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25 April 2022 | Story Elsabé Brits
Andre Roodt and Alice Brink
Prof Andreas Roodt and Prof Alice Brink are two of the inventors of the ‘Multinuclear complexes and their preparation patent.

According to the World Health Organisation (WHO), cancer is a leading cause of death worldwide, accounting for nearly 10 million deaths in 2020, or nearly one in six. The most common cancers are breast, lung, colon, rectum, and prostate cancers. There is a constant need to provide methods to diagnose and treat cancer-related tumours.  Current research strategies focus on eliminating cancer cells with the minimum damage to surrounding healthy cells.

A limitation of current technologies is that they are mostly based on the separate identification of cancer (diagnostic), followed by treatment (therapy) using chemotherapy and/or radiotherapy. To fit both needs at the same time and with similar or identical compounds, the principle of theranostic medicine was identified. This concept employs both diagnosing (by imaging) cancer and delivering therapy (treatment) simultaneously, which has been receiving increased attention internationally.

Collaborating with the University of Zurich
A University of the Free State (UFS) team, together with a team from the University of Zürich, conducted exciting research in this area and filed a patent titled ‘Multinuclear complexes and their preparation’. The patent was granted in South Africa and by the European Patent Office. It is being validated in selected European countries. The patent is pending in the USA, Japan, Hong Kong, and India. The inventors from the UFS are Prof Andreas Roodt, Prof Alice Brink, Dr Pennie Mokolokolo, and Dr Vincent Dumisani Kama. The approach that their technology takes is to enable the synthesis of a multinuclear compound/s, which may contain different pre-selected radioisotopes, to allow both imaging and therapy to the cancer site(s) with one and the same metal-organic complex.

So far, high-yield production of compounds has been successfully innovated, which contain both an imaging (in particular the widely utilised imaging isotope Technetium-99m) and therapeutic (typically the therapeutic isotope Rhenium-186) radioactive isotope(s), optionally carrying an additional cytotoxic agent. (Chemotherapy uses anti-cancer [cytotoxic] drugs to destroy cancer cells.)

Nuclear medicine technologies
In the next phase of the research, a lead compound portfolio of four to five model pharmaceuticals containing these metal nuclides with appropriate directing groups to target cancer sites will be designed and constructed. A number of these entities are known and can be introduced through different techniques. These will then undergo full characterisation and efficacy evaluation in biological models (in vitro), followed by extensive animal and human trials.

The technology will be delivered as a product or service in the way that current nuclear medicine technologies are delivered.

The fact that this product(s) contains both imaging and therapeutic radionuclides or cytotoxic modalities, enables detailed tracking of the pharmaceutical and monitoring of the tumours' response to the therapy. Not directly related to the patent, but an asset to it, is the fact that the incorporation of rhenium with a high atomic number (Z = 75) opens the additional opportunity to utilise the multinuclear compounds also as radiosensitisers. Synergistic effects, enhancing the therapeutic efficacy, can thus be expected in combination with radiotherapy.

The UFS would like to partner with a pharmaceutical company working in the field of nuclear medicine to commercialise this technology. Interested parties can contact Ravini Moodley at MoodleyR5@ufs.ac.za

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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