Synthesis, crystal structure, DNA binding and cleavage activities of oximato bridged cationic dinuclear copper(II) complex having labile ligands

Oximato bridged dinuclear copper(II) complex Cu(L)(CH3OH)](2)(ClO4)(2) with an oxime-Schiff base ligand, viz. 3-2-(dimethylamino)ethyl]imino]-2-butanoneoxime (HL), has been synthesized and structurally characterized. The dinuclear copper(II) complex crystallizes in monoclinic space group P2(1)/n with the unit cell parameters, a = 13.3564(9) angstrom, b = 12.0821(8) angstrom, c = 17.5045(11) angstrom, beta = 90.097, V = 2824.8(3) angstrom(3), Z = 4, R = 0.0769. The complex shows quasi-reversible cyclic voltammetric response at 0.844V (Delta E-p = 276 mV) at 100 mVs(-1). The binding studies of the complex with calf thymus DNA has been investigated using absorption spectrophotometry. Cleavage activity of the complex has been carried out on double stranded pBR 322 plasmid DNA by using gel electrophoresis experiments in the absence and in the presence of the oxidant, viz., H2O2.

Detailed properties of high redshift galaxies

Galaxies evolve throughout the history of the universe from the first star-forming sources, through gas-rich asymmetric structures with rapid star formation rates, to the massive symmetrical stellar systems observed at the present day. Determining the physical processes which drive galaxy formation and evolution is one of the most important questions in observational astrophysics. This thesis presents four projects aimed at improving our understanding of galaxy evolution from detailed measurements of star forming galaxies at high redshift.

We use resolved spectroscopy of gravitationally lensed z ≃ 2 - 3 star forming galaxies to measure their kinematic and star formation properties. The combination of lensing with adaptive optics yields physical resolution of ≃ 100 pc, sufficient to resolve giant Hii regions. We find that ~ 70 % of galaxies in our sample display ordered rotation with high local velocity dispersion indicating turbulent thick disks. The rotating galaxies are gravitationally unstable and are expected to fragment into giant clumps. The size and dynamical mass of giant Hii regions are in agreement with predictions for such clumps indicating that gravitational instability drives the rapid star formation. The remainder of our sample is comprised of ongoing major mergers. Merging galaxies display similar star formation rate, morphology, and local velocity dispersion as isolated sources, but their velocity fields are more chaotic with no coherent rotation.

We measure resolved metallicity in four lensed galaxies at z = 2.0 − 2.4 from optical emission line diagnostics. Three rotating galaxies display radial gradients with higher metallicity at smaller radii, while the fourth is undergoing a merger and has an inverted gradient with lower metallicity at the center. Strong gradients in the rotating galaxies indicate that they are growing inside-out with star formation fueled by accretion of metal-poor gas at large radii. By comparing measured gradients with an appropriate comparison sample at z = 0, we demonstrate that metallicity gradients in isolated galaxies must flatten at later times. The amount of size growth inferred by the gradients is in rough agreement with direct measurements of massive galaxies. We develop a chemical evolution model to interpret these data and conclude that metallicity gradients are established by a gradient in the outflow mass loading factor, combined with radial inflow of metal-enriched gas.

We present the first rest-frame optical spectroscopic survey of a large sample of low-luminosity galaxies at high redshift (L < L*, 1.5 < z < 3.5). This population dominates the star formation density of the universe at high redshifts, yet such galaxies are normally too faint to be studied spectroscopically. We take advantage of strong gravitational lensing magnification to compile observations for a sample of 29 galaxies using modest integration times with the Keck and Palomar telescopes. Balmer emission lines confirm that the sample has a median SFR ∼ 10 M_sun yr^−1 and extends to lower SFR than has been probed by other surveys at similar redshift. We derive the metallicity, dust extinction, SFR, ionization parameter, and dynamical mass from the spectroscopic data, providing the first accurate characterization of the star-forming environment in low-luminosity galaxies at high redshift. For the first time, we directly test the proposal that the relation between galaxy stellar mass, star formation rate, and gas phase metallicity does not evolve. We find lower gas phase metallicity in the high redshift galaxies than in local sources with equivalent stellar mass and star formation rate, arguing against a time-invariant relation. While our result is preliminary and may be biased by measurement errors, this represents an important first measurement that will be further constrained by ongoing analysis of the full data set and by future observations.

We present a study of composite rest-frame ultraviolet spectra of Lyman break galaxies at z = 4 and discuss implications for the distribution of neutral outflowing gas in the circumgalactic medium. In general we find similar spectroscopic trends to those found at z = 3 by earlier surveys. In particular, absorption lines which trace neutral gas are weaker in less evolved galaxies with lower stellar masses, smaller radii, lower luminosity, less dust, and stronger Lyα emission. Typical galaxies are thus expected to have stronger Lyα emission and weaker low-ionization absorption at earlier times, and we indeed find somewhat weaker low-ionization absorption at higher redshifts. In conjunction with earlier results, we argue that the reduced low-ionization absorption is likely caused by lower covering fraction and/or velocity range of outflowing neutral gas at earlier epochs. This result has important implications for the hypothesis that early galaxies were responsible for cosmic reionization. We additionally show that fine structure emission lines are sensitive to the spatial extent of neutral gas, and demonstrate that neutral gas is concentrated at smaller galactocentric radii in higher redshift galaxies.

The results of this thesis present a coherent picture of galaxy evolution at high redshifts 2 ≲ z ≲ 4. Roughly 1/3 of massive star forming galaxies at this period are undergoing major mergers, while the rest are growing inside-out with star formation occurring in gravitationally unstable thick disks. Star formation, stellar mass, and metallicity are limited by outflows which create a circumgalactic medium of metal-enriched material. We conclude by describing some remaining open questions and prospects for improving our understanding of galaxy evolution with future observations of gravitationally lensed galaxies.

Iso-specific Ziegler-Natta polymerization of α-olefins with a single-component organoyttrium catalyst

The synthesis of a sterically tailored ligand array (M)_2((C_5H_2-2-Si(CH_3)_3-4-C(CH_3)_3)S_2i(CH_3)_2]("M_2Bp") (M = Li, 16; K, 19) is described. Transmetallation of Li_2Bp with YCl_3(THF)_3 affords exclusively the C_2 symmetric product rac-[BpY(µ_2-Cl)_2Li(THF)_2], 20. A X-ray crystal structure of 20 has been determined; triclinic, P1, a= 13.110 (8), b = 17.163 (15), c = 20.623 (14) Å, α = 104.02 (7), β = 99.38 (5), γ = 100.24 (6)° , Z = 4, R = 0.056. Transmetallation of K_2Bp with YCl_3(THF)_3 affords the halide free complex rac-BpYCl, 23. The corresponding rac-BpLaCl, 28, is prepared in an anlogous manner. In all cases the achiral meso isomer is not obtained since only for the racemic isomers are the unfavorable steric interactions between the Si(CH3)_3 groups in the narrow portion of the [Cp-M'-Cp] wedge avoided. Alkylation of 20 or 23 with LiCH(Si(CH_3)_3)_2 affords rac-BpYCH(Si(CH_3)_3)_2, 26 in good yield. Alkylation of 28 with LiCH(Si(CH_3)_3)_2 affords rac-BpLaCH(Si(CH_3)_3)_2 29. Hydrogenation of 26 cleanly affords the bridging hydride species [BpY(µ_2-H)]_2, 27, as the homochiral (R,R) and (S,S) dimeric pairs. 26 is an efficient initiator for the polymerization of ethylene to high molecular weight linear polyethylene. 27 catalyzes the polymerization of propylene (25% v/v in methylcyclohexane) and neat samples of 1-butene, 1-pentene, 1-hexene to moderately high molecular weight polymers: polypropylene (M_n = 4,200, PDI 2.32, T_m 157 °C); poly-1-butene (M_n = 8,500, PDI 3.44, T_m 105 °C); poly-1-pentene (M_n = 20,000, PDI 1.99, T_m 73 °C); poly-1-hexene (M_n = 24,000, PDI 1.75, T_m < 25 °C). ^(13)C NMR spectra at the pentad analysis level indicates that the degree of isotacticity is 99% mmmm for all polymer samples. 27 is the first single component iso-specific α-olefin polymerization catalyst. The presumed origins of the high isospecificity are presented.

Reactions of oxygen containing ligands in the coordination sphere of permethylhafnocene and permethyltantalocene

A series of terl-butylperoxide complexes of hafnium, Cp*₂Hf(R)(OOCMe₃) (Cp* = ((η⁵-C₅Me₅); R = Cl, H, CH₃, CH₂CH₃, CH₂CH₂CH₃, CH₂CH₂CH₂CH₃, CH₂CHMe₂, CH=CHCMe₃, C₆H₅, meta-C₆H₃(CH₂)2) and Cp*(η⁵-C₅(CH₃)₄CH₂CH₂CH₂)Hf(OOCMe₃), has been synthesized. One example has been structurally characterized, Cp*₂Hf(OOCMe₃)CH₂CH₃ crystallizes in space group P2₁/c, with a = 19.890(7)Å, b = 8.746(4)Å, c = 17.532(6)Å, β = 124.987(24)°, V = 2498(2)ų, Z = 4 and R_F = 0.054 (2222 reflections, I > 0). Despite the coordinative unsaturation of the hafnium center, the terl-butylperoxide ligand is coordinated in a mono-dentate ligand. The mode of decomposition of these species is highly dependent on the substituent R. For R = H, CH₂CH₃, CH₂CH₂CH₃, CH₂CH₂CH₂CH₃, CH₂CHMe₂ a clean first order conversion to Cp*₂Hf(OCMe₃)(OR) is observed (for R CH₂CH₃, ΔHǂ = 19.6 kcal•mol^-1, ΔSǂ = -13 e.u.). These results are discussed in terms of a two step mechanism involving η²-coordination of the terl-butylperoxide ligand. Homolytic O-O bond cleavage is observed upon heating of Cp*₂Hf(OOCMe₃) R (R = C₆H₆, meta-C₆H₃(CH₃)₂). In the presence of excess 9,10-dihydroanthracene thermolysis of Cp*₂Hf(OOCMe₃)C₆H₆ cleanly affords Cp*₂Hf(C₆H₆)OH and HOCMe₃ (ΔHǂ = 22.6 kcal•mol^-1, ΔSǂ = -9 e.u.). The O-O bond strength in these complexes is thus estimated to be 22 kcal•mol^-1.

Cp*₂Ta(CH₂)H, Cp*₂Ta(CHC₆H₅)H, Cp*₂Ta(C₆H₄)H, Cp*₂Ta(CH₂=CH₂)H and Cp*₂Ta(CH₂=CHMe)H react, presumably through Cp*₂Ta-R intermediates, with H₂O to give Cp*₂Ta(O)H and alkane. Cp*₂Ta(O)H was structurally characterized: space group P2₁/n, a= 13.073(3)Å, b = 19.337(4)Å, c = 16.002(3)Å, β = 108.66(2)°, V = 3832(1)ų, Z = 8 and R_F = 0.0672 (6730 reflections). Reaction of terlbutylhydroperoxide with these same starting materials ultimately yields Cp*₂Ta(O)R and HOCMe₃. Cp*₂Ta(CH₂=CHR)OH species are proposed as intermediates in the olefin hydride reactions. Cp*₂Ta(O₂)R species can be generated from the reaction of the same starting materials and O₂. Lewis acids have been shown to promote oxygen insertion in these complexes.

I. The crystal structure of potassium bis(tricyanovinyl)amine. II. Nuclear magnetic resonance studies of alkali halide solutions. III. Elucidation of the intramolecular hydrogen bond in acetylacetone by the deuterium isotope effect on the chemical shift of the bridge hydrogen

Part I

Potassium bis-(tricyanovinyl) amine, K⁺N[C(CN)=C(CN)₂]₂^-, crystallizes in the monoclinic system with the space group Cc and lattice constants, a = 13.346 ± 0.003 Å, c = 8.992 ± 0.003 Å, B = 114.42 ± 0.02°, and Z = 4. Three dimensional intensity data were collected by layers perpendicular to b* and c* axes. The crystal structure was refined by the least squares method with anisotropic temperature factor to an R value of 0.064.

The average carbon-carbon and carbon-nitrogen bond distances in –C-CΞN are 1.441 ± 0.016 Å and 1.146 ± 0.014 Å respectively. The bis-(tricyanovinyl) amine anion is approximately planar. The coordination number of the potassium ion is eight with bond distances from 2.890 Å to 3.408 Å. The bond angle C-N-C of the amine nitrogen is 132.4 ± 1.9°. Among six cyano groups in the molecule, two of them are bent by what appear to be significant amounts (5.0° and 7.2°). The remaining four are linear within the experimental error. The bending can probably be explained by molecular packing forces in the crystals.

Part II

The nuclear magnetic resonance of ⁸¹Br and ¹²⁷I in aqueous solutions were studied. The cation-halide ion interactions were studied by studying the effect of the Li⁺, Na⁺, K⁺, Mg⁺⁺, Cs⁺ upon the line width of the halide ions. The solvent-halide ion interactions were studied by studying the effects of methanol, acetonitrile, and acetone upon the line width of ⁸¹Br and ¹²⁷I in the aqueous solutions. It was found that the viscosity plays a very important role upon the halide ions line width. There is no specific cation-halide ion interaction for those ions such as Mg⁺⁺, Di⁺, Na⁺, and K⁺, whereas the Cs⁺ - halide ion interaction is strong. The effect of organic solvents upon the halide ion line width in aqueous solutions is in the order acetone ˃ acetonitrile ˃ methanol. It is suggested that halide ions do form some stable complex with the solvent molecules and the reason Cs⁺ can replace one of the ligands in the solvent-halide ion complex.

Part III

An unusually large isotope effect on the bridge hydrogen chemical shift of the enol form of pentanedione-2, 4(acetylacetone) and 3-methylpentanedione-2, 4 has been observed. An attempt has been made to interpret this effect. It is suggested from the deuterium isotope effect studies, temperature dependence of the bridge hydrogen chemical shift studies, IR studies in the OH, OD, and C=O stretch regions, and the HMO calculations, that there may probably be two structures for the enol form of acetylacetone. The difference between these two structures arises mainly from the electronic structure of the π-system. The relative population of these two structures at various temperatures for normal acetylacetone and at room temperature for the deuterated acetylacetone were calculated.

稀土铁双核配合物的合成

本文通过LnCl_3·nTHF和[C_5H_4(SiMe_3)]Na反应得到了两类配合物[C_5H_4(SiMe_3)] LnCl_2·nTHF (Ln = Nd，Sm，Gd；n = 0，1，2)、[C_5H_4(SiMe_3)] LnCl_2·HCl·nTHF (Ln = Nd，Sm，Gd；n = 1，2)。通过元素分析、红外分析、质谱、核磁共振和热重分析确定了配合物的分子组成，特别是带氯化氢的产品在红外光谱中有1250 cm~(-1)，835 cm~(-1)，748 cm~(-1)自的三甲基硅基特征吸收峰。对氯化稀上进行了结构分析，结果发现LnCl_3·4THF (Ln = Sm，Gd)是与NdCl_3·4THF之间存在着变态关系。GdCl_3·4THF。晶体属单斜晶系，空间群为P21/C，晶胞参数为a = 30.765(7)，b = 8.219(3)，C = 17.534(3)A~·，β = 93.71(2)°；SmCl_3·4THF。晶体属单斜晶系，空间群为P21/C，晶胞参数为a = 30.921(13)，b = 8.287(7)，C = 17.665(8)，β = 94.17(4)°。LnCl_3·4THF的单位晶胞中存在着八个分子，每对分子互相等同，但每对分子内部两个分子之间互不等同。SmCl_3·2THF·DME晶体属单斜晶系，空间群为P21/a，晶胞参数为a = 13.547(8)，b = 8.607(4)，C = 16.029(9)A°，β = 90.53(5)°。铲原子与三个氯原子。两个四氢呋喃中的氧原子以及DME中的两个氧原子键合，形成七配位的配合物，但是配位多面体不是理想的五角双锥，而是形成了比五角双锥(D_(5h))对称性更低的多面体(C_(3v))。它能看作是在正八面体的一个面的中心加上第七个原子的结果，而且这八面体主要受到决定上述那个面的三个原子伸展开的畸变。在制备C_5H_5SiMe_3时，如果不用减压蒸馏，而在常压下直接蒸馏，则得到的不是C_5H_5SiMe_3而是它的二聚体(C_5H_5SiMe_3)_2。用红外光谱和核磁共振确定了它的组成和结构，特别是在1650 cm~(-1)处出现(C_5H_5SiMe_3)_2的孤立双键吸收峰。用C_5H_5SiMe_3和Ee(CO)_5回流反应制得了[C_5H_4(SiMe_3) Ee(CO)_2]_2。经过元素分析，红外光谱，质谱，顺磁共振确定了配合物的组成，红外光谱中有桥羰基的吸收峰，质谱图中498的离子峰的出现标志着上述二聚体的存在。用[C_5H_5Fe(CO)_2]_2作为制备双金属配合物的原料，用Na/Hg并还原[C_5H_5Fe(CO)_2]_2。反应时间为6-7小时得到中间体[C_5H_5Fe(CO)_2]_2Na·4THF的深紫红色晶体。反应时间加长，中间体被破坏，反应到15小时时生成了[C_5H_5Fe(CO)_2]Na·TMEDA的黄色晶体，特别是中间体的获得及晶体结构的测定对我们解释反应的机理非常重要。[C_5H_5Fe(CO)_2]_2Na·4THF为单斜晶系，空间群为P21/n，晶胞参数为a = 10.155(5)，b = 17.121(4)，C = 18.667(6)A°，β = 97.61(3)°，V = 3216.9A°~3， 2 = 4。铁的配位数为七，钠的配位数为六，钠离子和桥连羰基氧以配位键结合，每个钠离子连结着两个[C_5H_5Fe(CO)_2]_2~-，而每个[C_5H_5Fe(CO)_2]_2~-又连结着两个钠离子，组成一个无限链状分子，键状分子间以Van de W力结合。[C_5H_5Fe(CO)_2]Na·TMEDA正交晶系，空间群为P_(2,2,2,)。晶胞参数为a = 6.001(4)，b = 10.644(6)，C = 24.214(11)A~·。α = β = r = 90°。z = 4 V = 1546·7A°~3，铁的配位数为五。钠的配位数为四，钠离子和羰基氧以配位键结合，每个钠离子连结着两个[C_5H_5Fe(CO)_2]~-，每个[C_5H_5Fe(CO)_2]~-又连结着两个钠离子，体系就是以这种连结方式或正负电荷交替的形式无限螺旋分子，每个链节存在着两个[C_5H_5Fe(CO)_2]Na·TMEDA分子，链节的长度为a轴的轴长，说明螺旋分子以a轴轴长向上平移。用LnCl_3·nTHF和[C_5H_5Fe(CO)_2]Na反应制得了[C_5H_5Fe(CO)_2] LnCl_2·nTHF (Ln = Nd, Sm, Gd; n = 1, 2)，用[C_5H_5Fe(CO)_2] LnCl_2和[C_5H_4(SiMe_3)]Na或用[C_5H-4(SiMe_3)] LnCl_2和[C_5H_5Fe(CO)_2]Na得到[C_5H_5Fe(CO)_2] [C_5H_4(SiMe_3)] LnCl·nTHF (Ln = Nd, Sm, Gd; n = 0, 1, 3)，配合物[C_5H_5Fe(CO)_2] LnCl_2·nTHF及[C_5H_5Fe(CO)_2] [C_5H_4(SiMe_3)] LnCl·nTHF中存在着2000 cm~(-1)左右的终端羰基吸收峰及1766 cm~(-1)左右的桥连羰基吸收峰。说明稀土和铁之间是以羰基相连的。在TOTOE质谱仪上，配合物[C_5H_5Fe(CO)_2]Gd~·Cl·THF出现[C_5H_5Fe(CO)]GdCl_2、[Fe(CO)_2] Gd~+Cl_2的离子峰，配合物[C_5H_5Fe(CO)_2]-[C_5H_4(SiMe_3)] GdCl·THF出现[C_5H_5Fe(CO)_2] [C_5H_4]Gd~+Cl、[C_5H_5Fe(CO)_2]Gd~+Cl·[C_5H_4C(SiMe_3)] Gd~+Cl等离子峰。所有稀土有机配合物都溶于四氢呋喃、苯，对空气和水敏感。

正交晶系结构相角二价表达式的代数推导及其在晶体结构测定中的应用

本文用代数方法推导了正交晶系五十九个空间群的结构半不变量相同的二价表达式。就每一个空间群都得出了一系列公式。在222点群中的空间群都有形如以下三式的公式：E_(2h+2h';2k+2k'.0) = (N~(3/2)/g1)<(-1)~(α1)UE_(hkg))~2-1)UE_(h'k'α')|~2-1) >_(hkp;h'k'α') (0.1) E_(2h+2h'0.2α+α) = (N~(3/2)/g2)<(-1)~(α2)UE_(hkg))~2-1)UE_(h'k'α')|~2-1) >_(hkp;h'k'α') (0.2) E_(0.2h+2h'2α+2α) = (N~(3/2)/g3)<(-1)~(α3)UE_(hkg))~2-1)UE_(h'k'α')|~2-1) >_(hkp;h'k'α') (0.3) 其中g_i, α_i (i = 1, 2, 3) 与具体空间群有关。在mm2点群中的空间群都可得出六个公式，在mmm点群中的空间群都可得出二十八个公式。首先按照从低级到高级的顺序，将PT，P_(21)，P(2/N),C_(2/c)空间群的二价代数表达式进行了应用，然后将P_(2,2,2),P(na21)空间群的二价代数表达式进行了应用。由于未找到mmm点群空间群的结构实例，故为mmm点群空间群的公式未予应用附加地，推导了四方晶系I_(42a),I_(41/a)两空间群的公式，对I_(42a)的公式也进行了应用，由应用结果可得出：（一）代数方法推导的思路和数学方法是验证正确的，在含有主原子的结构中，由强度量算法的二十至三十个相角基本与正确值吻合（一般只有一、二个不等）。（二）在代数方法计算的同时，也进行了概率Σ_4元素的计算，可以得出，代数方法速度要快得多，特别是正交晶系中，时间上的优势更突出，数据剔除的依据也更比概率Σ_4关系明显。（三）代数方法在含有重原子的结构中比只含轻原子的结构中好用。这种特点和概率Σ_4关系一样。另外，和论文题目独立地，在低温条件下作者测定了杂多酸K_(11)[DY(SiMo_(11)O_(39))_2],28H_2O的晶体结构，晶体属单斜晶系的P_(21/n)空间群，Z = 4， 晶格参数为：a = 17.256(3), b = 26.817(4), C = 21.797(4)A, β = 104.39(1)°，最后的R = 0.0637。

环戊二烯基轻稀土氯化物的合成及其稳定性的研究

I LnCl_3-LiCl-THF配合物的研究深入地研究了氯化稀土和氯化锂于四氢呋喃溶液中，以不同的摩尔比，在不同条件下的反应。实验结果表明，反应速度随着稀土元素原子半径的减小，LiCl/LnCl_3摩尔比的增大，以及四氢呋喃用量的增加而加快。通过紫外质谱元素分析和X-射线单晶结构分析等证明，随着不同的LiCl/LnCl_3摩尔比和结晶条件的不同，可以得到不同组成的LnCl_3-LiCl-TNF配合物。对(LaCl)(THF)_2(μ_2-Cl)_4[Li(THF)_2]_2和(LaCl)DME(μ_3-Cl)(μ_2-Cl)_5(La·DME)Li(THF)_2晶体的结构分析表明，前者为单斜晶系，P21/C空间群。a=10.542(4), b=32.236(4), c=11.182(6)A °; β=113.50(3) °, V=3484.97 A °~3. Z=4, R=0.0471；后者为三斜晶系，PT空间群，晶胞参数是：a=11.123(3), b=16.564(5), c=8.653(3)A °;α=95.16(3), β=95.63(3), γ=74.71(3) °;V=1527.0A °~3。Z=2，R=0.0303。实验结果还表明，μ_2-和μ_3-氯桥键是LnCl_3-LiCl-THF类配合物中最基本、最重要的配位键，这种键是通过多重键的方式起着稳定分子结构的作用。当进行与有机配体的交换反应时，由于它们的特殊稳定性，能起到阻止轻稀土有机配合物歧化反应的作用。II环戊二烯基轻镧系氯化物的合成及其稳定性的研究对(G_5H_5)_3Ln·THF和LnCl_3·3LiCl-THF (Ln=La, Nd)溶液反应的研究表明，由于μ_2-氯桥键的作用，轻稀土环戊二烯基化合物中环戊二烯基的再分配反应，在0℃或室温下都能迅速进行。通过两者不同的摩尔比反应，经元素分析、红外光谱、~1H NMR和质谱鉴定，方便地合成了C_5H_5 LnCl_2·2LiCl·5THF和(C_5H_5)_2LnCl.LiCl·nTHF (Ln=La, Nd)等配合物。这一结果表明(C_5H_5)_2LnCl.LiCl·nTHF配合物不仅能稳定地存在于THF溶液中，而且能在一定条件下析出结晶。对(C_5H_5)_2LaCl.LiCl·4THF的晶体结构测定表明，该晶体属于正交晶系，Pc2m空间群。a=12.306(4), b=23.056(6), c=26.701(11)A°; V=7575.81A°~3;而(C_5H_5)_2LaCl·LiCl(DME)_2THF晶体则属于六方晶系，a=12.967(4), b=12.967(4), c=24.108(10)A°;V=3510 A°~3。通过(G_5H_5)_3Ln·THF与LnCl_3·3THF (Ln=La, Nd)的反应进一步研究了轻稀土环戊二烯基氯化物的稳定性。经元素分析，红外光谱和晶体结构分析表明合成了[(η~5-C_5H_5)_4La_3Cl_5·3THF]_2·9THF和(C_5H_5)_2 NdCl·THF配合物，前者属于三斜晶系，P1空间群。a=11.690(3), b=11.750(5), c=18.433(6)A°; α=98.75(3), β=95.62(3), γ=118.92(2)°; V=2147.06 A°~3. Z=1, R=0.099。对环戊二烯基轻稀土氯化物的稳定性进行了较详细地讨论。结果表明，THF的用量和化合物的溶解度是影响产物组成的决定因素。当THF的量不足以溶解所生成的产物时，就会歧化成溶解度最大((C_5H_5)_3Ln·THF)和最小(LnCl_3·nTHF)的两种组分。反之，环戊二烯基轻稀土化合物(Ln=La, Nd)中环戊二烯基的再分配反应就能顺利进行。经元素分析和结构测定，在((C_5H_5)_3Nd·THF)和NdCl_3·LiCl-THF溶液的反应体系中，偶然分离得到了[(η~5-C_5H_5)_4Nd_4(μ_4-o)(μ_2-Cl)_8] [Li(DMP)_2THF]_2这一不合常规的化合物，其晶体属于正交晶系，Pna2,空间群a=19.010(7), b=23.231(6), c=14.180(4); V=6261.91 A°~3。Z=4, R=0.054。说明在一定条件下,μ-氧桥键也起到了稳定分子结构的作用。推测了各类环戊二烯基轻稀土氯化物在THF中的合成反应机理,在LiCl存在的反应体系中Ln cl cl Li桥键能与环戊二烯基发生交换反应;在(C_5H_5)_3Ln·THF和LnCl_3·3THF的反应体系中,首先存在着LnCl_3分子之间的互相作用，因而易于形成双核或多核配合物。这类配合物以晶体形式析出时，易于发生结构上的变化，即化合物的结晶形态与溶液中的形态不一定相同。探索了环戊二烯基烯丙基稀土化合物新的合成方法。找到了真空加热脱水制备氯化稀土的最佳条件，其产物纯度在97%以上。通过加入Co_3O_4/Wo_3催化助燃剂的方法，提高了测定稀土有机化合物中碳含量的准确性。

结构因子相角的代数解法及K_8H_5[La(SiWMo_(10)O_(39))(SiW_3Mo_8O_(39))]·nH_2O的晶体结构

一 结构因子相角的代数解法晶体结构研究中的相角问题，一直是晶体学工作者努力探求的基本问题。几十年来，关于相角问题的研究已经取得了巨大的进展，直接法的成熟和普遍应用就是这个进展的显著标志。在直接法相角问题研究中，历来存在两种基本方法，即概率法和代数法。当前直接法的迅猛发展，则主要以概率法为基础，其应用的基本公式即是来自∑关系中的∑_2关系和由此发展出的TANGENT公式，并结合一系列的基本理论和辅助公式，从而使直接法的发展一直呈方兴未艾之势。与此形成鲜明对照的是，相角问题的代数法研究则有日趋下降之势，尤其近十年来则显著落后了。作者从近年来的∑关系研究中，看到要解决相角问题，代数法仍然有其潜在的应作价值，并认为在概率法可以得到应用的许多方面，在代数法那里都应找到对应的类似内容，而代数法在研究和应用中所表现出的不同于概率法的那些方面也正是在相角问题研究中最令人感兴趣的问题，这就是我们进行代数法研究的目的和出发点。（一）1.5和2.5阶代数式的提出及对±2~(II)型相角的估算。（二）一般类型相角的估算（三）结构相角通用代数式的推导。代数法不仅可用于结构半不变量O，π型相角的计算，而且可用于非结构半不变量的种种类型相角的估算，其中包括型和一般类型相角，而且其应用效果完全可以和概率法相比拟，在机时利用上前者有一定优势。通用代数式的获得将为代数法的普遍应用和计算机计算创造了方便条件。二稀土杂多酸根配合物K_8H_5[La(SiWMo_(10)O_(39))(SiW_3Mo_8O_(39))]·nH_2O的晶体结构采用低温技术，在-90 ℃的干燥氮气保护下，收集晶体衍射数据，以直接法解出结构。a = 17.485(5), b = 27.096(6), c = 21.642(5)A, β = 107.79(2)°, z = 4。最后的R值为0.097。中心离子La(III)同两个杂多酸根提供的8 个氧配合。而其中的W、Mo同氧的配位情况基本相同，者是与氧六配位，形成变形配位八面体。

卟啉LB膜结构表征和电性质研究

利用膜天平、紫外-可见分光光度计、红外光谱仪、电子显微镜以及X-射线衍射仪等手段研究了新合成的尚未见文献报道的材料的界面膜和LB膜的性质和结构，对卟啉LB膜导电特性和气敏特性也进行了初步研究，得到下述结论：（1）利用预处理的新方法研究了界面膜的性质，研究结果表明预处理过程能用于判别界面膜的存在状态。（2）随着取代基上碳原子数增加，分子在水面上占据表观截面积呈现增大趋势。（3）取代链的长度对膜的沉积类型有重要影响，短链取代卟啉仅能以Z型方式沉积，而长链取代卟啉能以Y或Z型方式沉积。（4）取代侧链的长度对卟吩环取向影响较小，几种化合物的取向角在30°- 40°之间。（5）花生酸与TPIAPP掺杂后可减弱卟啉分子在LB膜中的相互作用。（6）取代链长度对膜结构的有序性有影响。短链取代卟啉不能给出布拉格衍射峰。（7）混合膜中，由于卟啉的混杂使花生酸的相变向低温方向移动，并有熔程变长的现象。（8）所研究材料的LB膜面的内导电能力较差，加入NH_3和NO_2后膜的电导不发生显著变化。

毛蕊异黄酮类似物的合成及其对JAK/STAT信号途径调控的构效关系研究

干扰素（IFNs）是最早发现的具有广泛用途的一类细胞因子，IFN-α通过JAK/STAT信号途径调控机体一系列生理和病理反应。至今尚未发现类干扰素的小分子。我们前期研究发现天然产物毛蕊异黄酮可激活干扰素诱导的JAK/STAT信号途径。为发现类干扰素小分子、获得小分子探针，本课题拟建立成熟的JAK/STAT信号途径的筛选模型，合成毛蕊异黄酮及其类似物，研究这些化合物的构效关系，进而尝试通过共价键标记生物素或香豆素来直接研究它们与相关受体的作用。 从异香草醛出发经7步合成反应得到了毛蕊异黄酮。采用平行合成策略得到异黄酮类化合物；采用分支式合成策略，以取代苯乙酸作为合成砌块，获得具有与异黄酮类似结构的香豆素、3-芳基喹诺酮。与分离得到的黄酮类化合物，构建了一个包括异黄酮、黄酮、香豆素、3-芳基喹诺酮在内的化合物库。 建立了包含IFN-α刺激反应元件 (ISRE)的荧光素酶报告基因体系，通过筛选化合物库中的化合物，发现异黄酮骨架为激活JAK/STAT信号途径必须结构、毛蕊异黄酮7-位酚羟基被取代后活性丧失。根据以上结果，对毛蕊异黄酮3′-位标记物的合成进行了初步尝试。 发现山茱萸科植物青荚叶(Helwingia japonica (Thunb.) Dietr.)有抑制蛋白酪氨酸磷酸酯酶1B（PTP1B）的活性。从其地上部分95%乙醇提取物的乙酸乙酯部分分离得到5个化合物,应用波谱方法及与已知品对照的手段鉴定它们为p-menth-2-en-1β, 4β, 8-triol (Z-1)、blumenol A (Z-2)、2′,3′,4′,5′,6′-五羟基查尔酮(Z-3)、洋芹素7-O-β-D-吡喃葡萄糖苷(Z-4)、木犀草素7-O-β-D-吡喃葡萄糖苷(Z-5). Interferons (IFNs) are one kind of cytokines with broad functions. IFN-α mediates series physiological and pathological changes of human body via JAK/STAT pathway. Untill now, no IFNs-like small molecules are discovered. In our preliminary experiment, the natural product calycosin has been observed to activate JAK/STAT pathway. Therefore, we establish a luciferase reporter gene system and synthesize calycosin and its analogues to reveal their structure-activity relationship (SAR). Besides, in order to prove that calycosin activates JAK/STAT pathway through IFN receptor, we attempted to tag it with biotin or coumarin by covalent bonding. Calycosin was synthesized from isovanillin via seven steps. Other isoflavones were obtained by parallel synthesis; coumarins and quinolones were prepared through divergent synthesis, using substituted phenylacetic acids as building blocks. Combing with natural flavones, a small molecule library was established. A luciferase reporter gene system, consisting of 5 copies of the ISRE (interferon-stimulated response element), was used for screening of small molecules from that library. We found that the core-structure of isoflavone was necessary, and if the 7-OH is substituted, the activity slumps. According to our observation, we tried to tag biotin or coumarin at 3′-OH of calycosin. The 95% ethanol extract of the aerial parts of Helwingia japonica (Thunb.) Dietr. showed protein tyrosine phosphatase 1B (PTP1B) inhibitory activity. Five compounds were isolated. On the basis of spectral data or by comparison with authentic samples, they were identified as p-menth-2-en-1β,4β,8-triol (1), blumenol A (2), 2′,3′,4′,5′,6′-pentahydroxychalcone (3), apigenin 7-O-β-D-glucopyranoside (4), and luteolin 7-O-β-D-glucopyranoside (5).

Phoswich探测器测量重离子在生物组织中的核碎片

利用 HIRFL (兰州重离子研究装置 )产生的 5 5 Me V/ u的4 0 Ar17+ 离子束 ,用由 Cs I(Tl) +快塑料闪烁探测器组成的 Phoswich探测器 ,以 1.5 mm有机玻璃为等效生物组织材料 ,探索了研究等效生物组织中核碎片测量的方法。对实验中可能出现的问题及解决方法进行了探讨。结果表明探测器对 Z可分辨到 16。元素分辨率为 Z/ ΔZ约为 4 0。

低能铁离子注入氨基酸分子改性和质量沉积

用110keV Fe+注入L（+）-半胱氨酸薄膜样品,经盐酸溶解后通过缓慢蒸发育成纯物质单晶,并对其中一粒单晶用四圆衍射仪进行了X射线衍射分析.晶体属单斜晶系,空间群为C2,晶体学参数a=1.8534（4）nm,b=0.5234（1）nm,c=0.7212（1）nM,β=103.72（3）°,V=0.67965（3）nm3,Z=4,F（000）=144.0,Dclac=1.763 g·cm-3,μ（MoKα）=1.06mm-1,T=293（2）K.最终一致性因子R=0.0379,wR=0.0835.晶体化合物的化学式为[CH2CH（NH2）NO2]ClFe（Mr=180.38）.提纯了重离子束改性分子并直接证实注入铁离子在新分子中的质量沉积.相同注量的110 keV Fe+离子注入L（+）-半胱氨酸盐酸盐单晶水合物薄膜样品后的Fourier变换红外光谱分析表明,样品分子受到严重损伤,产生了很大变化.

~(28)Si+~(12)C中的两体反应与全熔合反应

利用ΔE E望远镜系统测量了 1 56 3MeV2 8Si+ 12 C反应 (近对称系统 )中出射的Z =4— 1 4的产物元素的能谱和角分布 ,并由此给出了这些产物的胁变截面图 .从理论上计算了Z =4— 1 1产物的实验室系最可几动能分布E1(θ)和各元素的质心系的总动能分布Et(Z) ,指出了这些产物主要来自系统的两体反应过程 .还给出了该反应系统的全熔合截面值为 (980± 68)mb ,并指出从低能数据外推到此能量下的全熔合截面值与实验值之差主要归因于两体过程 .

同中子素核9C、8B、7Be和6Li在中能区与28Si反应总截面的测量

放射性束流(RIB)装置拓广了实验核物理在同位旋(T_z)自由度上从稳定核直到滴线核的广袤空间。通常，位于β-稳定线及其附近的核，N／Z在1－1.5范围变化，其分离能E_s无论对于质子还是中子，总是在6-8 MeV之间；对于远离稳定线的非稳定核，N／Z可在0.5-4范围变化，如~9C的N／Z = 0.5，~(10)He的N／Z = 4，而且分离能E_s是在0-40 MeV之间变化的，开展对这些远离β-稳定线非稳定核性质、结构的研究是目前核物理的前沿之一。核反应总截面σ_R是表征原子核性质特征的一个基本物理量，从实验测得的核反应总截面中可以得到有关核结构和核内核子分布的信息。在由放射性束流所产生奇异核的结构与各种反应机制研究中，反应总截面的测量更是有其特殊的重要性，具有奇异核结构如晕核的一个典型的物理特征就是其反应总截面要比稳定核大得多，Tanihata等人最早就是通过对放射性束流的相互作用截面的测量发现了具有奇异结构的核，即中子晕核。由于反应总截面的测量对探测器的要求不高，而且数据分析过程相对较为简单，因而反应总截面的测量已经成为放射性束核物理的研究的一个非常重要实验手段。中子晕核以及中子皮核的发现促使人们去寻找质子晕核和质子皮核，由于最后一个质子的结合能非常小只有136，keV，并且有较大的电四极矩，因而使得~8B成为质子晕的最大热门候选核，有关~8B是否具有质子晕核结构的问题，许多实验科学家得出了相互矛盾的回答；而目前有关另外一个质子晕候选核~9C的实验数据非常少，目前还没有人从实验上对~9C是否为质子晕核这一问题进行肯定或否定的回答。因此非常有必要测量~9C和~8B的反应总截面。对反应总截面进行研究的一个非常有用理论就是Glauber模型，该模型考虑了库伦效应的多次散射理论。它是一种基于自由核子-核子(N-N)碰撞的与核物质密度相关的理论，因而能够从实验测量到的反应总截面中提取核物质分布的信息。该理论对中低能区的反应总截面描述却有一个缺憾：理论值比实验值都要小。本论文主要描述了利用透射法测量了中能区同中子素核~9C、~8B、~7Be及~6Li与~(28)Si的反应总截面，并介绍了重离子碰撞以及描述重离子性质的几种常用理论。在论文里对实验测量得到的结果进行了理论分析，这些理论包括半经验的Shen公式、Glauber模型、BUU模型以及SHF理论。如果将~9C和~8B当成具有正常核结构来处理，半经验的Shen公式和Glauber模型(HO密度分布)的理论计算值总是比实验值要小得多；对于Glauber模型的理论计算值和实验值的差异，Ozawa等定义了一个差值因子d，方德清等人对轻核系统的d值进行了详细的分析。一般认为，正常核的d值在20％以内，而对于具有晕或皮奇异结构的核，其d值则超过30％，甚至可达50％，因此可根据一个核的d值是否超过30％而且比相邻核的d值明显大这种半经验的方法来判断一个核是否具有奇异结构；利用d值的分析结果，我们认为：~9C和~8B都具有奇异核结构；对于BUU模型用同样的方法引进差值因子d值，对于~9C和~8B有相同的结论。用SHF理论计算得到B和C同位素的密度分布结果显示，~9C和~8B的密度分布比相邻的同位素扩展都要大得多。为减小Glauber模型计算的反应截面与实验值的差别，本论文还对Glauber模型的输入密度形式进行了修改，在原单一HO分布基础上加一个高斯分布的尾巴，并对丰质子的同中子素核~9C、~8B、~7Be及~6Li与~(28)Si靶以及~(12)C和丰中子的C同位素核~(13-16)C与~(12)C靶的反应截面重新进行了计算，结果显示在中能区的计算值比原来单一密度分布的计算结构有明显改善。