Neutrino Astronomy and Neutrino Oscillations:
Investigating neutrinos from cosmic sources like supernovae and understanding neutrino oscillations, shedding light on their masses and mixing angles, providing crucial insights into the universe's most energetic processes.
Dark Matter and Dark Energy Studies:
Exploring the nature of dark matter, its distribution in the universe, and the mysterious dark energy that drives the accelerated expansion of the cosmos, aiming to decipher their roles in shaping the universe's large-scale structure.
Gamma-Ray Astronomy and High-Energy Photon Detection:
Studying gamma-ray bursts, pulsars, and active galactic nuclei using high-energy photon detectors, unraveling the extreme astrophysical environments and cosmic particle acceleration mechanisms.
Cosmic Ray Research and Ultra-High-Energy Particles:
Investigating the origins of cosmic rays, their acceleration mechanisms, and detecting ultra-high-energy particles, providing insights into the most energetic astrophysical events and their impact on the universe.
Astrophysical Neutrino Telescopes and Multimessenger Astronomy:
Developing neutrino telescopes to detect astrophysical neutrinos and combining these observations with electromagnetic and gravitational wave signals
enabling a comprehensive understanding of cosmic events such as supernovae, gamma-ray bursts, and neutron star mergers.