From U Wisconsin IceCube Collaboration: “Looking for dark matter in the center of the Milky Way”

U Wisconsin ICECUBE neutrino detector at the South Pole

From U Wisconsin IceCube Collaboration

17 Mar 2020
Madeleine O’Keefe

We know very few things about dark matter: it makes up more than a quarter of all matter and energy in the universe; it clumps in specific pockets of space, like the centers of galaxies, including the Milky Way; and it has gravitational effects on the visible matter that surrounds it. Still, there are many things we want to learn, and since it has yet to be directly detected, scientists must find ways to study dark matter indirectly.

That’s where neutrinos might be able to help. These weakly interacting, nearly massless fundamental particles might be produced (according to some theories) when particles of dark matter annihilate with each other. If these theories are true, neutrino detectors—like the IceCube Neutrino Observatory at the South Pole and ANTARES in the Mediterranean Sea—can look for excess neutrinos coming from known dark matter hotspots. And if these sources produce more neutrinos than expected, it would support the theory that dark matter is connected to Standard Model particles.

So, the IceCube and ANTARES Collaborations recently probed one of these sources—the center of the Milky Way—by combining data from their respective neutrino telescopes. They did not find any unusual excesses of neutrinos, but they put stronger constraints on the dark matter annihilation cross-section averaged over the dark matter velocity. The results of the analysis are outlined in a paper submitted recently to Physical Review D.

This plot shows the upper limit on the thermally averaged self-annihilation cross section obtained by this combined analysis as a function of the dark matter mass for a specific annihilation channel and halo profile assumption. The limits from IceCube, ANTARES, VERITAS, Fermi-MAGIC, and HESS are also presented. Credit: IceCube and ANTARES Collaborations

Anteres Neutrino Telescope Underwater, a neutrino detector residing 2.5 km under the Mediterranean Sea off the coast of Toulon, France

CfA/VERITAS, a major ground-based gamma-ray observatory with an array of four Čerenkov Telescopes for gamma-ray astronomy in the GeV – TeV energy range. Located at Fred Lawrence Whipple Observatory,Mount Hopkins, Arizona, US in AZ, USA, Altitude 2,606 m (8,550 ft)

MAGIC Čerenkov telescopes at the Observatorio del Roque de los Muchachos (Garfia, La Palma, Spain)), Altitude 2,396 m (7,861 ft)

H.E.S.S. Čerenkov Telescope Array, located on the Cranz family farm, Göllschau, in Namibia, near the Gamsberg searches for cosmic rays, altitude, 1,800 m (5,900 ft)

The IceCube Neutrino Observatory is an array of 5,160 optical sensors buried in a cubic kilometer of ice beneath the South Pole. ANTARES (the Astronomy with a Neutrino Telescope and Abyss environmental RESearch project) is made up of 885 similar sensors installed underwater in the Mediterranean Sea off the coast of France. Both experiments detect light that is produced when neutrinos interact with a nucleus in the surrounding medium.

According to Nadège Iovine, an IceCube collaborator from Université Libre de Bruxelles and one of the leads on this analysis, the main motivation for this work was to improve the potential of detecting dark matter–produced neutrinos by combining datasets from the ANTARES and IceCube neutrino experiments. They specifically chose dark matter masses between 50 to 1000 GeV/c^2, a range for which each experiment had already independently obtained limits. The researchers also wanted to confirm that both experiments were operating under the same model assumptions and analysis methods.

So Iovine and her collaborators combined nine years of ANTARES data with three years of IceCube data. These datasets were from previous analyses carried out separately by each collaboration that were optimized for the search for dark matter in the Galactic Center. They then looked for neutrinos that could be produced by the annihilation of dark matter particles through various specific channels and under the assumptions of two different dark matter halo profiles.

They did not find evidence for dark matter; there were no excess neutrinos coming from the Galactic Center. Therefore, the researchers put limits on the dark matter annihilation cross section averaged over the speed of the particle—the thermally averaged dark matter self-annihilation cross section. The combined limits were improvements on the limits previously obtained by each experiment.

Ultimately, the analysis demonstrated the promising potential of combined analyses using datasets from both the ANTARES and IceCube neutrino telescopes. “This work brought to light the differences that can occur between two similar analyses and provides a benchmark for future combined analyses,” says Iovine.

Still, the hunt for dark matter is not over yet. Sebastian Baur, another IceCube scientist from Brussels, says, “With more years of data to come, a better understanding of the detector, and new statistical methods under development, we expect to further improve our results in the near future.”

See the full article here .


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IceCube is a particle detector at the South Pole that records the interactions of a nearly massless sub-atomic particle called the neutrino. IceCube searches for neutrinos from the most violent astrophysical sources: events like exploding stars, gamma ray bursts, and cataclysmic phenomena involving black holes and neutron stars. The IceCube telescope is a powerful tool to search for dark matter, and could reveal the new physical processes associated with the enigmatic origin of the highest energy particles in nature. In addition, exploring the background of neutrinos produced in the atmosphere, IceCube studies the neutrinos themselves; their energies far exceed those produced by accelerator beams. IceCube is the world’s largest neutrino detector, encompassing a cubic kilometer of ice.

IceCube employs more than 5000 detectors lowered on 86 strings into almost 100 holes in the Antarctic ice NSF B. Gudbjartsson, IceCube Collaboration

Lunar Icecube

IceCube DeepCore annotated

IceCube PINGU annotated

DM-Ice II at IceCube annotated