collaborators

5 papers

astro-ph.HE2026

Magnetic field dynamics in isolated neutron stars with an external dipole field

Aurora Capobianco, William Cook, Sebastiano Bernuzzi +2

Neutron stars can harbor extremely strong magnetic fields, yet the structure and stability of their magnetic field configuration remain poorly understood. Observations of pulsars i…

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.HE2026

Superfluid He aerogel experiments as a laboratory neutron star analogue

Samuli Autti, Vanessa Graber, Brynmor Haskell

Neutron stars make a unique astrophysical test bench for our understanding of quantum physics at kilometre scales. The rotation of a neutron star features glitches, sudden spin-ups…

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

Gravitational pulsars: correlations between the electromagnetic and the continuous gravitational wave signal

Marco Antonelli, Avishek Basu, Brynmor Haskell

Neutron stars emitting continuous gravitational waves may be regarded as gravitational pulsars, in the sense that it could be possible to track the evolution of their rotational pe…