Neutron Star Physics studies the structure and behavior of neutron stars, which are among the densest known objects in the universe. Neutron stars contain matter compressed beyond atomic nuclei densities. Their interiors involve exotic states of matter governed by nuclear and particle physics. Neutron star physics explores equations of state, magnetic fields, and rotational dynamics. Observations include pulsars, magnetars, and gravitational wave signals from mergers. Neutron stars provide insight into strong interactions and relativistic gravity. Their study connects astrophysics with nuclear physics and quantum theory. Neutron star physics remains a rapidly evolving field driven by multimessenger astronomy.
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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
Title : How the Rad Lab helped avert nuclear war
Thomas F Ramos, Lawrence Livermore National Laboratory, United States
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Omar Mohammed Daud Shakarneh, Novosibirsk State University of Architecture and Civil Engineering, Russian Federation
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 : Enhanced ferromagnetism in carbon dots polyaniline nanocomposite
Paulo Cesar De Morais, University of Brasilia, Brazil