2007/11/15 by Irina Sagert, Sagert, Irina, Mirjam Wietoska +6
Earth and Planetary Sciences · Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Geophysics and Gravity Measurements #Nuclear Theory (nucl-th) #Nuclear physics research studies #Pulsars and Gravitational Waves Research #astro-ph #nucl-th
paper · pdf · doi:10.48550/arxiv.0711.2402
10 pages, 3 figures, talk given at the International Symposium on Exotic States of Nuclear Matter (EXOCT07), Catania, Italy, June 11-15, 2007
arxiv created 2007/11/15 · openalex publication_date 2007/11/15 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Recent astrophysical observations of neutron stars and heavy-ion data are confronted with our present understanding of the equation of state of dense hadronic matter. Emphasis is put on the possible role of the presence of hyperons in the interior of compact stars. We argue that data from low-mass pulsars provide an important cross-check between high-density astrophysics and heavy-ion physics.