Dark Energy Models aim to explain the observed accelerated expansion of the universe. Dark energy is thought to comprise the majority of the universe’s energy content, yet its nature remains unknown. Models range from a cosmological constant to dynamic scalar fields that evolve over time. Some models attribute dark energy to vacuum energy, while others propose new fields or modifications to gravity. Dark energy models are constrained by astronomical observations such as supernova distances, cosmic microwave background measurements, and large-scale structure data. These models influence cosmic expansion history and the fate of the universe. Distinguishing between different dark energy models is one of the central challenges of modern cosmology. Understanding dark energy could fundamentally alter knowledge of spacetime, quantum physics, and gravity.
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