Contains fulltext : 237174.pdf (Author’s version preprint ) (Open Access
We analyze the inspiral dynamics of equal-mass precessing black-hole binaries using multi-timescale ...
Contains fulltext : 234090.pdf (Publisher’s version ) (Open Access
ntermediate mass black holes (IMBHs; 101.3 to 105Msolar) are thought to form as relics of Population...
Clouds of ultralight bosons-such as axions-can form around a rapidly spinning black hole, if the bla...
Contains fulltext : 156237.pdf (preprint version ) (Open Access
Contains fulltext : 132494.pdf (preprint version ) (Open Access
The tidal disruption of a star by a supermassive black hole (SMBH) is a highly energetic event with ...
Modeling ultra-close encounters between a white dwarf and a spinning, intermediate mass black hole r...
Ultralight bosons can form clouds around rotating black holes if their Compton wavelength is compara...
Contains fulltext : 205965.pdf (publisher's version ) (Open Access
Contains fulltext : 176277.pdf (publisher's version ) (Open Access
Contains fulltext : 173553.pdf (preprint version ) (Open Access
The deformability of a compact object under the presence of a tidal perturbation is encoded in the t...
Contains fulltext : 147309.pdf (preprint version ) (Open Access
star approaching a supermassive black hole (SMBH) can be torn apart in a tidal disruption event (TDE...
We analyze the inspiral dynamics of equal-mass precessing black-hole binaries using multi-timescale ...
Contains fulltext : 234090.pdf (Publisher’s version ) (Open Access
ntermediate mass black holes (IMBHs; 101.3 to 105Msolar) are thought to form as relics of Population...
Clouds of ultralight bosons-such as axions-can form around a rapidly spinning black hole, if the bla...
Contains fulltext : 156237.pdf (preprint version ) (Open Access
Contains fulltext : 132494.pdf (preprint version ) (Open Access
The tidal disruption of a star by a supermassive black hole (SMBH) is a highly energetic event with ...
Modeling ultra-close encounters between a white dwarf and a spinning, intermediate mass black hole r...
Ultralight bosons can form clouds around rotating black holes if their Compton wavelength is compara...
Contains fulltext : 205965.pdf (publisher's version ) (Open Access
Contains fulltext : 176277.pdf (publisher's version ) (Open Access
Contains fulltext : 173553.pdf (preprint version ) (Open Access
The deformability of a compact object under the presence of a tidal perturbation is encoded in the t...
Contains fulltext : 147309.pdf (preprint version ) (Open Access
star approaching a supermassive black hole (SMBH) can be torn apart in a tidal disruption event (TDE...
We analyze the inspiral dynamics of equal-mass precessing black-hole binaries using multi-timescale ...
Contains fulltext : 234090.pdf (Publisher’s version ) (Open Access
ntermediate mass black holes (IMBHs; 101.3 to 105Msolar) are thought to form as relics of Population...
DOI
Add to ORKG