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16 October 2025 | Story Lacea Loader

The University of the Free State (UFS) Executive Committee (Exco), Institutional Representative Council (ISRC), and Campus Student Representative Councils (CSRCs) of the three campuses met on 15 October 2025 and reached an agreement regarding the implementation of the phasing out of provisional registration. 
The discussions were held in light of the decision made by the UFS Council on 26 September 2025 to phase out the provisional registration – a decision that led to the recent protest actions on the three campuses the past week. 

In a spirit of working towards a fairer, more equitable, and sustainable financial support system for all academically deserving students, Exco and the student leadership agreed that provisional registration will be phased out over a period of two years (2026-2027). This phased approach allows the university time to assess the risks students are facing with a view to assisting students. This means that from 1 January 2026, all students will be on a fully registered system. 

In recognition of the challenges students face, the outcomes of the meeting reflect the university’s ongoing commitment, and it ensures that all students are supported within a financially sustainable framework. It also reaffirms the university’s commitment to expanding access through enhanced financial support while sustaining the UFS as a national asset for future generations. 

The Exco remains committed to ongoing engagement with student leadership through open dialogue that reflects the university’s values, appreciates the constructive approach taken by the student leadership, and remains dedicated to working collaboratively in the best interest of all students and the broader university community.

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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