activity
19942023
most citedMesoscopic pinning forces in neutron star crusts

88 citations · 666 across the 28 of their papers we have counts for

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Showing astro-ph.HEShow all

16 papers · 1 filter

astro-ph.HE2023★ 23 cited

Insights into the physics of neutron star interiors from pulsar glitches

Marco Antonelli, Alessandro Montoli, Pierre Pizzochero

The presence of superfluid phases in the interior of a neutron star affects its dynamics, as neutrons can flow relative to the non-superfluid (normal) components of the star with l…

astro-ph.HE2022★ 11 cited

Continuous gravitational wave emission from neutron stars with pinned superfluids in the core

Brynmor Haskell, Marco Antonelli, Pierre Pizzochero

We investigate the effect of a pinned superfluid component on the gravitational wave emission of a rotating neutron star. Pinning of superfluid vortices to the flux-tubes in the ou…

astro-ph.HE2022★ 14 cited

Two decades of X-ray observations of the isolated neutron star RX J1856.5-3754: detection of thermal and non-thermal hard X-rays and refined spin-down measurement

Davide De Grandis, Michela Rigoselli, Sandro Mereghetti +6

The soft X-ray pulsar RX J1856.5-3754 is the brightest member of a small class of thermally-emitting, radio-silent, isolated neutron stars. Its X-ray spectrum is almost indistingui…

astro-ph.HE2020★ 10 cited

Statistical estimates of the pulsar glitch activity

Alessandro Montoli, Marco Antonelli, Brynmor Haskell +1

A common way to calculate the glitch activity of a pulsar is an ordinary linear regression of the observed cumulative glitch history. This method however is likely to underestimate…

astro-ph.HE2020★ 18 cited

Bayesian estimate of the superfluid moments of inertia from the 2016 glitch in the Vela pulsar

Alessandro Montoli, Marco Antonelli, Fabio Magistrelli +1

The observation of the first pulse-to-pulse glitch in the Vela pulsar opens a new window on the internal dynamics of neutron stars. We study the minimal three-component model for p…

astro-ph.HE2020★ 28 cited

A universal formula for the relativistic correction to the mutual friction coupling time-scale in neutron stars

Lorenzo Gavassino, Marco Antonelli, Pierre Pizzochero +1

Vortex-mediated mutual friction governs the coupling between the superfluid and normal components in neutron star interiors. By, for example, comparing precise timing observations…