“The Missing Photons” –Predicted Dark Matter Signal Fails

Hubble Dark Matter


The planet’s frustrating dark-matter quest continues. An unidentified X-ray signature recently observed in nearby galaxies and galaxy clusters is not due to decay of dark matter, researchers report. The findings rule out previously proposed interpretations of dark matter particle physics.

Despite its cosmological abundance and the well-established astrophysical evidence of its existence, little about the mysterious material is known, including which subatomic particles make up dark matter. Some models of potential dark matter predict that they might slowly decay into ordinary matter. If so, the process of dark matter decay would produce faint photon emissions detectable by X-ray telescopes.

Is Dark Matter Only the Tip of an Invisible Universe of Unknown Forces?

Recent X-ray observations of nearby galaxy clusters have detected an unidentified X-ray emission line at 3.5 kiloelectronvolts (keV), which has been interpreted by some as a signature of dark matter decay – particularly a hypothetical dark matter particle known as the sterile neutrino. If this is correct, dark matter surrounding our Galaxy should decay and produce a similar X-ray emission line, spread faintly across the entire night sky.

“I Couldn’t Believe My Eyes”–A Strange Signal from One of the Largest Objects in the Cosmos

Christopher Dessert and colleagues searched for the 3.5 keV signal within the ambient halo of the Milky Way using data from the European Space Agency’s XMM-Newton space telescope. Dessert and colleagues analyzed blank-sky observations (parts of the sky away from large X-ray emitting regions) with a total exposure time of roughly a year, finding no evidence for the predicted 3.5 KeV line. According to the authors, the findings rule out the predicted signal strength by over an order of magnitude.

The Daily Galaxy, Max Goldberg, via Science/AAAS 

Image credit: Data gathered by the Hubble Space Telescope creates a map of dark matter.
(© NASA/ESA/Caltech)

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