3.3. Determination of Light Absorbance at Different Wavelengths from 190 to 900 nm with a Double-Blazed Shimadzu UV-2550PC UV-Vis Spectrophotometer.
Using a double-blazed Shimadzu UV-2550PC UV-Vis spectrophotometer, light absorbance was determined at different wavelengths from 190 to 900 nm. Light absorbance results for each alfalfa genotype, depending on the precursor and its exposure time, are summarised in graph figures 1,2,3 and 4. The results of light absorption for the ‘
Kometa’ genotype after 24 h exposure to AgNO
3 and HAuCl
4 are shown in
Figure 1.
The most significant changes in the light absorption results compared to the control for the ‘
Kometa’ genotype after 24 h of exposure to the precursors are summarised in
Table 1.
The results of light absorption for the ‘
la Bella’ genotype after 24 h of exposure to AgNO
3 and HauCl
4 are shown in
Figure 2.
The most significant changes in the light absorption results compared to the control for the ‘
la Bella’ genotype after 24 h of exposure to the precursors are summarised in
Table 2.
The results of light absorption for the ‘
Kometa’ genotype after 48 h of exposure to AgNO
3 and HAuCl
4 are shown in
Figure 3.
The most significant changes in the light absorption results compared to the control for the ‘
Kometa’ genotype after 48 h of exposure to the precursors are summarised in
Table 3.
The results of light absorption for the ‘
la Bella’ genotype after 48 h of exposure to AgNO
3 and HAuCl
4 are shown in
Figure 4.
The most significant changes in the light absorption results compared to the control for the ‘
la Bella’ genotype after 48 h of exposure to the precursors are summarised in
Table 4.
Double-blazed photo-spectroscopy showed that control samples of both alfalfa genotypes had a light absorption peak between 5.00 and 4.5 when the samples received light with a wavelength between 340 and 460 nm. When light was received with a wavelength exceeding 460 nm, the absorption intensity decreased in all control samples and reached a minimum at 900 nm (<1.00).
In both ‘Kometa’ and ‘la Bella’ samples of the experimental groups that received all concentrations of the HAuCl4 precursor for 24 h and almost all concentrations for 48 h, the wavelength period in which the maximum values of light absorption were observed decreased compared to the control group. The decrease depended on the precursor type and its concentration. As the concentration of the precursor increased, the maximum values of light absorption were shown less frequently than in the control groups.
Samples were found where the light absorption peak did not reach the maximum value of 5.00. These were ‘Kometa’ genotype samples that received 250 and 1000 mg/L of the AgNO3 precursor with an exposure time of 24 h. Additionally, ‘la Bella’ samples that received the AgNO3 precursor with concentrations of 250 and 500 mg/L and an exposure time of 24 h.
When the precursors were used for 48 h, samples were detected in which the light absorption peak did not reach the maximum value of 5.00. These results are shown in
Table 4. These were the ‘
Kometa’ genotype samples that received 100 and 200 mg/L of the HAuCl
4 precursor and samples that received 250 mg/L of the AgNO
3 precursor. The ‘
la Bella’ sample that received 50 mg/L of the HAuCl
4 precursor also differed significantly from the control. This was the only one of the HAuCl
4 samples to show such a considerable difference from the control. Additionally, ‘
la Bella‘ samples that received the AgNO
3 precursor at all concentrations showed low absorption peaks with a short wavelength period.
3.4. Determination of Light Absorbance Intensity at a Certain Wavelength by Spectrophotometry Using a NanoDrop1000 Spectrophotometer.
The absorbance of the light in the suspension solution was determined at light wavelengths of 470 and 350 nm for AgNO
3 samples and 450 and 650 nm for HAuCl
4 samples. The NanoDrop1000 spectrophotometer differs from the double-blazed Shimadzu UV-2550PC UV-Vis spectrophotometer, in that absorbance is determined at a specific wavelength rather than a period. Each sample measurement was repeated in triplicate, and the light absorbance was determined at the selected wavelengths.
Table 5 summarises the average data of the 3 measurements of light absorption for the control group and the experimental groups of seedlings of both genotypes after 24 h of exposure to precursors.
After statistical analysis of the data, the spectrophotometry results showed that ‘
Kometa’ samples that were irradiated with light at a wavelength of 450 or 650 nm after 24 h of exposure to 50 mg/L HAuCl
4 showed a statistically significant increase in light absorption. Samples exposed to 100 mg/L showed a statistically insignificant increase, but samples exposed to 200 mg/L HAuCl
4 showed a statistically insignificant decrease. ‘
Kometa’ genotype samples exposed to AgNO
3 showed statistically significant changes in light absorption measured at both 350 and 470 nm at all precursor concentrations. At concentrations of 250 and 500 mg/L, absorbance at a 470 nm wavelength was reduced compared to the control group, but at the highest concentration of this precursor (1000 mg/L), absorbance was increased. In contrast, in samples irradiated with a light wavelength of 350 nm, absorbance was significantly increased in all three experimental groups. These results are shown in
Table 5.
The light absorption results of the Medicago sativa L. genotype ‘la Bella’ were also very different. In samples with HAuCl4, illumination at 450 nm showed a statistically significant decrease in absorbance when the precursor was used at concentrations of 100 mg/L and 200 mg/L. However, at a light wavelength of 650 nm, a statistically significant effect on light absorption was seen only when the precursor was used at a high concentration (200 mg/L). Absorption was reduced in ‘la Bella’ samples that received AgNO3 and were irradiated with light wavelengths of 470 and 350 nm. Statistically significant light absorption decreased when AgNO3 was used at a concentration of 250 mg/L with light waves of 470 and 350 nm. However, the absorbance was not significantly affected at 470 nm with a high precursor concentration (100 mg/L), whereas the highest concentration (1000 mg/L) was able to reduce the absorbance statistically significantly. Overall, the results showed that the sample with 500 mg/L AgNO3 at 350 nm had a statistically significant increase, whereas the highest concentration (1000 mg/L) did not significantly affect absorption.
Almost all of the light absorption data at different wavelengths changed their light absorption values after 24 h of exposure to precursors compared to the control group, except for one sample (‘la Bella‘, 650 nm, HAuCl4, 100 mg/L). However, the results changed unevenly, as only a part of the results (15 of 24) showed statistically significant changes.
Table 6 shows the average data of the 3 measurements of light absorption for the control group and the experimental groups of seedlings of both genotypes after 48 h of exposure to precursors.
These results showed that the changes in light absorption did not fluctuate as often as was seen in the results after 24 h of precursor exposure in alfalfa. In samples of genotype ‘
Kometa’ that received HAuCl
4 acid for 48 h, light absorption was increased statistically significantly compared to the control group in both experimental groups (HAuCl
4 concentrations 50, 100 and 200 mg/L). An increase in absorbance was observed at both wavelengths of light (450 and 650 nm). In samples of ‘
Kometa’ genotype that received AgNO
3 nitrate for 48 h and were irradiated with light at a wavelength of 470 nm, light absorption was increased compared to the control group at all concentrations (50, 100 and 200 mg/L). However, this increase was not statistically significant. However, with light at a wavelength of 350 nm, its absorption in the ‘
Kometa’ samples increased statistically significantly. In ‘
la Bella’ genotype samples that received HAuCl
4 acid for 48 h, light absorption increased statistically significantly at all acid concentrations (50, 100 and 200 mg/L) compared to the control group. These samples were irradiated with light at a wavelength of 450 nm. However, samples treated with light at a wavelength of 650 nm and an acid concentration of 50 mg/L showed a decrease in absorbance compared to the control, but this was not statistically significant. Samples with the same light wave but a higher acid concentration (100 and 200 mg/L) showed a statistically significant decrease in light absorption compared to the control group. The consistency of the results between samples within the same experimental group was also demonstrated by the remaining samples with AgNO
3 chloride; however, these results did not rule out differences between the experimental groups. The results with AgNO
3 showed that light absorption decreased statistically significantly at all acid concentrations (250, 500 and 1000 mg/L) compared to the control group when irradiating the samples with light with a wavelength of 470 nm, but the results were completely opposite when using a wavelength of 350 nm, as light absorption at all acid concentrations (250, 500 and 1000 mg/L) increased statistically significantly compared to the control group. These results are shown in
Table 6.
Almost all of the results from light absorption data at different wavelengths after 48 h of exposure to precursors, except for 4 samples (‘Kometa’, AgNO3, 450 nm 100 mg/L, 200 mg/L, 1000 mg/L and ‘la Bella’ HAuCl4, 650 nm, 50 mg/L), changed their light absorbance values statistically significantly. This indicates that 48 h of exposure to the precursor caused changes in light absorption more often. HAuCl4 increased light absorption in ‘Kometa’ samples statistically significantly, while in ‘la Bella’ samples, light absorption both decreased and increased depending on the wavelength of the light. Using the AgNO3 precursor in all ‘Kometa’ and ‘la Bella’ samples (at 470 nm) reduced light absorption statistically significantly.
3.5. Visualisation of Medicago sativa L. Seedlings with Confocal Microscopy.
The alfalfa leaves and roots were visualised in both genotypes using a confocal laser scanning microscope after 24 and 48 h of exposure to the precursor. Control and experimental samples with the highest precursor concentrations (‘
Kometa’ leaves and roots of control, HAuCl
4 200 mg/L, AgNO
3 1000 mg/L and ‘
la Bella’ leaves and roots of control, HAuCl
4 200 mg/L, AgNO
3 1000 mg/L) were visualised. Light fluorescence was determined for all the mentioned samples, and all samples were imaged. Some of the images are shown in these results. The peak of light fluorescence in all samples was shown when the samples received light with wavelengths from 530 to 550 nm. The wavelength period of peak light fluorescence intensity in leaf and root cells of ‘
Kometa’ and ‘
la Bella’ after exposure to precursors is shown in
Table 7.
The confocal microscopy results showed that leaves of the ‘Kometa’ genotype from a control sample had some stoma and fragments of a chloroplast. The study used a thick leaf; thus, the leaf tissues and cells overlapped with each other. The maximum fluorescence intensity in ‘Kometa’ leaves for the control sample was about 350 nm, but for the root sample, the fluorescence peak was much higher, exceeding 900 nm.
An image of a ‘
Kometa’ genotype leaf after 24 h of exposure to 200 mg/L HAuCl
4 in leaves and roots are shown in
Figure 1(a).
Figure 1.
Image of root sample with 200 mg/L HAuCl4 from the ‘Kometa’ genotype (a). Image of root sample with HAuCl4 200 mg/L, from the ‘la Bella’ genotype (b). Image of ‘la Bella’ genotype root sample after exposure to 1000 mg/L AgNO3 (c). Image of ‘Kometa’ genotype root sample exposed to 1000 mg/L AgNO3 (d). Image of ‘la Bella’ genotype root sample exposed to 1000 mg/L AgNO3 (e).
Figure 1.
Image of root sample with 200 mg/L HAuCl4 from the ‘Kometa’ genotype (a). Image of root sample with HAuCl4 200 mg/L, from the ‘la Bella’ genotype (b). Image of ‘la Bella’ genotype root sample after exposure to 1000 mg/L AgNO3 (c). Image of ‘Kometa’ genotype root sample exposed to 1000 mg/L AgNO3 (d). Image of ‘la Bella’ genotype root sample exposed to 1000 mg/L AgNO3 (e).
Au particles were seen between the cells of the vascular tissue, which gave off bright fluorescence. The size of these particles could not be determined because they stuck together in many places and formed agglomerates, and some of the particles stuck around the root from the outside and could be seen in the image as larger spots. The maximum fluorescence intensity of these samples for both the leaves and roots increased significantly; thus, HAuCl4 entered the plant roots.
After 24 h of exposure to 1000 mg/L AgNO3, the leaves of the ‘Kometa’ genotype showed an increase in fluorescence intensity compared to the control, but no Ag particles were visible in either leaves or roots.
For the ‘la Bella’ genotype, the control had a maximum fluorescence intensity of about 850 nm for the leaves, but for the root sample, the fluorescence peak was lower, exceeding 650 nm.
An image of the ‘
la Bella’ genotype leaf after 24 h of growing with HAuCl
4 200 mg/L, and a diagram of light fluorescence in the leaf and root are demonstrated in
Figure 1 (b).
Some Au particles were seen between the cells of the vascular tissue, which gave off bright fluorescence. The intensity of these samples for both the leaf and root samples increased significantly; thus, HAuCl4 entered the roots of the plant. Some of the particles formed an agglomerate and were around the root from the outside, as shown in the image as one larger spot.
An image of a ‘
la Bella’ genotype leaf after 24 h of exposure to 1000 mg/L AgNO
3 is shown in
Figure 1 (c).
Some Ag particles in this sample were also seen between the cells of the vascular tissue, which gave off a bright fluorescence. The intensity of both the leaf and root samples increased significantly; thus, AgNO3 also entered the plant roots.
However, the ‘Kometa’ genotype leaves of the control sample and those treated for 48 h with 200 mg/L HAuCl4 showed nothing. In the root sample, vascular tissue cells were partially visible, but no Au particles were visible. The maximum fluorescence intensity in ‘Kometa’ leaves for the control sample was about 1350 nm, but for the root sample, the fluorescence peak was much higher, exceeding 3000 nm. However, in sample leaves and roots of ‘Kometa’ with 200 mg/L HAuCl4 acid, the fluorescence peak was much higher than that of the control, demonstrating that HAuCl4 acid entered the plant and interacted with it.
An image of a ‘
Kometa’ genotype leaf after 24 h of exposure to 1000 mg/L AgNO
3 is shown in
Figure 1 (d).
After 48 h of exposure to 1000 mg/L HAuCl4, ‘Kometa’ genotype leaves showed an increase in fluorescence intensity compared to the control. Ag particles were not visible in the leaf samples. In contrast, AgNO3 particles were visible in the root samples, although they were not abundant; they appeared to be more abundant in the sample medium concentration of silver nitrate.
After 48 h of exposure, leaves of the ‘la Bella’ genotype without any precursor (control) or 200 mg/L HAuCl4 showed nothing. In the root sample, vascular tissue cells were partially visible, and some Au particles could be seen between the tissues, but there were very few. The maximum fluorescence intensity in ‘la Bella’ leaves for the control sample was about 2500 nm, but for the root sample, the fluorescence peak was much lower, exceeding 600 nm. However, in the ‘la Bella’ leaves exposed to 200 mg/L HAuCl4, the fluorescence peak was much lower than the control, and the roots showed a higher fluorescence peak than the control, demonstrating that HAuCl4 acid entered the plant and affected the ‘la Bella’ genotype.
An image of the ‘
la Bella’ genotype leaf after 48 h of exposure to 1000 mg/L AgNO
3 is shown in
Figure 1 (e).
The ‘la Bella’ leaf and root samples exposed to AgNO3 (1000 mg/L) for 48 h did not show a significant increase in fluorescence intensity compared to the control. The same Ag particles were visible in the leaf sample. AgNO3 particles were also visible in the root sample, although there were not many of them.