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Secular effects of Ultralight Dark Matter on Binary Pulsars

Dark matter (DM) can consist of very light bosons behaving as a classical scalar field that experiences coherent oscillations. The presence of this DM field would perturb the dynamics of celestial bodies, either because the (oscillating) DM stress tensor modifies the gravitational potentials of the...

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Detalles Bibliográficos
Autores principales:	Blas, Diego, López Nacir, Diana, Sibiryakov, Sergey
Lenguaje:	eng
Publicado:	2019
Materias:	hep-ph Particle Physics - Phenomenology astro-ph.HE Astrophysics and Astronomy gr-qc General Relativity and Cosmology
Acceso en línea:	https://dx.doi.org/10.1103/PhysRevD.101.063016 http://cds.cern.ch/record/2695232

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