The SC-ETF method realizes orbital-free DFT for nuclear pasta by solving self-consistent Euler-Lagrange equations from a second-order ETF Skyrme functional, producing known and exotic 3D structures across inner-crust densities.
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4 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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2026 4verdicts
UNVERDICTED 4representative citing papers
Gross-Pitaevskii simulations show Josephson coupling creates a bound composite of one ^1S0 SQV and two ^3P2 HQVs that can depin from pinning sites.
Interband response enhances the neutron superfluid fraction in the crystalline crust, yielding effective ion masses close to the mass of quantum mechanically bound nucleons for realistic pairing gaps.
An effective two-band model of surface neutrons shows that nuclear spin-orbit coupling and density gradients at neutron-star pasta surfaces generate thermal spin polarization without magnetic fields.
citing papers explorer
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Three-dimensional orbital-free density functional theory description of nuclear pasta in the inner crust of neutron stars
The SC-ETF method realizes orbital-free DFT for nuclear pasta by solving self-consistent Euler-Lagrange equations from a second-order ETF Skyrme functional, producing known and exotic 3D structures across inner-crust densities.
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Formation of bound composite vortices of a singly-quantized $^1$S$_0$ vortex and half-quantized $^3$P$_2$ vortices in the $^1$S$_0$-$^3$P$_2$ coexisting phase in neutron stars
Gross-Pitaevskii simulations show Josephson coupling creates a bound composite of one ^1S0 SQV and two ^3P2 HQVs that can depin from pinning sites.
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Superfluid fraction and effective ion mass in the crystalline crust of a neutron star: role of interband response
Interband response enhances the neutron superfluid fraction in the crystalline crust, yielding effective ion masses close to the mass of quantum mechanically bound nucleons for realistic pairing gaps.
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Thermal Spin Polarization Driven by Nuclear Spin-Orbit Coupling in Neutron Star Pasta
An effective two-band model of surface neutrons shows that nuclear spin-orbit coupling and density gradients at neutron-star pasta surfaces generate thermal spin polarization without magnetic fields.