Secondary Ultraweak Luminescence from Humic Acids Induced by γ-Radiation

• Main Authors: Wieslaw Gorączko, Janusz Sławiński
• Format: Article
• Language: English
• Published: SAGE Publishing 2004-07-01
• Series: Dose-Response
• Online Access: https://doi.org/10.1080/15401420490507468

Humic substances (HSs) are products of biochemical transformations of plant and animal residues that make up a major fraction of the organic carbon of soil and aquatic systems in the environment. Because radioisotopes occur in the Earth's crust and because the entire biosphere is continuously exposed to cosmic radiation, ionizing radiation continually interacts with HSs. This chronic irradiation could have a significant ecological impact. However, very few publications are available that address possible consequences of chronic exposure of HSs to ionizing radiation from terrestrial and cosmic sources. This study was conducted to investigate possible impacts of exposure of HSs to ionizing radiation. Dried humic acid (HA) or its associated aqueous solution (in 0.1 M Na 2 CO 3 ) were exposed to absorbed γ-radiation in high doses of 1–90 kGy using a 60 Co source. Following the γ-ray exposures, a secondary, ultraweak radiation emanation with wavelengths in the spectral range λ = 340–650 nm was recorded as a long-lived chemiluminescence (CL) from the aqueous solutions; however, the CL was not observed after irradiating dry HA. Absorption spectra (for λ = 240–800 nm) of irradiated solutions indicated that polymerization/degradation processes were operating on the HA macromolecules. The effect of specific CL enhancers (luminol and lucigenin) on the intensity and kinetics of the CL implicated the participation of reactive oxygen species and free radicals in the CL and polymerization/degradation processes. For the range of absorbed doses used (1–10 kGy), the intensity of the induced CL was nonlinearly related to dose, suggesting that complex radical formation mechanisms were involved.