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Atmospheric plasma inactivation of biofilm-forming bacteria for food safety control

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journal contribution
posted on 2008-07-14, 11:35 authored by Mieke Vleugels, Gilbert Shama, Xu-Tao Deng, Elizabeth Greenacre, Tim Brocklehurst, Michael G. Kong
The ability of atmospheric pressure glow discharges (APGD) to inactivate microorganisms has been demonstrated in a number of previous studies. However, most of this work has been performed using microorganisms that do not form biofilms and with the microorganisms supported on abiotic surfaces that discourage cell growth. When microorganisms attach to the surface of a food, they can extract nutrients from the food and proliferate at the surface. Often this growth takes the form of biofilms which comprise three-dimensional (3-D) networks of polysaccharides that attach microorganisms to surfaces and serve to protect them from external stresses; fresh foods, such as salad crops, frequently harbor biofilms. We believe that the use of APGD offers a potential for inactivating microorganisms on the surface of fresh foods that cannot be readily treated by other methods without inducing unacceptable changes to these foods. As a first step toward a full evaluation of the viability of the APGD technology for food safety control, we consider in this paper two key issues, namely: 1) whether atmospheric glow discharges can inactivate biofilm-forming microorganisms and 2) whether plasma treatment causes significant discoloration to food surfaces. Using the biofilm-forming bacterium Pantoea agglomerans and bell peppers (Capsicum annuum) as a typical example of plant tissue, we show that atmospheric He-O2 plasmas can be effective inactivation agents without causing unacceptable levels of discoloration to the peppers, and that furthermore they are superior to the use of low-pressure ultraviolet sources.



  • Mechanical, Electrical and Manufacturing Engineering


VLEUGELA, M. ... et al, 2005. Atmospheric plasma inactivation of biofilm-forming bacteria for food safety control. IEEE Transactions on Plasma Science, 33(2), pp. 824-828



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