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18Th International Conference on General
18TH INTERNATIONAL CONFERENCE ON GENERAL RELATIVITY AND GRAVITATION (GRG18) 8 – 13 July 2007 7TH EDOARDO AMALDI CONFERENCE ON GRAVITATIONAL WAVES (AMALDI7) www.grg18.com 8 – 14 July 2007 www.Amaldi7.com Sydney Convention & Exhibition Centre • Darling Harbour • Sydney Australia INSPIRALLING BLACK HOLES RAPID EPANSION OF AN UNSTABLE NEUTRON STAR Credit: Seidel (LSU/AEI) / Kaehler (ZIB) Credit: Rezzolla (AEI) / Benger (ZIB) GRAZING COLLISION OF TWO BLACK HOLES VISUALISATION OF A GRAVITATIONAL WAVE HAVING Credit: Seidel (AEI) / Benger (ZIB) TEUKOLSKY'S SOLUTION AS INITIAL DATA Credit: Seidel (AEI) / Benger (ZIB) ROLLER COASTER DISTORTED BY SPECIAL RELATIVISTIC EFFECTS Credit: Michael Hush, Department of Physics, The Australian National University The program for GRG18 will incorporate all areas of General Relativity and Gravitation including Classical General Relativity; Numerical Relativity; Relativistic Astrophysics and Cosmology; Experimental Work on Gravity and Quantum Issues in Gravitation. The program for Amaldi7 will cover all aspects of Gravitational Wave Physics and Detection. PLENARY LECTURES Peter Schneider (Bonn) Donald Marolf USA Bernard Schutz Germany Bernd Bruegman (Friedrich-Schiller-University Jena) Gravitational lensing David McClelland Australia Robin Stebbins United States Numerical relativity Daniel Shaddock (JPL California Institute of Technology) Jorge Pullin USA Kimio Tsubono Japan Daniel Eisenstein (University of Arizona) Gravitational wave detection from space: technology challenges Norna Robertson USA Stefano Vitale Italy Dark energy Stan Whitcomb (California Institute of Technology) Misao Sasaki Japan Clifford Will United States Ground-based gravitational wave detection: now and future Bernard F Schutz Germany Francis Everitt (Stanford University) Susan M. Scott Australia LOCAL ORGANISING COMMITTEE Gravity Probe B and precision tests of General Relativity Chair: Susan M. -
Hamilton's Ricci Flow
The University of Melbourne, Department of Mathematics and Statistics Hamilton's Ricci Flow Nick Sheridan Supervisor: Associate Professor Craig Hodgson Second Reader: Professor Hyam Rubinstein Honours Thesis, November 2006. Abstract The aim of this project is to introduce the basics of Hamilton's Ricci Flow. The Ricci flow is a pde for evolving the metric tensor in a Riemannian manifold to make it \rounder", in the hope that one may draw topological conclusions from the existence of such \round" metrics. Indeed, the Ricci flow has recently been used to prove two very deep theorems in topology, namely the Geometrization and Poincar´eConjectures. We begin with a brief survey of the differential geometry that is needed in the Ricci flow, then proceed to introduce its basic properties and the basic techniques used to understand it, for example, proving existence and uniqueness and bounds on derivatives of curvature under the Ricci flow using the maximum principle. We use these results to prove the \original" Ricci flow theorem { the 1982 theorem of Richard Hamilton that closed 3-manifolds which admit metrics of strictly positive Ricci curvature are diffeomorphic to quotients of the round 3-sphere by finite groups of isometries acting freely. We conclude with a qualitative discussion of the ideas behind the proof of the Geometrization Conjecture using the Ricci flow. Most of the project is based on the book by Chow and Knopf [6], the notes by Peter Topping [28] (which have recently been made into a book, see [29]), the papers of Richard Hamilton (in particular [9]) and the lecture course on Geometric Evolution Equations presented by Ben Andrews at the 2006 ICE-EM Graduate School held at the University of Queensland. -
Inverse Mean Curvature Evolution of Entire Graphs
INVERSE MEAN CURVATURE EVOLUTION OF ENTIRE GRAPHS PANAGIOTA DASKALOPOULOS AND GERHARD HUISKEN n Abstract. We study the evolution of strictly mean-convex entire graphs over R by Inverse Mean Curvature flow. First we establish the global existence of starshaped entire graphs with superlinear growth at infinity. The main result in this work concerns the critical case of asymptotically conical entire convex graphs. In this case we show that there exists a time T < +1, which depends on the growth at infinity of the initial data, such that the unique solution of the flow exists for all t < T . Moreover, as t ! T the solution converges to a flat plane. Our techniques exploit the ultra-fast diffusion character of the fully-nonlinear flow, a property that implies that the asymptotic behavior at spatial infinity of our solution plays a crucial influence on the maximal time of existence, as such behavior propagates infinitely fast towards the interior. Contents 1. Introduction 1 2. The geometric equations and preliminaries 5 3. Self-similar solutions 10 4. The super-linear case and short time existence 13 5. Lp bounds on 1=H 23 6. L1 estimates on 1=H 29 7. Long time existence Theorem 1.1 40 References 41 arXiv:1709.06665v1 [math.DG] 19 Sep 2017 1. Introduction n n+1 We consider a family of immersions Ft : M ! R of n-dimensional mean convex hypersurfaces n+1 n in R . We say that Mt := Ft(M ) moves by inverse mean curvature flow if @ (1.1) F (z; t) = H−1(z; t) ν(z; t); z 2 M n @t where H(z; t) > 0 and ν(z; t) denote the mean curvature and exterior unit normal of the surface Mt at the point F (z; t). -
The Newtonian Limit of General Relativity
The Newtonian Limit of General Relativity Dissertation zur Erlangung des Doktorgrades der Naturwissenschaften an der Fakult¨atMathematik und Physik der Eberhard-Karls-Universit¨atT¨ubingen vorgelegt von Maren Reimold aus N¨ordlingen Unterst¨utztdurch das Evangelische Studienwerk Villigst e.V. T¨ubingen,September 3, 2010 Contents Deutsche Zusammenfassung 3 Introduction 5 0.1 Transitions from tangent and cotangent space and induced connections 8 0.2 Concepts of curvature . 9 0.3 Newton's theory of gravitation and Einstein's theory of relativity . 13 1 Frame theory 19 1.1 The structure of the frame theory . 19 1.2 Linear Algebra . 23 1.3 Transfer to the frame theory . 30 1.4 The case λ =0 ............................. 34 2 The Newtonian limit: definition and existence 63 2.1 Definition of the Newtonian limit . 63 2.2 Extension of spacetimes . 66 2.3 Examples . 66 2.4 Existence of a limit . 75 2.5 Static and spherically symmetric spacetimes . 82 3 Existence of genuine Newtonian limits 95 3.1 Transformation of coordinates . 96 3.2 Conditions for the curvature tensor . 103 3.3 Asymptotically flat spacetimes . 106 A Appendix 121 A.1 The Schwarzschild spacetime . 121 A.2 The Kerr spacetime . 128 Index 151 Bibliography 153 1 Deutsche Zusammenfassung So lange es die Allgemeine Relativit¨atstheoriegibt, so lange gibt es auch die zugeh¨origeFrage, inwieweit man die Newtonsche Gravitationstheorie als einen Spezialfall oder doch wenigstens als eine Grenzlage der Allgemeinen Relativit¨ats- theorie auffassen kann. Schon am 18. November 1915, eine Woche bevor -
Geometric Analysis
IAS/PARK CITY MATHEMATICS SERIES Volume 22 Geometric Analysis Hubert L. Bray Greg Galloway Rafe Mazzeo Natasa Sesum Editors American Mathematical Society Institute for Advanced Study Geometric Analysis https://doi.org/10.1090//pcms/022 IAS/PARK CITY MATHEMATICS SERIES Volume 22 Geometric Analysis Hubert L. Bray Greg Galloway Rafe Mazzeo Natasa Sesum Editors American Mathematical Society Institute for Advanced Study Hubert Lewis Bray, Gregory J. Galloway, Rafe Mazzeo, and Natasa Sesum, Volume Editors IAS/Park City Mathematics Institute runs mathematics education programs that bring together high school mathematics teachers, researchers in mathematics and mathematics education, undergraduate mathematics faculty, graduate students, and undergraduates to participate in distinct but overlapping programs of research and education. This volume contains the lecture notes from the Graduate Summer School program 2010 Mathematics Subject Classification. Primary 53-06, 35-06, 83-06. Library of Congress Cataloging-in-Publication Data Geometric analysis / Hubert L. Bray, editor [and three others]. pages cm. — (IAS/Park City mathematics series ; volume 22) Includes bibliographical references. ISBN 978-1-4704-2313-1 (alk. paper) 1. Geometric analysis. 2. Mathematical analysis. I. Bray, Hubert L., editor. QA360.G455 2015 515.1—dc23 2015031562 Copying and reprinting. Individual readers of this publication, and nonprofit libraries acting for them, are permitted to make fair use of the material, such as to copy select pages for use in teaching or research. Permission is granted to quote brief passages from this publication in reviews, provided the customary acknowledgment of the source is given. Republication, systematic copying, or multiple reproduction of any material in this publication is permitted only under license from the American Mathematical Society. -
Geometric Relativity
GRADUATE STUDIES IN MATHEMATICS 201 Geometric Relativity Dan A. Lee 10.1090/gsm/201 Geometric Relativity GRADUATE STUDIES IN MATHEMATICS 201 Geometric Relativity Dan A. Lee EDITORIAL COMMITTEE Daniel S. Freed (Chair) Bjorn Poonen Gigliola Staffilani Jeff A. Viaclovsky 2010 Mathematics Subject Classification. Primary 53-01, 53C20, 53C21, 53C24, 53C27, 53C44, 53C50, 53C80, 83C05, 83C57. For additional information and updates on this book, visit www.ams.org/bookpages/gsm-201 Library of Congress Cataloging-in-Publication Data Names: Lee, Dan A., 1978- author. Title: Geometric relativity / Dan A. Lee. Description: Providence, Rhode Island : American Mathematical Society, [2019] | Series: Gradu- ate studies in mathematics ; volume 201 | Includes bibliographical references and index. Identifiers: LCCN 2019019111 | ISBN 9781470450816 (alk. paper) Subjects: LCSH: General relativity (Physics)–Mathematics. | Geometry, Riemannian. | Differ- ential equations, Partial. | AMS: Differential geometry – Instructional exposition (textbooks, tutorial papers, etc.). msc | Differential geometry – Global differential geometry – Global Riemannian geometry, including pinching. msc | Differential geometry – Global differential geometry – Methods of Riemannian geometry, including PDE methods; curvature restrictions. msc | Differential geometry – Global differential geometry – Rigidity results. msc — Differential geometry – Global differential geometry – Spin and Spin. msc | Differential geometry – Global differential geometry – Geometric evolution equations (mean curvature flow, -
William A. Hiscock Michio Kaku Gordon Kane J-M Wersinger
WILLIAM A. HISCOCK From Wormholes to the Warp Drive: Using Theoretical Physics to Place Ultimate Bounds on Technology MICHIO KAKU M-Theory: Mother of All Superstrings GORDON KANE Anthropic Questions Peering into the Universe: Images from the Hubble Space Telescope J-M WERSINGER The National Space Grant Student Satellite Program: Crawl, Walk, Run, Fly! The Honor Society of Phi Kappa Phi was founded in 1897 and became a national organization Board of Directors through the efforts of the presidents of three state Wendell H. McKenzie, PhD universities. Its primary objective has been from National President the first the recognition and encouragement of Dept. of Genetics superior scholarship in all fields of study. Good Box 7614 NCSU character is an essential supporting attribute for Raleigh, NC 27695 those elected to membership. The motto of the Paul J. Ferlazzo, PhD Society is philosophia krateit¯oph¯ot¯on, which is National President-Elect freely translated as “Let the love of learning rule Northern Arizona University Phi Kappa Phi Forum Staff humanity.” Dept. of English, Bx 6032 Flagstaff, AZ 86011 Editor: JAMES P. KAETZ Donna Clark Schubert National Vice President Associate Editors: Troy State University Phi Kappa Phi encourages and recognizes aca- 101 C Wallace Hall STEPHANIE J. BOND demic excellence through several national pro- Troy, AL 36082 LAURA J. KLOBERG grams. Its flagship National Fellowship Program now awards more than $460,000 each year to Neil R. Luebke, PhD Copy Editor: student members for the first year of graduate Past President 616 W. Harned Ave. AMES ARRS study. In addition, the Society funds Study J T. -
Monotonicity Formulas for Parabolic Flows on Manifolds
COMMUNICATIONS IN ANALYSIS AND GEOMETRY Volume 1, Number 1, 127-137, 1993 MONOTONICITY FORMULAS FOR PARABOLIC FLOWS ON MANIFOLDS RICHARD S. HAMILTON Recently Michael Struwe [S] and Gerhard Huisken [Hu2] have independently derived monotonicity formulas for the Harmonic Map heat flow on a Euclidean domain and for the Mean Curvature flow of a hypersurface in Euclidean space. In this paper we show how to generalize these results to the case of flows on a general compact manifold, and we also give the analogous monotonicity for- mula for the Yang-Mills heat flow. The key ingredient is a matrix Harnack estimate for positive solutions to the scalar heat equation given in [H]. In [GrH] the authors show how to use the monotonicity formula to prove that rapidly forming singularities in the Harmonic Map heat flow are asymptotic to homo- thetically shrinking solitons; similar results may be expected in other cases, as Huisken does in [Hu2] for the Mean Curvature flow in Euclidean space. We only obtain strict monotonicity for a special class of metrics, but in general there is an error term which is small enough to give the same effect. (Chen Yummei and Michael Struwe [CS] give a different approach to the error on manifolds.) The special class of metrics are those which are Ricci parallel (so that DiRjk = 0) and have weakly positive sectional curvature (so that RijkiViWjVkWt > 0 for all vectors V and W). This holds for example if M is flat or a sphere or a complex projective space, or a product of such, or a quotient of a product by a finite free group of isometries. -
Numerical Relativity: Instituto De Ciencias Instituto De Ciencias UNAMUNAM Nuclearesnucleares on Overview of the Field and Recent Results on Black Hole Simulations
Numerical Relativity: Instituto de Ciencias Instituto de Ciencias UNAMUNAM NuclearesNucleares On overview of the field and recent results on black hole simulations Miguel Alcubierre Instituto de Ciencias Nucleares UNAM, Mexico SIAM Conference, Philadelphia, August 2010 Gravitational wave detectors InstitutoInstitutode de Ciencias Ciencias UNAM Nucleares UNAM NuclearesA global network of gravitational wave detectors in now either in an advanced state of construction, or actually taking data! The collision of compact objects (black holes, neutron stars) is considered one of the most promising sources for detection in the next few years. TAMA, Tokio VIRGO, Pisa LIGO,Washington GEO 600, Hanover LIGO, Louisiana The future: LISA (Laser Interferometer Space Antenna) Instituto de Ciencias Instituto de Ciencias UNAMUNAM NuclearesNucleares Einstein’s field equations Instituto de Ciencias Instituto de Ciencias UNAMUNAM NuclearesNucleares The dynamics of the gravitational field are described by the Einstein field equations: G 8 3,2,1,0 These equations relate the geometry of space‐time (the left hand side) with the distribution of mass and energy (the right hand side). Einstein’s equations form a system of 10 non‐linear, coupled, partial differential equations in 4 dimensions. Written on a general coordinate system they can have thousands of terms! Numerical relativity Instituto de Ciencias Instituto de Ciencias UNAMUNAM NuclearesNucleares There are books full of exact solutions to Einstein’s equations, but few of those solutions have a clear astrophysical interpretation. Exact solutions are typically found by asking for space‐time to have a high degree of symmetry: • Schwarzschild black hole: Static and spherically symmetric. • Kerr black hole: Stationary and axially symmetric. -
Convex Ancient Solutions of the Mean Curvature Flow
j. differential geometry 101 (2015) 267-287 CONVEX ANCIENT SOLUTIONS OF THE MEAN CURVATURE FLOW Gerhard Huisken & Carlo Sinestrari Abstract We study solutions of the mean curvature flow which are defined for all negative times, usually called ancient solutions. We give various conditions ensuring that a closed convex ancient solution is a shrinking sphere. Examples of such conditions are: a uniform pinching condition on the curvatures, a suitable growth bound on the diameter, or a reverse isoperimetric inequality. We also study the behaviour of uniformly k-convex solutions, and consider generalizations to ancient solutions immersed in a sphere. 1. Introduction In this paper, we study convex ancient solutions to the mean cur- vature flow. We recall that a family of smooth immersions F : M× n+1 (t0,t1) → R ,whereM is an n-dimensional manifold, is called a mean curvature flow if it satisfies ∂F (1.1) (p, t)=−H(p, t)ν(p, t),p∈M,t∈ (t0,t1), ∂t where H(p, t)andν(p, t) are the mean curvature and the outer normal respectively at the point F (p, t)ofthesurfaceMt = F (·,t)(M). The signs are chosen such that −Hν = H is the mean curvature vector and the mean curvature of a convex surface is positive. We assume that n ≥ 2andthatM is closed. A solution is called ancient if it is defined for t ∈ (−∞, 0). While mean curvature flow is parabolic and hence in general ill-posed backward in time, ancient solutions are of interest for several reasons: They arise as tangent flows near singularities of the flow and therefore model the as- ymptotic profile of the surfaces as they approach a singularity, see e.g. -
There Is Found Actual Science After the Opinions of Force Areas and Invisibility Cloaks
Things that were once just fantastic fiction of science fiction make up many of today's technologies. Did you know that Jules Verne, who was a nineteenth-century science fiction writer, has already dreamed about devices such as fax machines, a worldwide network, and moon rocket ships? Although we accepted these technologies today, Verne's contemporaries, even the leading physicists, laughed them, convinced them to be impossible. Even when you watch sci-fi movies that aren't that old, you can see that some of the technologies depicted today are considered rough, like large computers with lots of flashing bulbs. In some respects, the science of now has exceeded fiction yesterday, although it has not yet passed through other galaxies wearing catsuits. And are you wondering about what will technologies that seem impossible today be? Which of these is going to be achieved in the future and how? You are going to discover if you keep reading. Chapter 1 - There is found actual science after the opinions of force areas and invisibility cloaks. Do you recognize the force fields applied in Star Trek? Challenging energy barriers that preserve starships from rockets and enemy fire? Imaginary, isn't it? The one, that is known in classical physics, is force fields. As it understands, many objects can have an impact on other objects around them without direct contact with them. For example, a magnet pulls or pushes things in an exact field around it. In the nineteenth century, by Michael Faraday who was an English scientist named, it is told that uncovered the concept of force fields, invisible fields, or lines of force surrounding a magnet. -
The Alcubierre Warp Drive Using Lorentz Boosts According to the Harold White Spacetime Metric Potential Θ
The Alcubierre Warp Drive using Lorentz Boosts according to the Harold White Spacetime Metric potential θ. Fernando Loup, Rocha Daniel To cite this version: Fernando Loup, Rocha Daniel. The Alcubierre Warp Drive using Lorentz Boosts according to the Harold White Spacetime Metric potential θ.. 2012. hal-00768779 HAL Id: hal-00768779 https://hal.archives-ouvertes.fr/hal-00768779 Submitted on 23 Dec 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. The Alcubierre Warp Drive using Lorentz Boosts according to the Harold White Spacetime Metric potential θ. Fernando Loup ∗ Daniel Rocha † December 23, 2012 Abstract Warp Drives are solutions of the Einstein Field Equations that allows superluminal travel within the framework of General Relativity. The first of these solutions was discovered by the Mexican math- ematician Miguel Alcubierre in 1994.The Alcubierre warp drive seems to be very attractive because allows interstellar space travel at arbitrarily large speeds avoiding the time dilatation and mass increase paradoxes of Special Relativity. However it suffers from a very serious drawback:Interstellar space is not empty:It is fulfilled with photons and particle dusts and a ship at superluminal speeds would impact these obstacles in highly energetic collisions disrupting the warp field and placing the astronauts in danger.This was pointed out by a great number of authors like Clark,Hiscock,Larson,McMonigal,Lewis,O’Byrne, Barcelo,Finazzi and Liberati.