1996/05/28 by As. Abada, M. B. Gavela, M.B. Gavela +1 · 1 citation
Engineering · Physics and Astronomy · #Astrophysical Phenomena and Observations #Geophysics and Sensor Technology #Pulsars and Gravitational Waves Research #astro-ph #hep-ph
paper · pdf · doi:10.1016/0370-2693(96)01050-7
published as Phys.Lett. B387 (1996) 315-319 · 10 pages, Latex2e, two figures
arxiv created 1996/05/28 · openalex publication_date 1996/10/01 · arxiv updated 2009/11/30 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
Massless neutrinos are exchanged in a neutron star, leading to long range interactions. Many body forces of this type follow and we resum them. Their net contribution to the total energy is negligible as compared to the star mass. The stability of the star is not in danger, contrary to recent assertions.