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水合作用和空间(熵)压力对磷脂酰胆碱双层膜间相互作用的贡献:亚凝胶相实验

Contributions of hydration and steric (entropic) pressures to the interactions between phosphatidylcholine bilayers: experiments with the subgel phase.

作者信息

McIntosh T J, Simon S A

机构信息

Department of Cell Biology, Duke University Medical Center, Durham, North Carolina 27710.

出版信息

Biochemistry. 1993 Aug 17;32(32):8374-84. doi: 10.1021/bi00083a042.

Abstract

The total repulsive interaction between electrically neutral, fluid bilayer membranes is thought to have a number of components, including a hydration pressure, due to the reorientation of water by the bilayer, and steric (entropic) pressures due to bilayer undulations, head group motion, and molecular protrusions. For fully hydrated, crystalline bilayers these three steric pressures should be relatively small, and the major repulsive pressure present should be the hydration pressure. Therefore, to isolate the contribution of hydration pressure to the total interbilayer interaction, we have measured pressure-distance data by X-ray diffraction analysis of osmotically stressed dipalmitoylphosphatidylcholine (DPPC) multilayers in the subgel phase, where wide-angle and low-angle X-ray data show the bilayers are crystalline. As applied pressure was increased from 0 to 1 x 10(6) dyn/cm2, the interbilayer fluid space (df) decreased less than 1 A from its value at full hydration of 8.4 A. As the pressure was increased from 1 x 10(6) to 3 x 10(7) dyn/cm2, df decreased from about 8 to 4 A. For this range of df, the repulsive pressure decayed exponentially with df with a decay length of 1.4 A. Further increases in applied pressure did not appreciably decrease df, so that there was a sharp upward break in the pressure-distance curve at an interbilayer spacing of about 3 A. In contrast, pressure-distance relations for gel (L beta') phase and liquid-crystalline (L alpha) phase bilayers had much softer upward breaks at df < 5 A and extended to larger df at zero applied pressure. However, the pressure-distance curves for all three phases decayed exponentially with approximately the same decay length for 4 < df < 8 A. We interpret these data to mean the following: (1) the repulsion observed for df < 5 A is primarily a steric pressure whose range depends on head group motion; (2) the steric undulation pressure plays an important role in determining the hydration properties and the range of the total repulsive pressure for fluid membranes; (3) the same underlying mechanisms govern the repulsive pressure for all phases for 4 < df < 8 A; (4) these mechanisms include a pressure due to reorientation of water molecules; and (5) the hydration pressure component extents a maximum of about two water molecules from the bilayer surface for the subgel phase.

摘要

电中性的流体双层膜之间的总排斥相互作用被认为有多个组成部分,包括由于双层膜使水重新定向而产生的水合压力,以及由于双层膜波动、头部基团运动和分子突出而产生的空间(熵)压力。对于完全水合的晶体双层膜,这三种空间压力应该相对较小,主要的排斥压力应该是水合压力。因此,为了分离水合压力对双层膜间总相互作用的贡献,我们通过对亚凝胶相的渗透应激二棕榈酰磷脂酰胆碱(DPPC)多层膜进行X射线衍射分析,测量了压力-距离数据,其中广角和低角度X射线数据表明双层膜是晶体。当施加压力从0增加到1×10⁶达因/平方厘米时,双层膜间流体空间(df)从其在完全水合时8.4埃的值减少不到1埃。当压力从1×10⁶增加到3×10⁷达因/平方厘米时,df从约8埃减少到4埃。对于这个df范围,排斥压力随df呈指数衰减,衰减长度为1.4埃。施加压力的进一步增加并没有明显减小df,因此在双层膜间距约为3埃时,压力-距离曲线出现急剧向上的转折。相比之下,凝胶(Lβ')相和液晶(Lα)相双层膜的压力-距离关系在df<5埃时有更平缓的向上转折,并且在零施加压力下延伸到更大的df。然而,对于4<df<8埃,所有三个相的压力-距离曲线以大致相同的衰减长度呈指数衰减。我们对这些数据的解释如下:(1)对于df<5埃观察到的排斥主要是一种空间压力,其范围取决于头部基团运动;(2)空间波动压力在决定流体膜的水合性质和总排斥压力范围方面起重要作用;(3)对于4<df<8埃,相同的潜在机制控制所有相的排斥压力;(4)这些机制包括由于水分子重新定向产生的压力;(5)对于亚凝胶相,水合压力分量从双层膜表面延伸最多约两个水分子。

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