Simulated
Milky Way Galaxy. Credit: AIP/ A. Khalatyan
New
research shows that dark matter has a different distribution in our galaxy than
previously thought, and that advances dark matter's status as a potential
source of the observed gamma ray excess in the Milky Way's center.
High-resolution simulations reveal that the dark matter distribution in the
inner galaxy is not spherical, but flattened and asymmetrical. The findings
confirm the theory that the gamma ray excess is due to dark matter
annihilation.
Scientists have long suspected dark matter annihilation to be a source of these rays, but the rays'
spatial spread did not match the arrangement of dark matter they had predicted.
Another theory argues that ancient millisecond pulsars could produce the rays.
For
the new study published in Physical Review Letters, researchers modeled
the formation of Milky Way-like galaxies under environmental conditions similar
to those of Earth's cosmic neighborhood, thereby reproducing simulated Milky
Way-like galaxies that bear strong resemblance to the real thing.
They
found that dark matter does not radiate outwards from the Galactic Center but
is instead organized similar to that of stars, meaning the former could just as
equally have produced the excess gamma rays.
"When
the FERMI space telescope pointed to the galactic center, the results were startling. The
telescope measured too many gamma rays, the most energetic kind of light in the
universe. Astronomers around the world were puzzled, and competing theories
started pouring in to explain the so-called 'gamma ray excess,'" states
Noam Libeskind from the Leibniz Institute for Astrophysics Potsdam (AIP).
After
much debate, two ideas rose to the fore: either these gamma rays were the
result of millisecond pulsars (ultra-dense neutron stars that spin thousands of
times per second) or from dark matter particles smashing into each other and
annihilating. Both theories have their drawbacks. However, the new results
offered by scientists at the AIP collaborating with the Hebrew University in
Israel and Johns Hopkins University in the U.S. have shed new light on this
problem, effectively confirming the theory that the gamma ray excess is due to
dark matter annihilation.
The
Milky Way galaxy has long been known to live in a so-called dark matter halo, a
spherical region filled with dark matter around it. However, the extent to
which this halo is aspherical or ellipsoidal has not been appreciated.
Moorits Muru, lead author of the paper, says, "We analyzed simulations of the Milky Way and its dark matter halo and found that the flattening of this region is sufficient to explain the gamma ray excess as being due to dark matter particles self-annihilating. These calculations demonstrate that the hunt for dark matter particles (that can self-annihilate) should be encouraged and bring us one step closer to understanding the mysterious nature of these particles."
Source: Milky Way shows gamma ray excess due to dark matter annihilation, study suggests

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