MATTERS of GRAVITY Contents Editor
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
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. -
AC2 Report to IUPAP 2016.Pages
Report of Affiliated Commission AC.2 for 2015-16 submitted by Beverly K. Berger, Secretary The principal event of the year for the International Society on General Relativity and Gravitation (AC2) was the triennial GR conference. The 21st International Conference on General Relativity and Gravitation, GR21, was held 10 – 15 July 2016 at Columbia University. The scientific highlights of the meeting were talks and activities related to the first direct detection of gravitational waves by the LIGO Scientific Collaboration and the Virgo Collaboration—a momentous celebration of the Centennial of Einstein's first presentation of general relativity in November 1915. Approximately 650 registered participants attended the meeting. Sponsorship from IUPAP for this meeting, and AC2's own limited funds, assisted some of these participants. As usual, the conference had plenary talks in the morning, covering the whole field of AC2's interests. In the afternoons there were parallel contributed papers and poster sessions. There were 15 plenary talks (5 of the speakers being women) and 17 parallel sessions (7 of the chairs being women). Abstracts of all submissions became available online1 after the meeting. The abstracts of all parallel session talks and posters and the slides from the parallel session talks are available on the conference website.2 Slides from the plenary talks will be available soon. During the meeting, several prize winners were honored by AC2 and GWIC (WG11): The IUPAP Young Scientist Prize in General Relativity and Gravitation was first awarded at GR20 in 2013. The three winners since then, Jorge Santos, Stanford University and Cambridge University (2014), Nicolas Yunes, Montana State University (2015), and Ivan Agullo, Louisiana State University (2016) were recognized at the meeting. -
Consistent Discretizations and Quantum Gravity 3 Singularity, the Value of the Lapse Gets Modified and Therefore the “Lattice Spacing” Before and After Is Different
Proceedings of the II International Conference on Fundamental Interactions Pedra Azul, Brazil, June 2004 Canonical quantum gravity and consistent discretizations Rodolfo Gambini Instituto de F´ısica, Facultad de Ciencias, Igua esq. Mataojo, Montevideo, Uruguay Jorge Pullin Department of Physics and Astronomy, Louisiana State University, Baton Rouge, LA 70803 USA We review a recent proposal for the construction of a quantum theory of the gravita- tional field. The proposal is based on approximating the continuum theory by a discrete theory that has several attractive properties, among them, the fact that in its canonical formulation it is free of constraints. This allows to bypass many of the hard conceptual problems of traditional canonical quantum gravity. In particular the resulting theory im- plies a fundamental mechanism for decoherence and bypasses the black hole information paradox. Keywords: canonical, quantum gravity, new variables, loop quantization 1. Introduction Discretizations are very commonly used as a tool to treat field theories. Classically, when one wishes to solve the equations of a theory on a computer, one replaces arXiv:gr-qc/0408025v1 9 Aug 2004 the continuum equations by discrete approximations to be solved numerically. At the level of quantization, lattices have been used to regularize the infinities that plague field theories. This has been a very successful approach for treating Yang– Mills theories. The current approaches to non-perturbatively construct in detail a mathematically well defined theory of quantum gravity both at the canonical level 1 and at the path integral level 2 resort to discretizations to regularize the theory. Discretizing general relativity is more subtle than what one initially thinks. -
Jorge Pullin Horace Hearne Institute for Theoretical Physics Louisiana State University
Complete quantization of vacuum spherically symmetric gravity Jorge Pullin Horace Hearne Institute for Theoretical Physics Louisiana State University With Rodolfo Gambini University of the Republic of Uruguay In spite of their simplicity, spherically symmetric vacuum space-times are challenging to quantize. One has a Hamiltonian and (one) diffeomorphism constraint and, like those in the full theory, they do not form a Lie algebra. Therefore a traditional Dirac quantization is problematic. There has been some progress in the past: Kastrup and Thiemann (NPB399, 211 (1993)) using the “old” (complex) Ashtekar variables were able to quantize through a series of gauge fixings. The resulting quantization has waveforms Ψ(M), with M being a Dirac observable. There is no sense in which the singularity is “resolved”. Kucha ř (PRD50, 3961 (1994)) through a series of canonical transformation using the traditional metric variables isolated the single degree of freedom of the model (the ADM mass). Results similar to Kastrup and Thiemann’s. Campiglia, Gambini and JP (CQG24, 3649 (2007)) using modern Ashtekar variables gauge fixed the diffeomorphism constraint and rescaled the Hamiltonian constraint to make it Abelian. The quantization ends up being equivalent to those of Kastrup, Thiemann and Kucha ř. Various authors (Modesto, Boehmer and Vandersloot, Ashtekar and Bojowald, Campiglia, Gambini, JP) studied the quantization of the interior of a black hole using the isometry to Kantowski-Sachs and treating it as a LQC. The singularity is resolved. Gambini and JP (PRL101, 161301 (2008)) studied the semiclassical theory for the complete space-time of a black hole. The singularity is replaced by a region of high curvature that tunnels into another region of space-time. -
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 -
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. -
Grav19 April 8Th–12Th, 2019, C´Ordoba, Argentina
Grav19 April 8th–12th, 2019, Cordoba,´ Argentina Monday Tuesday Wednesday Thursday Friday 9:00-9:50 J. Pullin P. Ajith 8:45 F. Pretorius D. Siegel A. Perez´ 10:00-10:30 C OFFEE yLive streaming EHT/ESO C OFFEE 10:30-11:20 I. Agullo J. R. Westernacher 11:00 Coffee/discussion I. Racz´ J. Peraza 11:30-12:20 H. Friedrich O. Sarbach #12:00. S Liebling/L.Lehner F. Beyer F. Carrasco 12:20-14:00 **Reception Lunch** LUNCH 14:00-14:50 J. Frauendiener A. Rogers J. Jaramillo O. Moreschi 14:50-15:10 R. Gleiser B. Araneda A. Acena˜ C. del Pilar Quijada 15:10-15:30 T. Madler¨ L. Combi A. Giacomini E. Eiroa 15:30-15:50 P. Rioseco J. Bad´ıa enjoy I. Gentile G. Figueroa Aguirre 15:50-16:10 C OFFEE your C OFFEE 16:10-16:30 J. Oliva F. Canfora´ free M. Arganaraz˜ M. Ramirez 16:30-16:50 M. Rubio A. Petrov afternoon F. Abalos O. Fierro Mondaca 16:50-17:10 O. Baake G. Crisnejo P. Anglada M. J. Guzman´ 17:10-17:30 N. Miron´ Granese N. Poplawski 18:30-20:00 **Wine and Cheese** ?? 19:00hs. Jorge Pullin ?Gabriela Gonzalez: Public Lecture (Charla Publica,´ libre y gratuita). Friday, April 5: 20.00 HS at Observa- torio Astronomico´ de Cordoba:´ LAPRIDA 854, Auditorio MIRTA MOSCONI. ?? Jorge Pullin: La telenovela de las ondas gravitacionales: desde Newton en 1666 hasta Estocolmo 2017, Martes 9, 19:00HS en el SUM de la Plaza Cielo Tierra (Bv. Chacabuco 1300). -
Alejandro R. Corichi
Alejandro R. Corichi Instituto de Matematicas, UNAM, Apartado Postal 61-3, Morelia, Michoacan, 58090, M¶exico, Phone/Fax: +52 (55) 5623 2769/2732 , [email protected] , http://www.matmor.unam.mx/~corichi, Personal Mexican. Date of birth: 2nd of November of 1967. Married male with two children. Information Education The Pennsylvania State University, USA Ph.D. in Physics, August 1997. Thesis: Interplay between topology, gauge ¯elds and gravity. Adviser: Prof. Abhay Ashtekar. Facultad de Ciencias, UNAM, M¶exico Licenciado (Bs./M.Sc.) in Physics, October 1991. Thesis: Introduction to Geometrodynamics. Experience Visiting Professor Institute for Gravitation and the Cosmos Penn State University August 2008 { July 2009 I visited the Institute for Gravitation and the Cosmos at Penn State conducting research in quantum gravity. Researcher/Professor Institute of Mathematics Universidad Nacional Aut¶onomade M¶exico August 2005 { I joined the Institute for Mathematics, also at UNAM, where a quantum gravity group is now consolidating, including myself, R. Oeckl and J.A. Zapata. Head of the Department of Gravitation and Field Institute for Nuclear Sciences (ICN) Theory Universidad Nacional Aut¶onomade M¶exico September 2002 { August 2004. I served as head of the Department of Gravitation and Field Theory, consisting of 13 permanent faculty members, 4 postdoctoral associates and 20 graduate students. Research Associate Department of Physics and Astronomy University of Mississippi, USA September 2001 { August 2002 Conducted research in classical and quantum gravity. In quantum gravity, the statistical approach to semiclassical states in loop quantum gravity in collaboration with L. Bombelli and O. Winkler. Studies of coherent and semi-classical states for constrained systems. -
Curriculum Vitae
Curriculum Vitae Luis R. Lehner April 2020 1 Personal Data: Name and Surname: Luis R. LEHNER Marital Status: Married Date of Birth: July 17th. 1970 Current Address: Perimeter Institute for Theoretical Physics, 31 Caroline St. N. Waterloo, ON, N2L 2Y5 Canada Tel.: 519) 569-7600 Ext 6571 Mail Address: [email protected] Fax: (519) 569-7611 2 Education: • Ph.D. in Physics; University of Pittsburgh; 1998. Title: Gravitational Radiation from Black Hole spacetimes. Advisor: Jeffrey Winicour, PhD. • Licenciado en F´ısica;FaMAF, Universidad Nacional de C´ordoba;1993. Title: On a Simple Model for Compact Objects in General Relativity. Advisor: Osvaldo M. Moreschi, PhD. 3 Awards, Honors & Fellowships • \TD's 10 most influential Hispanic Canadian" 2019. • \Resident Theorist" for the Gravitational Wave International Committee 2018-present. • Member of the Advisory Board of the Kavli Institute for Theoretical Physics (UCSB) 2016-2020. • Executive Committee Member of the CIFAR programme: \Gravity and the Extreme Universe" 2017-present. • Member of the Scientific Council of the ICTP South American Institute for Fundamental Research (ICTP- SAIFR) 2015-present. • Fellow International Society of General Relativity and Gravitation, 2013-. • Discovery Accelerator Award, NSERC, Canada 2011-2014. • American Physical Society Fellow 2009-. • Canadian Institute for Advanced Research Fellow 2009-. 1 • Kavli-National Academy of Sciences Fellow 2008, 2017. • Louisiana State University Rainmaker 2008. • Baton Rouge Business Report Top 40 Under 40. 2007. • Scientific Board Member of Teragrid-NSF. 2006-2009. • Institute of Physics Fellow. The Institute of Physics, UK, 2004 -. • Phi Kappa Phi Non-Tenured Faculty Award in Natural and Physical Sciences. Louisiana State University, 2004. • Canadian Institute for Advanced Research Associate Member, 2004 -.