities throughout the programme. 8 The fourth edition of the European-Japanese Symposium on Symplectic Varieties and Moduli Spaces took place at ETH with the support of the ETH-ITS. It was organised by Junior Fellow Ulrike Rieß together with Chiara Camere (Università degli Studi di Milano), Daisuke Matsushita (Hokkaido University), Giovanni Mongardi (Università di Bologna), Hisanori Ohashi (Tokyo University of Science). It included minicourses of Claire Voisin and Yoshinori Namikawa and talks by participants. In addition, Senior Fellows Sandu Popescu and Gilles Brassard gave series of lectures on topics related to quantum information theory and foundation of quantum mechanics, see the Fellows’ report below for more details. 9 Former Senior Fellow Robert Brandenberger (left) discusses with Philippe Jetzer and ITS Colloquium Speaker Rainer Weiss (right). The ITS Science Colloquium The ITS Science Colloquium aims at exposing students and researchers in mathematics, theoretical computer science and theoretical natural sciences to new questions and research subjects of common interest to different disciplines. The first talk was by ETH physicist Renato Renner who asked whether quantum mechanics can be used to describe a physicist who herself uses quantum mechanics, a question based on the much discussed thought experiment recently proposed by Renner with Daniela Frauchiger. In another well-attended talk Nobel prize laureate Rainer Weiss, of the Massachusetts Institute of Technology, co-founder of the LIGO project, told us about the exploration of the Universe through gravitational waves. The third speaker of the academic year was Ranit Aharonov, of IBM Research, manager of Project Debater, an AI system that can engage humans in debates on complex topics. In her talk she addressed the question «How persuasive can a computer be?» Finally, Miranda Cheng, of the University of Amsterdam, told us the story of the 17 mysterious formulae written by Ramanujan in a 1920 letter, that marked the beginning of a theory that has recent application to various research areas, including the moonshine theory in mathematics and black holes in theoretical physics. 10 The audience at Renato Renner’s talk «Beyond Schrödinger’s cat». Programme 2018/2019 25.10.2018 Renato Renner, ETH Zurich Beyond Schrödinger’s cat 28.02.2019 Rainer Weiss, MIT and LIGO Exploring the universe with gravitational waves 07.03.2019 Ranit Aharonov, IBM research Project Debater – How persuasive can a computer be? 14.03.2019 Miranda Cheng, Amsterdam Mock modular forms are everywhere Videos of selected talks can be viewed on www.ethz.ch/eth-its/activities → 11 Fellows’ seminar The aim of the Fellows’ seminar, organized by Junior Fellows Johannes Noller and Ulrike Rieß, is to present the research of the Fellows of the ETH-ITS. It is open to all interested and the rule is that talks should be accessible to other Fellows, which are typically from a different field. Programme 2018/2019 09.10.2018 Sandu Popescu On conservation laws in quantum mechanics 16.10.2018 Pierrick
Recommended publications
  • Nobel Laureates Endorse Joe Biden
    Nobel Laureates endorse Joe Biden 81 American Nobel Laureates in Physics, Chemistry, and Medicine have signed this letter to express their support for former Vice President Joe Biden in the 2020 election for President of the United States. At no time in our nation’s history has there been a greater need for our leaders to appreciate the value of science in formulating public policy. During his long record of public service, Joe Biden has consistently demonstrated his willingness to listen to experts, his understanding of the value of international collaboration in research, and his respect for the contribution that immigrants make to the intellectual life of our country. As American citizens and as scientists, we wholeheartedly endorse Joe Biden for President. Name Category Prize Year Peter Agre Chemistry 2003 Sidney Altman Chemistry 1989 Frances H. Arnold Chemistry 2018 Paul Berg Chemistry 1980 Thomas R. Cech Chemistry 1989 Martin Chalfie Chemistry 2008 Elias James Corey Chemistry 1990 Joachim Frank Chemistry 2017 Walter Gilbert Chemistry 1980 John B. Goodenough Chemistry 2019 Alan Heeger Chemistry 2000 Dudley R. Herschbach Chemistry 1986 Roald Hoffmann Chemistry 1981 Brian K. Kobilka Chemistry 2012 Roger D. Kornberg Chemistry 2006 Robert J. Lefkowitz Chemistry 2012 Roderick MacKinnon Chemistry 2003 Paul L. Modrich Chemistry 2015 William E. Moerner Chemistry 2014 Mario J. Molina Chemistry 1995 Richard R. Schrock Chemistry 2005 K. Barry Sharpless Chemistry 2001 Sir James Fraser Stoddart Chemistry 2016 M. Stanley Whittingham Chemistry 2019 James P. Allison Medicine 2018 Richard Axel Medicine 2004 David Baltimore Medicine 1975 J. Michael Bishop Medicine 1989 Elizabeth H. Blackburn Medicine 2009 Michael S.
    [Show full text]
  • Ripples in Spacetime
    editorial Ripples in spacetime The 2017 Nobel prize in Physics has been awarded to Rainer Weiss, Barry C. Barish and Kip S. Thorne “for decisive contributions to the LIGO detector and the observation of gravitational waves”. It is, frankly, difficult to find something original to say about the detection of gravitational waves that hasn’t been said already. The technological feat of measuring fluctuations in the fabric of spacetime less than one-thousandth the width of an atomic nucleus is quite simply astonishing. The scientific achievement represented by the confirmation of a century-old prediction by Albert Einstein is unique. And the collaborative effort that made the discovery possible — the Laser Interferometer Gravitational-Wave Observatory (LIGO) — is inspiring. Adapted from Phys. Rev. Lett. 116, 061102 (2016), under Creative Commons Licence. Rainer Weiss and Kip Thorne were, along with the late Ronald Drever, founders of the project that eventually became known Barry Barish, who was the director Last month we received a spectacular as LIGO. In the 1960s, Thorne, a black hole of LIGO from 1997 to 2005, is widely demonstration that talk of a new era expert, had come to believe that his objects of credited with transforming it into a ‘big of gravitational astronomy was no interest should be detectable as gravitational physics’ collaboration, and providing the exaggeration. Cued by detections at LIGO waves. Separately, and inspired by previous organizational structure required to ensure and Virgo, an interferometer based in Pisa, proposals, Weiss came up with the first it worked. Of course, the passion, skill and Italy, more than 70 teams of researchers calculations detailing how an interferometer dedication of the thousand or so scientists working at different telescopes around could be used to detect them in 1972.
    [Show full text]
  • Recent Observations of Gravitational Waves by LIGO and Virgo Detectors
    universe Review Recent Observations of Gravitational Waves by LIGO and Virgo Detectors Andrzej Królak 1,2,* and Paritosh Verma 2 1 Institute of Mathematics, Polish Academy of Sciences, 00-656 Warsaw, Poland 2 National Centre for Nuclear Research, 05-400 Otwock, Poland; [email protected] * Correspondence: [email protected] Abstract: In this paper we present the most recent observations of gravitational waves (GWs) by LIGO and Virgo detectors. We also discuss contributions of the recent Nobel prize winner, Sir Roger Penrose to understanding gravitational radiation and black holes (BHs). We make a short introduction to GW phenomenon in general relativity (GR) and we present main sources of detectable GW signals. We describe the laser interferometric detectors that made the first observations of GWs. We briefly discuss the first direct detection of GW signal that originated from a merger of two BHs and the first detection of GW signal form merger of two neutron stars (NSs). Finally we present in more detail the observations of GW signals made during the first half of the most recent observing run of the LIGO and Virgo projects. Finally we present prospects for future GW observations. Keywords: gravitational waves; black holes; neutron stars; laser interferometers 1. Introduction The first terrestrial direct detection of GWs on 14 September 2015, was a milestone Citation: Kro´lak, A.; Verma, P. discovery, and it opened up an entirely new window to explore the universe. The combined Recent Observations of Gravitational effort of various scientists and engineers worldwide working on the theoretical, experi- Waves by LIGO and Virgo Detectors.
    [Show full text]
  • Rainer Weiss, Professor of Physics Emeritus and 2017 Nobel Laureate
    Giving to the Department of Physics by Erin McGrath RAINER WEISS ’55, PHD ’62 Bryce Vickmark Rai Weiss has established a fellowship in the Physics Department because he is eternally grateful to his advisor, the late Jerrold Zacharias, for all that he did for Rai, so he knows firsthand the importance of supporting graduate students. Rainer Weiss, Professor of Physics Emeritus and 2017 Nobel Laureate. Rainer “Rai” Weiss was born in Berlin, Germany in 1932. His father was a physician and his mother was an actress. His family was forced out of Germany by the Nazis since his father was Jewish and a Communist. Rai, his mother and father fled to Prague, Czecho- slovakia. In 1937 a sister was born in Prague. In 1938, after Chamberlain appeased Hitler by effectively giving him Czechoslovakia, the family was able to obtain visas to enter the United States through the Stix Family in St. Louis, who were giving bond to professional Jewish emigrants. When Rai was 21 years-old, he visited Mrs. Stix and thanked her for what she had done for his family. The family immigrated to New York City. Rai’s father had a hard time passing the medi- cal boards because of his inability to answer multiple choice exams. His mother, who Rai says “held the family together,” worked in a number of retail stores. Through the services of an immigrant relief organization Rai received a scholarship to attend the prestigious Columbia Grammar School. At the end of 1945, when Rai was 13 years old, he became fascinated with electronics and music.
    [Show full text]
  • The Titans of the Cosmos
    FALL 2018 Titans of the Cosmos Exploring the Mysteries of Neutron Star Mergers & Supermassive Black Holes 10 | Educating the next generation of innovators in science and industry 16 | Berkeley leads the way in data science education Research Highlights, Department News & More CONTENTS CHAIR’SLETTER RESEARCH HIGHLIGHTS2 Recent breakthroughs in faculty-led investigations PHOTO: BEN AILES PHOTO: TITANS OF THE COSMOS Fall classes are underway, our introductory courses ON THE COVER: Exploring the Mysteries of are packed, and we have good news on several fronts. Berkeley astrophysicist Daniel Kasen's research group uses Neutron Star Mergers and On July 1 we welcomed our newest faculty member, supercomputers at the National Supermassive Black Holes condensed matter theorist Mike Zalatel. In August the Energy Research Scientific Com- puting Center at LBNL to model 2018 Academic Rankings of World Universities were cosmic explosions. See page 4. announced, with Berkeley Physics second, between MIT CHAIR and Stanford – fine company. In September we learned Wick Haxton 4 that Professor Barbara Jacak will be awarded the 2019 MANAGING EDITOR & Tom Bonner Prize of the American Physical Society for DIRECTOR OF DEVELOPMENT her leadership of the PHENIX detector at Brookhaven’s Rachel Schafer Relativistic Heavy Ion Collider, and new graduate stu- CONTRIBUTING EDITOR & dent Nick Sherman will receive the LeRoy Apker Award SCIENCE WRITER for outstanding undergraduate research in theoretical Devi Mathieu PHYSICS INNOVATORS condensed matter and mathematical physics. Most re- DESIGN 10INITIATIVE cently, Assistant Professor Norman Yao has been named Sarah Wittmer Educating the Next a Packard Fellow, one of the most prestigious awards CONTRIBUTORS Generation of Innovators available in STEM disciplines.
    [Show full text]
  • A Brief History of Gravitational Waves
    Review A Brief History of Gravitational Waves Jorge L. Cervantes-Cota 1, Salvador Galindo-Uribarri 1 and George F. Smoot 2,3,4,* 1 Department of Physics, National Institute for Nuclear Research, Km 36.5 Carretera Mexico-Toluca, Ocoyoacac, Mexico State C.P.52750, Mexico; [email protected] (J.L.C.-C.); [email protected] (S.G.-U.) 2 Helmut and Ana Pao Sohmen Professor at Large, Institute for Advanced Study, Hong Kong University of Science and Technology, Clear Water Bay, 999077 Kowloon, Hong Kong, China. 3 Université Sorbonne Paris Cité, Laboratoire APC-PCCP, Université Paris Diderot, 10 rue Alice Domon et Leonie Duquet 75205 Paris Cedex 13, France. 4 Department of Physics and LBNL, University of California; MS Bldg 50-5505 LBNL, 1 Cyclotron Road Berkeley, CA 94720, USA. * Correspondence: [email protected]; Tel.:+1-510-486-5505 Abstract: This review describes the discovery of gravitational waves. We recount the journey of predicting and finding those waves, since its beginning in the early twentieth century, their prediction by Einstein in 1916, theoretical and experimental blunders, efforts towards their detection, and finally the subsequent successful discovery. Keywords: gravitational waves; General Relativity; LIGO; Einstein; strong-field gravity; binary black holes 1. Introduction Einstein’s General Theory of Relativity, published in November 1915, led to the prediction of the existence of gravitational waves that would be so faint and their interaction with matter so weak that Einstein himself wondered if they could ever be discovered. Even if they were detectable, Einstein also wondered if they would ever be useful enough for use in science.
    [Show full text]
  • Rainer Weiss Year: 1972 Journal Citation: Quarterly Progress Report, Research Laboratory of Electronics (MIT) No
    Author: Rainer Weiss Year: 1972 Journal Citation: Quarterly Progress Report, Research Laboratory of Electronics (MIT) No. 105, p.54. Title: Electronically Coupled Broadband Gravitational Antenna nLtr Cli/x = .*= /( 6\"iue lSApr'tla (v. GR-rvIT-{TrOriRESE-{P.CH) B. ELECTROAIAGNETICALLY COUPLED BR OADBAND GR.{,VIT.{TIONAL A\TE:i\A l. Intro duction The prediction of gravitational radiarion that travels at the speed of Ught has been an essential part of every gravitational theory since the discovery of special relativiiy. ^I In !918, Einstein, usirg a rveak-field appPoxirnationin bis very successful geometrical theory of gravity (the general theory of relativity), indicated the form that gravitational waves would take rn ihis theorj- and demonstrated that systems with titne-variant mass quadrupole moments u,ou]d lose energy by gravitational radiation. It was evident to Einstein that since gravitationaf radiation is extremely weak, the most likely measurable radiatj,on woulci come from astronomi,cal sources. For many years the subject of gravj.tational radiation remained the province of a few dedicated theorists; however, the recen! discovery of the pulsars and the pioneering and controve:'sial experiments of Weber-'' at the Universitt' of Maryland have engendered a new interest in ihe field. Weber has reported coincldent excitarions in two gravitational anter/tras separaied 1000 km. These antelrnas are high-Q resonard ba.rs tuned to 1.6 kHz. He attributes these excitattons to puLsesof graviiadonal radiadon emitted by broadband sources con- cenirated nesr the eenter of our galaxy. If Weberrs i$terpretatj.on of these events is corlect, the:'e is ar e!:ormous flnx of gravitationaL fadiation incident on the Earth.
    [Show full text]
  • Gravitational Waves WARNING!!!!
    Gravitational Waves WARNING!!!! ⚫ Terminology is treacherous! ⚫ There are gravitational waves (our topic) and there are gravity waves (a topic for a surfing class). Mix them to your peril. Gravitational waves ⚫ Movie The History ⚫ The history of gravitational waves is rocky. Einstein argued in 1916 that gravitational waves must exist – if the space-time is dynamic, there must be ripples on it. ⚫ Einstein derived the approximate formula for the gravitational waves from two orbiting bodies. ⚫ In 1922 Eddington (that one) argued that gravitational waves were not real and just a mathematical artefact. The History ⚫ In 1936 Einstein wrote a paper with Nathan Rosen reversing his original view; they concluded that all gravitational waves should collapse into black holes. ⚫ The paper was submitted to Physics Review but was returned after the referee pointed out a mistake in it. ⚫ Einstein got berserk in response, writing an angry letter to the editor and promising never to publish in Physics Review again. The History ⚫ Einstein was later persuaded by Infeld of his mistake and corrected the paper. Rosen never conceded. ⚫ In 1957 Richard Feymann (a very famous particle physicist) presented a “sticky bead” argument that convinced most people that gravitational waves are real. The Challenge ⚫ The primary challenge with gravitational waves is that in GR there is no (unambiguous) mathematical expression for its energy. ⚫ Since locally space-time is Minkowski, in the local inertial reference frame the energy of gravitational waves is zero. I.e., that energy is non-local, one cannot claim that the energy of gravitational waves is … at his location, only that the total energy is such and such.
    [Show full text]
  • Highlights of Modern Physics and Astrophysics
    Highlights of Modern Physics and Astrophysics How to find the “Top Ten” in Physics & Astrophysics? - List of Nobel Laureates in Physics - Other prizes? Templeton prize, … - Top Citation Rankings of Publication Search Engines - Science News … - ... Nobel Laureates in Physics Year Names Achievement 2020 Sir Roger Penrose "for the discovery that black hole formation is a robust prediction of the general theory of relativity" Reinhard Genzel, Andrea Ghez "for the discovery of a supermassive compact object at the centre of our galaxy" 2019 James Peebles "for theoretical discoveries in physical cosmology" Michel Mayor, Didier Queloz "for the discovery of an exoplanet orbiting a solar-type star" 2018 Arthur Ashkin "for groundbreaking inventions in the field of laser physics", in particular "for the optical tweezers and their application to Gerard Mourou, Donna Strickland biological systems" "for groundbreaking inventions in the field of laser physics", in particular "for their method of generating high-intensity, ultra-short optical pulses" Nobel Laureates in Physics Year Names Achievement 2017 Rainer Weiss "for decisive contributions to the LIGO detector and the Kip Thorne, Barry Barish observation of gravitational waves" 2016 David J. Thouless, "for theoretical discoveries of topological phase transitions F. Duncan M. Haldane, and topological phases of matter" John M. Kosterlitz 2015 Takaaki Kajita, "for the discovery of neutrino oscillations, which shows that Arthur B. MsDonald neutrinos have mass" 2014 Isamu Akasaki, "for the invention of
    [Show full text]
  • 69Th Lindau Nobel Laureate Meeting Programme MEETING APPS
    69th Lindau Nobel Laureate Meeting Programme MEETING APPS The Lindau Meetings offer three different apps, available on Android and Apple app stores: Lindau Nobel Laureate Meetings The meeting guide • Up-to-date programme info & details • Session abstracts and poster abstracts • Ask questions during panel discussions • Participate in surveys • Interactive maps • Social media integration Lindau Alumni Network Stay in contact with your peers • News • Direct messages • Participant profiles • Alumni events All young scientists have been invited to join the Lindau Alumni Network. Lindau Science Trail Explore the Lindau Science Trail • Interactive map • Rich content & detailed background information • Tours & quizzes 2 TABLE OF CONTENTS Scientific Programme page 10 About the Meetings page 37 Supporters page 42 Maps page 50 Good to Know page 62 3 WELCOME In 1951, the idea of two doctors from the small town of Lindau became real- ity: They had the vision of reuniting European scientists after years of sepa- ration during World War II. Together with Count Lennart Bernadotte from nearby Mainau Island, Franz Karl Hein and Gustav Wilhelm Parade realised the first “European Meeting of Nobel Laureates” with seven Nobel Laure- ates. Only two years later, the first students were invited – the rest is history. This summer, 39 Nobel Laureates and 580 young scientists from 89 coun- tries will join the 69th Lindau Nobel Laureate Meeting. Never before have so many countries been represented in this extraordinary exchange. All you excellent scientists from around the world have one thing in common: your passion for physics. We hope you will experience the special “Lindau Spir- it”– as more than 30.000 Lindau Alumni did before you.
    [Show full text]
  • Mathematics People
    NEWS Mathematics People “In 1972, Rainer Weiss wrote down in an MIT report his Weiss, Barish, and ideas for building a laser interferometer that could detect Thorne Awarded gravitational waves. He had thought this through carefully and described in detail the physics and design of such an Nobel Prize in Physics instrument. This is typically called the ‘birth of LIGO.’ Rai Weiss’s vision, his incredible insights into the science and The Royal Swedish Academy of Sci- challenges of building such an instrument were absolutely ences has awarded the 2017 Nobel crucial to make out of his original idea the successful Prize in Physics to Rainer Weiss, experiment that LIGO has become. Barry C. Barish, and Kip S. Thorne, “Kip Thorne has done a wealth of theoretical work in all of the LIGO/Virgo Collaboration, general relativity and astrophysics, in particular connected for their “decisive contributions to with gravitational waves. In 1975, a meeting between the LIGO detector and the observa- Rainer Weiss and Kip Thorne from Caltech marked the tion of gravitational waves.” Weiss beginning of the complicated endeavors to build a gravi- receives one-half of the prize; Barish tational wave detector. Rai Weiss’s incredible insights into and Thorne share one-half. the science and challenges of building such an instrument Rainer Weiss combined with Kip Thorne’s theoretical expertise with According to the prize citation, gravitational waves, as well as his broad connectedness “LIGO, the Laser Interferometer with several areas of physics and funding agencies, set Gravitational-Wave Observatory, is the path toward a larger collaboration.
    [Show full text]
  • Nobel Laureate Kip Thorne, Nobel Prize 2017. LIGO and Gravitational
    Abstract: My 60 Year Romance with the Warped Side of the Universe - And What It Has Taught Me about Physics Education Already in the 1950s and 60s, when I was a student, Einstein’s general relativity theory suggested that there might be a “warped side” of our universe: objects and phenomena made not from matter, but from warped spacetime. These include, among others, black holes, wormholes, backward time travel, gravitational waves, and the big-bang birth of the universe. I have devoted most of my career to exploring this warped side through theory and computer simulations, and to developing plans and technology for exploring the warped side observationally, via gravitational waves. Most of my classroom teaching, mentoring, writing, and outreach to nonscientists, has revolved around the warped side; and from this I have developed some strong views about physics education. In this talk I will discuss those views, in the context of personal anecdotes about my warped-side research, teaching, mentoring, writing, and outreach. Bio: Kip Thorne was born in 1940 in Logan, Utah, USA, and is currently the Feynman Professor of Theoretical Physics, Emeritus at the California Institute of Technology (Caltech). From 1967 to 2009, he led a Caltech research group working in relativistic astrophysics and gravitational physics, with emphasis on relativistic stars, black holes, and especially gravitational waves. Fifty three students received their PhD’s under his mentorship, and he mentored roughly sixty postdoctoral students. He co-authored the textbooks Gravitation (1973, with Charles Misner and John Archibald Wheeler) and Modern Classical Physics (2017, with Roger Blandford), and was sole author of Black Holes and Time Warps: Einstein’s Outrageous Legacy.
    [Show full text]