Inside Neutron Stars: Mapping the Boundary Between Matter and the Unknown

New research combines theoretical models with astronomical observations to refine our understanding of the extreme conditions within neutron stars and the elusive transition between hadronic and quark matter.




![The study demonstrates that magnetic field-dependent spectroscopic measurements, combined with a third-order perturbative scattering model and Schrieffer-Wolff transformation, reveal a renormalized [latex]\mathcal{J}_{\pm}[/latex] value of approximately 0.62, accurately capturing the complex interplay between the overscreened Kondo peak, the ferromagnetic Kondo dip, and the effective magnetic field-a result confirmed by a minimized [latex]\chi^{2}[/latex] of 0.23 under conditions of 54mK sample temperature, -20mV bias voltage, and 1nA current-thereby establishing a refined understanding of Kondo physics in these systems.](https://arxiv.org/html/2604.07174v1/Figure_3.png)
![The study demonstrates a quantifiable relationship between entanglement entropy and lattice information in [latex] B=0 [/latex] meson-meson and [latex] B=1 [/latex] meson-baryon scattering, suggesting a fundamental connection between these properties in particle interactions.](https://arxiv.org/html/2604.06716v1/baryons2025_proceeding_v2.jpg)