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Nuclear pasta
Astromaterial Science and Nuclear Pasta
Phase Transitions and the Casimir Effect in Neutron Stars
Arxiv:1707.04966V3 [Astro-Ph.HE] 17 Dec 2017
The Nuclear Physics of Neutron Stars
Beyond Nuclear Pasta: Phase Transitions and Neutrino Opacity of Non-Traditional Pasta
Nuclear Pasta with a Touch of Quantum Towards Fully Antisymmetrised Dynamics for Bulk Fermion Systems
Defects in Nuclear Pasta David Reagan David
The Crust of Merging Neutron Stars
Unified Equation of State for Neutron Stars on a Microscopic Basis
Pasta-Phase Transitions in the Inner Crust of Neutron Stars∗
Neutron Stars from Crust to Core Within the Quark-Meson Coupling Model
Relativistic Density Functional Theory for Finite Nuclei and Neutron Stars
Neutron Stars
Supernovae • Types Ib, Ic: No H Lines Due to Shell Loss (Type Ia Already Discussed) Type II: Plenty of H Left (Standard End Stage of SG)
A Neutron Star Is Born
Nuclear Pasta in Supernovae and Neutron Stars
Neutron Stars' Hidden Nuclear Pasta
Nuclear Pasta Phases Within the Quark-Meson Coupling Model
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
Pdf/2015LRP/2015 LRPNS 091815.Pdf[23] C
Arxiv:1911.06334V2 [Hep-Ph] 20 Mar 2020
Molecular Dynamics Simulations of Nuclear Pasta
Inner Workings: Physicists Look to a New Telescope to Understand
A Brief Review of Nuclear Pasta Models and Theoretical Predictions