Gravitational Physics Personnel:C. R. Evans B. Brill T. Garrett M. Peppers ResearchSources of Gravitational Radiation Interests:Numerical Relativity &

Slides:



Advertisements
Similar presentations
Regularization of the the second-order gravitational perturbations produced by a compact object Eran Rosenthal University of Guelph - Canada Amos Ori Technion.
Advertisements

Spacetime Approach to Force-Free Magnetospheres Sam Gralla University of Maryland Collaborators: Daniel Brennan (UMD undergrad) Ted Jacobson (UMD prof)
Holographic Superconductors with Higher Curvature Corrections Sugumi Kanno (Durham) work w/ Ruth Gregory (Durham) Jiro Soda (Kyoto) arXiv: , to.
Numerical Relativity & Gravitational waves I.Introduction II.Status III.Latest results IV.Summary M. Shibata (U. Tokyo)
07 Nov 2003Gravitational Wave Phenomenology Workshop1 Numerical Relativity Deirdre ShoemakerCornell University  The role of numerical relativity in gravitational-wave.
Recent results with Goddard AMR codes Dae-Il (Dale) Choi NASA/Goddard, USRA Collaborators J. Centrella, J. Baker, J. van Meter, D. Fiske, B. Imbiriba (NASA/Goddard)
Toward Binary Black Hole Simulations in Numerical Relativity Frans Pretorius California Institute of Technology BIRS Workshop on Numerical Relativity Banff,
(In)Stabilities and Complementarity in AdS/CFT Eliezer Rabinovici The Hebrew University, Jerusalem Based on works with J.L.F Barbon Based on work with.
Pennsylvania State University Joint work at Southampton University Ulrich Sperhake Ray d’Inverno Robert Sjödin James Vickers Cauchy characteristic matching.
ASYMPTOTIC STRUCTURE IN HIGHER DIMENSIONS AND ITS CLASSIFICATION KENTARO TANABE (UNIVERSITY OF BARCELONA) based on KT, Kinoshita and Shiromizu PRD
Numerical simulations of gravitational singularities.
Non-axisymmetric modes of differentially rotating neutron stars Andrea Passamonti Southampton, 13 December 2007 University of Southampton In collaboration.
Gravitational Collapse in Axisymmetry Collaborators: Matthew Choptuik, CIAR/UBC Eric Hircshmann, BYU Steve Liebling, LIU APS Meeting Albuquerque, New Mexico.
Scott Johnson, John Rossman, Charles Harnden, Rob Schweitzer, Scott Schlef Department of Physics, Bridgewater State College // Bridgewater MA, Mentor:
Trajectory and Invariant Manifold Computation for Flows in the Chesapeake Bay Nathan Brasher February 13, 2005.
EGM20091 Perturbative analysis of gravitational recoil Hiroyuki Nakano Carlos O. Lousto Yosef Zlochower Center for Computational Relativity and Gravitation.
ANALYSIS OF PDE & GENERAL RELATIVITY Sergiu Klainerman June, 2000.
Gravitational Radiation Energy From Radial In-fall Into Schwarzschild and Kerr Geometries Project for Physics 879, Professor A. Buonanno, University of.
Some Interesting Topics on QNM QNM in time-dependent Black hole backgrounds QNM of Black Strings QNM of colliding Black Holes.
Spin, Charge, and Topology in low dimensions BIRS, Banff, July 29 - August 3, 2006.
Gravitational Perturbations of Higher Dimensional Rotating Black Holes Harvey Reall University of Nottingham Collaborators: Hari Kunduri, James Lucietti.
Special Relativistic Analogues of Black Strings?? Matthew Wm Choptuik CIAR Cosmology & Gravity Program Dept of Physics & Astronomy, UBC Vancouver BC The.
(SPH) Simulations of Binary Neutron Star Coalescence Examining the Mass Ratio Dependence of Post-Newtonian Smoothed Particle Hydrodynamics Jonathon Meyers,
Lamb shift in Schwarzschild spacetime Wenting Zhou & Hongwei Yu Department of Physics, Hunan Normal University, Changsha, Hunan, China.
The Astrophysics of Gravitational Wave Sources Conference Summary: Ground-Based Detectors ( Hz) Kimberly New, LANL.
Schwarzschild Perturbations in the Lorenz Gauge Leor Barack (Soton) Carlos Lousto (UTB)
2次ゲージ不変摂動論定式化の進行状況 Kouji Nakamura (Grad. Univ. Adv. Stud. (NAOJ)) References : K.N. Prog. Theor. Phys., vol.110 (2003), 723. (gr-qc/ ). K.N. Prog.
1 Yasushi Mino Theoretical AstroPhysics Including Relativity (TAPIR), CalTech Index 1: Introduction: LISA project 2: MiSaTaQuWa.
Forming Nonsingular Black Holes from Dust Collapse by R. Maier (Centro Brasileiro de Pesquisas Físicas-Rio de Janeiro) I. Damião Soares (Centro Brasileiro.
Black hole production in preheating Teruaki Suyama (Kyoto University) Takahiro Tanaka (Kyoto University) Bruce Bassett (ICG, University of Portsmouth)
A New Code for Axisymmetric Numerical Relativity Eric Hircshmann, BYU Steve Liebling, LIU Frans Pretorius, UBC Matthew Choptuik CIAR/UBC Black Holes III.
Stabilizing moduli with flux in brane gas cosmology Jin Young Kim (Kunsan National Univ.) CosPA 2009, Melbourne Based on arXiv: [hep-th]; PRD 78,
ACKNOWLEDGMENTS This research was supported by the National Science Foundation of China (NSFC) under grants , , , the Specialized.
Dynamics of Colliding Branes and Black Brane Production Dynamics of Colliding Branes and Black Brane Production Yu-ichi Takamizu (Waseda univ, Japan) With.
Objective of numerical relativity is to develop simulation code and relating computing tools to solve problems of general relativity and relativistic astrophysics.
“Einstein Gravity in Higher Dimensions”, Jerusalem, Feb., 2007.
“Models of Gravity in Higher Dimensions”, Bremen, Aug , 2008.
Perturbations of Higher-dimensional Spacetimes Jan Novák.
Cosmological Perturbations in the brane worlds Kazuya Koyama Tokyo University JSPS PD fellow.
Albert-Einstein-Institut Black Hole Initial Data for Evolution Distorted Black Holes: “Brill Wave plus Black Hole” (NCSA model)
1+log slicing in gravitational collapse. Ingredients of successful binary black hole simulations Pretorius Generalized harmonic coordinates Excision ____________________________.
Self-Force and the m-mode regularization scheme Sam Dolan (with Leor Barack) University of Southampton BriXGrav, Dublin 2010.
1 Steklov Mathematical Institute RAS G. Alekseev G. Alekseev Cosmological solutions Dynamics of waves Fields of accelerated sources Stationary axisymmetric.
1 Calculating Gravitational Wave Signatures from Black Hole Binary Coalescence Joan Centrella Laboratory for High Energy Astrophysics NASA/GSFC The Astrophysics.
On finding fields and self force in a gauge appropriate to separable wave equations (gr-qc/ ) 2006 Midwest Relativity Meeting Tobias Keidl University.
2008 Yousuke Takamori ( Osaka City Univ. ) with Hideki Ishihara, Msashi Kimura, Ken-ichi Nakao,(Osaka City Univ.) Masaaki Takahashi(Aichi.
1 Building Bridges: CGWA Inauguration 15 December 2003 Lazarus Approach to Binary Black Hole Modeling John Baker Laboratory for High Energy Astrophysics.
Initial data for binary black holes: the conformal thin- sandwich puncture method Mark D. Hannam UTB Relativity Group Seminar September 26, 2003.
Cactus Workshop - NCSA Sep 27 - Oct Cactus For Relativistic Collaborations Ed Seidel Albert Einstein Institute
Gravitational collapse of massless scalar field Bin Wang Shanghai Jiao Tong University.
Black Holes Pierre Cieniewicz. What are they? A Black Hole (BH) is a place in space from which nothing can escape The reason for this is gravity Some.
Math 445: Applied PDEs: models, problems, methods D. Gurarie.
Gravitational Self-force on a Particle in the Schwarzschild background Hiroyuki Nakano (Osaka City) Norichika Sago (Osaka) Wataru Hikida (Kyoto, YITP)
Bosenova collapse of axion cloud around a rotating black hole Hirotaka Yoshino Tohoku University (September 27, 2011) Hideo Kodama (KEK)
1 Yasushi Mino ( 蓑 泰 志 ) WUGRAV, Washington University at St. Louis Index 1: Introduction 2: Self-force in a Linear Perturbation.
Hawking radiation as tunneling from squashed Kaluza-Klein BH Ken Matsuno and Koichiro Umetsu (Osaka city university) (Kyoto sangyo university) Phys. Rev.
Quantum mechanics and the geometry of spacetime Juan Maldacena PPCM Conference May 2014.
1 Merging Black Holes and Gravitational Waves Joan Centrella Chief, Gravitational Astrophysics Laboratory NASA Goddard Space Flight Center Observational.
Based on Phys. Rev. D 92, (R) (2015) 中科大交叉学科理论研究中心
Innermost stable circular orbits around squashed Kaluza-Klein black holes Ken Matsuno & Hideki Ishihara ( Osaka City University ) 1.
Statements of the interest in LCGT data analysis Ping Xi Shanghai United Center for Astrophysics (SUCA), Shanghai Normal University.
1 Toward the 2 nd order self-force Eran Rosenthal University of Guelph, Canada.
BLACK HOLES SIMULATION and visualization
3 rd Karl Schwarzschild Meeting, Germany 24 July 2017
Spacetime solutions and their understandings
Thermodynamic Volume in AdS/CFT
Detection of gravitational waves from binary black hole mergers
Charged black holes in string-inspired gravity models
Global Defects near Black Holes
29 faculty 65 grad students.
Presentation transcript:

Gravitational Physics Personnel:C. R. Evans B. Brill T. Garrett M. Peppers ResearchSources of Gravitational Radiation Interests:Numerical Relativity & Black Hole Dynamics Critical Phenomena in Gravitational Collapse Gravitational Wave Signal Analysis

Gravitational Physics Numerical Integration of 1 st Order Hyperbolic Systems on Black Hole Spacetimes (Brill & Evans) Numerical Implementation and Stability of Black Hole Excision (Garrett & Evans) Ultimate Goal:Simulate Binary Black Hole Mergers in 3 dimensions (3D) Near-Term:Treat Hyperbolic Systems in General Spacetimes in 3D Remove Black Hole Interior from Computational Domain Achieve Stability at the Horizon Achieve Efficient, Scalable Computation on Parallel Computers Employ More General Spatial Coordinate Systems

Gravitational Physics Numerical Integration of Scalar Field on a Schwarzschild Black Hole Black Hole Interior is Excised from the Computational Domain Late-time Quasi-normal Mode Develops

Gravitational Physics Numerical Integration of Scalar Field on a Kerr Black Hole Black Hole Interior is Excised from the Computational Domain Late-time Spiral Quasi-normal Mode Develops

Gravitational Physics Accomplishments: Integration of scalar fields in 1 st order form on black hole spacetimes Stable black hole excision in special coordinate systems Development of a general time-dependent, 2 nd order, operator splitting method Development of a scalable code using MPI on an IBM SP cluster (720 proc’s) Current Activities: Working to develop a black hole excision technique (causal differencing) that can be used with more general spatial coordinate systems Working to extend integrations to 1 st order hyperbolic tensor wave systems Extension to dynamic black holes

Gravitational Physics Ultimate Goal: Merger of Kerr Black Holes Holes Precess Orbit Precesses Frame Dragging Non-Kerr Remnant

Gravitational Physics Related Publications Evans, C.R. & Coleman, J.S. 1994, “Critical Phenomena and Self-Similarity in the Gravitational Collapse of Radiation Fluid,” Phys. Rev. Lett., 72, Abrahams, A.M. & Evans, C.R. 1993, “Critical Behavior and Scaling in Vacuum Axisymmetric Gravitational Collapse,” Phys. Rev. Lett., 70, Abrahams, A.M., Rezzolla, L., Rupright, M.E., et al., 1998, “Gravitational wave extraction and outer boundary conditions by perturbative matching,” Phys. Rev. Lett., 80, Cook, G.B., Huq, M.F., Klasky, S.A., Scheel, M.A., et al., 1998, “Boosted 3-dimensional Black Hole Evolutions with Singularity Excision,” Phys. Rev. Lett., 80, Abrahams, A.M. and Evans, C.R. 1990, “Gauge Invariant Treatment of Gravitational Radiation near the Source: Analysis and Numerical Simulations,” Phys. Rev., D42, Gomez, R., Lehner, L., Marsa, R., Winicour, J., et al., 1998, “Stable characteristic evolution of generic 3-dimensional single-black-hole spacetimes,” Phys. Rev. Lett., 80,