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astro-ph.SR2026
Temperature-resolved sensitivities of production to helium-burning reactions in pair-instability supernovae
Hiroki Kawashimo, Nobuya Nishimura, Yudai Suwa
We propose a temperature-resolved Monte Carlo (MC) approach to identify the temperature regimes in which low-energy helium-burning reaction rates most strongly affect nucleosynthes…
astro-ph.HE2026
Evidence of Nuclear Urca Process in the Ocean of Neutron-Star Superburst MAXI J1752457
Hao Huang, Akira Dohi, Amira Aoyama +2
We propose that the rapid cooling of the neutron star following its X-ray superburst in MAXI J1752457 over a period of 4 days, observed by two Japanese satellites, MAXI and Ninj…