Observability of Isolated Stellar-mass Black Holes
Stellar-mass black holes (BHs) represent the natural end states of massive stars. It is estimated that 10 ^8 stellar-mass BHs are present in the Milky Way galaxy, a significant fraction of which are expected to be isolated.
Lena Murchikova, Kailash C. Sahu
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Energy Extraction from Loop Quantum Black Holes: The Role of Magnetic Penrose Process and Quantum Gravity Effects with Astrophysical Insights [PDF]
Tursunali Xamidov +3 more
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PRIMORDIAL BLACK HOLES, ASTROPHYSICAL SYSTEMS AND THE EDDINGTON–WEINBERG RELATION [PDF]
Salvatore Capozziello +2 more
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The cosmic expansion rate can be directly measured with gravitational-wave (GW) data of the compact binary mergers by jointly constraining the mass function of the population and the cosmological model via the so-called spectral sirens.
Yin-Jie Li +3 more
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We present the results of the first fully cosmological hydrodynamical simulations studying the merger-driven model for massive black hole (BH) seed formation via direct collapse.
Lucio Mayer +3 more
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Recoiling black holes: electromagnetic signatures, candidates, and astrophysical implications [PDF]
S. Komossa
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Find the Gap: Black Hole Population Analysis with an Astrophysically Motivated Mass Function [PDF]
Eric J. Baxter +3 more
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The Delayed Radio Emission in the Black Hole X-Ray Binary MAXI J1348-630
We explore the coupling between the accretion flow and the jet in black hole X-ray binary MAXI J1348-630 by analyzing the X-ray and radio observations during its 2019 outburst.
Bei You +4 more
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The most powerful astrophysical events: Gravitational-wave peak luminosity of binary black holes as predicted by numerical relativity [PDF]
D. Keitel +11 more
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Non-Stationary Astrophysical Stochastic Gravitational-Wave Background: A New Probe to the High Redshift Population of Binary Black Holes [PDF]
Mohit Raj Sah, Suvodip Mukherjee
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