Determining the Hubble constant from gravitational wave observations
about
Short GRB and binary black hole standard sirens as a probe of dark energyGravitational Wave Detection by Interferometry (Ground and Space).The Hubble Constant.Gravitational-Wave Data Analysis. Formalism and Sample Applications: The Gaussian Case.Advanced technologies for future ground-based, laser-interferometric gravitational wave detectors.The Post-Newtonian Approximation for Relativistic Compact Binaries.Spin-induced orbital precession and its modulation of the gravitational waveforms from merging binariesThe last three minutes: Issues in gravitational-wave measurements of coalescing compact binariesPrecision cosmology from future lensed gravitational wave and electromagnetic signals.Anisotropies of Gravitational-Wave Standard Sirens as a New Cosmological Probe without Redshift Information.Detectability of Gravitational Waves from High-Redshift Binaries.Gamma-ray-burst beaming and gravitational-wave observations.Measuring a cosmological distance-redshift relationship using only gravitational wave observations of binary neutron star coalescences.Beyond concordance cosmology with magnification of gravitational-wave standard sirens.Imprint of accretion disk-induced migration on gravitational waves from extreme mass ratio inspirals.Algorithm to search for gravitational radiation from coalescing binaries.Strong-field point-particle limit and the equations of motion in the binary pulsar.Prospects for Multiband Gravitational-Wave Astronomy after GW150914.Toward an Internally Consistent Astronomical Distance ScaleGalactic distribution of merging neutron stars and black holes - prospects for short gamma-ray burst progenitors and LIGO/VIRGOImplementation and testing of the first prompt search for gravitational wave transients with electromagnetic counterpartsGravitational-Wave Data Analysis. Formalism and Sample Applications: The Gaussian CasePost-Newtonian SPH calculations of binary neutron star coalescence: Method and first resultsReducing the gravitational lensing scatter of type Ia supernovae without introducing any extra biasHunting Gravitational Waves with Multi-Messenger Counterparts: Australia’s RoleHow gravitational waves could solve some of the Universe’s deepest mysteries
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Determining the Hubble constant from gravitational wave observations
description
article publié dans la revue scientifique Nature
@fr
scientific article published in Nature
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована в Nature у вересні 1986
@uk
name
Determining the Hubble constant from gravitational wave observations
@en
Determining the Hubble constant from gravitational wave observations
@nl
type
label
Determining the Hubble constant from gravitational wave observations
@en
Determining the Hubble constant from gravitational wave observations
@nl
prefLabel
Determining the Hubble constant from gravitational wave observations
@en
Determining the Hubble constant from gravitational wave observations
@nl
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P1433
P1476
Determining the Hubble constant from gravitational wave observations
@en
P2093
Bernard F. Schutz
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P304
P356
10.1038/323310A0
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P577
1986-09-01T00:00:00Z
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1051965609