Observational consistency and future predictions for a 3.5 keV ALP to photon line

Pedro D. Alvarez, Joseph P. Conlon, Francesca V. Day, M. C.David Marsh, Markus Rummel

Research output: Contribution to journalArticlepeer-review

15 Scopus citations

Abstract

Abstract Motivated by the possibility of explaining the 3.5 keV line through dark matter decaying to axion-like particles that subsequently convert to photons, we study ALP-photon conversion for sightlines passing within 50 pc of the galactic centre. Conversion depends on the galactic centre magnetic field which is highly uncertain. For fields at low or mid-range of observational estimates (10-100 μG), no observable signal is possible. For fields at the high range of observational estimates (a pervasive poloidal mG field over the central 150 pc) it is possible to generate sufficient signal to explain recent observations of a 3.5 keV line in the galactic centre. In this scenario, the galactic centre line signal comes predominantly from the region with z> 20 pc, reconciling the results from the Chandra and XMM-Newton X-ray telescopes. The dark matter to ALP to photon scenario also naturally predicts the non-observation of the 3.5 keV line in stacked galaxy spectra. We further explore predictions for the line flux in galaxies and suggest a set of galaxies that is optimised for observing the 3.5 keV line in this model.

Original languageEnglish
Article number013
JournalJournal of Cosmology and Astroparticle Physics
Volume2015
Issue number4
DOIs
StatePublished - 2015
Externally publishedYes

ASJC Scopus subject areas

  • Astronomy and Astrophysics

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