Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Probing The Longest Dark Matter Lifetimes with the Line Emission Mapper

Journal Article · · TBD
OSTI ID:2202852
 [1];  [2]
  1. Fermilab; Chicago U., KICP; Chicago U., Astron. Astrophys. Ctr.
  2. Fermilab; Chicago U., KICP
In the next decade, the proposed Line Emission Mapper (LEM) telescope concept is poised to revolutionize Galactic and extragalactic X-ray sensitivity. The instruments aboard LEM feature unprecedented eV scale energy resolution and an effective area of 1600 cm$^2$ at 0.5 keV. Such features are ideally suited to explore decaying dark matter candidates that predict X-ray signals, including axion-like particles and sterile neutrinos. We present the first forecast of LEM sensitivity to dark matter decays and find sensitivity to lifetimes beyond $$\sim 10^{32}$$ s in the keV range, surpassing current limits by several orders of magnitude. Notably, our results show that LEM will be the first ever instrument to probe such long dark matter lifetimes in any mass range for any decay channel.
Research Organization:
Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
DOE Contract Number:
AC02-07CH11359
OSTI ID:
2202852
Report Number(s):
FERMILAB-PUB-23-455-T; arXiv:2307.00041; oai:inspirehep.net:2673901
Journal Information:
TBD, Journal Name: TBD
Country of Publication:
United States
Language:
English

Similar Records

Line emission mapper microcalorimeter spectrometer
Journal Article · Wed Oct 18 20:00:00 EDT 2023 · Journal of Astronomical Telescopes, Instruments, and Systems · OSTI ID:2349606

Development of the microcalorimeter and anticoincidence detector for the Line Emission Mapper x-ray probe
Journal Article · Tue Oct 17 20:00:00 EDT 2023 · Journal of Astronomical Telescopes, Instruments, and Systems · OSTI ID:2403637

Hidden axion dark matter decaying through mixing with QCD axion and the 3.5 keV X-ray line
Journal Article · Sun Nov 30 23:00:00 EST 2014 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22382098