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Fundamental physics with the square kilometre array
The Square Kilometre Array (SKA) is a planned large radio interferometer designed to
operate over a wide range of frequencies, and with an order of magnitude greater sensitivity …
operate over a wide range of frequencies, and with an order of magnitude greater sensitivity …
The Process of Stellar Tidal Disruption by Supermassive Black Holes: The First Pericenter Passage
Tidal disruption events (TDEs) are among the brightest transients in the optical, ultraviolet,
and X-ray sky. These flares are set into motion when a star is torn apart by the tidal field of a …
and X-ray sky. These flares are set into motion when a star is torn apart by the tidal field of a …
Observational signatures of supermassive black hole binaries
Despite solid theoretical and observational grounds for the pairing of supermassive black
holes (SMBHs) after galaxy mergers, definitive evidence for the existence of close (sub …
holes (SMBHs) after galaxy mergers, definitive evidence for the existence of close (sub …
GW× LSS: chasing the progenitors of merging binary black holes
Are the stellar-mass merging binary black holes, recently detected by their gravitational
wave signal, of stellar or primordial origin? Answering this question will have profound …
wave signal, of stellar or primordial origin? Answering this question will have profound …
Electromagnetic chirp of a compact binary black hole: A phase template for the gravitational wave inspiral
Z Haiman - Physical Review D, 2017 - APS
The gravitational waves (GWs) from a binary black hole (BBH) with masses 10 4≲ M≲ 10 7
M⊙ can be detected with the Laser Interferometer Space Antenna (LISA) once their orbital …
M⊙ can be detected with the Laser Interferometer Space Antenna (LISA) once their orbital …
Tidal disruption events from supermassive black hole binaries
We investigate the pre-disruption gravitational dynamics and post-disruption hydrodynamics
of the tidal disruption of stars by supermassive black hole (SMBH) binaries. We focus on …
of the tidal disruption of stars by supermassive black hole (SMBH) binaries. We focus on …
X-ray flares from the stellar tidal disruption by a candidate supermassive black hole binary
Optical transient surveys have led to the discovery of dozens of stellar tidal disruption events
(TDEs) by massive black hole in the centers of galaxies. Despite extensive searches, X-ray …
(TDEs) by massive black hole in the centers of galaxies. Despite extensive searches, X-ray …
Broad-band X-ray observations of the 2018 outburst of the changing-look active galactic nucleus NGC 1566
We study the nature of the changing-look active galactic nucleus NGC 1566 during its 2018
June outburst. During the outburst, the X-ray intensity of the source rises up to∼ 25–30 …
June outburst. During the outburst, the X-ray intensity of the source rises up to∼ 25–30 …
[PDF][PDF] Disc origin of broad optical emission lines of the TDE candidate PTF09djl
An otherwise dormant supermassive black hole (SMBH) in a galactic nucleus flares up when
it tidally disrupts a star passing by. Most of the tidal disruption events (TDEs) and candidates …
it tidally disrupts a star passing by. Most of the tidal disruption events (TDEs) and candidates …
Single progenitor model for GW150914 and GW170104
The merger of stellar-mass black holes (BHs) is not expected to generate detectable
electromagnetic (EM) emission. However, the gravitational wave (GW) events GW150914 …
electromagnetic (EM) emission. However, the gravitational wave (GW) events GW150914 …