Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Max Planck SocietyDE1.2k papers
- Centre National de la Recherche ScientifiqueFR1k papers
- National Institute for AstrophysicsIT820 papers
- European Southern ObservatoryCL784 papers
- Center for Astrophysics Harvard & SmithsonianUS755 papers
- Max Planck Institute for Extraterrestrial PhysicsDE722 papers
- Ludwig-Maximilians-Universität MünchenDE639 papers
- Space Research InstituteRU602 papers
- Osservatorio Astronomico di PadovaIT600 papers
- California Institute of TechnologyUS581 papers
- Trieste Astronomical ObservatoryIT566 papers
- University of California, BerkeleyUS566 papers
19 papers · 1 filter
Arc Statistics with Realistic Cluster Potentials. I. Method and First Results
M. Bartelmann, A. Weiss
{}From the lensing properties of a numerically simulated cluster, from the statistical properties of the giant arcs produced by the cluster, and from comparing the cluster properti…
Shell Effects in Nuclei Near Neutron Drip
M. M. Sharma, G. A. Lalazissis, W. Hillebrandt +1
Shell effects in nuclei close to the neutron-drip lines have been investigated. It has been demonstrated in the relativistic mean-field theory that nuclei very far from stability m…
Trapped surfaces in spherical expanding open universes
Uwe Brauer, Edward Malec, Niall Ó Murchadha
Consider spherically symmetric initial data for a cosmology which, in the large, approximates an open Friedmann-Lema{\^ı}tre universe. Further assume that the data i…
A gravitational lens model for B1422+231
R. Kormann, P. Schneider, M. Bartelmann
We construct a simple elliptical gravitational lens model for the quadruple lens B1422+231 and show that the details of the configuration cannot be easily understood in terms of th…
Large-scale correlations between QSOs and IRAS galaxies
M. Bartelmann, P. Schneider
We demonstrate that high-redshift 1-Jansky radio sources are correlated with foreground IRAS galaxies on angular scales of several 10 arc minutes on a statistical significance leve…
Lagrangian theory of gravitational instability of Friedman-Lemaitre cosmologies - generic third-order model for non-linear clustering
Thomas Buchert
The Lagrangian perturbation theory on Friedman-Lemaitre cosmologies investigated and solved up to the second order in earlier papers (Buchert 1992, Buchert \& Ehlers 1993) is evalu…
Formation of spiral and elliptical galaxies in a CDM cosmogony
Matthias Steinmetz, Ewald Mueller
The formation of galaxies in a CDM cosmogony is investigated by following the evolution of dark and baryonic matter and of the frequency- dependent spatially averaged radiation fie…
The large-scale structure in a universe dominated by cold plus hot dark matter
Y. P. Jing, H. J. Mo, G. Boerner +1
Using numerical simulations, we investigate the large-scale gravitational clustering in a flat universe dominated by cold plus hot dark matter (i.e., $Ω_0=\ocdm+\ohdm+\obaryon=1$).…
Blow-Up of Test Fields Near Cauchy Horizons
J. Rauch, A. D. Rendall
The behaviour of test fields near a compact Cauchy horizon is investigated. It is shown that solutions of nonlinear wave equations on Taub spacetime with generic initial data canno…
Global existence of classical solutions to the Vlasov-Poisson system in a three dimensional, cosmological setting
Gerhard Rein, Alan D. Rendall
The initial value problem for the Vlasov-Poisson system is by now well understood in the case of an isolated system where, by definition, the distribution function of the particles…
A regularity theorem for solutions of the spherically symmetric Vlasov-Einstein system
Gerhard Rein, Alan D. Rendall, Jack Schaeffer
In a previous paper two of the authors (G. R. and A. D. R.) showed that there exist global, classical solutions of the spherically symmetric Vlasov-Einstein system for small initia…
Gravitational waves in general relativity: XIV. Bondi expansions and the ``polyhomogeneity'' of \Scri
Piotr T. Chrusciel, Malcolm A. H. MacCallum, David B. Singleton
The structure of polyhomogeneous space-times (i.e., space-times with metrics which admit an expansion in terms of ) constructed by a Bondi--Sachs type method is ana…
On the Definition of Averagely Trapped Surfaces
Sean A. Hayward
Previously suggested definitions of averagely trapped surfaces are not well-defined properties of 2-surfaces, and can include surfaces in flat space-time. A natural definition of a…
On ``hyperboloidal'' Cauchy data for vacuum Einstein equations and obstructions to smoothness of ``null infinity''
Lars Andersson, Piotr T. Chrusciel
Various works have suggested that the Bondi--Sachs--Penrose decay conditions on the gravitational field at null infinity are not generally representative of asymptotically flat spa…
Maximal Hypersurfaces in Asymptotically Stationary Space-Times
P. T. Chrusciel, R. Wald
Existence of maximal hypersurfaces and of foliations by maximal hypersurfaces is proven in two classes of asymptotically flat spacetimes which possess a one parameter group of isom…
Global Structure of a Black-Hole Cosmos and its Extremes
Dieter R. Brill, Sean A. Hayward
We analyze the global structure of a family of Einstein-Maxwell solutions parametrized by mass, charge and cosmological constant. In a qualitative classification there are: (i) gen…
Quasi-Local Gravitational Energy
Sean A. Hayward
A dynamically preferred quasi-local definition of gravitational energy is given in terms of the Hamiltonian of a `2+2' formulation of general relativity. The energy is well-defined…
The Newtonian Limit for Asymptotically Flat Solutions of the Vlasov-Einstein System
Alan D. Rendall
It is shown that there exist families of asymptotically flat solutions of the Einstein equations coupled to the Vlasov equation describing a collisionless gas which have a Newtonia…
General Laws of Black-Hole Dynamics
Sean A. Hayward
A general definition of a black hole is given, and general `laws of black-hole dynamics' derived. The definition involves something similar to an apparent horizon, a trapping horiz…