The GW-Neutrino Window: Probing the Engines of the Extreme Universe
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| Format: | Recurso digital |
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Zenodo
2025
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| _version_ | 1866901227883724800 |
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| author | Revista, Zen ASTRO, 10 |
| author_facet | Revista, Zen ASTRO, 10 |
| contents | Multi-messenger astronomy, leveraging gravitational waves (GWs) and high-energy neutrinos, opens an unparalleled "GW-Neutrino Window" into the most extreme astrophysical phenomena. This paper explores the profound potential of this emerging observational paradigm to decipher the fundamental physics governing the engines of the universe, such as merging compact objects, core-collapse supernovae, and active galactic nuclei. We review the current status of GW and neutrino detection, outlining the theoretical framework for their joint emission from high-energy transient events. By correlating signals across these distinct cosmic messengers, we can precisely localize sources, probe the immediate environments of newly formed black holes and neutron stars, constrain their equations of state, and unravel the mechanisms of relativistic jet formation and particle acceleration. The synergistic operation of current and next-generation observatories, including advanced GW detectors and neutrino telescopes like IceCube-Gen2 and POEMMA, promises to revolutionize our understanding of the high-energy universe, offering unique insights into the origin of cosmic rays and the nature of matter under extreme conditions. This multi-messenger approach is crucial for addressing long-standing questions in astrophysics and cosmology. |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_17755290 |
| institution | Zenodo |
| language | |
| publishDate | 2025 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | The GW-Neutrino Window: Probing the Engines of the Extreme Universe Revista, Zen ASTRO, 10 Multi-messenger astronomy, leveraging gravitational waves (GWs) and high-energy neutrinos, opens an unparalleled "GW-Neutrino Window" into the most extreme astrophysical phenomena. This paper explores the profound potential of this emerging observational paradigm to decipher the fundamental physics governing the engines of the universe, such as merging compact objects, core-collapse supernovae, and active galactic nuclei. We review the current status of GW and neutrino detection, outlining the theoretical framework for their joint emission from high-energy transient events. By correlating signals across these distinct cosmic messengers, we can precisely localize sources, probe the immediate environments of newly formed black holes and neutron stars, constrain their equations of state, and unravel the mechanisms of relativistic jet formation and particle acceleration. The synergistic operation of current and next-generation observatories, including advanced GW detectors and neutrino telescopes like IceCube-Gen2 and POEMMA, promises to revolutionize our understanding of the high-energy universe, offering unique insights into the origin of cosmic rays and the nature of matter under extreme conditions. This multi-messenger approach is crucial for addressing long-standing questions in astrophysics and cosmology. |
| title | The GW-Neutrino Window: Probing the Engines of the Extreme Universe |
| url | https://doi.org/10.5281/zenodo.17755290 |