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04 April 2019 | Story Ruan Bruwer | Photo Varsity Cup
Lubabalo Dobela
Flyhalf Lubabalo Dobela will be an important cog in the wheel for the Shimlas against the Maties in the semi-final stage of the Varsity Cup. He has been named Player that Rocks twice this year.

The Shimlas (University of the Free State) will go into the semi-final against the unbeaten Maties with confidence, knowing that they can compete against them, said coach Hendro Scholtz.

The Shimlas will travel to Stellenbosch for the Varsity Cup clash on Monday (8 April). They qualified for the play-offs thanks to a 38-14 victory over the University of Johannesburg (UJ) in the final round of the competition on Monday 1 April 2019.

The Free State students lost to the Maties by 59-14 two weeks ago, and although the score reflects a big hiding, the Shimlas stood tall for most of the encounter.

“With 18 minutes remaining, we trailed by only ten points (14-24). We can gain confidence from that. We learned a couple of things about them. We will have to stop their driving mall and be sharp when it comes to our discipline. They will hurt us if we concede penalties,” said Scholtz.

According to him, it is important to get off to a good start. “You often sit with students who have other things to think about apart from rugby, such as upcoming tests, which can hamper their concentration. Against UJ in the wet, it was important to play the conditions right, and I think it made the players concentrate that little bit more.”

The Shimlas won four of their eight group matches and will look back on their defeats against the Pukke and Ixias as matches that they could easily have won on another day.

It is the fifth time in the 12 years of the Varsity Cup that the Shimlas have reached the final-four stage, with one win in 2015 over the Ikeys.

The Shimlas will be without two of their key men among the forwards – the injured flank Janco Cloete and hooker Hanno Snyman.

News Archive

Two scientists part of team that discovers the source of the highest energy cosmic rays at the centre of the Milky Way
2016-03-22

Description: Giant molecular clouds  Tags: Giant molecular clouds

Artist's impression of the giant molecular clouds surrounding the Galactic Centre, bombarded by very high energy protons accelerated in the vicinity of the central black hole and subsequently shining in gamma rays.
Artist's impression: © Dr Mark A. Garlick/ H.E.S.S. Collaboration

Spotlight photo:
Dr Brian van Soelen and Prof Pieter Meintjes of the UFS Department of Physics.
Photo: Charl Devenish

H.E.S.S. (High Energy Stereoscopic System) scientists publically revealed their latest galactic discovery in the international science journal, Nature, on 16 March 2016. These scientists were able to pinpoint the most powerful source of cosmic radiation – which, up to now, remained a mystery.

Part of this team of scientists are Prof Pieter Meintjes and Dr Brian van Soelen, both in the University of the Free State (UFS) Department of Physics. Dr Van Soelen explains that they have discovered a proton PeVatron – a source that can accelerate protons up to energies of ~1 PeV (10^15 eV) – at the centre of the Milky Way. The supermassive black hole called Sagittarius A has been identified as the most plausible source of this unprecedented acceleration of protons.

The protons are accelerated to Very High Energy (VHE) gamma rays. The energy of these protons are 100 times larger than those achieved by the Large Hadron Collider at CERN (the European Organization for Nuclear Research).

According to Dr Van Soelen, the fact that this research has been published in Nature demonstrates the importance and pioneering nature of the research conducted by H.E.S.S. The H.E.S.S. observatory – operational in Namibia – is a collaboration between 42 scientific institutions in 12 countries.

In 2006, H.E.S.S. was awarded the Descartes Prize of the European Commission – the highest recognition for collaborative research – and in 2010 the prestigious Rossi Prize of the American Astronomical Society. The extent of the observatory’s significance places it among the ranks of the Hubble Space Telescope and the telescopes of the European Southern Observatory in Chile.

“The next generation VHE gamma-ray telescope,” Dr Van Soelen says, “will be the Cherenkov Telescope Array (CTA), which is currently in the design and development stage.” Both Dr Van Soelen and Prof Meintjes are part of this project as well.

H.E.S.S. has issued a complete statement about the paper published in Nature.

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