Cosmic Rays are high-energy particles originating from outer space that strike Earth’s atmosphere. They consist mainly of protons, atomic nuclei, and a small fraction of electrons and antiparticles. Cosmic rays are produced by energetic astrophysical processes such as supernova explosions and active galactic nuclei. Studying cosmic rays provides insight into particle acceleration mechanisms and extreme environments in the universe. When cosmic rays interact with the atmosphere, they generate cascades of secondary particles. Detection methods include ground-based detectors and satellite experiments. Cosmic ray research connects astrophysics, particle physics, and atmospheric science. It also helps probe fundamental interactions at energies beyond current accelerators.
Title : Photoaligned azodye nanolayers: New trends for liquid crystal devices
Vladimir Chigrinov, Hong Kong University of Science and Technology, Hong Kong
Title : Where is modern physics heading? Why constants of nature matter
Alexander Unzicker, Pestalozzi Gymnasium Munchen, Germany
Title : Global photochemical model CHARM-DE of the earth’s atmosphere for altitudes 0-130 km
Alexei Krivolutsky, Central Aerological Observatory (CAO), Russian Federation
Title : Nonlinear plasma wave excitation in cylindrical semiconductor waveguides
Amir Sohail, COMSATS University Islamabad, Pakistan
Title : Characterization of quaternary alloy
Yarub Al Douri, European Academy of Sciences, Belgium
Title : Using physics to eliminate implant infection in over 25000 patients to date
Thomas J Webster, Brown University, United States