Elsevier

Carbohydrate Polymers

Volume 44, Issue 3, March 2001, Pages 269-271
Carbohydrate Polymers

Short Communication
Free radical formation in UV- and gamma-irradiated cassava starch

https://doi.org/10.1016/S0144-8617(00)00268-XGet rights and content

Abstract

Cassava starch is degraded by UV irradiation, particularly when previously acidified with lactic acid. Gamma irradiation also induces starch degradation through the formation of free radicals. The aim of this work was to confirm the hypothesis that free radicals are formed in starch through UV treatment and to compare free radical formation and the extent of degradation in native or acidified starches as a result of UV and gamma irradiation. Both types of irradiation result in a decrease in starch intrinsic viscosity. Electronic spin resonance (ESR) shows that radicals formed in UV irradiated samples are similar to those produced by gamma irradiation.

Introduction

The treatment of starch by UV light, with or without a photosensitizer (Phillips & Rickards, 1969), induces changes in its functional properties: it increases water binding capacity and solubility (Gholap, Marondeze & Tomasik, 1993) and decreases hot paste viscosity (Fiedorowicz, Tomasick & Lim, 1999). The latter phenomenon can also be observed after treatment with natural sunlight, particularly with cassava starch that has been previously acidified with lactic acid (Mestres and Rouau, 1997, Fiedorowicz et al., 1999, Nunes, 1994, Plata-Oviedo and Camargo, 1998).

Sunlight or UV irradiation do not seem to alter the crystalline structure of starch; the gelatinization enthalpy remains mainly unchanged (Mestres and Rouau, 1997, Fiedorowicz et al., 1999). However, irradiation decreases the intrinsic viscosity (Merlin and Fouassier, 1981, Mestres and Rouau, 1997) and could also promote starch cross-linking under oxygen (Fiedorowicz et al., 1999). UV photodegradation of starch results in glycosidic bond cleavages, with a shortening of the amylose chain and a debranching of the amylopectin chain, through free radical formation (Merlin & Fouassier, 1981). Some studies suggest that free radicals produced by UV irradiation are identical to those produced during thermal treatments (Tomasick & Zaranyika, 1995) or to those generated by additives such as sulphite or ascorbic acid (Sriburi, Hill & Barclay, 1999). However, the starch photodegradation mechanism remains unclear.

Electronic spin resonance (ESR) experiments have made a major contribution to our understanding of the mechanism of starch degradation after gamma irradiation. It has been reported that gamma irradiation induces free radicals at the C1 position on the glucose molecule (Raffi and Agnel, 1983, Raffi et al., 1985). The aim of this work was to confirm the hypothesis that free radicals are formed in starch after UV treatment and to compare free radical formation and the extent of starch degradation after UV and gamma irradiation.

Section snippets

Materials and methods

Cassava starch (Manihot esculenta Crantz) used was a commercial sample from Lorenz Co. (São Paulo, Brazil). Amylopectin was extracted from the starch according the method described by Banks and Greenwood (1967). Dextrin 10 derived from corn starch was obtained from Fluka BioChemika.

The cassava starch, amylopectin and dextrin were acidified with lactic acid (Sigma L1250) solution (2% w/w) for 10 min at room temperature then dried in an oven at 25°C for 24 h, giving a final water content of 12%

ESR

The native cassava starch did not show any ESR signal. The ESR patterns of the cassava starch samples after UV or gamma radiation (Fig. 1) showed different shapes depending on water content and storage time after irradiation. They can present two main signals, AA′ and BB′ (Table 1), according to the notation of the signals already found in gamma-irradiated starches (Raffi & Agnel, 1983), or a main BB′ signal; these two signals are singlets. Merlin and Fouassier (1981) also noted the presence of

Acknowledgements

The authors thank the Brazilian Ministry of Education for its research grant.

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