Dark Energy Models
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.
Thomas F Ramos
Lawrence Livermore National Laboratory, United States
Ephraim Suhir
Portland State University, United States
Alexander Unzicker
Pestalozzi Gymnasium Munchen, Germany
Thomas J Webster
Brown University, United States
Jon H Brasher
Stelleo Scientific Foundation, United States
Jason Liu
West Windsor-Plainsboro High School North, United States
Tom Lawrence
Ronin Institute of Independent Scholarship 2.0, United KingdomSubmit your abstract Today
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Vladimir Chigrinov, Hong Kong University of Science and Technology, Hong Kong
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Thomas J Webster, Brown University, United States
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Omar Mohammed Daud Shakarneh, Novosibirsk State University of Architecture and Civil Engineering, Russian Federation
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Alexei Krivolutsky, Central Aerological Observatory (CAO), Russian Federation
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Paulo Cesar De Morais, University of Brasilia, Brazil