Results 51 to 60 of about 3,576 (162)
With the growing number of binary black hole (BBH) mergers detected by LIGO/Virgo/KAGRA, several systems have become difficult to explain via isolated binary evolution, having components in the pair-instability mass gap, high orbital eccentricities, and ...
Rachel C. Zhang +3 more
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Laboratory sources of gravitational waves
Abstract We consider the possibility of generating and subsequently detecting artificial gravitational waves in a laboratory based on different approaches. As one of the methods for creating gravitational waves, we investigate oscillations of the ions of the crystal lattice of a dielectric under the influence of high-power laser ...
I V Fomin +5 more
openaire +1 more source
Localizing Dynamically Formed Black Hole Binaries in Milky Way Globular Clusters with LISA
The dynamical formation of binary black holes (BBHs) in globular clusters (GCs) may contribute significantly to the observed gravitational-wave (GW) merger rate.
Zeyuan Xuan, Kyle Kremer, Smadar Naoz
doaj +1 more source
Fast Radio Bursts: Electromagnetic Counterparts to Extreme Mass-ratio Inspirals
Recent observations discovered that some repeating fast radio bursts (FRBs) show a large value and complex variations of Faraday rotation measures (RMs).
Rui-Nan Li +3 more
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Machine Learning Confirms GW231123 is a “Lite” Intermediate Mass Black Hole Merger
The LIGO–Virgo–KAGRA Collaboration recently reported GW231123, a black hole merger with total mass of around 190–265 M _⊙ . This event adds to the growing evidence of “lite” intermediate mass black hole (IMBH) discoveries of postmerger black holes ≳100 M
Chayan Chatterjee +4 more
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Multimessenger observations of gravitational waves and electromagnetic emission from compact object mergers offer unique insights into the structure of neutron stars, the formation of heavy elements, and the expansion rate of the Universe.
Nayyer Raza +7 more
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Gravitational Waves from Gravitational Collapse
Gravitational-wave emission from stellar collapse has been studied for nearly four decades. Current state-of-the-art numerical investigations of collapse include those that use progenitors with more realistic angular momentum profiles, properly treat ...
Chris L. Fryer, Kimberly C.B. New
doaj
Structure and Skewness of the Effective Inspiral Spin Distribution of Binary Black Hole Mergers
The detection of gravitational waves has brought to light a population of binary black holes that merge within a Hubble time. Multiple formation channels can contribute to this population, making it difficult to definitively associate particular ...
Sharan Banagiri +4 more
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Gravitational wave denoising of binary black hole mergers with deep learning
Gravitational wave detection requires an in-depth understanding of the physical properties of gravitational wave signals, and the noise from which they are extracted.
Wei Wei, E.A. Huerta
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Anisotropic stochastic gravitational wave background (SGWB) serves as a potential probe of the large-scale structure (LSS) of the universe. In this work, we explore the anisotropic SGWB from local ( z < ∼ 0.085) merging stellar mass compact binaries ...
Zhencheng Li +6 more
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