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20032022
most citedInspiral, merger and ringdown of unequal mass black hole binaries: a multipolar analysis

425 citations · 4.2k across the 51 of their papers we have counts for

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Showing 2018Show all

9 papers · 1 filter

gr-qc2018

On the stability of scalarized black hole solutions in scalar-Gauss-Bonnet gravity

Hector O. Silva, Caio F. B. Macedo, Thomas P. Sotiriou +3

Scalar-tensor theories of gravity where a new scalar degree of freedom couples to the Gauss-Bonnet invariant can exhibit the phenomenon of spontaneous black hole scalarization. The…

gr-qc2018

Follow-up signals from superradiant instabilities of black hole merger remnants

Shrobana Ghosh, Emanuele Berti, Richard Brito +1

Superradiant instabilities can trigger the formation of bosonic clouds around rotating black holes. If the bosonic field growth is sufficiently fast, these clouds could form shortl…

gr-qc2018

Wide nutation: binary black-hole spins repeatedly oscillating from full alignment to full anti-alignment

Davide Gerosa, Alicia Lima, Emanuele Berti +3

Within the framework of 2PN black-hole binary spin precession, we explore configurations where one of the two spins oscillates from being completely aligned with the orbital angula…

gr-qc2018

Multi-mode black hole spectroscopy

Vishal Baibhav, Emanuele Berti

The first two LIGO/Virgo observing runs have detected several black hole binary mergers. One of the most exciting prospects of future observing runs is the possibility to identify…

astro-ph.HE2018

Expanding the LISA Horizon from the Ground

Kaze W. K. Wong, Ely D. Kovetz, Curt Cutler +1

The Laser Interferometer Space Antenna (LISA) gravitational-wave (GW) observatory will be limited in its ability to detect mergers of binary black holes (BBHs) in the stellar-mass…

astro-ph.EP2018

On the possibility of detecting ultra-short period exoplanets with LISA

Kaze W. K. Wong, Emanuele Berti, William E. Gabella +1

Cunha et al. (2018) recently reexamined the possibility of detecting gravitational waves from exoplanets, claiming that three ultra-short period systems would be observable by LISA…