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Gravitational waves from hot young rapidly rotating neutron stars

- B. Owen, L. Lindblom, C. Cutler, B. Schutz, A. Vecchio, N. Andersson
- Physics
- 20 April 1998

Gravitational radiation drives an instability in the r-modes of young rapidly rotating neutron stars. This instability is expected to carry away most of the angular momentum of the star by… Expand

The Einstein Telescope: a third-generation gravitational wave observatory

- M. Punturo, M. Abernathy,
+132 authors Kazuhiro Yamamoto - Physics
- 7 October 2010

Advanced gravitational wave interferometers, currently under realization, will soon permit the detection of gravitational waves from astronomical sources. To open the era of precision gravitational… Expand

Sensitivity studies for third-generation gravitational wave observatories

- S. Hild, M. Abernathy,
+136 authors K. Yamamoto - Physics, Geology
- 4 December 2010

Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope (ET), a… Expand

Modelling magnetically deformed neutron stars

- B. Haskell, L. Samuelsson, K. Glampedakis, N. Andersson
- Physics
- 12 May 2007

Rotating deformed neutron stars are important potential sources for ground-based gravitational wave interferometers such as LIGO, GEO600 and VIRGO. One mechanism that may lead to significant… Expand

THE R-MODE INSTABILITY IN ROTATING NEUTRON STARS

- N. Andersson, K. Kokkotas
- Physics
- 27 October 2000

In this review we summarize the current understanding of the gravitational-wave driven instability associated with the so-called r-modes in rotating neutron stars. We discuss the nature of the… Expand

Einstein gravitational wave Telescope conceptual design study

- M. Abernathy, F. Acernese,
+169 authors L. Rezzolla - Physics
- 20 May 2011

This document describes the Conceptual Design of a third generation gravitational wave observatory named Einstein Telescope (“ET”). The design of this new research infrastructure has been realised… Expand

Towards gravitational wave asteroseismology

- N. Andersson, K. Kokkotas
- Physics, Geology
- 28 November 1997

We present new results for pulsating neutron stars. We have calculated the eigenfrequencies of the modes that one would expect to be the most important gravitational wave sources: the fundamental… Expand

Relativistic Fluid Dynamics: Physics for Many Different Scales

- N. Andersson, G. Comer
- PhysicsLiving reviews in relativity
- 1 May 2006

TLDR

Dynamics of perturbations of rotating black holes

- W. Krivan, P. Laguna, P. Papadopoulos, N. Andersson
- Physics
- 24 February 1997

We present a numerical study of the time evolution of perturbations of rotating black holes. The solutions are obtained by integrating the Teukolsky equation written as a first order in time, coupled… Expand

Mutual friction in superfluid neutron stars

- N. Andersson, T. Sidery, G. Comer
- Physics
- 3 October 2005

We discuss vortex-mediated mutual friction in the two-fluid model for superfluid neutron star cores. Our discussion is based on the general formalism developed by Carter and collaborators, which… Expand

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