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23 October 2019 | Story Valentino Ndaba | Photo Valentino Ndaba
Dr Patience book
From left: Prof Melanie Walker (SARChI Chair and Director of Higher Education and Human Development Research Group), Dr Patience Mukwambo (author of the monograph), and Dr Mikateko Hoppener, Senior Researcher in the group.

“A quality higher-education learning experience is a transformative experience for both students and lecturers who develop their minds in criticality, as well as social and self-identity, in addition to other skills and competencies.” This was the message from Dr Patience Mukwambo at the launch of her recently published book – ‘Quality in Higher Education as a Tool for Human Development: Enhancing Teaching and Learning in Zimbabwe’.

The book is a product of her doctoral research and was launched by the office of the SARChI Chair in Higher Education and Human Development, where Dr Mukwambo is a full-time researcher and was introduced at an event held at the Bloemfontein campus of the University of the Free State (UFS) on 21 October 2019. 

Depressing higher-education system

Dr Mukwambo was joined in conversation by Prof Brian Raftopoulos, a Mellon Senior Research Mentor in the Centre for Humanities Research at University of the Western Cape. 

Both scholars testified to the concept of critical thinking, alluding to the depressing state of education in Zimbabwe due to limitations posed by a non-expanding economy and a repressive political space. 

Prof Raftopoulos told the audience the idea of critical thinking has a long genealogy in radical thought which has deepened its roots in modern-day society. 

“What you have seen through the introduction of STEM (Science, Technology, Engineering, and Mathematics), is the increasing idea of functionalising education for a work economy. More often than not, you will hear the state saying it is up to school-leavers to create their own jobs,” said Prof Raftopoulos. According to Dr Mukwambo, part of the challenge is that “critical thinking is omitted on purpose and therefore universities lack a moral compass to work from”.

“While the broader economy might be constraining there are opportunities to develop critical thinking in the classroom, although it might not be uniform across all universities,” said Dr Mukwambo.

Equipping graduates with critical-thinking skills contributes to a range of benefits, such as improved wellbeing, economic outcomes, political engagement, and human capital formation. Quality in teaching and learning is therefore indeed a step in the right direction, towards social justice.


News Archive

UFS physicists publish in prestigious Nature journal
2017-10-16

Description: Boyden Observatory gravitational wave event Tags: Boyden Observatory, gravitational wave event, Dr Brian van Soelen, Hélène Szegedi, multi-wavelength astronomy 
Hélène Szegedi and Dr Brian van Soelen are scientists in the
Department of Physics at the University of the Free State.

Photo: Charl Devenish

In August 2017, the Boyden Observatory in Bloemfontein played a major role in obtaining optical observations of one of the biggest discoveries ever made in astrophysics: the detection of an electromagnetic counterpart to a gravitational wave event.
 
An article reporting on this discovery will appear in the prestigious science journal, Nature, in October 2017. Co-authors of the article, Dr Brian van Soelen and Hélène Szegedi, are from the Department of Physics at the University of the Free State (UFS). Both Dr Van Soelen and Szegedi are researching multi-wavelength astronomy.
 
Discovery is the beginning of a new epoch in astronomy
 
Dr van Soelen said: “These observations and this discovery are the beginning of a new epoch in astronomy. We are now able to not only undertake multi-wavelength observations over the whole electromagnetic spectrum (radio up to gamma-rays) but have now been able to observe the same source in both electromagnetic and gravitational waves.”
 
Until recently it was only possible to observe the universe using light obtained from astronomical sources. This all changed in February 2016 when LIGO (Laser Interferometer Gravitational-Wave Observatory) stated that for the first time they had detected gravitational waves on 14 September 2015 from the merger of two black holes. Since then, LIGO has announced the detection of two more such mergers. A fourth was just reported (27 September 2017), which was the first detected by both LIGO and Virgo. However, despite the huge amount of energy released in these processes, none of this is detectable as radiation in any part of the electromagnetic spectrum. Since the first LIGO detection astronomers have been searching for possible electromagnetic counterparts to gravitational wave detections. 
 
Large international collaboration of astronomers rushed to observe source
 
On 17 August 2017 LIGO and Virgo detected the first ever gravitational waves resulting from the merger of two neutron stars. Neutron star mergers produce massive explosions called kilonovae which will produce a specific electromagnetic signature. After the detection of the gravitational wave, telescopes around the world started searching for the optical counterpart, and it was discovered to be located in an elliptical galaxy, NGC4993, 130 million light years away. A large international collaboration of astronomers, including Dr Van Soelen and Szegedi, rushed to observe this source.
 
At the Boyden Observatory, Dr Van Soelen and Szegedi used the Boyden 1.5-m optical telescope to observe the source in the early evening, from 18 to 21 August. The observations obtained at Boyden Observatory, combined with observations from telescopes in Chile and Hawaii, confirmed that this was the first-ever detection of an electromagnetic counterpart to a gravitational wave event. Combined with the detection of gamma-rays with the Fermi-LAT telescope, this also confirms that neutron star mergers are responsible for short gamma-ray bursts.  
 
The results from these optical observations are reported in A kilonova as the electromagnetic counterpart to a gravitational-wave source published in Nature in October 2017.
 
“Our paper is one of a few that will be submitted by different groups that will report on this discovery, including a large LIGO-Virgo paper summarising all observations. The main results from our paper were obtained through the New Technology Telescope, the GROND system, and the Pan-STARRS system. The Boyden observations helped to obtain extra observations during the first 72 hours which showed that the light of the source decreased much quicker than was expected for supernova, classifying this source as a kilonova,” Dr Van Soelen said.

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