3.1 UV-Vis analysis of the extracted humic acids
Ultraviolet and visible spectroscopic measurements of the humic acids were made among 200 to 800 nm. E4/E6 value is the ratio of optical densities at specific wavelength of 450 and 650 nm used to conclude the degree of aromatization with normal Mw, size along with the O2 contents in HS [28]. The E4/E6 ratio has inverse relation with the degree of condensation, aromaticity, and degree of humification of humic substances [29].
Table 3.1: Effect of co-solvent on yield of humic acids and their spectroscopic properties
Coal sample
|
Solvent
|
E4/E6
|
ߡlog K
|
LS-93
|
KOH
|
2.35
|
0.601
|
3.2 Elemental analysis
Rendering to the foundation of organic material and place of development, the elemental configuration of humic constituents, in addition to their assets may fluctuate. The elemental investigation is significant meanwhile it delivers knowledge around the overall conformation of the particle, even though defining the humic acid molecular formula epitomizes a task. The presence of carbon content is lower as compared to the oxygen content. It is observed that the higher proportions of H/C and O/C and lower ratio N/C. The composition of humic acid having lower content of aliphatic means that there is a large content of aromatic groups which indicated the larger phenolic and carboxylic groups. These phenolic and carboxylic groups are the cause of formation of complexes. If the aromatic rings and humification is reduced, then the concentration of metal complexed is improved for alpha and gamma compositions at both pH in comparison beta places complex formation rises by the improved portions of carboxylic assemblies. It was shown that with the decrease of humification in humic acids, then the solidity of complexes at alpha and beta places reduces [26].
Table 3.2: Elemental composition and atomic ratios of humic Acid isolated from sample
Elements (%)
|
Atomic Ratio
|
C
|
40.50
|
H/C
|
1.65
|
H
|
5.25
|
N/C
|
0.13
|
N
|
7.23
|
O/C
|
0.81
|
O
|
45.35
|
|
|
|
|
|
|
Table 3.3: Physical state, color and melting points of humic metal complexes
HA complexes
|
Physical state
|
Color
|
Melting point
|
HA-Zn
|
Crystalline solid
|
Black
|
181°C
|
HA-Fe
|
Crystalline solid
|
Black
|
184°C
|
HA-Mg
|
Crystalline solid
|
Black
|
173°C
|
3.3 Vibrational assignments of FTIR
Fourier transform infrared spectroscopy (FTIR) is very applicable for studies of metals and humic acid interactions, reveals imperative features of divalent positive ions complexation, as well as offering limitations concerning the organizational description and it is also effective for identifying the functional groups presence.
Vibration peaks of FTIR analysis of HA and HA-Metal complexes
Bond stretching
|
Wave number (cm-1)
|
C-H
|
2950 – 2850
|
O-H
|
3540 – 3035
|
C-O
|
1200 -1215
|
C=O
|
1650 – 1550
|
C=C
|
1678 – 1688
|
COOH
|
1760-1690
|
Zn
|
500
|
Fe
|
490
|
Mg
|
480
|
Complexes with main vibrational assignments
Owing to the fact that humic substances establish numerous known binding sites such as amine (-NH), hydroxyl (-OH), carboxyl (-COOH) and metal ions of various metals (heavy metals) have revealed strong attractions [30]. Carboxyl, hydroxyl groups, aromatic, and alcoholic, hydroxyls have been considered to be the main functional groups observed in HA (the main portion of humic substances) for metal complexation [31, 32]. We also will concentrate on its most interesting FTIR bands of such major groups that could play a key role in binding ions.
The FTIR of the HA-Zn complexes prepared using the ion-exchange method is shown in Figure 2. Around 1583 cm-1 and 1384 cm-1, the two intensive bands can be identified. Symmetric (COO-) and antisymmetric (COO-) stretching vibrations, respectively [33] Carboxylate groups, can be attributed to these absorptions, suggesting that the HA-Zn complex of humic substances is formed predominantly by metal-carboxylate bonds. It would be difficult to classify the involvement of other functional groups (such as diketone groups and phenolic hydroxyls etc.) in metal complexing on the basis of FTIR analysis.
The approximate difference between the antisymmetric (COO-) and symmetric (COO-) carboxylate stretching frequencies of zinc (200 cm-1) was proposed, suggesting that perhaps the metal-oxygen bonds throughout the zinc bonds are much more covalent. Figure 4.2 suggests that the value was (199 cm-1) between all these bands, thereby confirming the active formation of the HA-Zn complex. The most significant aspect of the FTIR spectrum of HA substances was stated to be the existence of a peak approximately at 1700 cm-1 due to C= O stretching [34].
Furthermore, in order to form a metal ion-complex, the interaction between both the metal cation and carboxylic groups results in the disappearing of absorption peaks at 1700 cm-1 - 1720 cm-1 and the emergence of new bands at around 1583 cm-1 and 1384 cm-1 allocated to COO- and it’s stretching respectively. The absence of this group also means that the majority of COOH groups have been converted into the COO type. In contrast to the (COO-stretching) the band near about 1617 cm-1 of pure HA along with the change to lower frequencies, which also confirms the formation of HA-Zn and the band at about 1583 cm-1 (COO-stretching) turn out to be ever more intense for HA-Zn complexes [33]. It was studied by the use of Fourier transform infrared spectroscopy that the humic acids which are highly mummified have a tendency of bidentate linking complexation. If the humic acids are less humified than in this situation zinc tended to cause bidentate linking chelation [26]. The recent work describes the formation and description of complexes between humic substances particularly humic acid and fulvic acid isolated from wastes of hens and the zinc, copper, and iron ions [14]. The soil solution was appraised and is affected by deliver of such metals in a buffer solution. It was found that complex formation occurs due to the presence of carboxylic and phenolic groups [14].
The FTIR spectra of HA-Mg complex are shown in Figure 4.2. The peaks of the symmetric (COO-) and antisymmetric (COO-) stretching vibrations were identified after the analysis of HA. These groups of carboxylate groups, can be familiar to absorptions around 1566 cm-1 and 1381 cm-1 this suggesting that the HA-Mg complex of humic substances is formed mostly by metal-carboxylate bonds. Furthermore, in order to the peaks of FTIR obtained 1566 cm-1 and 1381 cm-1 with disappearing of the absobtion band at range of 1700 cm-1 - 1720 cm-1 of metal ion-complex, that was due to the interaction between both the metal cation (Mg2+) and carboxylic groups. The absence of this group also means that the majority of COOH groups have been transformed into the COO type. In comparison to the (COO-stretching) band near 1617 cm-1 of pure HA along with the change to lower frequencies, which also confirms the formation of HA-Mg, we obtained the band at 1566 cm-1 (COO-stretching) becomes ever more intense for the HA-Mg complexes.
Iron ion (Fe2+) had a greater effect of the blocking sites. According to the pure HA there were intense peaks in the range of 3000 cm-1 to 2700 cm-1. After the formation of the HA-Fe complex, these intense peaks were disappearing and obtained peaks in the region of 1566 cm-1 and 1381 cm-1. Which indicate the deformation of H stretching Furthermore the below 1000 cm-1 band indicates the presence of nitrogenous ring structures in the complex due to the pyrimidine and purine of HA. It also provided a binding site for the metal ion with HA. The FTIR spectra of the HA-Fe complexes are shown in Figure 4. The peaks of the stretching of carboxylic groups were identified by the analysis of the FTIR. Absorptions of about 1566 cm-1 and 1381 cm-1 can be standard in these classes of carboxylate groups, representing that the HA-Fe complex of humic substances is formed primarily by bonds of metal-carboxylate. The similar peaks values change for Fe-HA complexation were noted in already investigation [35].
Table 3.4: Comparative shifting of FTIR peaks of functional groups in HA and HA-Metal complexes
Functional groups
|
HA
|
HA-Zn
|
HA-Fe
|
HA-Mg
|
O-H
3540 – 3035
|
3390 cm-1
|
3250 cm-1
|
3270 cm-1
|
3345 cm-1
|
C-H
2950 – 2850
|
2919 cm-1
|
Nil
|
2925 cm-1
|
2921 cm-1
|
COOH
1760-1500
|
1600 cm-1
|
1574 cm-1
|
1570 cm-1
|
1566 cm-1
|
3.4 Thermo gravimetric analysis
Metal-humic complexes increase the stability of metals which frequently permitting the metals to persist in solution to be with ease accessible without influencing the uptake of plants. Interaction between humic acid and metals like Na, K, Mg, and Zn is investigated with special emphasis. Humic acid enriched with these elements is useful in organomineral fertilization. Organomineral fertilization is the combination of organic matter (HA) and mineral matter having more advantages in order to availability of macro (Mg), and micro (Zn) nutrients that are needed at initial phases of plant development [23].
Humic acid showed mass loss graphs as a function of the temperature at two major peaks: the first one at a lower temperature approximately 280 °C), as well as the second at temperature of above 400 °C. Elimination of water contents happened up to 200 °C accompanied by the elimination of main functional groups present in the sample between 250 to 280 °C
The mass loss at lower temperature was happened because metal ions interrupt the bond linkage between the humic substances and the individual components, due to which spread the individuals so it become reactive with heat and dissociate its structure. The decomposition carbohydrates present in the HA and the mass loss of the main functional groups as methyl, carboxylic, alcoholic groups and methylene was happened near about 300°C.
After the thermal analysis it is indicated that the HA has higher the value of the decomposition affinity with respect to the temperature as compared to the complexes as HA-Zn, HA-Fe and HA-Mg. However, the entropic contribution of the HA-Metal complexes smaller than according for the HA, hence the metal ions increase the thermal stability of the Humic products in the light of the above figures. It is also observed that decreases of large amount of the entropy in the process of degradation of humic acid, which combine with metal ions.
The maximum weight loss of HA complex occurs in the range of 300‒500 ºC indicating the thermal degradation. Sharma & Dubey (2014) reported the thermal degradation of complex in air atmosphere, 2.50 % weight lost at 105°C indicates the dehydration of HA complex. The maximum weight loss of about 91.6 % between 330 ºC to 590 ºC indicating both homogeneous combustion of volatiles and heterogeneous combustion of fixed carbon. Compared N2 and Ar atmospheres with CO2 atmosphere could considerably promote the combustion reaction and burnout temperature (Guo-dong et al. 2016). Thermo gravimetric analysis of HA complex showed great weight loss in temperature ranges from 400°C to 700°C and HA complex showed lower TG behavior due to high content of inert materials such as ash and low volatile content. HA complex started losing moisture from temperature 30–170°C (Dwivedi et al. 2019). Rathnam et al. measured the reactivity of Australian HA complex under simulated air (O2/N2) and oxy-fuel (O2/CO2) atmospheres using a TGA under non-isothermal conditions up to 1473 K.
3.5 The X-ray Diffraction analysis
In particular, broad bands between 3.5 Å (assigned to the more compact carbon network, i.e. aromatic structure) as 04.31 Å are found throughout the diffraction spectra of HA (attributed to the structure of aliphatic carbons). In Figures 4.9 X-ray diffractograms of the HA are shown, and also their corresponding complexes. Many other fine and well-developed peaks typical of the crystalline structures are given by the diffractograms.
Furthermore, because it is a macromolecule which may differ in composition and does not yet have a fully defined crystal lattice, experiments concerning the aromatic rings are recorded throughout the literature on the basis of the percentage used for understanding. The patterns are referred to the horizontal chains' aliphatic groups, whereas the other bands are attributed to the aromatic rings inside an order close to that of the graphite plan (002). This research was effectively used by [14]. Researchers who reinforced the effects of this kind of technique, whereby BG= band G (correlates to the 2nd angle of 25.50 °, or 00.35 nm mostly in X-ray diffracto-gram); Bγ= band γ (correlates to either the 2nd angle of 20.50 °, either 00.43 nm mostly in X-ray diffracto-gram); BG= peak area= high level area of band G; Bγ= peak area = peak area of band γ. HA had identical aromatic carbon contents ratios, with HA having a 05.25 percent higher disparity. The substance of humification as well as aromaticity, furthermore, is not only relevant to something like the qualitative structure including its functional groups, as well as to the structural reorganisation of certain substances, such as the changes that arise because when humic fraction is metal-complex. We emphasise that the given peaks aren't all that extreme and for HA-Zn, HA-Fe and FA-Mg complexes, which would have hindered the measurement of the aromatic as well as aliphatic carbon.