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03 September 2018 Photo Thabo Kessah
Burnout affects productivity in higher education
Elizabeth Nchapi’s study says burnout has adverse results for both employer and employee.

Staff members who are chronically exhausted may develop a cynical attitude towards their work and are likely to underperform, therefore feeling incompetent or experiencing a sense of reduced accomplishment. This is according to a research study by Elizabeth Nchapi, Head: Finances, on the University of the Free State’s Qwaqwa Campus. The study, which formed part of her Master of Arts (Higher Education Studies), also gives a comprehensive view on potential consequences for individuals and the organisation itself.

“The study was informed by my experience as a finance professional working at a higher-education institution where most of the research on burnout has mainly been around academic staff, hence this study focused on administrative staff,” she said.

Work environment stressors for administration staff

“Administrative staff in this sector have a responsibility to provide quality service not only to the academic core business of the institution, but also to the external stakeholders. Their working conditions require extensive multitasking, as they may often be expected to perform external roles or in fields other than their regular functions. Given that they continuously work under these circumstances, members may increasingly suffer from pressure leading to stress and burnout, which is a state of mental and physical exhaustion caused by one’s work environment.”

Work-environment stressors that lead to burnout, according to the study, include work overload, student interaction, team conflict, role ambiguity, job insecurity, lack of organisational support, lack of motivation, and workplace bullying.

Results of burnout

“Some of the potential consequences of burnout that have been identified as serious health problems may include, among others, sleep disturbances, anxiety, depression, and respiratory infections,” said Nchapi.

“Previous studies have shown that burnout does not only impact employees’ physical and psychological well-being. It also has significant consequences for the organisations and the employers. These include absenteeism, alcohol abuse, and poor organisational commitment, which ultimately result in poor performance,” she added.

The study further emphasises that personal and organisational consequences cut across the lines of gender, age, race, and employment levels. 

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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