Fermi data tantalize with new clues to dark matter

Apr 03, 2014 by Francis Reddy
At left is a map of gamma rays with energies between 1 and 3.16 GeV detected in the galactic center by Fermi's LAT; red indicates the greatest number. Prominent pulsars are labeled. Removing all known gamma-ray sources (right) reveals excess emission that may arise from dark matter annihilations. Credit: T. Linden, Univ. of Chicago

(Phys.org) —A new study of gamma-ray light from the center of our galaxy makes the strongest case to date that some of this emission may arise from dark matter, an unknown substance making up most of the material universe. Using publicly available data from NASA's Fermi Gamma-ray Space Telescope, independent scientists at the Fermi National Accelerator Laboratory (Fermilab), the Harvard-Smithsonian Center for Astrophysics (CfA), the Massachusetts Institute of Technology (MIT) and the University of Chicago have developed new maps showing that the galactic center produces more high-energy gamma rays than can be explained by known sources and that this excess emission is consistent with some forms of dark matter.

"The new maps allow us to analyze the excess and test whether more conventional explanations, such as the presence of undiscovered pulsars or cosmic-ray collisions on gas clouds, can account for it," said Dan Hooper, an astrophysicist at Fermilab in Batavia, Ill., and a lead author of the study. "The signal we find cannot be explained by currently proposed alternatives and is in close agreement with the predictions of very simple models."

The galactic center teems with gamma-ray sources, from interacting binary systems and isolated pulsars to supernova remnants and particles colliding with interstellar gas. It's also where astronomers expect to find the galaxy's highest density of dark matter, which only affects normal matter and radiation through its gravity. Large amounts of dark matter attract normal matter, forming a foundation upon which visible structures, like galaxies, are built.

No one knows the true nature of dark matter, but WIMPs, or Weakly Interacting Massive Particles, represent a leading class of candidates. Theorists have envisioned a wide range of WIMP types, some of which may either mutually annihilate or produce an intermediate, quickly decaying particle when they collide. Both of these pathways end with the production of gamma rays—the most energetic form of light—at energies within the detection range of Fermi's Large Area Telescope (LAT).

When astronomers carefully subtract all known gamma-ray sources from LAT observations of the galactic center, a patch of leftover emission remains. This excess appears most prominent at energies between 1 and 3 billion electron volts (GeV)—roughly a billion times greater than that of visible light—and extends outward at least 5,000 light-years from the galactic center.

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This animation zooms into an image of the Milky Way, shown in visible light, and superimposes a gamma-ray map of the galactic center from NASA's Fermi. Raw data transitions to a view with all known sources removed, revealing a gamma-ray excess hinting at the presence of dark matter. Credit: NASA Goddard; A. Mellinger, CMU; T. Linden, Univ. of Chicago

Hooper and his colleagues conclude that annihilations of with a mass between 31 and 40 GeV provide a remarkable fit for the excess based on its gamma-ray spectrum, its symmetry around the galactic center, and its overall brightness. Writing in a paper submitted to the journal Physical Review D, the researchers say that these features are difficult to reconcile with other explanations proposed so far, although they note that plausible alternatives not requiring dark matter may yet materialize.

"Dark matter in this mass range can be probed by direct detection and by the Large Hadron Collider (LHC), so if this is dark matter, we're already learning about its interactions from the lack of detection so far," said co-author Tracy Slatyer, a theoretical physicist at MIT in Cambridge, Mass. "This is a very exciting signal, and while the case is not yet closed, in the future we might well look back and say this was where we saw dark matter annihilation for the first time."

The researchers caution that it will take multiple sightings – in other astronomical objects, the LHC or in some of the direct-detection experiments now being conducted around the world—to validate their dark matter interpretation.

"Our case is very much a process-of-elimination argument. We made a list, scratched off things that didn't work, and ended up with dark matter," said co-author Douglas Finkbeiner, a professor of astronomy and physics at the CfA, also in Cambridge.

"This study is an example of innovative techniques applied to Fermi data by the science community," said Peter Michelson, a professor of physics at Stanford University in California and the LAT principal investigator. "The Fermi LAT Collaboration continues to examine the extraordinarily complex central region of the galaxy, but until this study is complete we can neither confirm nor refute this interesting analysis."

While the great amount of dark matter expected at the galactic center should produce a strong signal, competition from many other complicates any case for a detection. But turning the problem on its head provides another way to attack it. Instead of looking at the largest nearby collection of dark matter, look where the signal has fewer challenges.

Dwarf galaxies orbiting the Milky Way lack other types of gamma-ray emitters and contain large amounts of dark matter for their size – in fact, they're the most dark-matter-dominated sources known. But there's a tradeoff. Because they lie much farther away and contain much less total dark matter than the center of the Milky Way, dwarf galaxies produce a much weaker signal and require many years of observations to establish a secure detection.

For the past four years, the LAT team has been searching dwarf galaxies for hints of dark matter. The published results of these studies have set stringent limits on the mass ranges and interaction rates for many proposed WIMPs, even eliminating some models. In the study's most recent results, published in Physical Review D on Feb. 11, the Fermi team took note of a small but provocative gamma-ray excess.

"There's about a one-in-12 chance that what we're seeing in the dwarf galaxies is not even a signal at all, just a fluctuation in the gamma-ray background," explained Elliott Bloom, a member of the LAT Collaboration at the Kavli Institute for Particle Astrophysics and Cosmology, jointly located at the SLAC National Accelerator Laboratory and Stanford University. If it's real, the signal should grow stronger as Fermi acquires additional years of observations and as wide-field astronomical surveys discover new dwarfs. "If we ultimately see a significant signal," he added, "it could be a very strong confirmation of the dark matter signal claimed in the ."

Explore further: Possible evidence for dark matter particle presented

More information:Paper: "The characterization of the gamma-ray signal from the central Milky Way: A compelling case for annihilating dark matter"
' Paper: "Dark matter constraints from observations of 25 Milky Way satellite galaxies with the Fermi Large Area Telescope"

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zorro6204
not rated yet Apr 03, 2014
One thing I don't get from the Bullet cluster observations is why the gas became disconnected with the stars, and the stars stayed with the dark matter, which are by far the biggest contribution to mass, apparently. If the dark matter is concentrated at the center of galaxies, that helps explain how the gas got blown off, it would seem more difficult for that to happen if the dark matter was distributed like a cloud. On the other hand, it becomes more difficult to explain galactic rotation if the mass is concentrated, one would think the outer parts would be slower.

Or, there is no dark matter and these observations are an emergent phenomena of some deeper process that is associated with concentrated areas of "ordinary" mass.
osnova
Apr 03, 2014
This comment has been removed by a moderator.
barakn
5 / 5 (11) Apr 03, 2014
Zorro6204 - It's all about whether things collide or not. Dark matter doesn't collide with anything (except perhaps itself), and stars are so far apart that they are unlikely to collide with each other, and they are also pretty resistant to being blown around by radiation pressure. This means that once set on a trajectory, stars and dark matter are likely to keep on going. Gas, on the other hand...
zorro6204
5 / 5 (1) Apr 03, 2014
Yeah, I see your point. But even gas is very diffuse in space, and besides, why would collisions of such tiny particles completely displace the gas from the dark matter clump? I could see the larger dark matter assembly stealing gas from the other galaxy, but for the gas to go completely adrift from both centers of mass, that seems odd.
pandora4real
not rated yet Apr 03, 2014
When WIMPS collide... Could be a best seller.

Seriously, my photo hobby is imaging dwarf local group members and I'm interested in their anomalous concentration of dark matter (apparently). Doesn't that speak to the possibility of more physics existing in the black hole-dark matter interaction, i.e. once associated they stay associated. That would suggest the mechanism for gas distribution vis a vis dark matter and dark matter distribution vis a vis black holes may be two very different processes.

Which I think most the other comments could agree with.
zorro6204
not rated yet Apr 03, 2014
Maybe it's a field interaction, like the dark matter field becomes coupled to fields associated with ordinary matter, they get bound together, and perhaps the interaction is stronger at concentrations of mass, and maybe not in a linear fashion. Like the Higgs field, where it took a lot of energy to make the particle emerge and confirm the existence of the field, it could be very difficult to see that interaction. I don't know, we're missing a bunch of stuff, and I don't like it.
rah
1 / 5 (7) Apr 03, 2014
So, if I'm not mistaken, this is all fabricated crap.
osnova
Apr 05, 2014
This comment has been removed by a moderator.
IMP-9
5 / 5 (1) Apr 07, 2014
These gamma rays are produced with stellar binaries.


Where is your evidence to support the assertion that this can explain this spectral feature?
yyz
5 / 5 (2) Apr 07, 2014
"These gamma rays are produced with stellar binaries, which are more common near galactic center."

Gamma ray binaries are rare beasts in the Milky Way galaxy. As of 2013 only five GR binaries were known and (surprise surprise) they are not concentrated about the galactic center:

http://arxiv.org/abs/1307.7083

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