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12 May 2020 | Story Prof Francis Petersen | Photo Sonia Small
Prof Francis Petersen.

In a rapidly changing, uncertain and complex world, the role that universities are playing as the engines of social mobility, as drivers of the economy and as generators of new ideas, is now more critical than ever.  Due to the universal nature of knowledge, universities are global in scope – a space that encourages new ideas, controversy, inquiry, and argument and challenges orthodox views, but they are also deeply entrenched in their local environment, influenced by socio-economic and political dynamics.  There is an expectation that universities should exhibit great levels of responsiveness and public accountability, with higher levels of trust in higher education, and between higher education and government, and higher education and the public.  The challenge for both higher education and government is to allow institutional autonomy without oppressive accountability.  

Over the past few years, the purpose of universities has been challenged in relation to their role in society, their advocacy for speaking truth to power, their continuous strive to be great universities without being elitist, and their ability to function in an age of populism. The Trump administration and, more recently, Brexit have demonstrated that there is a decline in the respect for evidence and advice from subject-specific experts.  It seems (as in the case of the Trump administration) as if empirical reality does not matter, nor does empirical reasoning form the basis of public policy – a political place that is becoming increasingly anti-intellectual.  Emotion and personal belief have been shown to carry more weight than objective facts and evidence in terms of influencing public opinion.  Fake news and ‘the alternative truth’ have also challenged the fundamental principles of a university – academic freedom and the generation of new knowledge in the pursuit of truth.

A digitally unequal society
The COVID-19 pandemic has shown deep fault lines in our society – stark poverty and inequality – that universities should engage with (and they do); however, they cannot eliminate it on their own, but can be part of the solution.  South Africa is the most unequal society in the world.  Before the COVID-19 pandemic, the South African economy was already in deep trouble, with sovereign downgrades by all the rating agencies and with an unemployment rate close to 30%.   The national lockdown, in an attempt to ‘flatten the infection curve’ and hence manage the response of the national health system to COVID-19 cases, has added to the pressure on the economy.  It is envisaged that a large number of people (estimated between 3 and 7 million South Africans) will lose their jobs after the national lockdown period, adding to poverty and an already high unemployment rate.  Even during the lockdown period, there are many South Africans living in crowded spaces, hence finding it difficult to practise social distancing, may not have running water and proper sanitation, and possibly do not have regular access to food.  

As schools and the post-school education and training sectors move online with their learning, it further shows how digitally unequal our society really is – access to connectivity, data, and an appropriate digital device is a challenge, and electricity is not evenly distributed or is non-existent in our society.  These institutions, within the environment of digital inequality, are ensuring that digital equity is maintained as far as possible.  Many churches, business leaders, and certain politicians have called for a different social pact between business, labour, and government to address the state of the economy – any such action, however, must be supplemented by concrete measures for social reform.

Regaining trust in universities
But perhaps this pandemic has also created an opportunity for science and evidence to regain credibility in informing government decisions and public trust, and for universities to demonstrate respect for evidence. During the initial stages (early March) of COVID-19 in South Africa, the epidemiologists and virologists have shown through confirmed data from the National Institute of Communicable Diseases (NICD) that South Africa was in the early phase of the infection curve – also interpreted to be the relatively low-risk phase of the curve; this would be the right time to apply the principle of social distancing.  It allowed certain organisations (such as universities) to pro-actively suspend part of their activities so as to minimise the number of people in their operational environment, well before the national lockdown was announced on 26 March – a decision based on science.

Through data and proper analyses, the NICD, other scientific bodies and the Ministerial Advisory Committee on COVID-19 provided evidence-based information to government and the public, from which meaningful decisions could be taken.  The South African government has made it perfectly clear that decisions around COVID-19 will be made based on the science associated with this pandemic – a stance to be applauded.  Hence, the risk-adjusted approach of ‘opening up’ the economy through easing the lockdown measures but constantly monitoring the infection curve is an excellent example of risk management while continuously assessing the risks.

Universities, science laboratories, and pharmaceutical companies around the globe are hard at work to develop an effective vaccine for COVID-19, which is another opportunity to demonstrate how science can assist in protecting people from this terrible virus. Universities are making advances in personal protective equipment (PPE), the development of new technologies for non-ICU provision of oxygen to COVID-19 patients, more advanced methods of testing (for the virus) to reduce turnaround times, and various other scientific studies.  

This platform is giving universities a renewed impetus to use science and scientific developments to advance societal agendas such as climate change, poverty and inequality, public health and social justice (ethics of care) – and more immediate – assisting in re-building a strong South African economy.  It is an opportunity for the public and politicians to regain trust in universities, but it is also an opportunity for universities to profile their public intellectuals so that the value of science and evidence-based output is part of policy debates and informed decision-making.  However, in doing so, universities must strengthen their relationship with society at large, be inquiry-driven, and at the same time be learning and co-creating.

Prof Francis Petersen is Rector and Vice-Chancellor of the University of the Free State.

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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