纳米颗粒物的中枢神经毒性效应

随着纳米科技的迅速发展,纳米颗粒物的安全性评价备受人们关注,而由于中枢神经系统有可能是纳米颗粒作用的潜在靶器官,纳米颗粒的中枢神经毒性效应已成为研究热点.本文首先总结了纳米颗粒进入中枢神经系统的可能途径,从生物整体水平和细胞水平分析了纳米颗粒对中枢神经系统的毒性效应研究以及可能的机制.最后讨论了目前的实验研究中所存在的问题与缺陷,并对纳米颗粒的中枢神经毒性效应方面的研究方向进行了探讨.     

量子点毒性效应的研究进展

量子点（quantum dots,QDs）作为一种新型的纳米材料已备受关注．由于其独特的荧光特性,量子点已经成功地应用于生命科学等领域．近年来,量子点的生物学毒性效应及其环境影响成为新的研究热点．本文综述了量子点毒性效应的相关研究,并对该领域的前景及研究方向进行了评述和展望．     

富勒烯：美丽世界的尊贵访客

回顾了富勒烯科学的发展简史,从国际国内两个视角论述了富勒烯科学的发展现状,对富勒烯在化妆品等领域的应用前景进行了展望。     

环境中典型人工纳米颗粒物毒性效应

随着纳米技术和纳米材料在工业和生活中的大规模应用,大量的人工纳米颗粒物将不可避免地释放到环境介质(如水体、土壤、沉积物等)中。纳米颗粒物所具有的独特性质已引发人们对它们可能造成的健康风险和环境危害的关注和讨论。本文对目前环境中存在的几种主要典型人工纳米颗粒物的性质、来源、纳米毒性及影响纳米毒性的因素进行详细介绍,阐述了纳米颗粒物对生物的可能致毒机理。在分析纳米颗粒物毒性影响因素过程中,提出了纳米材料在环境中相关毒性研究展望。最后文中总结目前纳米材料在环境中的行为和毒性研究中所存在和面临的问题,并在此基础上提出将来纳米材料毒性的研究方向(如纳米材料的定量结构-活性关系,纳米材料表征技术及慢性毒性研究等)及需要改进的相关建议。     

富勒烯(C60/70)-丙烯酸的自由基共聚

富勒烯及其衍生物在超导、光电、磁学等领域展现出奇特性能[1],富勒烯的化学修饰成为化学工作者们关注的热点之一,而其中合成含富勒烯的新型聚合物是一个非常重要的方面.     

富勒烯：美丽世界的尊贵访客

A brief review is given on the history of fullerene science. The international and domestic development of fullerene science is discussed. Also given are perspectives on the potential applications of fullerene in cosmetics.     

纳米毒理学研究中的放射分析方法

随着纳米技术及其应用的迅速发展,纳米材料对生命体和生态环境的影响引起了社会公众、纳米产品生产厂家、科研工作者和各国政府的密切关注。纳米毒理学已成为纳米技术和毒理学的重要分支。纳米毒理学研究依赖于多种分析方法,用于纳米材料物理化学特性的表征及检测生命体中的纳米材料。放射分析方法由于其高灵敏度、高准确度、原位和体内分析能力,在纳米毒理学研究中能够发挥重要作用。本文综述了放射分析方法在纳米毒理学研究中应用的最新进展,重点介绍了针对不同纳米材料的放射性标记技术。     

富勒烯衍生物纳米颗粒水悬液对细菌生长的抑制作用

富勒烯纳米颗粒的生物学效应受到了广泛关注。本文首次测定了二加成亚甲基富勒烯[60]二膦酸四乙酯(bis-methanophosphonate fullerene, BMPF)的纳米水悬液（nano-BMPF）和富勒醇纳米水悬液（nano-fullerol）对细菌生长的影响。结果显示,nano-BMPF和nano-fullerol在黑暗条件下可抑制革兰氏阳性菌金黄色葡萄球菌的生长,且呈现浓度梯度依赖性,半抑制浓度IC50值分别为9.1 μM和4.2 μM;nano-fullerol对金黄色葡萄球菌生长的抑制可能与活性氧无关, nano-BMPF对金黄色葡萄球菌生长的抑制则可能与超氧阴离子自由基(O2.-)有关。在黑暗条件下二者对革兰氏阴性菌大肠杆菌的生长无影响。以上结果表明,这2种富勒烯衍生物纳米颗粒作为抗生素在生物医用领域具有潜在的应用前景。     

无机类富勒烯MoS2纳米材料的制备与表征

The Inorganic Fullerene-like MoS2 was obtained by a simple precipitation method using the polyethylenegly colas the dispersant,The hydroxylamine hydrochloride as the reductant, and (NH4)2S as the sulfursource. Themorphology and structure of the product were characterized by Powder X-ray Diffraction (XRD), Scanning Electron Microscopy (SEM) and High-resolution Transmission Electron Microscopy (HRTEM). The results suggest that the polyethylene glycol dispersant can be adsorbed on the particle surface of the reaction precursor, amorphous MoS2 powders, to form a relative isolated environment. This isolated environment may induce an obstruct effect which helps the precursor nano-particles transfer to the IF structure in the subsequent calcinations process.     

C_(60)/C_(70)及其衍生物(C_(60)Cl_n/C_(70)Cl_n)在丁二烯阴离子聚合中的偶联作用

Fullerene(富勒烯)独特的结构和性质吸引了高分子界广泛的关注.迄今,已通过和自由基共聚[1]、活性自由基聚合[2]、阳离子聚合[3]、阴离子聚合[4～8]以及配位聚合[9～13]等诸多方法相结合制备出了种类繁多的富勒烯高分子衍生物.不仅如此,富勒烯家族的重要分支--富勒烯卤化物,其独特的分子结构和具有的新性质也甚引起人们的重视[14,15].     

卤化富勒烯研究进展

自从C60被发现并能被大量制备以来,富勒烯化学已成为有机化学学科发展最快的领域之一.富勒烯通过多加成反应形成具有独特结构和性能的富勒烯卤化物和全氟烷基化物,为设计合成新型富勒烯基功能材料开辟了新方向.本文综述了近几年来在卤化富勒烯和全氟烷基化富勒烯的合成方法、结构及性能方面取得的最新进展,重点介绍了氟化富勒烯及其衍生化反应,并展望了该领域今后的发展趋势.     

卤化富勒烯研究进展

自从C60被发现并能被大量制备以来,富勒烯化学已成为有机化学学科发展最快的领域之一。富勒烯通过多加成反应形成具有独特结构和性能的富勒烯卤化物和全氟烷基化物,为设计合成新型富勒烯基功能材料开辟了新方向。本文综述了近几年来在卤化富勒烯和全氟烷基化富勒烯的合成方法、结构及性能方面取得的最新进展,重点介绍了氟化富勒烯及其衍生化反应,并展望了该领域今后的发展趋势。     

富勒烯合成化学研究进展

富勒烯是一类由12个五元环和若干六元环组成的笼状分子, 自20世纪80年代中期被发现以来就以其独特的结构和新奇的性质而成为科学界研究的热点, 25年来, 无论在基础研究还是在实际应用领域都有了长足的进步, 人们在发展富勒烯合成新方法和寻找富勒烯新结构方面做了大量的工作。本文对富勒烯的各种宏量合成方法进行了回顾, 并概述了迄今已发表的60余种富勒烯新结构,包括各种富勒烯空笼、内嵌富勒烯、富勒烯笼外修饰衍生物及氮杂富勒烯等结构。     

Octapalladium Strings Trap C60 and C70 Fullerenes Affording Metal-Chain-Wired Bucky Balls

Reactions of Pd₈ strings supported by meso-Ph₂PCH₂P(Ph)CH₂P(Ph)CH₂PPh₂ (meso-dpmppm) ligands, [Pd₈(meso-dpmppm)₄(L)₂]⁴⁺ (L=CH₃CN ( 1 ), XylNC ( 2 )) with C₆₀ resulted in the exclusive formation of unprecedented metal-chain-wired C₆₀ bucky balls, [{Pd₄(meso-dpmppm)₂(L)}₂(C₆₀)]⁴⁺ (L=CH₃CN ( 11 ), XylNC ( 12 )), in which a C₆₀ fullerene is trapped in the central Pd–Pd junction, as unambiguously established by spectroscopic, X-ray crystallographic, and theoretical techniques. The similar reaction of Pd₈ strings supported by rac-dpmppm, [Pd₈(rac-dpmppm)₄(CH₃CN)₂]⁴⁺ ( 3 ) also afforded a racemic mixture of [{Pd₄((R*,R*)-dpmppm)₂(CH₃CN)}₂(C₆₀)]⁴⁺ ( 13 ) without scrambling the Pd₄ fragments with (R,R)- and (S,S)-dpmppm ligands. Consequently, those of enantiopure chiral Pd₈ strings, [Pd₈((R*,R*)-dpmppm)₄(CH₃CN)₂]⁴⁺, certainly afforded chiral bucky balls of [{Pd₄((R*,R*)-dpmppm)₂(CH₃CN)}₂(C₆₀)]⁴⁺ ( 13 _RR and 13 _SS ), that exhibit mirror-image circular dichroism spectra. The reactions of 1 and 2 were also applied for trapping a C₇₀ fullerene to give 2 : 1 adducts of [{Pd₄(meso-dpmppm)₂(L)}₂(C₇₀)]⁴⁺ (L=CH₃CN ( 21 ), XylNC ( 22 )). These results provide useful information for creating a platform to develop dimensionally and chirality controlled metal–carbon nanocomposite materials.     

富勒烯的化学研究进展

本文评述了富勒烯化学研究的新进展, 从[ 60 ]、[ 70 ]富勒烯的化学修饰、富勒烯金属包合物、掺杂富勒烯、碳纳米管以及富勒烯的化学合成等几个方面着重介绍了国际上富勒烯研究的热点, 对进一步研究的方向进行了讨论。     

Fullerenes in Space

In 1985 the football structure of C₆₀, buckminsterfullerene was proposed and subsequently confirmed following its macroscopic synthesis in 1990. From the very beginning the role of C₆₀ and C₆₀⁺ in space was considered, particularly in the context of the enigmatic diffuse interstellar bands. These are absorption features found in the spectra of reddened star light. The first astronomical observations were made around one hundred years ago and despite significant efforts none of the interstellar molecules responsible have been identified. The absorption spectrum of C₆₀⁺ was measured in a 5 K neon matrix in 1993 and two prominent bands near 9583 Å and 9645 Å were observed. On the basis of this data the likely wavelength range in which the gas phase C₆₀⁺ absorptions should lie was predicted. In 1994 two diffuse interstellar bands were found in this spectral region and proposed to be due to C₆₀⁺. It took over 20 years to measure the absorption spectrum of C₆₀⁺ under conditions similar to those prevailing in diffuse clouds. In 2015, sophisticated laboratory experiments led to the confirmation that these two interstellar bands are indeed caused by C₆₀⁺, providing the first answer to this century old puzzle. Here, we describe the experiments, concepts and astronomical observations that led to the detection of C₆₀⁺ in interstellar space.