Titlebook: Handbook of Gravitational Wave Astronomy; Cosimo Bambi,Stavros Katsanevas,Konstantinos D. Ko Reference work 2022 Springer Nature Singapore

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Third-Generation Gravitational-Wave Observatoriesored. A greatly more sensitive third generation of observatories is currently being planned: The Einstein Telescope in Europe and Cosmic Explorer in the USA. The Einstein Telescope is envisaged as an underground observatory in the shape of an equilateral triangle with a side length of 10 km located

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Research and Development for Third-Generation Gravitational Wave Detectorss were from instruments of the second generation of detectors – the first generation of kilometer-scale ground based detectors operated as planned, but did not conclusively observe gravitational waves. The second-generation detectors (Advanced LIGO and Advanced Virgo) opened the field, and the third

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Isolated Neutron Starsobservations is, however, a challenging endeavor, as the radiation is only emitted by the outermost layers and is scattered by the interstellar medium. Gravitational waves, on the other hand, while challenging to detect, interact weakly with matter and are likely to carry a clean imprint of the high

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-Process Nucleosynthesis from Compact Binary Mergersing at high speed in space. Being matter coming from the violent disruption of a neutron star, these ejecta are initially very dense, hot, and extremely rich in neutrons. The few available protons form heavy nuclei (“seeds”) that absorb the more abundant free neutrons, increasing their size. The neu

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