Titlebook: Compact Objects in the Universe; Eleftherios Papantonopoulos,Nikolaos Mavromatos Book 2024 The Editor(s) (if applicable) and The Author(s)

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https://doi.org/10.1007/978-981-19-0928-3context of the same theory which also possess interesting observable features such as photon rings and echoes. Moving beyond this class of theories, we then address the more extended scalar-tensor Horndeski theory, briefly mention the types of black-hole solutions that arise, and demonstrate that an

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Transformation Using Cotyledon Explantsications in black holes and exotic horizonless compact objects. We will show that quasinormal modes generically suffer from spectral instabilities, explore how such phenomena can further affect black-hole spectroscopy, and discuss potential ringdown imprints and waveform stability issues in current

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Marcy Main,Bronwyn Frame,Kan Wangtomic nucleus, and mergers that emit both gravitational and electromagnetic waves probe the formation of short gamma ray bursts and the nucleosynthesis of heavy elements. Other searches are constraining more and more the emission of isolated sources and the possible background of gravitational waves

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Mark A. Smedley,Wendy A. Harwoodverse in large scales using the . observational method. For identifying individually fast radio sources, the . (ABDUS) project has been proposed and developed and will combine the current BINGO construction with the main single-dish telescope and stations of phased-array and outrigger, which will re

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https://doi.org/10.1007/978-1-4939-1658-0r range. In particular cases, they also generate characteristic oscillatory patterns that are transferred in the spectrum of secondary GWs, which are potentially observable by operating or designed experiments. We demonstrate these effects through the calculation of the primordial power spectrum and

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Black-Hole Spectroscopy: Quasinormal Modes, Ringdown Stability and the Pseudospectrumications in black holes and exotic horizonless compact objects. We will show that quasinormal modes generically suffer from spectral instabilities, explore how such phenomena can further affect black-hole spectroscopy, and discuss potential ringdown imprints and waveform stability issues in current