Nuclear pasta
Top View
- Arxiv:2006.04963V3 [Nucl-Th] 29 Sep 2020 Believed to Occur in the Inner Cores of Very High Mass Neu- Verted Sphere) When Calculating the Neutrino Emissivity
- In Neutron Star Crusts
- A Density Functional Equation of State for Use in Astrophysical Phenomena
- Supernovae Neutrino-Pasta Interaction
- FRIB 400 Whitepaper
- Chuck Horowitz, Indiana U., First Compact Star Merger, ECT*, Oct. 2019 Neutron Rich Matter
- The State of Matter in Simulations of Core-Collapse Supernovae—Reflections and Recent Developments
- Neutron Stars
- An Introduction to Neutron Stars
- Nuclear Astrophysics in the Multimessenger Era: a Partnership Made in Heaven∗
- Study of Dense QCD Matter and Its Application to Physics of Compact Stars
- Study of Electron Gas on a Neutron-Rich Nuclear Pasta Enrique Ramirez-Homs University of Texas at El Paso, [email protected]
- Prospect of Experimental Nuclear Physics (In Japan) --Personal View
- Phases of Dense Matter in Compact Stars
- Evolution of Quasiperiodic Structures in a Non-Ideal Hydrodynamic Description of Phase Transitions
- Neutron Rich Matter and Neutron Star Crusts
- Crustal Cooling in the Neutron Star Low-Mass X-Ray Binary KS 1731−260 by Rachael L
- The Crusts of Accreting Neutron Stars 0.01 Edward Brown, Michigan State University 1