Gravitational wave sources in the era of multi-frequency gravitational wave astronomy
Monica Colpi, Alberto Sesana

TL;DR
This paper discusses the diverse sources of gravitational waves across multiple frequency bands, emphasizing their potential to revolutionize our understanding of cosmic phenomena from stellar evolution to the early universe.
Contribution
It provides a comprehensive overview of prospective gravitational wave sources across different frequencies and highlights their scientific significance and expected signals.
Findings
Identification of key gravitational wave sources across frequency bands
Potential insights into star and black hole formation and evolution
Implications for understanding fundamental physics and the early universe
Abstract
The focus of this Chapter is on describing the prospective sources of the gravitational wave universe accessible to present and future observations, from kHz, to mHz down to nano-Hz frequencies. The multi-frequency gravitational wave universe gives a deep view into the cosmos, inaccessible otherwise. It has as main actors core-collapsing massive stars, neutron stars, coalescing compact object binaries of different flavours and stellar origin, coalescing massive black hole binaries, extreme mass ratio inspirals, and possibly the very early universe itself. Here, we highlight the science aims and describe the gravitational wave signals expected from the sources and the information gathered in it. We show that the observation of gravitational wave sources will play a transformative role in our understanding of the processes ruling the formation and evolution of stars and black holes,…
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