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04 March 2025 | Story Tshepo Tsotetsi | Photo Supplied
Prof Tameshnie Deane
Prof Tameshnie Deane, Vice-Dean of Research, Postgraduate Studies and Internationalisation in the UFS Faculty of Law.

A judgment by Prof Tameshnie Deane, Vice-Dean of Research, Postgraduate Studies and Internationalisation at the University of the Free State’s (UFS) Faculty of Law, has been published in South African Criminal Law Reports (SACLR), in recognition of its groundbreaking contribution to South African domestic violence law.

Prof Deane’s May 2024 judgment in the case GD v NB (2025(1) SACR 179) challenged a restrictive Supreme Court of Appeal (SCA) precedent and expanded the interpretation of ‘domestic relationships’ under the Domestic Violence Act. Her ruling has not only reshaped legal understanding but also reinforced the UFS’s commitment to impactful legal scholarship.

South African Criminal Law Reports is a monthly report of criminal law and procedure cases from superior courts in Southern Africa. The cases highlighted in each issue are chosen for their importance to criminal law practitioners.

Challenging established precedents

Prof Deane’s judgment effectively challenged a precedent set by the SCA in Daffy v Daffy (2012), marking a significant shift in legal interpretation under the Domestic Violence Act 116 of 1998 (DVA).

The GD v NB case revolves around domestic violence and the issuance of a protection order under the DVA. The appellant (the person who appealed the original court’s decision), who was married to the sister of the respondent (the person who must answer the claims), argued that their relationship did not fall under the domestic relationship criteria for a protection order. This argument relied heavily on the SCA’s decision in Daffy v Daffy, where the court had narrowly defined a ‘domestic relationship’ as being limited to cohabitation or close familial ties. In the Daffy case, two brothers were denied protection under the DVA, as their strained business relationship was deemed insufficient to fall under the scope of domestic violence protections.

Expanding the definition of domestic relationships

Prof Deane, however, disagreed with the restrictive interpretation applied in that case. “I concluded that this constrictive interpretation of a ‘domestic relationship’ seemingly ignores the intended aims of the DVA,” she explained. In her judgment, she argued that the DVA was intended to offer protection in a wide range of domestic relationships, and that the previous ruling failed to consider the evolving dynamics of modern familial ties.

By drawing on the broader, evolving understanding of domestic violence, Prof Deane expanded the definition of a “domestic relationship” to include relationships based on familial obligations, even where they may not involve cohabitation or direct consanguinity (direct blood relation). She cited specific details in the GD v NB case where the appellant and respondent were involved in the care of the respondent’s mother. “The relationship between the appellant and respondent extends beyond business matters to include familial obligations,” she noted. The ruling in GD v NB granted the appellant a protection order, acknowledging that their relationship met the broader definition of domestic violence protection under the DVA.

Adapting the law to contemporary realities

Her judgment reinforced that domestic violence can occur in diverse familial structures and that protection under the DVA should not be limited by narrow definitions. “Society is constantly changing, and the law must adapt accordingly to ensure relevance and that the widest possible protections are afforded to those in a wide range of domestic relationships,” Prof Deane emphasised. Her judgment serves as a response to South Africa’s high rates of domestic violence, ensuring that the law accommodates and responds to the diverse situations in which domestic violence occurs.

This landmark ruling contributes significantly to the ongoing development of South African law, furthering the protection of domestic violence victims and ensuring that the DVA is applied in a way that reflects the realities of contemporary society. Prof Deane’s decision highlights the importance of the law adapting to social changes, offering broader protection and safeguarding the rights of vulnerable individuals within complex and varied domestic environments. This judgment also positions the UFS as a leader in advancing legal thought and contributing meaningfully to the evolution of South African law.

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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