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researcher

D. I. Jones

9 papers hereh-index 4270 citations7 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author2
  • last author4

Across the 8 of 9 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE4
  • astro-ph.SR3
  • astro-ph2
same name
  • D. I. Jones — 43 papers
  • D. I. Jones — 10 papers
  • D. I. Jones — 3 papers
  • D. I. Jones — 2 papers
  • D. I. Jones — 2 papers
  • D. I. Jones — 1 paper

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20002026
most citedGravitational waves from neutron stars: Promises and challenges

219 citations · 731 across the 9 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

4 papers · 1 filter

astro-ph.HE2026

Numerical calculations of neutron star mountains supported by crustal lattice pressure

T. J. Hutchins, D. I. Jones

Gravitational waves may set the spin frequencies of neutron stars in low-mass X-ray binaries (LMXBs). One mechanism for facilitating such emission is the formation of a mass asymme…

astro-ph.HE2024★ 1 cited

Crustal lattice pressure as a source of neutron star mountains

D. I. Jones, T. J. Hutchins

The spin frequencies of neutron stars in low-mass X-ray binaries may be limited by the emission of gravitational waves. A candidate for producing such steady emission is a mass asy…

astro-ph.HE2019★ 39 cited

Magnetar birth: rotation rates and gravitational-wave emission

S. K. Lander, D. I. Jones

Understanding the evolution of the angle χ between a magnetar's rotation and magnetic axes sheds light on the star's birth properties. This evolution is coupled with that of the…

astro-ph.HE2018★ 54 cited

Neutron-star spindown and magnetic inclination-angle evolution

S. K. Lander, D. I. Jones

A rotating fluid star, endowed with a magnetic field, can undergo a form of precessional motion: a sum of rigid-body free precession and a non-rigid response. On secular timescales…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.