BEYOND SPACE and TIME the Secret Network of the Universe: How Quantum Geometry Might Complete Einstein’S Dream
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The Metaphysical Baggage of Physics Lee Smolin Argues That Life Is More
The Metaphysical Baggage of Physics Lee Smolin argues that life is more fundamental than physical laws. BY MICHAEL SEGAL ILLUSTRATION BY LOUISA BERTMAN JANUARY 30, 2014 An issue on tme would not be complete without a conversaton with Lee Smolin. High school dropout, theoretcal physicist, and founding member of the Perimeter Insttute for Theoretcal Physics in Waterloo, Canada, Smolin’s life and work refect many of the values of this magazine. Constantly probing the edges of physics, he has also pushed beyond them, into economics and the philosophy of science, and into popular writng. Not one to shy away from a confrontaton, his 2008 bookThe Trouble with Physicstook aim at string theory, calling one of the hotest developments in theoretcal physics of the past 50 years a dead end. In his thinking on tme too, he has taken a diferent tack from the mainstream, arguing that the fow of tme is not just real, but more fundamental than physical law. He spoke to me on the phone from his home in Toronto. How long have you been thinking about tme? The whole story starts back in the ’80s when I was puzzling over the failure of string theory to uniquely tell us the principles that determine what the laws of physics are. I challenged myself to invent a way that nature might select what the laws of physics turned out to be. I invented a hypothesis called Cosmological Natural Selecton, which was testable, which made explicit predictons. This wasn’t my main day job; my main day job was working on quantum gravity where it’s assumed that tme is unreal, that tme is an illusion, and I was working, like anybody else, on the assumpton that tme is an illusion for most of my career. -
Information Loss, Made Worse by Quantum Gravity?
ORIGINAL RESEARCH published: 20 May 2015 doi: 10.3389/fphy.2015.00033 Information loss, made worse by quantum gravity? Martin Bojowald * Department of Physics, Institute for Gravitation and the Cosmos, The Pennsylvania State University, University Park, PA, USA Quantum gravity is often expected to solve both the singularity problem and the information-loss problem of black holes. This article presents an example from loop quantum gravity in which the singularity problem is solved in such a way that the information-loss problem is made worse. Quantum effects in this scenario, in contrast to previous non-singular models, do not eliminate the event horizon and introduce a new Cauchy horizon where determinism breaks down. Although infinities are avoided, for all practical purposes the core of the black hole plays the role of a naked singularity. Recent developments in loop quantum gravity indicate that this aggravated information loss problem is likely to be the generic outcome, putting strong conceptual pressure on the theory. Edited by: Keywords: signature change, loop quantum gravity, black holes, information loss, effective theory Martin Anthony Hendry, University of Glasgow, UK Reviewed by: 1. Introduction Davood Momeni, L.N. Gumilyov Eurasian National There is a widespread expectation that quantum gravity, once it is fully developed and understood, University, Kazakhstan will resolve several important conceptual problems in our current grasp of the universe. Among the Jerzy Lewandowski, most popular ones of these problems are the singularity problem and the problem of information Uniwersytet Warszawswski, Poland loss. Several proposals have been made to address these questions within the existing approaches *Correspondence: to quantum gravity, but it is difficult to see a general scenario emerge. -
A Singing, Dancing Universe Jon Butterworth Enjoys a Celebration of Mathematics-Led Theoretical Physics
SPRING BOOKS COMMENT under physicist and Nobel laureate William to the intensely scrutinized narrative on the discovery “may turn out to be the greatest Henry Bragg, studying small mol ecules such double helix itself, he clarifies key issues. He development in the field of molecular genet- as tartaric acid. Moving to the University points out that the infamous conflict between ics in recent years”. And, on occasion, the of Leeds, UK, in 1928, Astbury probed the Wilkins and chemist Rosalind Franklin arose scope is too broad. The tragic figure of Nikolai structure of biological fibres such as hair. His from actions of John Randall, head of the Vavilov, the great Soviet plant geneticist of the colleague Florence Bell took the first X-ray biophysics unit at King’s College London. He early twentieth century who perished in the diffraction photographs of DNA, leading to implied to Franklin that she would take over Gulag, features prominently, but I am not sure the “pile of pennies” model (W. T. Astbury Wilkins’ work on DNA, yet gave Wilkins the how relevant his research is here. Yet pulling and F. O. Bell Nature 141, 747–748; 1938). impression she would be his assistant. Wilkins such figures into the limelight is partly what Her photos, plagued by technical limitations, conceded the DNA work to Franklin, and distinguishes Williams’s book from others. were fuzzy. But in 1951, Astbury’s lab pro- PhD student Raymond Gosling became her What of those others? Franklin Portugal duced a gem, by the rarely mentioned Elwyn assistant. It was Gosling who, under Franklin’s and Jack Cohen covered much the same Beighton. -
Covariant Phase Space for Gravity with Boundaries: Metric Vs Tetrad Formulations
Covariant phase space for gravity with boundaries: metric vs tetrad formulations J. Fernando Barbero G.c,d Juan Margalef-Bentabola,c Valle Varob,c Eduardo J.S. Villaseñorb,c aInstitute for Gravitation and the Cosmos and Physics Department. Penn State University. PA 16802, USA. bDepartamento de Matemáticas, Universidad Carlos III de Madrid. Avda. de la Universidad 30, 28911 Leganés, Spain. cGrupo de Teorías de Campos y Física Estadística. Instituto Gregorio Millán (UC3M). Unidad Asociada al Instituto de Estructura de la Materia, CSIC, Madrid, Spain. dInstituto de Estructura de la Materia, CSIC, Serrano 123, 28006, Madrid, Spain E-mail: [email protected], [email protected], [email protected], [email protected] Abstract: We use covariant phase space methods to study the metric and tetrad formula- tions of General Relativity in a manifold with boundary and compare the results obtained in both approaches. Proving their equivalence has been a long-lasting problem that we solve here by using the cohomological approach provided by the relative bicomplex framework. This setting provides a clean and ambiguity-free way to describe the solution spaces and associated symplectic structures. We also compute several relevant charges in both schemes and show that they are equivalent, as expected. arXiv:2103.06362v2 [gr-qc] 14 Jun 2021 Contents I Introduction1 II The geometric arena2 II.1 M as a space-time2 II.2 From M-vector fields to F-vector fields3 II.3 CPS-Algorithm4 IIIGeneral Relativity in terms of metrics5 IV General relativity in terms of tetrads8 V Metric vs Tetrad formulation 13 V.1 Space of solutions 13 V.2 Presymplectic structures 14 VI Conclusions 15 A Ancillary material 16 A.1 Mathematical background 16 A.2 Some computations in the metric case 19 A.3 Some tetrad computations 21 Bibliography 22 I Introduction Space-time boundaries play a prominent role in classical and quantum General Relativity (GR). -
Pos(Rio De Janeiro 2012)002 † ∗ [email protected] Speaker
Loop Quantum Gravity and the Very Early Universe PoS(Rio de Janeiro 2012)002 Abhay Ashtekar∗† Institute for Gravitational Physics and Geometry, Physics Department, Penn State, University Park, PA 16802, U.S.A. E-mail: [email protected] This brief overview is addressed to beginning researchers. It begins with a discussion of the distinguishing features of loop quantum gravity, then illustrates the type of issues that must be faced by any quantum gravity theory, and concludes with a brief summary of the status of these issues in loop quantum gravity. For concreteness the emphasis is on cosmology. Since several introductory as well as detailed reviews of loop quantum gravity are already available in the literature, the focus is on explaining the overall viewpoint and providing a short bibliography to introduce the interested reader to literature. 7th Conference Mathematical Methods in Physics - Londrina 2012, 16 to 20 April 2012 Rio de Janeiro, Brazil ∗Speaker. †A footnote may follow. c Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence. http://pos.sissa.it/ Loop Quantum Gravity Abhay Ashtekar Loop quantum gravity (LQG) is a non-perturbative approach aimed at unifying general rela- tivity and quantum physics. Its distinguishing features are: i) Background independence, and, ii) Underlying unity of the mathematical framework used to describe gravity and the other three basic forces of nature. It is background independent in the sense that there are no background fields, not even a space-time metric. All fields —whether they represent matter constituents, or gauge fields that mediate fundamental forces between them, or space- time geometry itself— are treated on the same footing. -
A Realist Vision of the Quantum World
A realist's vision of the quantum world Kragh, Helge Stjernholm Published in: American Scientist Publication date: 2019 Document version Publisher's PDF, also known as Version of record Document license: Unspecified Citation for published version (APA): Kragh, H. S. (2019). A realist's vision of the quantum world. American Scientist, 107, 374-376. https://www.americanscientist.org/article/a-realist-vision-of-the-quantum-world Download date: 24. sep.. 2021 A reprint from American Scientist the magazine of Sigma Xi, The Scientific Research Honor Society This reprint is provided for personal and noncommercial use. For any other use, please send a request to Permissions, American Scientist, P.O. Box 13975, Research Triangle Park, NC, 27709, U.S.A., or by electronic mail to [email protected]. ©Sigma Xi, The Scientific Research Hornor Society and other rightsholders Scientists’ Nightstand has been the most successful theory of nature, and quantum mechanics The Scientists’ Nightstand, A Realist Vision precludes the sort of realism to which American Scientist’s books of the Quantum Smolin aspires. He describes three dif- section, offers reviews, review ferent kinds of anti-realists: The radical essays, brief excerpts, and more. World anti-realists, such as Niels Bohr, who For additional books coverage, believe that the properties we ascribe please see our Science Culture Helge Kragh to atoms and elementary particles are blog channel, which explores EINSTEIN’S UNFINISHED REVOLUTION: not inherent in them but are created by how science intersects with other The Search for What Lies Beyond the our interactions with them and exist areas of knowledge, entertain- Quantum. -
Peircean Cosmogony's Symbolic Agapistic Self-Organization As an Example of the Influence of Eastern Philosophy on Western Thinking
Peircean Cosmogony's Symbolic Agapistic Self-organization as an Example of the Influence of Eastern Philosophy on Western Thinking Brier, Søren Document Version Accepted author manuscript Published in: Progress in Biophysics & Molecular Biology DOI: 10.1016/j.pbiomolbio.2017.09.010 Publication date: 2017 License CC BY-NC-ND Citation for published version (APA): Brier, S. (2017). Peircean Cosmogony's Symbolic Agapistic Self-organization as an Example of the Influence of Eastern Philosophy on Western Thinking. Progress in Biophysics & Molecular Biology, (131), 92-107. https://doi.org/10.1016/j.pbiomolbio.2017.09.010 Link to publication in CBS Research Portal General rights Copyright and moral rights for the publications made accessible in the public portal are retained by the authors and/or other copyright owners and it is a condition of accessing publications that users recognise and abide by the legal requirements associated with these rights. Take down policy If you believe that this document breaches copyright please contact us ([email protected]) providing details, and we will remove access to the work immediately and investigate your claim. Download date: 02. Oct. 2021 Peircean Cosmogony's Symbolic Agapistic Self-organization as an Example of the Influence of Eastern Philosophy on Western Thinking Søren Brier Journal article (Accepted manuscript) CITE: Brier, S. (2017). Peircean Cosmogony's Symbolic Agapistic Self-organization as an Example of the Influence of Eastern Philosophy on Western Thinking. Progress in Biophysics & Molecular -
Physics Needs Philosophy. Philosophy Needs Physics. Carlo Rovelli
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by PhilSci Archive Physics needs philosophy. Philosophy needs physics. Carlo Rovelli Extended version of a keynote talk at the XVIII UK-European Conference on the Foundation of Physics, given at the London School of Economics the 16 July 2016 Published on Foundations of Physics, 48, 481-491, 2018 Abstract Contrary to claims about the irrelevance of philosophy for science, I argue that philosophy has had, and still has, far more influence on physics than is commonly assumed. I maintain that the current anti-philosophical ideology has had damaging effects on the fertility of science. I also suggest that recent important empirical results, such as the detection of the Higgs particle and gravitational waves, and the failure to detect supersymmetry where many expected to find it, question the validity of certain philosophical assumptions common among theoretical physicists, inviting us to engage in a clearer philosophical reflection on scientific method. 1. Against Philosophy is the title of a chapter of a book by one of the great physicists of the last generation: Steven Weinberg, Nobel Prize winner and one of the architects of the Standard Model of elementary particle physicsi. Weinberg argues eloquently that philosophy is more damaging than helpful for physics—although it might provide some good ideas at times, it is often a straightjacket that physicists have to free themselves from. More radically, Stephen Hawking famously wrote that “philosophy is dead” because the big questions that used to be discussed by philosophers are now in the hands of physicistsii. -
Loop Quantum Gravity: the First 25 Years Carlo Rovelli
Loop quantum gravity: the first 25 years Carlo Rovelli To cite this version: Carlo Rovelli. Loop quantum gravity: the first 25 years. Classical and Quantum Gravity, IOP Publishing, 2011, 28 (15), pp.153002. 10.1088/0264-9381/28/15/153002. hal-00723006 HAL Id: hal-00723006 https://hal.archives-ouvertes.fr/hal-00723006 Submitted on 7 Aug 2012 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Loop quantum gravity: the first twenty five years Carlo Rovelli Centre de Physique Th´eorique de Luminy∗, Case 907, F-13288 Marseille, EU (Dated: January 27, 2011) I give a synthetic presentation of loop quantum gravity. I spell-out the aims of the theory and compare the results obtained with the initial hopes that motivated the early interest in this research direction. I give my own perspective on the status of the program and attempt of a critical evaluation of its successes and limits. I. INTRODUCTION The history of quantum gravity is full of great hopes later disappointed. I remember as a young student sitting in a major conference where a world-renowned physicists Loop gravity is not quite twenty-five years old, but announced that the final theory of quantum gravity and is getting close to such a venerable age: several basic everything had finally been found. -
Laudatio for Professor Abhay Ashtekar
Laudatio for Professor Abhay Ashtekar Professor Ashtekar is a remarkable ¯gure in the ¯eld of Ein- stein's gravity. This being the Einstein Year and, moreover, the World Year of Physics, one can hardly think of anyone more ¯tting to be honoured for his research and his achievements { achievements that have influenced the most varied aspects of gravitational theory in a profound way. Prof. Ashtekar is the Eberly Professor of Physics and the Di- rector of the Institute for Gravitational Physics and Geometry at Penn State University in the United States. His research in gravitational theory is notable for its breadth, covering quantum gravity and generalizations of quantum mechanics, but also clas- sical general relativity, the mathematical theory of black holes and gravitational waves. Our view of the world has undergone many revisions in the past, two of which, arguably the most revolutionary, were ini- tiated by Einstein in his annus mirabilis, 1905. For one thing, the theory of special relativity turned our notion of space and time on its ear for speeds approaching that of light. At the same time, Einstein's explanation of the photoelectric e®ect heralded the coming of quantum theory. Many of the best minds in theo- retical physics, including Einstein himself, have been trying for years to ¯nd a uni¯ed theory of relativity and quantum theory. Such a theory, often called quantum gravity, could, for example, provide an explanation for the initial moments of our universe just after the big bang. Especially noteworthy is Prof. Ashtekar's work on the canon- ical quantization of gravitation, which is based upon a reformu- lation of Einstein's ¯eld equations that Ashtekar presented 1986. -
MATTERS of GRAVITY, a Newsletter for the Gravity Community, Number 3
MATTERS OF GRAVITY Number 3 Spring 1994 Table of Contents Editorial ................................................... ................... 2 Correspondents ................................................... ............ 2 Gravity news: Open Letter to gravitational physicists, Beverly Berger ........................ 3 A Missouri relativist in King Gustav’s Court, Clifford Will .................... 6 Gary Horowitz wins the Xanthopoulos award, Abhay Ashtekar ................ 9 Research briefs: Gamma-ray bursts and their possible cosmological implications, Peter Meszaros 12 Current activity and results in laboratory gravity, Riley Newman ............. 15 Update on representations of quantum gravity, Donald Marolf ................ 19 Ligo project report: December 1993, Rochus E. Vogt ......................... 23 Dark matter or new gravity?, Richard Hammond ............................. 25 Conference Reports: Gravitational waves from coalescing compact binaries, Curt Cutler ........... 28 Mach’s principle: from Newton’s bucket to quantum gravity, Dieter Brill ..... 31 Cornelius Lanczos international centenary conference, David Brown .......... 33 Third Midwest relativity conference, David Garfinkle ......................... 36 arXiv:gr-qc/9402002v1 1 Feb 1994 Editor: Jorge Pullin Center for Gravitational Physics and Geometry The Pennsylvania State University University Park, PA 16802-6300 Fax: (814)863-9608 Phone (814)863-9597 Internet: [email protected] 1 Editorial Well, this newsletter is growing into its third year and third number with a lot of strength. In fact, maybe too much strength. Twelve articles and 37 (!) pages. In this number, apart from the ”traditional” research briefs and conference reports we also bring some news for the community, therefore starting to fulfill the original promise of bringing the gravity/relativity community closer together. As usual I am open to suggestions, criticisms and proposals for articles for the next issue, due September 1st. Many thanks to the authors and the correspondents who made this issue possible. -
150 Abhay Ashtekar
ICTS PUBLIC LECTURE BIG BANG, BLACK HOLES AND GRAVITATIONAL WAVES Illustrations of Paradigm Shifts in Fundamental Science Big Bang, Black Holes and Gravitational Waves now appear as compelling – even obvious – consequences of general relativity. Therefore, it may seem surprising that none of these ideas were readily accepted. Not only was there considerable debate, but in fact leading figures were often arguing on what turned out to be the “wrong side” of history. These developments provide excellent lessons for younger researchers on how science un-folds. Paradigm shifts in science occur when younger researchers have the courage not to accept ideas merely because they are mainstream; patience to systematically develop novel avenues they deeply believe in; and maturity to accept that a variety of factors – not all logical or even science related – can drive or slow down scientific progress. ABHAY ASHTEKAR Pennsylvania State University Abhay Ashtekar is the Eberly Professor of Physics and the Director of the Institute for Gravitational Physics and Geometry at Pennsylvania State University. His research interests span different aspects of General Relativity, Quantum Gravity and Black Holes. The recipient of the Einstein Prize and the Senior Research Prize of the Humboldt Foundation, his work is widely recognized. He is an elected member of the US National Academy of Sciences, Elected Fellow of the American Association for Advancement of Science, American Physical Society and Honorary Fellow of the Indian Academy of Sciences, and has served as the president of International Society for General Relativity and Gravitation. 4 pm, 21 August, 2019 ICTS, Bengaluru Register online https://bit.ly/AbhayAshtekar BG Image – Frame from a simulation of the merger of two black holes and the resulting emission of gravitational radiation (colored fields).