arXiv · astro-ph/0605106
EXO 0748-676 Rules out Soft Equations of State for Neutron Star Matter
Abstract
The interiors of neutron stars contain matter at very high densities, in a state that differs greatly from those found in the early universe or achieved at terrestrial experiments. Matter in these conditions can only be probed through astrophysical observations that measure the mass and radius of neutron stars with sufficient precision. Here I report for the first time a unique determination of the mass and radius of the neutron star EXO 0748-676, which appears to rule out all the soft equations of state of neutron star matter. If this object is typical, then condensates and unconfined quarks do not exist in the centers of neutron stars.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
F. Ozel. 2006-05-03. EXO 0748-676 Rules out Soft Equations of State for Neutron Star Matter. https://doi.org/10.1038/nature04858
Cite the original work for its findings. Save a collection to share your selection of sources.