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Ian Hawke

Researcher at University of Southampton

Publications -  81
Citations -  3107

Ian Hawke is an academic researcher from University of Southampton. The author has contributed to research in topics: Numerical relativity & General relativity. The author has an hindex of 24, co-authored 74 publications receiving 2762 citations. Previous affiliations of Ian Hawke include Albert Einstein Institution & Max Planck Society.

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Evolutions in 3D numerical relativity using fixed mesh refinement

TL;DR: This work presents results of 3D numerical simulations using a finite difference code featuring fixed mesh refinement (FMR), in which a subset of the computational domain is refined in space and time.
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Scientific objectives of Einstein Telescope

Bangalore Suryanarayana Sathyaprakash, +225 more
TL;DR: The advanced interferometer network will herald a new era in observational astronomy, and there is a very strong science case to go beyond the advanced detector network and build detectors that operate in a frequency range from 1 Hz to 10 kHz, with sensitivity a factor 10 better in amplitude as discussed by the authors.
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Three-dimensional relativistic simulations of rotating neutron-star collapse to a Kerr black hole

TL;DR: In this article, a conformal traceless formulation of the Einstein equations is presented for the study of the gravitational collapse of uniformly rotating neutron stars to Kerr black holes, where the initial stellar models are modeled as relativistic polytropes with angular velocities ranging from slow rotation to the mass shedding limit.

Einstein gravitational wave Telescope conceptual design study

Matthew Abernathy, +171 more
TL;DR: In this article, the conceptual design of a third generation gravitational wave observatory named the Einstein Telescope (ET) has been described with the support of the European Community's Seventh Framework Programme (FP7/2007-2013) under grant agreement n 211743.
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3D collapse of rotating stellar iron cores in general relativity including deleptonization and a nuclear equation of state.

TL;DR: This work focuses on gravitational wave (GW) emission from rotating collapse, bounce, and early postbounce phases and indicates that the GW signature of these phases is much more generic than previously estimated.