Neutron Stars with Less Mass Than a White Dwarf Might Exist
SMRTR summary
Researchers are searching for small neutron stars below 1.4 solar masses using gravitational wave data. While no evidence was found, the study sets an upper limit of 2,000 observable mergers involving neutron stars up to 70% of the Sun's mass, potentially improving our understanding of neutron star physics.
SMRTR provides this summary for quick context. The original article belongs to Hacker News.
Read the original article