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06 February 2024 | Story Dr Munita Dunn-Coetzee | Photo SUPPLIED
Munita Dunn-Coetzee
Dr Munita Dunn-Coetzee is Director: Student Counselling and Development, Division of Student Affairs, University of the Free State.

Opinion Article by Dr Munita Dunn-Coetzee, Director: Student Counselling and Development, Division of Student Affairs, University of the Free State.

The discovery of two hidden rooms with disturbing images and materials at Wilgenhof Men’s Residence (Stellenbosch University) last month has rekindled conversations about hazing and hazing practices. Wilgenhof, with a manifesto emphasising it as a place of belonging where all are free to be themselves, is described as a ‘house of horrors’, as punishment was seemingly doled out to male students as determined by an informal disciplinary committee.

Hazing is an ancient, universal practice. In society, whether past or modern, the need to join a group is an aspect of humanity. Hazing in educational institutions tends to occur as part of the hidden curriculum and manifests in a cyclical nature, for example, at the beginning of an academic year. A number or practices are associated with joining groups – it may take the form of a rite of passage, a ceremony, hazing, or paying a fee. The goal of participating in hazing activities is to be admitted and accepted in the group. By participating, prospective members can also prove their commitment to the group. When people freely choose to undergo a difficult initiation, it often increases their commitment and group cohesion – they need to believe the price of membership was worth it. The whole point of hazing is to build solidarity between members of a group.

Successfully navigating intimate, reciprocal relationships

The cohort of students joining higher education in South Africa typically fall in the 18- to 25-year-old range, and thus within the developmental phase of emerging adulthood. Erik Erikson, a German American child psychoanalyst known for his theory on psychosocial development of human beings, emphasised that this stage of development is about successfully navigating intimate, reciprocal relationships with others. A developmental need at university is therefore to fit in, to belong to a group, and to be part of campus activities – it brings security and protection. Hazing, however traumatising or painful, fulfils a developmental need.

Research has shown that the length of time for young people to actually create a personal identity has increased to the mid-to-late 20s. Emerging adulthood in Western culture can therefore be a time of shifting identities. This brings about a continued risk of experimentation with unhealthy behaviour. They are no longer minors and are faced with two additional life challenges: increased adult responsibilities and decreased familial support. From the onset of puberty through age 25, the adolescent brain undergoes profound changes in structure and function. A core element in the journey to adulthood involves the attainment of autonomy – on an emotional and behavioural level – learning to make your own decisions and manage your own emotions. Another developmental need is thereby met through hazing practices. 

Psychological consequences of hazing

While a few hazing rituals may appear mildly risky, many rituals cross the line. It is believed that humans are psychologically wired to form social groups in response to a threat, and this is what makes hazing effective in creating group identity. Despite the fact that hazing is potentially fatal and emotionally damaging, it is also believed that new students should have the same hazing experience as their predecessors. The hazing culture is therefore reproduced and enforced.

The psychological consequences of hazing can be rife. The concept of hazing is built upon psychological manipulation, degradation, and humiliation. Negative consequences that might have lasting effects include sleep problems, difficulty forming relationships, difficulty trusting others, decreased self-esteem, depressive tendencies, anxiety, self-harming tendencies, as well as academic underperformance. Unfortunately, hazing can also consist of social isolation, forced exercise, excessive drinking, and activities with a sexual innuendo. This results in embarrassing, abusive, exploitative, and dangerous activities. 

A student who has experienced hazing might feel a loss of control and empowerment, feeling more like a victim than before the hazing. This may appear directly after the hazing or later. Students who might have experienced traumatic events prior to hazing are more at risk for negative psychological reactions to hazing. This also applies to students witnessing hazing. They may experience feelings of guilt and shame for not having intervened to assist the hazing victim. And ironically, those who initiate hazing are not horrible, malicious human beings. They may believe the actions are expected of them and that they are carrying on a tradition for their residence. Those who haze others may also experience some of the same psychological consequences. We need to also remember that these psychological consequences would be significantly exacerbated should a student pass away due to a hazing-related activity. 

Will you still send him?

The focus thus far has been on the student, but what about the student’s parents, caregivers, and support system? Within the South African education system, not all South Africans have access to higher education. As a student finishing Grade 12, your dream is to enter tertiary education and to become the one breaking the cycle of poverty. Despite claiming that a university is a welcoming community assisting students to optimise their potential, hazardous hazing activities – such as the current discourse on Wilgenhof’s ‘house of horrors’ – have far-reaching negative physical and psychological consequences for both parents and students. 

Joining any group or team should not mean sacrificing your psychological health and well-being. It should be optimising your sense of self and enriching you systemically. If your son has been accepted at Wilgenhof Men’s Residence for 2024, will you still send him?

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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