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A peek at the birth of the universe

July 24, 2019

The Square Kilometre Array (SKA) is set to become the largest radio telescope on Earth. Bielefeld University researchers together with the Max Planck Institute for Radio Astronomy (MPIfR) and international partners have now examined the SKA-MPG telescope--a prototype for the part of the SKA that receives signals in the mid-frequency range. The study, published today (24 July) in the journal Monthly Notices of the Royal Astronomical Society, shows that the telescope is not only a prototype to test the SKA design, but can also be used on its own to provide insights into the origin of the Universe. The German Federal Ministry of Education and Research (BMBF) is funding the work on the SKA-MPG through a joint research project coordinated by Bielefeld University.

'The SKA-MPG telescope in South Africa will help us to understand the cosmic background Radiation,' says Dr Aritra Basu, lead author of the study and physicist in Bielefeld University's Astroparticle Physics and Cosmology Working Group. The cosmic background radiation is light in the microwave range that was produced shortly after the Big Bang, and exploring it provides information about the origin of the Universe. 'However, measurements of the cosmic background radiation are distorted by other effects in the foreground, such as ultrafast electrons in the magnetic field of the Milky Way. In order to measure cosmic background radiation, we need to know more about these effects. Our study shows that the new telescope is excellent for investigating foreground radiation with ultra precision,' says Basu.

The SKA-MPG telescope was jointly developed by the Max Planck Institute for Radio Astronomy (MPIfR) in Bonn and MT-Mechatronics GmbH. The abbreviation 'MPG' stands for the Max Planck Society, which is funding the telescope. The radio telescope has a diameter of 15 metres and can receive signals between 1.7 and 3.5 GHz. It is currently being assembled in the South Africa's Karoo desert. Gundolf Wieching of the MPIfR, project leader of the telescope, expects first regular scientific use in autumn 2019.

The radio telescope is primarily designed as a prototype for a part of the SKA that receives signals from a medium radio frequency range. If the prototype performs well in a series of tests, around 200 such telescopes will be built for the SKA in South Africa. The SKA will observe medium as well as low radio frequencies. This second instrument will consist of thousands of small radio antennae that can be combined to simulate a huge radio telescope. The two parts of the SKA will then collect Signals over one square kilometre in Australia and South Africa--hence the name 'Square Kilometre Array'. 'Even with our prototype, we are able to look deep into the Universe thanks to a clever design for the telescope and new developments in receiver and backend technology,' says Dr Hans-Rainer Klöckner, astrophysicist at the MPIfR. 'I am curious to see what we will discover once 200 of these telescopes are synchronised for the SKA.' The SKA will be used, for example, to explore gravitational waves and dark energy, or to test Einstein's theory of relativity under extreme conditions.

The SKA will be the first global science organisation with locations on three continents: Australia, Africa, and Europe. In addition, data centres are being set up around the world. A special challenge lies in dealing with the enormous volume of data: the SKA will collect over 600 petabytes of observation data per year-- equivalent to the storage capacity of more than half a million laptops.

The German research institutions involved in the preparatory work for the SKA have joined forces in the 'German Long Wavelength Consortium', including Bielefeld University. The consortium's projects also include D-MeerKAT, in which the prototype SKA-MPG telescope is being evaluated--for example by the recently published study. The German Federal Ministry of Education and Research is funding D-MeerKAT as a joint research project. Professor Dr Dominik Schwarz, head of the Bielefeld Astroparticle Physics and Cosmology Working Group, coordinates D-MeerKAT. 'Our investigations with the SKA-MPG telescope are an important independent contribution to modern cosmology--with a lot of work and a bit of luck, we may be able to open a new window into understanding the Big Bang,' says Schwarz.
-end-
Original publication:

Aritra Basu, Dominik J. Schwarz, Hans-Rainer Klöckner, Sebastian von Hausegger, Michael Kramer, Gundolf Wieching, Blakesley Burkhart: CMB foreground measurements through broad-band radio spectro-polarimetry: prospects of the SKA-MPG telescope. MNRAS, https://doi.org/10.1093/mnras/stz1637, appeared on 24 July 2019. Reprint in arXiv: https://arxiv.org/pdf/1906.04788.pdf.

Further information is available online at:

* "Square Kilometre Array: The Cosmology Engine" (Press release published on 20/1/2015): https://ekvv.uni-bielefeld.de/blog/uninews/entry/square_kilometre_array_the_cosmology

* Website of the D-MeerKAT consortium: https://www.glowconsortium.de/index.php/en/meerkat-about/d-meerkat

* Website of the SKA project: https://www.skatelescope.org/

Bielefeld University

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