Urca process
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- Exotic Cooling on Neutron Stars with Different Surface Compositions
- Arxiv:1905.07308V1 [Astro-Ph.HE] 17 May 2019 Iiso H Asadrdu Fnurnsas Nlight in Stars
- A Moon-Sized, Highly Magnetised and Rapidly Rotating White Dwarf May Be
- Direct URCA Process in Neutron Stars with Strong Magnetic Fields
- Neutron Star Cooling Within the Equation of State with Induced Surface Tension
- Curriculum Vitae Anthony L
- In-Medium Enhancement of the Modified Urca Neutrino Reaction Rates
- Some Theoretical Aspects of Magnetars
- Determining the Nature of Super Fluidity and Superconductivity in Dense Matter from Neutron Star Observations
- The Great Wall: Urca Cooling Layers in the Accreted NS Crust
- From Early Convective Phases to Ignition: the Convective Urca Process
- Prospects for Multi-Messenger Extended Emission from Core-Collapse Supernovae in the Local Universe
- Astrophysical Constraints on Dense Matter in Neutron Stars
- The Structure of Compact Stars Spring 2017
- An Introduction to Neutron Stars
- Contents Contents
- Nuclear Pairing Gaps and Neutron Star Cooling
- Copyright by Michael Jaramillo 2020