output
19922026
most citedObservation of Gravitational Waves from a Binary Black Hole Merger

14.2k citations

Showing 2020 · gr-qcShow all

30 papers · 2 filters

gr-qc2020★ 71 cited

All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systems

The LIGO Scientific Collaboration, the Virgo Collaboration, R. Abbott +1369

Rapidly spinning neutron stars are promising sources of persistent, continuous gravitational waves. Detecting such a signal would allow probing of the physical properties of matter…

gr-qc2020★ 26 cited

Deep learning for clustering of continuous gravitational wave candidates II: identification of low-SNR candidates

Banafsheh Beheshtipour, Maria Alessandra Papa

Broad searches for continuous gravitational wave signals rely on hierarchies of follow-up stages for candidates above a given significance threshold. An important step to simplify…

gr-qc2020★ 34 cited

Results from high-frequency all-sky search for continuous gravitational waves from small-ellipticity sources

Vladimir Dergachev, Maria Alessandra Papa

We present the results of an all-sky search for continuous gravitational wave signals with frequencies in the 1700-2000 Hz range from neutron stars with ellipticity of 1e-8. The se…

gr-qc2020★ 370 cited

Challenges and Opportunities of Gravitational Wave Searches at MHz to GHz Frequencies

N. Aggarwal, O. D. Aguiar, A. Bauswein +22

The first direct measurement of gravitational waves by the LIGO and Virgo collaborations has opened up new avenues to explore our Universe. This white paper outlines the challenges…

gr-qc2020★ 11 cited

Possibility of primordial black holes as the source of gravitational wave events in the advanced LIGO detector

E. Khalouei, H. Ghodsi, S. Rahvar +1

The analysis of gravitational Wave (GW) data from advanced LIGO provides the mass of each companion of binary black holes as the source of GWs. The mass of events corresponding to…

gr-qc2020★ 53 cited

Quasinormal modes and their overtones at the common horizon in a binary black hole merger

Pierre Mourier, Xisco Jiménez Forteza, Daniel Pook-Kolb +2

It is expected that all astrophysical black holes in equilibrium are well described by the Kerr solution. Moreover, any black hole far away from equilibrium, such as one initially…