collaborators

5 papers

astro-ph.HE2026

Probing Neutron Star Interiors and the Properties of Cold Ultra-dense Matter with the SKAO

Avishek Basu, Vanessa Graber, Marcus E. Lower +19

Matter inside neutron stars is compressed to densities several times greater than nuclear saturation density, while maintaining low temperatures and large asymmetries between neutr…

astro-ph.HE2025

Probing neutron star interiors and the properties of cold ultra-dense matter with the SKAO

Avishek Basu, Vanessa Graber, Marcus E. Lower +19

Matter inside neutron stars is compressed to densities several times greater than nuclear saturation density, while maintaining low temperatures and large asymmetries between neutr…

astro-ph.HE2025

PSR J0537-6910: Exponential recoveries detected for 12 glitches

E. Zubieta, C. M. Espinoza, D. Antonopoulou +4

Pulsar glitches are unresolved increments of the rotation rate that sometimes trigger an enhancement of the spin-down rate. On occasions, the augmented spin-down decays gradually i…

astro-ph.HE2025

Braking index of the frequently glitching PSR J05376910

Erbil Gügercinoğlu, Onur Akbal, M. Ali Alpar +2

The pulsar J05376910 undergoes spin-up glitches more frequently than any other known pulsar, at a rate of roughly thrice per year. Its glitches are typically large and accompani…

astro-ph.HE2025

Signatures of magnetic flux expulsion from neutron star cores

S. K. Lander, K. N. Gourgouliatos, Z. Wadiasingh +1

Shortly after a neutron star is born, the protons in its core begin to form a superconductor. In terrestrial materials, the hallmark of superconductivity is an associated expulsion…