Losing Equilibrium: on the Existence of Abraham Wald's Fixed-Point Proof of 1935
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The Emergence of Gravitational Wave Science: 100 Years of Development of Mathematical Theory, Detectors, Numerical Algorithms, and Data Analysis Tools
BULLETIN (New Series) OF THE AMERICAN MATHEMATICAL SOCIETY Volume 53, Number 4, October 2016, Pages 513–554 http://dx.doi.org/10.1090/bull/1544 Article electronically published on August 2, 2016 THE EMERGENCE OF GRAVITATIONAL WAVE SCIENCE: 100 YEARS OF DEVELOPMENT OF MATHEMATICAL THEORY, DETECTORS, NUMERICAL ALGORITHMS, AND DATA ANALYSIS TOOLS MICHAEL HOLST, OLIVIER SARBACH, MANUEL TIGLIO, AND MICHELE VALLISNERI In memory of Sergio Dain Abstract. On September 14, 2015, the newly upgraded Laser Interferometer Gravitational-wave Observatory (LIGO) recorded a loud gravitational-wave (GW) signal, emitted a billion light-years away by a coalescing binary of two stellar-mass black holes. The detection was announced in February 2016, in time for the hundredth anniversary of Einstein’s prediction of GWs within the theory of general relativity (GR). The signal represents the first direct detec- tion of GWs, the first observation of a black-hole binary, and the first test of GR in its strong-field, high-velocity, nonlinear regime. In the remainder of its first observing run, LIGO observed two more signals from black-hole bina- ries, one moderately loud, another at the boundary of statistical significance. The detections mark the end of a decades-long quest and the beginning of GW astronomy: finally, we are able to probe the unseen, electromagnetically dark Universe by listening to it. In this article, we present a short historical overview of GW science: this young discipline combines GR, arguably the crowning achievement of classical physics, with record-setting, ultra-low-noise laser interferometry, and with some of the most powerful developments in the theory of differential geometry, partial differential equations, high-performance computation, numerical analysis, signal processing, statistical inference, and data science. -
Arxiv:Gr-Qc/0304042V1 9 Apr 2003
Do black holes radiate? Adam D Helfer Department of Mathematics, Mathematical Sciences Building, University of Missouri, Columbia, Missouri 65211, U.S.A. Abstract. The prediction that black holes radiate due to quantum effects is often considered one of the most secure in quantum field theory in curved space–time. Yet this prediction rests on two dubious assumptions: that ordinary physics may be applied to vacuum fluctuations at energy scales increasing exponentially without bound; and that quantum–gravitational effects may be neglected. Various suggestions have been put forward to address these issues: that they might be explained away by lessons from sonic black hole models; that the prediction is indeed successfully reproduced by quantum gravity; that the success of the link provided by the prediction between black holes and thermodynamics justifies the prediction. This paper explains the nature of the difficulties, and reviews the proposals that have been put forward to deal with them. None of the proposals put forward can so far be considered to be really successful, and simple dimensional arguments show that quantum–gravitational effects might well alter the evaporation process outlined by Hawking. arXiv:gr-qc/0304042v1 9 Apr 2003 Thus a definitive theoretical treatment will require an understanding of quantum gravity in at least some regimes. Until then, no compelling theoretical case for or against radiation by black holes is likely to be made. The possibility that non–radiating “mini” black holes exist should be taken seriously; such holes could be part of the dark matter in the Universe. Attempts to place observational limits on the number of “mini” black holes (independent of the assumption that they radiate) would be most welcome. -
Jacob Wolfowitz 1910–1981
NATIONAL ACADEMY OF SCIENCES JACOB WOLFOWITZ 1910–1981 A Biographical Memoir by SHELEMYAHU ZACKS Any opinions expressed in this memoir are those of the author and do not necessarily reflect the views of the National Academy of Sciences. Biographical Memoirs, VOLUME 82 PUBLISHED 2002 BY THE NATIONAL ACADEMY PRESS WASHINGTON, D.C. JACOB WOLFOWITZ March 19, 1910–July 16, 1981 BY SHELEMYAHU ZACKS ACOB WOLFOWITZ, A GIANT among the founders of modern Jstatistics, will always be remembered for his originality, deep thinking, clear mind, excellence in teaching, and vast contributions to statistical and information sciences. I met Wolfowitz for the first time in 1957, when he spent a sab- batical year at the Technion, Israel Institute of Technology. I was at the time a graduate student and a statistician at the building research station of the Technion. I had read papers of Wald and Wolfowitz before, and for me the meeting with Wolfowitz was a great opportunity to associate with a great scholar who was very kind to me and most helpful. I took his class at the Technion on statistical decision theory. Outside the classroom we used to spend time together over a cup of coffee or in his office discussing statistical problems. He gave me a lot of his time, as though I was his student. His advice on the correct approach to the theory of statistics accompanied my development as statistician for many years to come. Later we kept in touch, mostly by correspondence and in meetings of the Institute of Mathematical Statistics. I saw him the last time in his office at the University of Southern Florida in Tampa, where he spent the last years 3 4 BIOGRAPHICAL MEMOIRS of his life. -
Meeting Program
22nd Midwest Relativity Meeting September 28-29, 2012 Chicago, IL http://kicp-workshops.uchicago.edu/Relativity2012/ MEETING PROGRAM http://kicp.uchicago.edu/ http://www.uchicago.edu/ The 22nd Midwest Relativity Meeting will be held Friday and Saturday, September 28 and 29, 2012 at the University of Chicago. The format of the meeting will follow previous regional meetings, where all participants may present a talk of approximately 10-15 minutes, depending on the total number of talks. We intend for the meeting to cover a broad range of topics in gravitation physics, including classical and quantum gravity, numerical relativity, relativistic astrophysics, cosmology, gravitational waves, and experimental gravity. As this is a regional meeting, many of the participants will be from the greater United States Midwest and Canada, but researchers and students from other geographic areas are also welcome. Students are strongly encouraged to give presentations. The Blue Apple Award, sponsored by the APS Topical Group in Gravitation, will be awarded for the best student presentation. We gratefully acknowledge the generous support provided by the Kavli Institute for Cosmological Physics (KICP) at the University of Chicago. Organizing Committe Daniel Holz Robert Wald University of Chicago University of Chicago 22nd Midwest Relativity Meeting September 28-29, 2012 @ Chicago, IL MEETING PROGRAM September 28-29, 2012 @ Kersten Physics Teaching Center (KPTC), Room 106 Friday - September 28, 2012 8:15 AM - 8:55 AM COFFEE & PASTRIES 8:55 AM - 9:00 AM WELCOME -
List of Participants
Exploring Theories of Modified Gravity October 12-14, 2015 KICP workshop, 2015 Chicago, IL http://kicp-workshops.uchicago.edu/2015-mg/ LIST OF PARTICIPANTS http://kicp.uchicago.edu/ http://www.nsf.gov/ http://www.uchicago.edu/ The Kavli Institute for Cosmological Physics (KICP) at the University of Chicago is hosting a workshop this fall on theories of modified gravity. The purpose of workshop is to discuss recent progress and interesting directions in theoretical research into modified gravity. Topics of particular focus include: massive gravity, Horndeski, beyond Horndeski, and other derivatively coupled theories, screening and new physics in the gravitational sector, and possible observational probes of the above. The meeting will be relatively small, informal, and interactive workshop for the focused topics. Organizing Committee Scott Dodelson Wayne Hu Austin Joyce Fermilab, University of Chicago University of Chicago University of Chicago Hayato Motohashi Lian-Tao Wang University of Chicago University of Chicago Exploring Theories of Modified Gravity October 12-14, 2015 @ Chicago, IL 1. Tessa M Baker UPenn / University of Oxford 2. John Boguta University of Illinois Chicago 3. Claudia de Rham Case Western Reserve University 4. Cedric Deffayet CNRS 5. Scott Dodelson Fermilab, University of Chicago 6. Matteo R Fasiello Stanford 7. Maya Fishbach University of Chicago 8. Gregory Gabadadze New York University 9. Salman Habib Argonne National Laboratory 10. Kurt Hinterbichler Perimeter Institute for Theoretical Physics 11. Daniel Holz KICP 12. Wayne Hu University of Chicago 13. Lam Hui Columbia University 14. Elise Jennings Fermilab 15. Austin Joyce University of Chicago 16. Nemanja Kaloper University of California, Davis 17. Rampei Kimura New York University 18. -
On the Backreaction of Scalar and Spinor Quantum Fields in Curved Spacetimes
On the Backreaction of Scalar and Spinor Quantum Fields in Curved Spacetimes Dissertation zur Erlangung des Doktorgrades des Department Physik der Universität Hamburg vorgelegt von Thomas-Paul Hack aus Timisoara Hamburg 2010 Gutachter der Dissertation: Prof. Dr. K. Fredenhagen Prof. Dr. V. Moretti Prof. Dr. R. M. Wald Gutachter der Disputation: Prof. Dr. K. Fredenhagen Prof. Dr. W. Buchmüller Datum der Disputation: Mittwoch, 19. Mai 2010 Vorsitzender des Prüfungsausschusses: Prof. Dr. J. Bartels Vorsitzender des Promotionsausschusses: Prof. Dr. J. Bartels Dekan der Fakultät für Mathematik, Informatik und Naturwissenschaften: Prof. Dr. H. Graener Zusammenfassung In der vorliegenden Arbeit werden zunächst einige Konstruktionen und Resultate in Quantenfeldtheorie auf gekrümmten Raumzeiten, die bisher nur für das Klein-Gordon Feld behandelt und erlangt worden sind, für Dirac Felder verallgemeinert. Es wird im Rahmen des algebraischen Zugangs die erweiterte Algebra der Observablen konstruiert, die insbesondere normalgeordnete Wickpolynome des Diracfeldes enthält. Anschließend wird ein ausgezeichnetes Element dieser erweiterten Algebra, der Energie-Impuls Tensor, analysiert. Unter Zuhilfenahme ausführlicher Berechnungen der Hadamardkoe ?zienten des Diracfeldes wird gezeigt, dass eine lokale, kovariante und kovariant erhaltene Konstruktion des Energie- Impuls Tensors möglich ist. Anschließend wird das Verhältnis der mathematisch fundierten Hadamardreg- ularisierung des Energie-Impuls Tensors mit der mathematisch weniger rigorosen DeWitt-Schwinger -
Adalékok Wald Ábrahám Életrajzához Additions to Abraham Wald's Biography Adăugări La Biografia Lui Abraham Wald FERENC Márta, LŐRINCZ Annamária, OLÁH-GÁL Róbert
Adalékok Wald Ábrahám életrajzához Additions to Abraham Wald's biography Adăugări la biografia lui Abraham Wald FERENC Márta, LŐRINCZ Annamária, OLÁH-GÁL Róbert Sapientia Erdélyi Magyar Tudományegyetem, Csíkszeredai Kar, [email protected], [email protected], [email protected] Összefoglaló Száz évvel Bolyai János születése után Kolozsváron született egy másik nagy, de sajnos ke- vébé ismert matematikus, Wald Ábrahám. Wald Ábrahám ortodox-zsidó (hasszid) családban született. Sajnos nagyon kevés dokumentum maradt meg Wald életéről. A modern statisztikák- ban és az ökonometriában Wald nevét sok tétel őrzi. Ebben a cikkben eredeti dokumentumokat mutatunk be Wald Ábrahám életéről, nevezetesen: a kolozsvári piarista gimnázium matrikulai nyilvántartását, és 3 Wald Ábrahám által Alexits Györgynek magyarul írt levelet. A levéltári anyagok bemutatása forrásközlés. A cikk végén hangsúlyozzuk Wald Ábrahám szellemi és anyagi örökségének megőrzésének fontosságát. Wald örökségének megőrzéséhez emléktáblát kellene felállítani a Waldek szülői házának falán, Kolozsváron. Abstract One hundred years after the birth of János Bolyai, another well-known mathematician, Ábrahám Wald, was born in Cluj-Napoca. Ábrahám Wald was born into a Jewish-Orthodox family. Unfortu- nately, we don't have many documents about Wald's life. In modern statistics and econometrics many theorems of Wald's name are related. In this article we present original documents about the life of Ábrahám Wald, namely: the matriculation register from the Piarist High School in Cluj, and 3 letters of Ábrahám Wald written to György Alexits in Hungarian. Our presentation is an authentic first publi- cation. At the end of this article, we emphasize the importance of commemorating the intellectual and material heritage of Ábrahám Wald. -
2015MRM Scientific Program.Pdf
Thursday, October 1 Afternoon Welcoming Remarks 1:00 p.m. – 1:10 p.m. Vicky Kalogera, Center for Interdisciplinary Exploration and Research in Astrophysics Special General Relativity Invited Talks 1:10 p.m. – 5:10 p.m. Chair: Vicky Kalogera 1:10 2:00 Stu Shapiro, University of Illinois Compact Binary Mergers as Multimessenger Sources of Gravitational Waves 2:00 2:50 Lydia Bieri, University of Michigan Mathematical Relativity Chair: Shane Larson 3:30 4:20 Eva Silverstein, Stanford University Quantum gravity in the early universe and at horizons 4:20 5:10 Rainer Weiss, MIT A brief history of gravitational waves: theoretical insight to measurement Public lecture 7:30 p.m. – 9:00 p.m. 7:30 9:00 John D. Norton, University of Pittsburgh Einstein’s Discovery of the General Theory of Relativity Friday, October 2 Morning, Session One Gravitational Wave Sources 9:00 a.m. – 10:30 a.m. Chair: Vicky Kalogera 9:00 9:12 Carl Rodriguez*, Northwestern University Binary Black Hole Mergers from Globular Clusters: Implications for Advanced LIGO 9:12 9:24 Thomas Osburn*, UNC Chapel Hill Computing extreme mass ratio inspirals at high accuracy and large eccentricity using a hybrid method 9:24 9:36 Eliu Huerta, NCSA, University of Illinois at Urbana-Champaign Detection of eccentric supermassive black hole binaries with pulsar timing arrays: Signal-to-noise ratio calculations 9:36 9:48 Katelyn Breivik*, Northwestern University Exploring galactic binary population variance with population synthesis 9:48 10:00 Eric Poisson, University of Guelph Fluid resonances and self-force 10:00 10:12 John Poirier, University of Notre Dame Gravitomagnetic acceleration of accretion disk matter to polar jets John Poirier and Grant Mathews 10:12 10:24 Philippe Landry*, University of Guelph Tidal Deformation of a Slowly Rotating Material Body *Student 2015 Midwest Relativity Meeting 1 Friday, October 2 Morning, Session Two Gravitational Wave/Electromagnetic Detections 11:00 a.m. -
Passmore, J. (1967). Logical Positivism. in P. Edwards (Ed.). the Encyclopedia of Philosophy (Vol. 5, 52- 57). New York: Macmillan
Passmore, J. (1967). Logical Positivism. In P. Edwards (Ed.). The Encyclopedia of Philosophy (Vol. 5, 52- 57). New York: Macmillan. LOGICAL POSITIVISM is the name given in 1931 by A. E. Blumberg and Herbert Feigl to a set of philosophical ideas put forward by the Vienna circle. Synonymous expressions include "consistent empiricism," "logical empiricism," "scientific empiricism," and "logical neo-positivism." The name logical positivism is often, but misleadingly, used more broadly to include the "analytical" or "ordinary language philosophies developed at Cambridge and Oxford. HISTORICAL BACKGROUND The logical positivists thought of themselves as continuing a nineteenth-century Viennese empirical tradition, closely linked with British empiricism and culminating in the antimetaphysical, scientifically oriented teaching of Ernst Mach. In 1907 the mathematician Hans Hahn, the economist Otto Neurath, and the physicist Philipp Frank, all of whom were later to be prominent members of the Vienna circle, came together as an informal group to discuss the philosophy of science. They hoped to give an account of science which would do justice -as, they thought, Mach did not- to the central importance of mathematics, logic, and theoretical physics, without abandoning Mach's general doctrine that science is, fundamentally, the description of experience. As a solution to their problems, they looked to the "new positivism" of Poincare; in attempting to reconcile Mach and Poincare; they anticipated the main themes of logical positivism. In 1922, at the instigation of members of the "Vienna group," Moritz Schlick was invited to Vienna as professor, like Mach before him (1895-1901), in the philosophy of the inductive sciences. Schlick had been trained as a scientist under Max Planck and had won a name for himself as an interpreter of Einstein's theory of relativity. -
THE EPIC STORY of MAXIMUM LIKELIHOOD 3 Error Probabilities Follow a Curve
Statistical Science 2007, Vol. 22, No. 4, 598–620 DOI: 10.1214/07-STS249 c Institute of Mathematical Statistics, 2007 The Epic Story of Maximum Likelihood Stephen M. Stigler Abstract. At a superficial level, the idea of maximum likelihood must be prehistoric: early hunters and gatherers may not have used the words “method of maximum likelihood” to describe their choice of where and how to hunt and gather, but it is hard to believe they would have been surprised if their method had been described in those terms. It seems a simple, even unassailable idea: Who would rise to argue in favor of a method of minimum likelihood, or even mediocre likelihood? And yet the mathematical history of the topic shows this “simple idea” is really anything but simple. Joseph Louis Lagrange, Daniel Bernoulli, Leonard Euler, Pierre Simon Laplace and Carl Friedrich Gauss are only some of those who explored the topic, not always in ways we would sanction today. In this article, that history is reviewed from back well before Fisher to the time of Lucien Le Cam’s dissertation. In the process Fisher’s unpublished 1930 characterization of conditions for the consistency and efficiency of maximum likelihood estimates is presented, and the mathematical basis of his three proofs discussed. In particular, Fisher’s derivation of the information inequality is seen to be derived from his work on the analysis of variance, and his later approach via estimating functions was derived from Euler’s Relation for homogeneous functions. The reaction to Fisher’s work is reviewed, and some lessons drawn. -
Karl Menger Seymour Kass
comm-menger.qxp 4/22/98 9:44 AM Page 558 Karl Menger Seymour Kass Karl Menger died on October 5, 1985, in Chicago. dents were Nobel Laureates Richard Kuhn and Except in his native Austria [5], no obituary no- Wolfgang Pauli. He entered the University of Vi- tice seems to have appeared. This note marks ten enna in 1920 to study physics, attending the lec- years since his passing. tures of physicist Hans Thirring. Hans Hahn Menger’s career spanned sixty years, during joined the mathematics faculty in March 1921, which he published 234 papers, 65 of them be- and Menger attended his seminar “News about fore the age of thirty. A partial bibliography ap- the Concept of Curves”. In the first lecture Hahn pears in [15]. His early work in geometry and formulated the problem of making precise the topology secured him an enduring place in math- idea of a curve, which no one had been able to ematics, but his reach extended to logic, set the- articulate, mentioning the unsuccessful attempts ory, differential geometry, calculus of variations, of Cantor, Jordan, and Peano. The topology used graph theory, complex functions, algebra of in the lecture was new to Menger, but he “was functions, economics, philosophy, and peda- completely enthralled and left the lecture room gogy. Characteristic of Menger’s work in geom- in a daze” [10, p. 41]. After a week of complete etry and topology is the reworking of funda- engrossment, he produced a definition of a curve mental concepts from intrinsic points of view and confided it to fellow student Otto Schreier, (curve, dimension, curvature, statistical metric who could find no flaw but alerted Menger to re- spaces, hazy sets). -
1 (Information) Paradox Lost Tim Maudlin
(Information) Paradox Lost Tim Maudlin Department of Philosophy New York University New York, NY 10003 Abstract Since Stephen Hawking’s original 1975 paper on black hole evaporation there has been a consensus that the problem of “loss of information” is both deep and troubling, and may hold some conceptual keys to the unification of gravity with the other forces. I argue that this consensus view is mistaken. The so-called “information loss paradox” arises rather from the inaccurate application of foundational principles, involving both mathematical and conceptual errors. The resources for resolving the “paradox” are familiar and uncontroversial, and have been pointed out in the literature. The problem ought to have been dismissed 40 years ago. Recent radical attempts to “solve” the problem are blind alleys, solutions in search of a problem. 1 Introductory Incitement There is no “information loss” paradox. There never has been. If that seems like a provocation, it’s because it is one. Few problems have gotten as much attention in theoretical foundations of physics over the last 40 years as the so-called information loss paradox. But the “solution” to the paradox does not require any new physics that was unavailable in 1975, when Stephen Hawking posed the problem [1]. Indeed, the complete solution can be stated in a single sentence. And it has been pointed out, most forcefully by Robert Wald. The claim above ought to be frankly incredible. How could a simple solution have gone unappreciated by so many theoretical physicists—among them very great physicists—over such a long period of time? Probably no completely satisfactory non-sociological explanation is possible.