Evidence of Nuclear Urca Process in the Ocean of Neutron-Star Superburst MAXI J1752 - 457
astro-ph.HE, nucl-ex, nucl-th
Submitted: 2026-02-22
Updated: 2026-10-12
Sources
- Heating in the Accreted Neutron Star Ocean: Implications for Superburst Ignition
- Nuclear Reactions in the Crusts of Accreting Neutron Stars
- Urca Nuclide Production in Type-I X-ray Bursts and Implications for Nuclear Physics Studies
- The Thermal Evolution following a Superburst on an Accreting Neutron Star
- Long Type I X-ray Bursts and Neutron Star Interior Physics
- Long tails on thermonuclear X-ray bursts from neutron stars: a signature of inward heating?
- The cooling phase of Type-I X-ray bursts in 4U 1636-53
- The cooling rate of neutron stars after thermonuclear shell flashes
- Flux decay during thermonuclear X-ray bursts analysed with the dynamic power-law index method
- Model of heat diffusion in the outer crust of bursting neutron stars
- Superburst Models for Neutron Stars with Hydrogen and Helium-Rich Atmospheres
- A catalogue of unusually long thermonuclear bursts on neutron stars
- Models of Type I X-Ray Bursts in 4U 1820-30
- Impacts of the direct URCA and Superfluidity inside a Neutron Star on Type-I X-Ray Bursts and X-Ray Superbursts
- Constraining Accreted Neutron Star Crust Shallow Heating with the Inferred Depth of Carbon Ignition in X-ray Superbursts
- Thermonuclear superburst of MAXI J1752$-$457 observed with NinjaSat and MAXI
- Strong neutrino cooling by cycles of electron capture and $\beta^-$ decay in neutron star crusts
- A strong shallow heat source in the accreting neutron star MAXI J0556-332
- Urca cooling pairs in the neutron star ocean and their effect on superbursts
- Nuclear Physics of the Outer Layers of Accreting Neutron Stars
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