Golm / Burjassot / Trieste / Beirut / St. Louis / /
Country
Germany / United States / Italy / Spain / Greece / /
Facility
Washington University / Albert Einstein Institute / Aristotle University of Thessaloniki / Louisiana State University / /
IndustryTerm
stationary equilibrium solutions / rotational kinetic energy / self-gravitating systems / wrong weak solution / kinetic energy / gravitational binding energy / rest-mass energy / curvilinear coordinate systems / internal energy / excision algorithm / energy density / thermal energy / rotational energy / larger central energy densities / energy density ec / binary systems / physical systems / numerical solution / energy / stress-energy tensor / /
Organization
International School for Advanced Studies / Center for Computation and Technology / SISSA / Albert-Einstein-Institut / Aristotle University of Thessaloniki / Louisiana State University / Albert Einstein Institute / INFN / Department of Physics / Washington University / Universidad de Valencia / Max-Planck-Institut f¨ur Gravitationsphysik / /
Three-dimensional relativistic simulations of rotating neutron-star collapse to a Kerr black hole Luca Baiotti,1 Ian Hawke,2 Pedro J. Montero,1 Frank L¨offler,2 Luciano Rezzolla,1, 3 Nikolaos Stergioulas,4 Jos´e A. Fon