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Published in 2019 at "Astrophysics and Space Science"
DOI: 10.1007/s10509-019-3657-2
Abstract: This communication aims to expose further the assertions made in microscopic theory of black hole (MTBH) to the physics of intermediate mass black holes (IMBHs). The MTBH explores the most important spontaneous breaking of gravitation…
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Keywords:
study 137;
intermediate mass;
black hole;
mass ... See more keywords
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Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staa1338
Abstract: Coalescence of intermediate-mass black holes (IMBHs) as a result of the migration toward galactic centers via dynamical friction may contribute to the formation of supermassive BHs. Here we reinvestigate the gaseous dynamical friction, which was…
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Keywords:
black holes;
intermediate mass;
gaseous dynamical;
mass black ... See more keywords
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Published in 2022 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stad1544
Abstract: While it is well established that supermassive black holes (SMBHs) co-evolve with their host galaxy, it is currently less clear how lower-mass black holes, so-called intermediate-mass black holes (IMBHs), evolve within their dwarf galaxy hosts.…
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Keywords:
dwarf galaxies;
population statistics;
intermediate mass;
mass black ... See more keywords
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Published in 2017 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stx1755
Abstract: Tidal disruption events (TDEs) of stars by single or binary supermassive black holes (SMBHs) brighten galactic nuclei and reveal a population of otherwise dormant black holes. Adopting event rates from the literature, we aim to…
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Keywords:
intermediate mass;
black holes;
mass;
mass black ... See more keywords
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Published in 2018 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stx2762
Abstract: We investigate the lack of observed low mass black hole binary systems at short periods ( 200 and
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Keywords:
mass black;
low mass;
black hole;
selection effects ... See more keywords
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Published in 2020 at "Physical Review D"
DOI: 10.1103/physrevd.102.123014
Abstract: Long-term viscous neutrino-radiation hydrodynamics simulations in full general relativity are performed for a massive disk surrounding spinning stellar-mass black holes with mass $M_{\rm BH}=4$, $6$, and $10M_\odot$ and initial dimensionless spin $\chi \approx 0.8$. The…
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Keywords:
black holes;
disk;
stellar mass;
mass ... See more keywords
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Published in 2020 at "Physical Review D"
DOI: 10.1103/physrevd.102.124037
Abstract: Stellar-mass black hole binaries (SBHBs), like those currently being detected with the ground-based gravitational-wave (GW) observatories LIGO and Virgo, are also an anticipated GW source for LISA. LISA will observe them during the early inspiral…
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Keywords:
stellar mass;
black hole;
mass;
mass black ... See more keywords
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Published in 2021 at "Physical Review D"
DOI: 10.1103/physrevd.104.123501
Abstract: We demonstrate that cosmic string loops may provide a joint resolution of two mysteries surrounding recently observed black holes. For a string tension in an appropriate range, large radius string loops have the potential to…
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Keywords:
string loops;
black holes;
intermediate mass;
mass black ... See more keywords
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Published in 2021 at "Physical review letters"
DOI: 10.1103/physrevlett.126.021103
Abstract: We present the first search for gravitational waves from the coalescence of stellar mass and subsolar mass black holes with masses between 20-100 M_{⊙} and 0.01-1 M_{⊙}(10-10^{3} M_{J}), respectively. The observation of a single subsolar mass black hole…
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Keywords:
gravitational waves;
black holes;
search gravitational;
mass black ... See more keywords
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Published in 2021 at "Physical review letters"
DOI: 10.1103/physrevlett.126.071101
Abstract: Solar-mass black holes with masses in the range of ∼1-2.5 M_{⊙} are not expected from conventional stellar evolution, but can be produced naturally via neutron star (NS) implosions induced by capture of small primordial black holes…
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Keywords:
black holes;
mass black;
mass;
bhs ... See more keywords
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Published in 2019 at "Astronomy Reports"
DOI: 10.1134/s1063772919060052
Abstract: Under certain conditions, stars close to intermediate-mass black holes (IMBHs) can form close binary systems with these objects, in which the Roche lobe can be filled by the star and intense accretion of the star’s…
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Keywords:
black holes;
intermediate mass;
mass black;
mass ... See more keywords