New research reveals that the mysterious masses of particles inside neutron stars could play a major role in determining how quickly these extreme cosmic objects lose their heat. Neutron stars are among the strangest and most extreme objects in the universe. Formed when massive stars collapse at the end of their lives, these incredibly dense objects pack more mass than the Sun into a sphere roughly the size of a city. Their interiors contain matter under extraordinary pressure and density, creating physical conditions that cannot be easily reproduced in laboratories on Earth. Although neutron stars are born extremely hot, they gradually lose their heat over time. Surprisingly, some neutron stars cool much faster than others. Scientists have been studying this difference for years, and new research suggests that the answer may lie in the unusual properties of particles inside these stellar objects. A study by researchers Sugiyama and Dohi has investigated how the effective masses of par...