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Explore the theoretical formation mechanisms of sub-solar mass neutron stars within collapsar disk environments in this 15-minute conference talk. Examine how these exotic compact objects might form during the collapse of massive stars, focusing on the unique conditions within the accretion disks surrounding newly formed black holes. Learn about the physical processes that could lead to neutron star formation with masses below that of our Sun, challenging conventional understanding of stellar remnant mass distributions. Discover the implications of these theoretical models for gravitational wave astronomy, stellar evolution theory, and our broader understanding of compact object populations in the universe. Gain insights into cutting-edge research connecting stellar black hole lifecycles, massive star evolution, and the formation of unusual neutron star populations that could be detectable through future observational campaigns.
