Neutrino detection is an area of research that focuses on the identification and measurement of neutrinos, which are subatomic particles that have very little mass and no electric charge. Neutrinos are produced in various astrophysical processes, such as nuclear reactions in the Sun, supernovae explosions, and high-energy cosmic ray interactions. Detection of neutrinos is challenging because they interact very weakly with matter, making them difficult to detect. Various detection techniques are used, including scintillation detectors, water Cherenkov detectors, and radio detectors. Neutrino detection plays a crucial role in studying fundamental properties of neutrinos, as well as in astrophysics and particle physics research.