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Showing 1 to 5 of 5 for “"Black hole orbits"”.

  1. High precision calculation of generic extreme mass ratio inspirals

    Orbits around black holes evolve due to gravitational-wave emission, losing energy and angular momentum, and driving the orbiting body to slowly spiral into the black hole. Recent theoretical advances now make it possible to model the impact of this wave emission on generic (eccentric and inclined) …

    mit Repository record for High precision calculation of generic extreme mass ratio inspirals (opens in a new tab)

  2. Exploring the Possibility of Floating Orbits for Extreme Mass Ratio Binary Black Holes

    <p>A binary black hole system, where each black hole orbits the system's center of mass, loses energy by emission of gravitational waves. This causes both black holes to spiral in towards each other. However, if the binary were to, by some mechanism, gain orbital energy at the same rate that it …

    arkansas Repository record for Exploring the Possibility of Floating Orbits for Extreme Mass Ratio Binary Black Holes (opens in a new tab)

  3. Gravitomagnetic effects in compact binary systems : a study of spin-enhanced orbits around Kerr black holes

    … even chaotic-near the homoclinic set of orbits, which lie close to the separatrix dividing stable and unstable orbits. In this thesis we present a study of the spin-induced evolution of inclined, eccentric Kerr black hole orbits. The evolution of the orbital energy, angular momentum, and …

    mit Repository record for Gravitomagnetic effects in compact binary systems : a study of spin-enhanced orbits around Kerr black holes (opens in a new tab)

  4. Numerical relativity in higher-dimensional space-times

    … such as that involved in the merger of black holes, we use numerical relativity to solve the Einstein equations. In this thesis we develop and demonstrate several diagnostic tools and new initial data for use in numerical relativity simulations of higher dimensional spacetimes, and use …

    cambridge Repository record for Numerical relativity in higher-dimensional space-times (opens in a new tab)

  5. Making better binary models and modeling distorted black holes using black hole perturbation theory

    … I discuss the application and development of black hole perturbation theory both from an observational standpoint via gravitational waves and also tidal distortions of black hole horizons. The promise of gravitational wave astronomy depends on our ability to accurately model gravitational wave …

    mit Repository record for Making better binary models and modeling distorted black holes using black hole perturbation theory (opens in a new tab)