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21 July 2020 | Story Nitha Ramnath | Photo UFS photo archive

The Department of Business Management within the Faculty of Economic and Management Sciences is one of four successful recipients of the Nurturing Emerging Scholars Programme (NESP), which aims to recruit honours graduates who demonstrate academic ability and express an early interest in the possibility of an academic career. 

 “The NESP is a mechanism that addresses a potential shortcoming in the department in the medium to long term. Most of the academics in the department specialise either in entrepreneurship or marketing. As such, the availability of academics with interdisciplinary business knowledge who can teach and do research across the different sub-fields of business management is limited,” says Prof Brownhilder Neneh, Associate Professor in the Department of Business Management.

Once graduates enter the programme – as NESP master’s graduates they form part of a resource pool from which new academics can be recruited. 

Prof Neneh continues: “Considering the imminent retirement of academics in the department, the NESP provides an opportunity to recruit an academic who is able to work with experienced academics, gain experience, and ‘prepare’ the person to become an expert across the different fields in the department.”

“This programme would assist in succession planning within the department as well as training individuals within academia,” she says. 

According to Prof Neneh, access to this funding opportunity will further strengthen and expand the path that the department has embarked upon as far as striving for excellence in teaching, research, and community engagement is concerned, thereby contributing to address key societal challenges. “Appointing an NESP candidate would be an ideal opportunity to recruit an academic who will be able to work with the senior staff and gain experience and teaching/research competencies relevant to the 4IR, and ‘prepare’ the person to become the business management expert in the department,” she says.

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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