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A aron Brown was working as a CIA case officer in 2018 when he wrote a post for an agency blog warning about what he called ...

Neutron skin thickness in atomic nuclei is a fundamental property that provides critical insights into the equation of state (EOS) of infinite nuclear matter. This field has seen extensive ...

Fifty experts on nuclear physics, particle physics and astrophysics met at CERN from 9 to 13 June to discuss how to use ...

"This discovery heralds a broader understanding of the diversity in massive stars' deaths and a need for deeper investigations into the whole landscape of stellar evolution." ...

More information: Kota Hayashi et al, Jet from Binary Neutron Star Merger with Prompt Black Hole Formation, Physical Review Letters (2025). DOI: 10.1103/PhysRevLett.134.211407 ...

A computer simulation shows how two neutron stars of unequal mass merge, form a black hole and spit out a jet of high energy matter.

When white dwarfs—the hot remnants of stars like our sun—are orbited closely by another star, they sometimes steal mass away ...

Letter Published: 01 July 1968 Rotating Neutron Stars, Pulsars and Supernova Remnants F. PACINI Nature 219, 145–146 (1968) Cite this article ...