Binary pulsars as probes for spin-2 ultralight dark matter

DOI10.1088/1475-7516/2020/01/053zbMath1489.83026arXiv1909.13814OpenAlexW3098417525MaRDI QIDQ5067833

Diana López Nacir, Federico R. Urban, Juan Manuel Armaleo

Publication date: 4 April 2022

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

Full work available at URL: https://arxiv.org/abs/1909.13814

zbMATH Keywords

dark matter theorymillisecond pulsars

Mathematics Subject Classification ID

Oscillation, zeros of solutions, mean value theorems, etc. in context of PDEs (35B05) Two-body problems (70F05) Perturbations in context of PDEs (35B20) Galactic and stellar structure (85A15) Dark matter and dark energy (83C56) Bosonic systems in quantum theory (81V73)

Related Items

Pulsar timing array constraints on spin-2 ULDM ⋮ Pulsar timing residual induced by ultralight tensor dark matter ⋮ Towards a direct detection of the spin of dark matter ⋮ Cosmological gravitational particle production of massive spin-2 particles ⋮ Higher spin dark matter

Cites Work

• Vector fuzzy dark matter, fifth forces, and binary pulsars
• Gravity
• Binary and millisecond pulsars
• Partial masslessness of higher spins in (A)dS
• On partially massless bimetric gravity
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