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Displaying 58 speakers out of 58
A. SINTES (University of Balearic Islands)
Searching for Continuous GW Signals
A. VECCHIO (University of Birmingham)
Detection Theory
Detection Methods
A. WATTS (University of Southampton)
The Dynamics of Differentially Rotating Neutron Stars
B.S. SATHYAPRAKASH (Cardiff University)
Characterization of the Detector
Searching for binaries in interferometer data: Current status and future prospects
C. BONA (Universitat de les Illes Balears)
The Z4 Formalism in Numerical Relativity
C. KIM (Northwestern University)
Binary Pulsar Coalescence Rates and Detection Rates for GW Detectors
D. POLLNEY (Albert-Einstein-Institute)
3+1 Formulations for Numerical Relativity
D. ROSINSKA (Observatoire de Paris)
GWs from Binary Neutron Stars
D. SHOEMAKER (Cornell University)
Nonlinear generation of harmonics in highly distorted black holes
E. BERTI (University of Thessaloniki)
Asymptotic black hole quasinormal modes and the area quantum
E. SEIDEL (Albert-Einstein-Institute)
Numerical Relativity Lab. III.
Numerical Relativity Lab. IV.
Open Discussion II.
Three years of GW research in Europe
G. COMER (Saint Louis University)
Do Neutron Star Gravitational Waves Carry Superfluid Imprints?
G. FAYE (Jena University)
A skeleton solution of the Einstein field equations for bh binaries
G. SCHAEFER (University of Jena)
PN I.: gravitating bodies
PN II.: generation of GWs
PN III.: the gravitational radiation field
H. ASADA (Hirosaki University)
Equation of Motion for Compact Binaries with Strong Internal Gravity
H. DIMMELMEIER (MPA, Garching, Germany)
GWs from Supernova Core Collapse: Present Status and Developments
I. HAWKE (Albert-Einstein-Institute)
Dynamics in neutron star collapse to a black hole
J. MILLER (SISSA)
Overview of the School
Astrophysical Sources of GWs
The Hulse-Taylor Binary System
FINAL REMARKS
J. PONS (University of Valencia)
Proto-NSs: do they Pulsate and Rotate as "standard" NSs
J. THORNBURG (Albert-Einstein-Institute)
A Fast Apparent-Horizon Finder for 3D Cartesian Grids in Numerical Relativity
K. GLAMPEDAKIS (Cardiff University)
Spacetime Modes of Rotating Compact Stars
K. KOKKOTAS (University of Thessaloniki)
Introduction to Relativistic perturbations & asteroseismology
Instabilities in Relativistic Stars
Open Discussion I.
High Frequency GW Astronomy
K. OOHARA (Niigata University)
General Relativistic Numerical Simulations of Coalescing Binary NSs
K. URYU (SISSA)
Equilibrium Solutions of Binary Neutron Stars in Quasi-Circular Orbit
L. CADONATI (MIT)
The LIGO Detector: Status Report
L. GUALTIERI (La Sapienza, Roma)
Neutrino-transport effects on proto-NSs oscillations and on GW frequencies
L. LUSANNA (INFN, Firenze)
Background-Independent GWs in Post-Minkowskian Spacetimes
L. REZZOLLA (SISSA)
Solution of Hyperbolic Equations I.
Solution of Hyperbolic Equations II.
HRSC Methods in Numerical Relativistic Hydrodynamics
M. CERDONIO (INFN, Padova University)
The "dual" GW Detector
M. COLPI (Milano-Bicocca University)
Unveiling Binary Black Holes in Globular Clusters
M. FREITAG (ARI, Heidelberg)
Stellar Dynamics for LISA: Stars Captured by a Massive Black Hole
M. SAIJO (Kyoto University)
Collapse of a Differentially Rotating Supermassive Star
N. ANDERSSON (University of Southampton)
Introduction to Newtonian Perturbation Theory
Lagrangian Perturbation Theory
Towards Stability Criteria for Rotating Superfluid Stars
A REVIEW OF THE POSTER SESSION
N. BISHOP (Unisa)
Initial Data from a Non-conformal Decomposition of the Constraints
N. KANDA (Osaka University)
Search for GW Events and Data Quality Evaluation on TAMA300
N. SETO (Caltech)
GW Cosmology Around 1Hz
N. STERGIOULAS (University of Thessaloniki)
Equilibrium and Pulsations of Differentially Rotating Neutron Stars
O. BENHAR (INFN, Rome)
Neutron Star Matter EOS: where do we stand?
O. JENNRICH (ESA/ESTEC)
Resonant Bar Detectors
Ground-based Interferometers
Space Interferometers
O. MORESCHI (Cordoba University)
First-order Gravitational Radiation Reaction of a System of Compact Objects
O. REULA (Cordoba University)
Novel Techniques for Numerical Relativity: Application to BH Excision
P. ASTONE (INFN, Rome)
The Explorer and Nautilius GW Detectors: recent results and future plans
P. CERDA-DURAN (University of Valencia)
Improved dynamics and GWs from relativistic core collapse simulations
P. DIENER (Albert-Einstein-Institute)
Numerical Relativity Lab. I.
Numerical Relativity Lab. II.
Finding Event Horizons in Numerical Spacetimes
P. GRANDCLEMENT (Northwestern University)
Families of Initial Data for Binary Black Holes
P. LAGUNA (Penn State University)
Dirty Binary Black Hole Evolutions
P. RAPAGNANI (La Sapienza, Roma)
The Virgo Detector: Status Report
R. BALASUBRAMANIAN (Cardiff University)
Data Analysis Lab. I.
Data Analysis Lab. II.
R. D'INVERNO (University of Southampton)
Introduction to Tensors
Field equations of GR
Exact Solutions in GR
Introduction to GWs I.
Introduction to GWs II.
S. BONAZZOLA (Meudon, Paris)
A constrained scheme for Einstein equations: Application on slow evolution of bhs
S. CHAKRABARTI (Bose Institute)
Simultaneous Observations of EM and GWs from Coalescing Compact Objects
S. KARINO (University of Tokyo)
Dynamical Instability of Differentially Rotating Polytropes
S. VITALE (Trento University)
The LISA Detector: Status Report
T. FONT (University of Valencia)
A Light-cone Approach to Axisymmetric Stellar Core Collapse
T. HARADA (Queen Mary College)
Computing GWs from Slightly Nonspherical Stellar Collapse
V. FERRARI (La Sapienza, Roma)
WELCOME AND OPENING OF THE CONFERENCE
W. TICHY (Penn State University)
Gauge Conditions for Binary Black Holes Puncture Data
Y. KOJIMA (Hiroshima University)
Probing compact stars with GWs

Organizers

J. Miller, L. Rezzolla, V. Ferrari