Tuesday, March 10, 2015
Unexpected Gamma-Ray Emission From Dwarf Galaxy May Point to New Understanding of Dark Matter
A newly discovered dwarf galaxy orbiting our own Milky Way has offered up a surprise — it appears to be radiating gamma rays, according to an analysis by physicists at Carnegie Mellon, Brown and Cambridge universities. The exact source of this high-energy light is uncertain at this point, but it just might be a signal of dark matter lurking at the galaxy’s center.
“Something in the direction of this dwarf galaxy is emitting gamma rays. There’s no conventional reason this galaxy should be giving off gamma rays, so it’s potentially a signal for dark matter,” said Alex Geringer-Sameth, a postdoctoral research associate in CMU’s Department of Physics and the paper’s lead author.
The galaxy, named Reticulum 2, was discovered within the past few weeks in the data of the Dark Energy Survey, an experiment that maps the southern sky in the hope of understanding the accelerated expansion of the universe. At approximately 98,000 light-years from Earth, Reticulum 2 is one of the nearest dwarf galaxies yet detected. Using publicly available data from NASA’s Fermi Gamma-ray Space Telescope, Carnegie Mellon’s Geringer-Sameth and Matthew Walker, and Brown’s Savvas Koushiappas have shown gamma rays coming from the direction of the galaxy in excess of what would be expected from normal background.
“In the search for dark matter, gamma rays from a dwarf galaxy have long been considered a very strong signature,” said Koushiappas, an assistant professor of physics at Brown. “It seems like we may now be detecting such a thing for the first time.”
The researchers have submitted their analysis to the journal Physical Review Letters, and posted it on arXiv [arXiv:1503.02320]. They caution that while these preliminary results are exciting, there’s more work to be done to confirm a dark matter origin.
No one knows exactly what dark matter is, but it is thought to account for around 80 percent of the matter in the universe. Scientists know that dark matter exists because it exerts gravitational effects on visible matter, which explains the observed rotation of galaxies and galaxy clusters as well as the fluctuations in the cosmic microwave background.
“The gravitational detection of dark matter tells you very little about the particle behavior of the dark matter,” said Walker, assistant professor of physics and a member of CMU’s McWilliams Center for Cosmology. “But now we may have a non-gravitational detection that shows dark matter behaving like a particle, which is a holy grail of sorts.”
A leading theory suggests that dark matter particles are WIMPs, or Weakly Interacting Massive Particles. When pairs of WIMPs meet, they annihilate one another, giving off high-energy gamma rays. If that’s true, then there should be a lot of gamma rays emanating from places where WIMPs are thought to be plentiful, like the dense centers of galaxies. The trouble is, the high-energy rays also originate from many other sources, including black holes and pulsars, which makes it difficult to untangle a dark matter signal from the background noise.
That’s why dwarf galaxies are important in the hunt for the dark matter particle. Dwarfs are thought to lack other gamma-ray-producing sources, so a gamma ray flux from a dwarf galaxy would make a very strong case for dark matter.
“They’re basically very clean and quiet systems,” Koushiappas said.
Scientists have been looking at them for signs of gamma rays for the last several years using NASA’s Fermi Gamma-ray Space Telescope. There’s never been a convincing signal, until now.
Over the past few years Geringer-Sameth, Koushiappas and Walker have been developing an analysis technique that searches for weak signals in the gamma ray data that could be due to dark matter annihilation. With the discovery of Reticulum 2, Geringer-Sameth turned his attention to that part of the sky. He looked at all of the gamma rays coming from the direction of the dwarf galaxy as well as gamma rays coming from adjacent areas of the sky to provide a background level.
“There did seem to be an excess of gamma rays, above what you would expect from normal background processes, coming from the direction of this galaxy,” Geringer-Sameth said. “Given the way that we think we understand how gamma rays are generated in this region of the sky, it doesn’t seem that those processes can explain this signal.”
Further study of this dwarf galaxy’s attributes could reveal hidden sources that may be emitting gamma rays, but the researchers are cautiously optimistic.
“The fact that there are gamma rays and also a clump of dark matter in the same direction makes it quite interesting,” Walker said.
The above image represents a region of the sky surrounding the newly discovered dwarf galaxy Reticulum 2. The brightness in the center indicates a strong gamma-ray signal coming from the direction of Reticulum 2. The image was generated using the authors’ search algorithm applied to Fermi gamma-ray data.
Image Credit: NASA/DOE/Fermi-LAT Collaboration/Geringer-Sameth & Walker/Carnegie-Mellon University/Koushiappas/Brown University