Page 3: 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.

Do the fastest-spinning pulsars contain quark matter?

Neutron stars are so named because in the simplest of models they are made of neutrons. They form when the core of a large star collapses, and the weight of gravity causes atoms to collapse. Electrons are squeezed together ...

Do we really know what becomes a Type Ia supernova?

Lots of things out in the universe can cause a supernova, from the gravitational collapse of a massive star, to the collision of white dwarfs. But most of the supernovae we observe are in other galaxies, too distant for us ...

Why are black holes stable against their own gravity?

Neutron stars are timelike matter with a maximum mass of about 2.34 solar masses in quantum chromodynamics (the strong color force). Black holes are spacelike matter that have no maximum mass, but a minimum mass of 2.35 solar ...

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