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Green-blue-brown cloud, in which the outlines of skyscrapers, a turbine, laboratory equipment and a network diagram of a human head with a torso can be seen © UA Ruhr
Cosmic Neutrino Detector

Hundreds of new ‘eyes’ buried in the Antarctic ice

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  • UA Ruhr
  • Research
Group photo of the IceCube consortium © Colton Hill​​​/​​IceCube NSF
A total of 51 scientists and technicians buried 670 new sensors and calibration devices in the Antarctic ice, including researchers from Ruhr University Bochum and TU Dortmund University.
Since 2009, researchers have been using the IceCube Neutrino Observatory at the South Pole to search for cosmic ray sources. Now, during the Antarctic summer, the team has taken advantage of the conditions to install an important upgrade. Fifty-one scientists and technicians successfully deployed 670 sensors and calibration devices in the Antarctic ice. These new components will significantly improve the detector’s capability at lower neutrino energies. Physicists from TU Dortmund University and Ruhr University Bochum were involved in the IceCube upgrade, and two TU researchers were present on site. The RAPP Center is a joint research initiative in astro-, particle and plasma physics, connecting scientists from the three universities in the Ruhr area.

The current upgrade is an important milestone on the path toward the future IceCube-Gen2 facility. It is expected to significantly increase sensitivity and open up new scientific opportunities. Researchers at TU Dortmund University are working closely with partners from Ruhr University Bochum in the IceCube consortium; the two universities are currently applying together as Ruhr Innovation Lab in the Excellence Strategy. A total of nine German universities and the two research institutes KIT and DESY are members of the consortium.

Hundreds of glass spheres 2,600 meters deep in the ice

The German partners have jointly contributed to the design, testing, and deployment of the new sensor technology. A pressure-resistant glass sphere, called a multi-PMT digital optical module (mDOM), houses multiple photomultiplier tubes (PMTs). These PMTs record the faint flashes of light produced when neutrinos occasionally interact with matter in the ice. The modules are deployed like pearls on a string: long cables carrying more than 100 devices were lowered into individual boreholes up to 2,600 meters deep. There, the ice serves as both the target and the detection medium for the ghostly cosmic particles. Alongside the new optical modules, the upgrade also included new calibration devices and cameras. These instruments provide controlled reference measurements and in-situ monitoring, which helps characterize the optical properties of the ice and the detector response under real operating conditions more accurately.

Participation of RAPP researchers

Around five thousand PMTs were tested and calibrated at TU Dortmund University as part of Johannes Werthebach’s Ph.D. thesis before being forwarded for integration and assembly into complete mDOMs. Scientists from Ruhr University Bochum contributed to improving the ice characterization through a new camera system. TU physicist Johannes Werthebach and Dr. Alicia Fattorini participated in the deployment at the South Pole. Werthebach worked specifically on the upgrade and supported critical installation steps, such as freezing the glass modules in the boreholes. Fattorini, an IceCube winterover, helped ensure the observatory's continuous year-round operation under extreme conditions.

Groundwork for the Future
Looking ahead, the newly installed calibration devices and camera systems will reduce systematic uncertainties and improve the reconstruction of neutrino events. These improvements will enhance future measurements and enable the improved reconstruction and reanalysis of the complete IceCube data set already collected. This will strengthen IceCube’s overall physics reach and lay important groundwork for the next-generation IceCube-Gen2 observatory.

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