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首页> 外文期刊>The Journal of Chemical Physics >CROSSED BEAM REACTION OF ATOMIC CARBON, C(P-3(J)), WITH THE PROPARGYL RADICAL, C3H3((XB2)-B-2) - OBSERVATION OF DIACETYLENE, C4H2(X-1-SIGMA(G)(+))
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CROSSED BEAM REACTION OF ATOMIC CARBON, C(P-3(J)), WITH THE PROPARGYL RADICAL, C3H3((XB2)-B-2) - OBSERVATION OF DIACETYLENE, C4H2(X-1-SIGMA(G)(+))

机译:原子碳C(P-3(J))与丙基自由基C3H3((XB2)-B-2)的束流反应-对苯二甲酸,C4H2(X-1-SIGMA(G)(+)的观察)

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The reaction of ground-state carbon, C(P-3(j)), with the propargyl radical, C3H3((XB2)-B-2), is investigated at an average collision energy of 42.0 kJmol(-1) employing the crossed molecular beams technique and a universal mass spectrometric detector. The laboratory angular distribution and time-of-flight spectra of the C4H2 product are recorded at m/e = 50. Forward-convolution fitting of our data reveals the formation of diacetylene, HCCCCH, in its X-1 Sigma(g)(+) electronic ground state. The reaction dynamics are governed by an initial attack of C(P-3(j)) to the pi-electron density at the acetylenic carbon atom of the propargyl radical, followed by a [1,2]-hydrogen migration to the n-C4H3 isomer. A final carbon-hydrogen bond rupture yields atomic hydrogen and diacetylene through a tight exit transition state located 30-60 kJmol(-1) above the products. This first successful crossed molecular beams study of a reaction between an atom and a free radical marks the beginning of the next generation of crossed beams experiments elucidating the formation of molecular species in combustion processes, chemical vapor deposition, in the interstellar medium, outflows of carbon stars, and hydrocarbon-rich planetary atmospheres via radical-radical reactions. (C) 1997 American Institute of Physics. [S0021-9606(97)04144-5]. [References: 27]
机译:研究了基态碳C(P-3(j))与炔丙基C3H3((XB2)-B-2)在平均碰撞能为42.0 kJmol(-1)下的反应。交叉分子束技术和通用质谱检测器。在m / e = 50的情况下记录了C4H2产物的实验室角分布和飞行时间谱。我们数据的正向卷积拟合揭示了乙炔HCCCCH在其X-1 Sigma(g)(+ )电子基态。反应动力学受C(P-3(j))对炔丙基自由基炔碳原子上pi电子密度的初始攻击所控制,然后由[1,2]氢迁移至n- C4H3异构体。最终的碳氢键断裂通过位于产物上方30-60 kJmol(-1)的紧密出口过渡态产生原子氢和丁二炔。首次成功的交叉分子束研究是原子与自由基之间的反应,标志着下一代交叉束实验的开始,该实验阐明了燃烧过程中分子物质的形成,化学气相沉积,星际介质中碳的流出恒星和自由基引起的富含碳氢化合物的行星大气。 (C)1997美国物理研究所。 [S0021-9606(97)04144-5]。 [参考:27]

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