Maynard-Casely Helen E, Yevstigneyev Nikita S, Duyker Samuel G, Ennis Courtney
Australian Nuclear Science and Technology Organisation, Locked Bag 2001, Kirrawee DC, NSW, 2232, Australia.
Department of Chemistry, University of Otago, Dunedin, 9054, New Zealand.
Phys Chem Chem Phys. 2021 Dec 22;24(1):122-128. doi: 10.1039/d1cp04477j.
The crystal structure of propanal has been determined using powder X-ray diffraction (PXRD), where this common laboratory aldehyde is measured to crystallise in spacegroup 21/, = 4 with a unit cell = 8.9833(6) Å, = 4.2237(2) Å, = 9.4733(6) Å and = 97.508(6)°, resulting in a volume of 356.37(4) Å at 100 K and atmospheric pressure. The thermal expansion observed from 100 K until the sample melted (∼164 K) was found to be anisotropic. An additional neutron diffraction study was carried out, reaching a temperature of 3 K and found no further phase transformations from the determined structure at lower temperatures. The investigated temperature regime correlates to astronomical surfaces, including outer Solar System bodies and interstellar dust mantles, where propanal is thought to be generated by energetic processing of composite molecular ices. Results from the structure determination were applied to model propanal ice using periodic density functional theory for the calculation of intermolecular frequencies, where the simulated far-infrared spectrum of solid propanal can now be used for future molecular astronomy.
已使用粉末X射线衍射(PXRD)确定了丙醛的晶体结构,这种常见的实验室醛被测定为在空间群21/中结晶,α = 4,晶胞参数a = 8.9833(6) Å,b = 4.2237(2) Å,c = 9.4733(6) Å,β = 97.508(6)°,在100 K和大气压下体积为356.37(4) ų。从100 K到样品熔化(约164 K)观察到的热膨胀是各向异性的。还进行了一项额外的中子衍射研究,温度达到3 K,未发现低于该温度下确定结构的进一步相变。所研究的温度范围与天文表面相关,包括太阳系外天体和星际尘埃幔,在这些地方丙醛被认为是由复合分子冰的高能处理产生的。结构测定结果被应用于使用周期性密度泛函理论对丙醛冰进行建模,以计算分子间频率,其中固体丙醛的模拟远红外光谱现在可用于未来的分子天文学研究。