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06 February 2020 | Story Lacea Loader

During meetings between the management of the University of the Free State (UFS) and the Bloemfontein Campus Student Representative Council (CSRC) the week of 27 January 2020, an agreement regarding accredited and non-accredited accommodation was reached. Although it has been communicated to students on the university’s campuses earlier this week, it is important to clarify the agreement: 

• For 2020, students on the three campuses of the UFS who receive funding from the National Student Financial Aid Scheme (NSFAS) and who live in accredited and non-accredited accommodation, will receive the monthly accommodation allowance that will be paid directly into the student’s bank account.  Please note that the matter of the lease agreement is between the student and the service provider and the UFS does not take responsibility for payments to any supplier. The payments will only be made once funds are received from NSFAS.  

• Registered NSFAS beneficiaries must log in on Self Service and apply online for the private accommodation allowance. The application process requires that the lease agreement should be uploaded on the Self-Service portal. This lease agreement must be signed by both the student and the service provider. 

• Approved private accommodation applicants will receive their private accommodation allowance payment during the first week of each month for a period of 10 months, depending on the date of approval and the rental period.

• If the service provider does not have a lease agreement, students can download a basic lease agreement form here. This form must be signed by the student and the service provider.

• A process will be in place to verify the accommodation during 2020, as required by the Department of Higher Education, Science and Technology (DHET).  This process will start with the completion of the application form for accreditation by the service provider.  The application form can be obtained here.



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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