Gravitational Waves are ripples in spacetime generated by accelerating massive objects, such as merging black holes or neutron stars. Predicted by general relativity, gravitational waves propagate at the speed of light and carry information about their sources. Their detection provides a new way of observing the universe, independent of electromagnetic radiation. Gravitational wave astronomy has opened a new observational window into extreme astrophysical events. These waves encode information about strong gravitational fields and relativistic dynamics. Studying gravitational waves tests general relativity under extreme conditions. This field has rapidly advanced with the development of sensitive detectors. Gravitational waves represent a major breakthrough in modern physics and astrophysics.
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Vladimir Chigrinov, Hong Kong University of Science and Technology, Hong Kong
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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
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Amir Sohail, COMSATS University Islamabad, Pakistan
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Yarub Al Douri, European Academy of Sciences, Belgium
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Thomas J Webster, Brown University, United States