PINNs are used to non-parametrically infer the neutron star EOS from NICER and pulsar data, producing M_max = 2.06 M_sun, R_1.4 = 12.85 km, and a reproducible speed-of-sound softening at 2-4 rho_0 consistent with quark-hadron crossover.
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7 Pith papers cite this work. Polarity classification is still indexing.
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A redefinition of the symmetry energy expansion that incorporates finite strangeness consistent with SU(3) flavor symmetry and remains valid beyond typical neutron-star central densities.
A first-principles FRG approach to two-flavor QCD derives low-energy constants for the pion, sigma-meson and scalar diquark without parameters beyond QCD itself, including new diquark properties for color-superconducting models.
Network analysis of Mathlib reveals 50.9% coupling between human taxonomies and logical dependencies, median 1.6% import usage by developers, and centrality driven by infrastructure rather than mathematical content.
A constrained evolutionary pipeline identifies over 14,000 causal EoS reconciling GW170817 and GW190814 with non-monotonic sound speeds, M_max 2.3-2.8 solar masses, and R_1.4 around 12 km.
DM admixture in isentropic neutron stars can mimic quark-matter conformality signatures via competition between thermal effects and dark sector softening.
The MUSES Calliope engine computes multi-dimensional QCD equations of state, merges them consistently, and feeds them into viscous hydrodynamic simulations of heavy-ion collisions with movable critical points and critical scaling in transport coefficients.
citing papers explorer
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Neutron Star Equation of State via Physics Informed Neural Network
PINNs are used to non-parametrically infer the neutron star EOS from NICER and pulsar data, producing M_max = 2.06 M_sun, R_1.4 = 12.85 km, and a reproducible speed-of-sound softening at 2-4 rho_0 consistent with quark-hadron crossover.
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Symmetry Energy Expansion with Strange Dense Matter
A redefinition of the symmetry energy expansion that incorporates finite strangeness consistent with SU(3) flavor symmetry and remains valid beyond typical neutron-star central densities.
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Scalar diquarks in the QCD vacuum
A first-principles FRG approach to two-flavor QCD derives low-energy constants for the pion, sigma-meson and scalar diquark without parameters beyond QCD itself, including new diquark properties for color-superconducting models.
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The Network Structure of Mathlib
Network analysis of Mathlib reveals 50.9% coupling between human taxonomies and logical dependencies, median 1.6% import usage by developers, and centrality driven by infrastructure rather than mathematical content.
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Reconciling GW170817 and GW190814 with a Nonmonotonic Sound-Speed Equation of State
A constrained evolutionary pipeline identifies over 14,000 causal EoS reconciling GW170817 and GW190814 with non-monotonic sound speeds, M_max 2.3-2.8 solar masses, and R_1.4 around 12 km.
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Observables and conformal properties of dark matter admixed isentropic neutron stars
DM admixture in isentropic neutron stars can mimic quark-matter conformality signatures via competition between thermal effects and dark sector softening.
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Studying the QCD Matter produced in Heavy-Ion Collisions using the MUSES Calculation Engine
The MUSES Calliope engine computes multi-dimensional QCD equations of state, merges them consistently, and feeds them into viscous hydrodynamic simulations of heavy-ion collisions with movable critical points and critical scaling in transport coefficients.