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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

268 31- PDF

Gravitational Radiation Instability in Hot Young Neutron Stars

- L. Lindblom, B. Owen, S. Morsink
- Physics
- 13 March 1998

We show that gravitational radiation drives an instability in hot young rapidly rotating neutron stars. This instability occurs primarily in the l=2 r-mode and will carry away most of the angular… Expand

259 23- PDF

The effect of viscosity on neutron star oscillations

- C. Cutler, L. Lindblom
- Physics
- 1 March 1987

The rate at which neutron star oscillations are damped by the presence of viscosity and thermal conductivity in the neutron matter is computed. Fully relativistic equations are used to describe the… Expand

138 15

A New Generalized Harmonic Evolution System

- L. Lindblom, M. Scheel, L. Kidder, Robert Owen, O. Rinne
- Physics
- 15 December 2005

A new representation of the Einstein evolution equations is presented that is first order, linearly degenerate and symmetric hyperbolic. This new system uses the generalized harmonic method to… Expand

231 13- PDF

Stability and causality in dissipative relativistic fluids

- W. Hiscock, L. Lindblom
- Physics
- 1 July 1983

The standard theory of relativistic dissipative fluid mechanics developed by Eckart contains several undesirable features: thermal and viscous fluctuations propagate acausally; there exist generic… Expand

303 13

Second-order rotational effects on the r-modes of neutron stars.

- L. Lindblom, G. Mendell, B. Owen
- Physics
- 18 February 1999

Techniques are developed here for evaluating the r-modes of rotating neutron stars through second order in the angular velocity of the star. Second-order corrections to the frequencies and… Expand

67 13- PDF

Effect of hyperon bulk viscosity on neutron-star r-modes

- L. Lindblom, B. Owen
- Physics
- 25 October 2001

Neutron stars are expected to contain a significant number of hyperons in addition to protons and neutrons in the highest density portions of their cores. Following the work of Jones, we calculate… Expand

109 7- PDF

Determining the nuclear equation of state from neutron-star masses and radii

- L. Lindblom
- Physics
- 20 October 1992

A method is developed for determining the nuclear equation of state directly from a knowledge of the masses and radii of neutron stars. This analysis assumes only that equilibrium neutron-star matter… Expand

119 7

Spectral representations of neutron-star equations of state

- L. Lindblom
- Physics
- 3 September 2010

Methods are developed for constructing spectral representations of cold (barotropic) neutron-star equations of state. These representations are faithful in the sense that every physical equation of… Expand

66 7- PDF

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