Kathy Romer 38-Published-27.06.20.pdf (2.34 MB)
The XMM Cluster Survey: new evidence for the 3.5-keV feature in clusters is inconsistent with a dark matter origin
journal contribution
posted on 2023-06-07, 07:40 authored by Sunayana Bhargava, Paul GilesPaul Giles, Kathy RomerKathy Romer, T Jeltema, Julian Mayers, Alberto Bermeo, M Hilton, Reese WilkinsonReese Wilkinson, Carlos Fernando Vergara Cervantes, C A Collins, M Manolopoulou, Philip Rooney, S Rosborough, K Sabirli, J P Stott, E Swann, P T P VianaThere have been several reports of a detection of an unexplained excess of X-ray emission at ?3.5 keV in astrophysical systems. One interpretation of this excess is the decay of sterile neutrino dark matter. The most influential study to date analysed 73 clusters observed by the XMM–Newton satellite. We explore evidence for a ?3.5-keV excess in the XMM-PN spectra of 117 redMaPPer galaxy clusters (0.1 < z < 0.6). In our analysis of individual spectra, we identify three systems with an excess of flux at ?3.5 keV. In one case (XCS J0003.3+0204), this excess may result from a discrete emission line. None of these systems are the most dark matter dominated in our sample. We group the remaining 114 clusters into four temperature (TX) bins to search for an increase in ?3.5-keV flux excess with TX – a reliable tracer of halo mass. However, we do not find evidence of a significant excess in flux at ?3.5 keV in any TX bins. To maximize sensitivity to a potentially weak dark matter decay feature at ?3.5 keV, we jointly fit 114 clusters. Again, no significant excess is found at ?3.5 keV. We estimate the upper limit of an undetected emission line at ?3.5 keV to be 2.41 × 10-6 photons cm-2 s-1, corresponding to a mixing angle of sin?2(2?) = 4.4 × 10-11, lower than previous estimates from cluster studies. We conclude that a flux excess at ?3.5 keV is not a ubiquitous feature in clusters and therefore unlikely to originate from sterile neutrino dark matter decay.
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- Published
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- Published version
Journal
Monthly Notices of the Royal Astronomical SocietyISSN
0035-8711Publisher
Oxford University PressExternal DOI
Issue
1Volume
497Page range
656-671Pages
15.0Department affiliated with
- Physics and Astronomy Publications
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- Yes
Peer reviewed?
- Yes
Legacy Posted Date
2020-08-04First Open Access (FOA) Date
2020-08-04First Compliant Deposit (FCD) Date
2020-08-03Usage metrics
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