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22 February 2024 | Story André Damons | Photo SUPPLIED
Prof Robert Bragg
Prof Robert Bragg is a researcher in the Department of Microbiology and Biochemistry at the University of the Free State (UFS) and believes hospital-acquired infections (HAIs) might already be “Disease X”.

During the World Governments Summit, the World Health Organisation (WHO) warned world leaders about the likelihood of a Disease X outbreak, saying it is “a matter of when, not if” a new pathogen and pandemic will strike. If there is an outbreak of this disease tomorrow, the world still would not be ready. 

During his speech earlier this month at the summit in Dubai, Tedros Adhanom Ghebreyesus, Director-General of the WHO, said COVID-19 was a Disease X – a new pathogen causing a new disease. He said: “There will be another Disease X, or a Disease Y or a Disease Z. And as things stand, the world remains unprepared for the next Disease X, and the next pandemic. If it struck tomorrow, we would face many of the same problems we faced with COVID-19.”

Though Disease X is a hypothetical placeholder representing yet-to-be-encountered pathogens, Prof Robert Bragg, researcher in the Department of Microbiology and Biochemistry at the University of the Free State (UFS), believes hospital-acquired infections (HAI) might already be “Disease X”. He says data shows that deaths from HAIs will become the leading cause of human deaths. This problem is rapidly growing as most of the pathogens which people contract while in hospital are now resistant to antibiotics, making them very difficult to treat.  

Prof Bragg, whose main research is in disease-control, first in the agricultural industry, and now human health, also previously warned about a disease that would make COVID-19, which killed more than seven million people to date globally, look like a dress rehearsal. His PhD student, Samantha Mc Carlie, investigating how bacteria become resistant to disinfectant and sanitiser products. This is a serious problem for the future, as disinfection could be our last line of defence.

Heading for a crisis in health care

“The world is rapidly heading for a crisis in health care regarding hospital-acquired infections. It is common knowledge that we are quickly running out of antibiotics (and antifungals) to treat bacterial and yeast infections. Without antibiotics and antifungals, the outcome of many of these bacterial and yeast hospital-acquired infections will be very severe. They will, unfortunately, in many cases, result in the death of the patient,” says Prof Bragg. 

According to him, the WHO suggests that 30% of patients in ICUs in developed countries and 70% in underdeveloped countries will contract a HAI. Of these, the mortality rate can be as high as 70%. 

“Most of these infections are caused by multiple drug resistance strains of bacteria such as Enterococcus faecium, Staphylococcus aureus, Klebsiella pneumoniae, Acinetobacter baumannii, Pseudomonas aeruginosa and Enterobacter species. Additional bacteria and yeast, which can also cause HAIs, such as Serratia species, are also becoming a concern due to their intrinsic higher levels of disinfectant resistance.”

Prof Bragg explains that in 2014, a high-profile review was first published, commissioned by the UK Prime Minister, entitled, “Antimicrobial Resistance: Tackling a crisis for the Health and Wealth of Nations” (the AMR Review). This review estimated that antimicrobial resistance (AMR) could cause 10 million deaths annually by 2050 (The Review on Antimicrobial Resistance 2016). This is the same number of deaths caused by cancer today, making AMR the leading cause of human mortality by 2050. When it was finalised, this report was highly criticised as an over-dramatisation, as when this prediction was made, the number of mortalities related to HAIs was around 700 000 – a very long way off 10 000 000. However, according to recent estimates, five years later, in 2019, 1.27 million deaths were directly attributed to drug-resistant infections globally, and this had reached 4.95 million deaths associated with bacterial AMR (including those directly attributable to AMR) by 2022 (Murray et al. 2022). 

The overuse of disinfectants during the COVID-19 pandemic, according to Prof Bragg and Mc Calie, has contributed to the crisis by fostering resistant strains and contaminating environments. Based on the current trajectory of mortalities, the 10 million mark will be reached way before 2050.

Need for a paradigm shift

The researchers say an urgent need to change the paradigm in medicine from “treatment” to “prevention” is necessary and that the old saying ‘prevention is better than cure’ has never been truer. 

According to Bragg: “The golden era of antibiotics is rapidly coming to an end. It is highly unlikely that we will discover new antibiotics, and even if we do, the likelihood that the bacteria will already have or will be able to develop resistance in a very short time is highly likely. 

“We need to think of what happed with quinolones, where we thought we had won the war with a groundbreaking new antimicrobial agent. The bacteria did not have millions of years of evolution to develop resistance to quinolone, yet in only three years, the first resistant bacteria were isolated. There is currently great excitement around AI-derived new antibiotics. However, the end result is likely to be the same. We need an alternative to treatment – in other words, a paradigm shift.” 

Improved biosecurity 

Prof Bragg says highly improved biosecurity is the only viable option for disease control in a post-antibiotic era. By using good biosecurity in poultry production, he says the mortality rates were reduced by 50%. 

Research has shown a direct link between the environmental microbial load in a hospital and HAIs; with a lower microbial load linked to lower incidence of HAIs including C. difficile infections (Boyce et al. 2008; Suleyman et al. 2018; Umemura et al., 2022). Therefore, the new paradigm is to reduce microbial contamination in the hospital environment to prevent HAIs. If there are fewer dangerous microorganisms in an environment, patient and staff exposure to these microorganisms will decrease, reducing the level of HAIs for staff and patients. However, to reduce the microbial loads in healthcare settings, effective cleaning and disinfection products need to be used. 

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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