Results 11 to 20 of about 8,250 (145)
Partial Tidal Disruptions of Main-sequence Stars by Intermediate-mass Black Holes
We study close encounters of a 1 M _⊙ middle-age main-sequence star (modeled using MESA) with massive black holes through hydrodynamic simulations, and explore in particular the dependence of the outcomes on the black hole mass.
Fulya Kıroğlu +5 more
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Entropy of the Universe and Hierarchical Dark Matter
We discuss the relationship between dark matter and the entropy of the universe, with the premise that dark matter exists in the form of primordial black holes (PBHs) in a hierarchy of mass tiers. The lightest tier includes all PBHs with masses below one
Paul H. Frampton
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Intermediate Mass Black Holes: Their Motion and Associated Energetics
There is a lot of current astrophysical evidence and interest in intermediate mass black holes (IMBH), ranging from a few hundred to several thousand solar masses.
C. Sivaram, Kenath Arun
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The search for robust evidence of intermediate-mass black holes (IMBHs) is crucial for understanding the black hole seeding process and the formation of supermassive black holes in the early Universe.
Jingbo Sun +27 more
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Tidal disruption of white dwarfs by intermediate mass black holes
Modeling ultra-close encounters between a white dwarf and a spinning, intermediate mass black hole requires a full general relativistic treatment of gravity. This paper summarizes results from such a study.
Bode T. +3 more
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Interpretable Machine Learning for Finding Intermediate-mass Black Holes
Definitive evidence that globular clusters (GCs) host intermediate-mass black holes (IMBHs) is elusive. Machine-learning (ML) models trained on GC simulations can in principle predict IMBH host candidates based on observable features.
Mario Pasquato +6 more
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Supermassive Black Hole Growth in Hierarchically Merging Nuclear Star Clusters
Supermassive black holes are prevalent at the centers of massive galaxies, and their masses scale with galaxy properties, increasing evidence suggesting that these trends continue to low stellar masses.
Konstantinos Kritos +7 more
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Intermediate-mass black holes (IMBHs) have not been detected beyond any reasonable doubt through either dynamical or accretion signatures. Gravitational waves (GWs) represent an unparalleled opportunity to survey the sky and detect mergers of IMBHs ...
Giacomo Fragione, Abraham Loeb
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Detecting Intermediate-mass Black Holes Using Quasar Microlensing
Recent studies suggest that numerous intermediate-mass black holes (IMBHs) may wander undetected across the Universe, emitting little radiation. These IMBHs largely preserve their birth masses, offering critical insights into the formation of heavy black
Zihao Wu, Luis C. Ho
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On the Tidal Capture of White Dwarfs by Intermediate-mass Black Holes in Dense Stellar Environments
Intermediate-mass black holes (IMBHs) are the missing link between stellar-mass and supermassive black holes, widely believed to reside in at least some dense star clusters, but not yet observed directly.
Claire S. Ye +2 more
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