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Characterization of carbonaceous materials for their accessibility to methane-a concept of accessible pore size distribution

机译:碳质材料表征其可接近甲烷的能力-可访问孔径分布的概念

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Structural determination of coal and carbon based materials has been a subject of great interest to adsorption and coal scientists for many decades. The structural parameters, such as void volume, surface area, pore-size and pore-size distribution, have been determined from various theories or approaches. For example, void volume is usually determined by the helium expansion method, surface area from the BEt theory and the pore size from various classical theories such as the Hovarth-Kawazoe (HK), SaitoFoley (SF), Dubinin-Stoeckli (DS), Barrett-JoynerHalenda (BJH), Broekhoff-de Boer (BdB) theories, etc. More recently, tools such as Density Functional theory and Monte Carlo molecular simulation, have been applied to these problems, and these have helped to remove many of the difficulties associated with the limited applicability of the classical theories, for example to microporous solids (HK, SF, DS) or to mesoporous solids (BJH and BdB). Other problems associated with the classical approach are (i) the possibility of helium adsorption in fine pores, (ii)the improper assumptions inherent in the BET theory and (iii) the assumption of a specific geometry for the pore in the determination of pore size distribution, for example the HK and DS equations are designed for slits, SF theory is for cylinders, and BJH and BdB were developed for slits and cylinders (extension to spherical pores is also possible). Real solids do not conform to these geometries and therefore by making these assumptions about pore shape, the pore size distribution is treated qualitatively and can only be used as an indicator to compare one sample against the others in the same family. With these limitations inherent either in the theories or in the way the procedure is carried out, the derived information on pore volume, surface area and pore size distribution will have a limited value. Here we present a development of a consistent and coherent means to derive pore volume, surface area and pore size distribution. Recognizing the fact that these structural parameters depend on the molecular probe, we give examples of both methane and argon as molecular probes. By assuming known atomic configurations for the carbonaceous solids, we show how the void volume, geometrical area and pore size can be obtained as accessible quantities using Monte Carlo integration. The inaccessible solid volume is simply the difference between the total system volume and the accessible void volume. The challenge that faces us ahead is the experimental determination of these accessible parameters.
机译:煤炭和碳基材料的结构测定是对许多数十年来吸附和煤科学家感兴趣的主题。已经从各种理论或方法确定了结构参数,例如空隙体积,表面积,孔径和孔径分布。例如,空隙体积通常由氦膨胀方法,来自BET理论的表面积和来自各种古典理论的孔径,例如Hovarth-Kawazoe(HK),Saitoley(SF),Dubinin-Stoeckli(DS), Barrett-Joynerhalenda(BJH),Broekhoff-de Boer(BDB)理论等。最近,密度泛函理论和蒙特卡罗分子模拟等工具已应用于这些问题,这些问题有助于消除许多困难与经典理论的有限适用性相关,例如微孔固体(HK,SF,DS)或中孔固体(BJH和BDB)。与经典方法相关的其他问题是(i)在细孔中的氦吸附的可能性,(ii)BET理论中固有的不适当的假设和(iii)在测定孔径时对孔的特定几何形状的假设分布,例如,HK和DS方程设计用于狭缝,SF理论是用于圆柱体,而BJH和BDB是为狭缝和圆柱体开发的(也可以延伸到球形孔隙)。真实固体不符合这些几何形状,因此通过使这些关于孔形状的假设,定性处理孔径分布,并且只能用作指示器,以将一个样品与同一家族中的其他样品进行比较。通过在理论中固有的这些限制,或者在进行过程的方式中,孔隙体积,表面积和孔径分布的衍生信息将具有有限的值。在这里,我们展示了一致的和相干方法来衍生孔体积,表面积和孔径分布。认识到这些结构参数取决于分子探针的事实,我们提供甲烷和氩气作为分子探针的实例。通过假设用于碳质固体的已知原子构型,我们展示了如何使用Monte Carlo集成作为可接近量获得空隙体积,几何区域和孔径。无法访问的固体体积是总系统体积和可移空隙体积之间的差异。我们面临的挑战是对这些可访问参数的实验确定。

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