activity
20002024
most citedA lower limit of 50 microgauss for the magnetic field near the Galactic Centre

169 citations · 1k across the 24 of their papers we have counts for

collaborators

24 papers

astro-ph.HE2024★ 1 cited

Multimessenger observations and the science enabled: Continuous waves and their progenitors, equation of state of dense matter

D. I. Jones, K. Riles

Rotating and oscillating neutron stars can give rise to long-lived Continuous Gravitational Waves (CGWs). Despite many years of searching, the detection of such a CGW signal remain…

astro-ph.HE2022★ 13 cited

Measuring neutron-star distances and properties with gravitational-wave parallax

Magdalena Sieniawska, David Ian Jones, Andrew Lawrence Miller

Gravitational-wave astronomy allows us to study objects and events invisible to electromagnetic waves. So far, only signals triggered by coalescing binaries have been detected. How…

astro-ph.HE2022★ 13 cited

Precession of magnetars: dynamical evolutions and modulations on polarized electromagnetic waves

Yong Gao, Lijing Shao, Gregory Desvignes +3

Magnetars are conjectured to be highly magnetized neutron stars (NSs). Strong internal magnetic field and elasticity in the crust may deform the stars and lead to free precession.…

astro-ph.HE2022★ 39 cited

On the diversity of magnetar-driven kilonovae

Nikhil Sarin, Conor M. B. Omand, Ben Margalit +1

A non-negligible fraction of binary neutron star mergers are expected to form long-lived neutron star remnants, dramatically altering the multi-messenger signatures of a merger. He…

gr-qc2022★ 16 cited

Rotating Love: The dynamical tides of spinning Newtonian stars

Pantelis Pnigouras, Fabian Gittins, Amlan Nanda +2

We carefully develop the framework required to model the dynamical tidal response of a spinning neutron star in an inspiralling binary system, in the context of Newtonian gravity,…

astro-ph.HE2020★ 16 cited

Does elasticity stabilise a magnetic neutron star?

Prasanta Bera, D. I. Jones, Nils Andersson

The configuration of the magnetic field in the interior of a neutron star is mostly unknown from observations. Theoretical models of the interior magnetic field geometry tend to be…