Observability of dark matter substructure with pulsar timing correlations

DOI10.1088/1475-7516/2020/12/033zbMath1484.85024arXiv2005.03030OpenAlexW3021122280WikidataQ112669626 ScholiaQ112669626MaRDI QIDQ5027098

Kathryn M. Zurek, Tanner Trickle, Harikrishnan Ramani

Publication date: 3 February 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2005.03030

zbMATH Keywords

dark matter theoryparticle physics-cosmology connectionmillisecond pulsarsdark matter experiments

Mathematics Subject Classification ID

Measures of association (correlation, canonical correlation, etc.) (62H20) Black holes (83C57) Nuclear physics (81V35) Galactic and stellar structure (85A15) Dark matter and dark energy (83C56)

Related Items (3)

Pulsar timing array constraints on spin-2 ULDM ⋮ Dark photon stars: formation and role as dark matter substructure ⋮ The effects of relativistic hidden sector particles on the matter power spectrum

Cites Work

• Binary and millisecond pulsars

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