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Neutrinos are elementary particles that interact with other particles through the weak nuclear force, making them incredibly difficult to detect due to their extremely small mass and lack of electric charge. Despite their elusive nature, neutrinos play a pivotal role in astrophysics and cosmology. Modern research in high-energy astrophysics, astronomy, and cosmology reveals that neutrinos are integral to understanding a variety of fundamental processes, such as stellar explosions, the origin of cosmic rays, and the nature of dark matter. This article aims to explore the role of neutrinos in astrophysics, their impact on cosmic processes, and their significance for our understanding of the universe on large scales.
To investigate the role of neutrinos in astrophysics and cosmology, we employed theoretical physics approaches, numerical simulations, and observational data from neutrino detectors such as IceCube, Super-Kamiokande, and ANTARES, as well as data from cosmic telescopes. This research also draws upon cosmological data, particularly the cosmic microwave background (CMB), which provides insights into the early stages of the universe. Additionally, we examined the impact of neutrinos on processes like supernova explosions, cosmic ray propagation, and the potential link between neutrinos and dark matter. The methods of particle physics, along with computational models of astrophysical systems, were utilized to gain a comprehensive understanding of the role neutrinos play in the cosmos.
| Abstract Category | Astrophysics & Cosmology |
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