Kostas Glampedakis
12 ta ish
University of Tübingen
Mapping spacetimes with LISA: inspiral of a test body in a ‘quasi-Kerr’ field
Kostas Glampedakis, Stanislav Babak
MaqolaOchiq kirish20068 iqtibosABICan supermassive black hole shadows test the Kerr metric?
Kostas Glampedakis, George Pappas
MaqolaOchiq kirish20216 iqtibosABIThe Einstein Telescope: a third-generation gravitational wave observatory
M. Punturo, M. R. Abernathy, F. Acernese +97
Maqola20106 iqtibosABI“Kludge” gravitational waveforms for a test-body orbiting a Kerr black hole
Stanislav Babak, Hua Fang, J. R. Gair +2
MaqolaOchiq kirish20075 iqtibosABIScattering of scalar waves by rotating black holes
Kostas Glampedakis, Nils Andersson
MaqolaOchiq kirish20015 iqtibosABISensitivity studies for third-generation gravitational wave observatories
S. Hild, M. R. Abernathy, F. Acernese +97
MaqolaOchiq kirish20113 iqtibosABIHYDROMAGNETIC INSTABILITIES IN RELATIVISTIC NEUTRON STARS
P. D. Lasky, Burkhard Zink, Kostas D. Kokkotas +1
MaqolaOchiq kirish20113 iqtibosABIPost-Kerr black hole spectroscopy
Kostas Glampedakis, George Pappas, Hector O. Silva +1
MaqolaOchiq kirish20173 iqtibosABIIs a black hole shadow a reliable test of the no-hair theorem?
Kostas Glampedakis, George Pappas
MaqolaOchiq kirish20233 iqtibosABICrust-core coupling in rotating neutron stars
Kostas Glampedakis, Nils Andersson
MaqolaOchiq kirish20062 iqtibosABI