绿色合成姬松茸介导的银纳米粒子,提高酪氨酸羟化酶的催化效率,实现潜在的生物医学意义

IF 1.9 4区 物理与天体物理 Q2 BIOLOGY Origins of Life and Evolution of Biospheres Pub Date : 2024-07-11 DOI:10.1007/s11084-024-09647-4
Sikander Ali, Laraib Fatima, Muhammad Usman Ahmad, Qaiser Farid Khan, Muhammad Umar Hayyat, Zafar Siddiq, Sanjaykumar Patel, Tawaf Ali Shah, Yousef A. Bin Jardan, Youssouf Ali Younous, Mohammed Bourhia
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引用次数: 0

摘要

本研究涉及利用食用菌姬松茸作为还原剂,生物制造 AgA-AgNPs 以提高稳定性和催化效率,从而生产左旋多巴。为获得最大的酪氨酸羟化酶(TH)活性,对蘑菇生物量(2.5%,w/v)、提取介质(蛋白胨-碱性)和温度(90 ℃)等参数进行了优化。将酪氨酸羟化酶固定在 AgNPs 上可提高其活性。颜色从浅黄色变为深棕色证实了 AgA-AgNPs 的形成。此外,紫外可见光谱在 260 纳米处显示出表面等离子共振带。傅立叶变换红外光谱(FTIR)显示了官能团的存在,这些官能团在生成 NPs 的过程中发挥了重要作用。X 射线衍射 (XRD) 证实了霉菌合成的 AgNPs 的结晶性质,并显示出与 38.8° (111)、46.5° (200)、64.1° (220) 和 77.5o (311) 相对应的峰值。AgA-AgNPs 的 Zeta 电位为 -9.16 mv。AgA-AgNPs 的扫描电子显微镜(SEM)图像证实其粒径在 88.49 ± 3.83 nm 之间。从 A. arvensis 提取的固定化 TH 在最佳温度(20 ℃)下可重复使用 3 个周期。AgA-AgNPs 的左旋多巴产量提高了 2.54 倍。此外,与游离酶相比,固定化 TH 在 90 分钟的生物转化过程中消耗了更多的左旋酪氨酸,即 0.554 ± 0.022 mg/ml。因此,将 A. arvensis 提取的 TH 固定在 AgNPs 上可提高其活性、稳定性和催化效率。AgA-AgNPs 具有合成多巴胺的潜力,可在药物输送或生物医学应用中发挥重要作用。
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Green synthesis of Agaricus avensis-mediated silver nanoparticles for improved catalytic efficiency of tyrosine hydroxylase towards potential biomedical implications

The present study deals with the bio-fabrication of AgA-AgNPs utilizing edible mushroom Agaricus arvensis as a reductant for improved stability and catalytic efficiency towards L-dopa production. The parameters optimized for achieving maximum tyrosine hydroxylase (TH) activity were the mushroom biomass (2.5%, w/v), media for extraction (peptone-saline), and temperature (90 ℃). The activity of tyrosine hydroxylase (TH) was enhanced by its immobilization on AgNPs. The change in color from light yellow to dark brown confirmed the formation of AgA-AgNPs. In addition, the UV–Vis spectrum showed a surface plasmon resonance band at 260 nm. Fourier transform infrared (FTIR) indicated presence of functional groups, which play an important role in production of NPs. X-ray diffraction (XRD) confirmed the crystalline nature of mycosynthesized AgNPs and showed peaks corresponding to 38.8° (111), 46.5° (200), 64.1° (220), and 77.5o (311). AgA-AgNPs exhibited −9.16 mv zeta potential. Scanning Electron Microscopy (SEM) images of AgA-AgNPs confirmed particle size between 88.49 ± 3.83 nm. Immobilized TH extracted from A. arvensis showed reusability at optimized temperature (20 ℃) for 3 cycles. A 2.54-fold higher production of L-dopa was examined with AgA-AgNPs. Furthermore, immobilized TH consumed more L-tyrosine i.e. 0.554 ± 0.022 mg/ml as compared to the free enzyme at 90 min of biotransformation. Hence, the immobilization of A. arvensis extracted TH on AgNPs increased its activity as well as its stability and catalytic efficiency. AgA-AgNPs has a potential of dopamine synthesis and can play a significant role in drug delivery or biomedical applications.

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来源期刊
CiteScore
3.20
自引率
15.00%
发文量
12
审稿时长
>12 weeks
期刊介绍: The subject of the origin and early evolution of life is an inseparable part of the general discipline of Astrobiology. The journal Origins of Life and Evolution of Biospheres places special importance on the interconnection as well as the interdisciplinary nature of these fields, as is reflected in its subject coverage. While any scientific study which contributes to our understanding of the origins, evolution and distribution of life in the Universe is suitable for inclusion in the journal, some examples of important areas of interest are: prebiotic chemistry and the nature of Earth''s early environment, self-replicating and self-organizing systems, the theory of the RNA world and of other possible precursor systems, and the problem of the origin of the genetic code. Early evolution of life - as revealed by such techniques as the elucidation of biochemical pathways, molecular phylogeny, the study of Precambrian sediments and fossils and of major innovations in microbial evolution - forms a second focus. As a larger and more general context for these areas, Astrobiology refers to the origin and evolution of life in a cosmic setting, and includes interstellar chemistry, planetary atmospheres and habitable zones, the organic chemistry of comets, meteorites, asteroids and other small bodies, biological adaptation to extreme environments, life detection and related areas. Experimental papers, theoretical articles and authorative literature reviews are all appropriate forms for submission to the journal. In the coming years, Astrobiology will play an even greater role in defining the journal''s coverage and keeping Origins of Life and Evolution of Biospheres well-placed in this growing interdisciplinary field.
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