arXiv · hep-ph/9806433
Detecting supersymmetric Q-balls with neutron stars
Abstract
Supersymmetric Q-balls trapped in neutron stars or white dwarfs may cause the stars to explode. Trapping of Q-balls in neutron stars is shown to be less likely, but trapping in neutron star progenitors more likely than hitherto assumed, making neutron stars very sensitive Q-ball "detectors". White dwarfs only trap potentially dangerous Q-balls in a narrow parameter range.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Jes Madsen. 1998-06-22. Detecting supersymmetric Q-balls with neutron stars. https://doi.org/10.1016/s0370-2693(98)00789-8
Cite the original work for its findings. Save a collection to share your selection of sources.