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      Dynamical boson stars

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          Abstract

          The idea of stable, localized bundles of energy has strong appeal as a model for particles. In the 1950s, John Wheeler envisioned such bundles as smooth configurations of electromagnetic energy that he called geons, but none were found. Instead, particle-like solutions were found in the late 1960s with the addition of a scalar field, and these were given the name boson stars. Since then, boson stars find use in a wide variety of models as sources of dark matter, as black hole mimickers, in simple models of binary systems, and as a tool in finding black holes in higher dimensions with only a single Killing vector. We discuss important varieties of boson stars, their dynamic properties, and some of their uses, concentrating on recent efforts.

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          Observation of Gravitational Waves from a Binary Black Hole Merger

          On September 14, 2015 at 09:50:45 UTC the two detectors of the Laser Interferometer Gravitational-Wave Observatory simultaneously observed a transient gravitational-wave signal. The signal sweeps upwards in frequency from 35 to 250 Hz with a peak gravitational-wave strain of \(1.0 \times 10^{-21}\). It matches the waveform predicted by general relativity for the inspiral and merger of a pair of black holes and the ringdown of the resulting single black hole. The signal was observed with a matched-filter signal-to-noise ratio of 24 and a false alarm rate estimated to be less than 1 event per 203 000 years, equivalent to a significance greater than 5.1 {\sigma}. The source lies at a luminosity distance of \(410^{+160}_{-180}\) Mpc corresponding to a redshift \(z = 0.09^{+0.03}_{-0.04}\). In the source frame, the initial black hole masses are \(36^{+5}_{-4} M_\odot\) and \(29^{+4}_{-4} M_\odot\), and the final black hole mass is \(62^{+4}_{-4} M_\odot\), with \(3.0^{+0.5}_{-0.5} M_\odot c^2\) radiated in gravitational waves. All uncertainties define 90% credible intervals.These observations demonstrate the existence of binary stellar-mass black hole systems. This is the first direct detection of gravitational waves and the first observation of a binary black hole merger.
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            Black holes in higher dimensional space-times

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              Evolution of three-dimensional gravitational waves: Harmonic slicing case

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                Author and article information

                Contributors
                steve.liebling@liu.edu
                carlos.palenzuela@uib.es
                Journal
                Living Rev Relativ
                Living Rev Relativ
                Living Reviews in Relativity
                Springer International Publishing (Cham )
                1433-8351
                13 November 2017
                13 November 2017
                2017
                : 20
                : 1
                : 5
                Affiliations
                [1 ]GRID grid.259180.7, Long Island University, ; Brookville, NY 11548 USA
                [2 ]ISNI 0000000118418788, GRID grid.9563.9, Universitat de les Illes Balears, ; 07122 Palma de Mallorca, Baleares Spain
                Author information
                http://orcid.org/0000-0002-5008-6119
                Article
                7
                10.1007/s41114-017-0007-y
                5684349
                fe906383-0973-413c-906c-d860ef07547c
                © The Author(s) 2017

                Open AccessThis article is distributed under the terms of the Creative Commons Attribution 4.0 International License ( http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.

                History
                : 12 June 2017
                : 13 September 2017
                Categories
                Review Article
                Custom metadata
                © The Author(s) 2017

                numerical relativity,boson stars,solitons
                numerical relativity, boson stars, solitons

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