SEARCHING FOR keV STERILE NEUTRINO DARK MATTER WITH X-RAY MICROCALORIMETER SOUNDING ROCKETS
High-resolution X-ray spectrometers onboard suborbital sounding rockets can search for dark matter candidates that produce X-ray lines, such as decaying keV-scale sterile neutrinos. Even with exposure times and effective areas far smaller than XMM-Newton and Chandra observations, high-resolution, wi...
| Main Authors: | , , , , , , , , , , , |
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| Other Authors: | |
| Format: | Article |
| Language: | en_US |
| Published: |
IOP Publishing
2016
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| Online Access: | http://hdl.handle.net/1721.1/100732 https://orcid.org/0000-0002-3243-727X https://orcid.org/0000-0001-5268-8423 https://orcid.org/0000-0002-4435-4623 https://orcid.org/0000-0001-9285-5556 |
| Summary: | High-resolution X-ray spectrometers onboard suborbital sounding rockets can search for dark matter candidates that produce X-ray lines, such as decaying keV-scale sterile neutrinos. Even with exposure times and effective areas far smaller than XMM-Newton and Chandra observations, high-resolution, wide field of view observations with sounding rockets have competitive sensitivity to decaying sterile neutrinos. We analyze a subset of the 2011 observation by the X-ray Quantum Calorimeter instrument centered on Galactic coordinates l = 165°, b = -5° with an effective exposure of 106 s, obtaining a limit on the sterile neutrino mixing angle of sin[superscript 2] 2ϴ < 7.2 x 10[superscript -10] at 95% CL for a 7 keV neutrino. Better sensitivity at the level of sin[superscript 2] 2ϴ ~ 2.1 x 10[superscript -10] at 95% CL for a 7 keV neutrino is achievable with future 300-s observations of the galactic center by the Micro-X instrument, providing a definitive test of the sterile neutrino interpretation of the reported 3.56 keV excess from galaxy clusters. |
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