Page 2: Research news on Gravitational collapse

Gravitational collapse as a research area investigates the nonlinear dynamical evolution of self-gravitating systems under general relativity and, where appropriate, Newtonian gravity, focusing on conditions under which matter configurations become unstable and contract to form compact objects or singularities. It encompasses analytical and numerical studies of stability thresholds, critical phenomena, horizon formation, equation-of-state dependence, and the role of angular momentum, radiation, and magnetic fields. The field also addresses cosmic censorship, gravitational-wave signatures, and the interplay between microphysical processes (e.g., nuclear and particle interactions) and macroscopic spacetime dynamics in contexts such as stellar core collapse, supernovae, and black hole formation.

Pulsars could have tiny mountains

Imagine a star so dense that a teaspoon of its material would weigh as much as Mount Everest, spinning hundreds of times per second while beaming radio waves across the universe. These are pulsars, the collapsed cores of ...

Webb reveals intricate layers of interstellar dust and gas

Once upon a time, the core of a massive star collapsed, creating a shockwave that blasted outward, ripping the star apart as it went. When the shockwave reached the star's surface, it punched through, generating a brief, ...

Neutron star 'mountains' would cause ripples in space-time

Collapsed dead stars, known as neutron stars, are a trillion times denser than lead, and their surface features are largely unknown. Nuclear theorists have explored mountain building mechanisms active on the moons and planets ...

Planets can form in even the harshest conditions

According to the most widely held astronomical model (the nebular hypothesis), new stars are born from massive clouds of dust and gas (aka a nebula) that experience gravitational collapse. The remaining dust and gas form ...

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