通过气相质子转移反应优先破坏含有NH2的复杂星际分子
1Depts. of Chemistry & Astronomy, University of Virginia, Charlottesville, VA 22904, USA. rgarrod@virginia.edu.
复杂的含分子,如氨基,对于前生物化学至关重要,但很少被检测到. 新的研究表明,与氨的气相反应可以破坏这些分子,影响它们在太空中的检测能力.
科学领域:
- 天体化学是天体化学.
- 天体生物学 天体生物学
- 星际介质的化学介质
背景情况:
- 含的星际分子,特别是氨基,是前生物化学研究的关键目标.
- 它们在恒星和行星形成区域的检测是不一致的,尽管模型预测了它们的高丰度.
- 含氧的复杂有机分子 (COM) 通常比含NH2的物种更丰富.
研究的目的:
- 研究气相质子转移反应对复杂有机分子 (COM) 破坏的影响.
- 了解氨 (NH3) 在含的星际分子化学演变中的作用.
- 评估这些反应对氨酸和其他NH2载体物种的检测能力的影响.
主要方法:
- 模拟气相质子转移反应,涉及氨和各种COMs.
- 分析这些反应对星际分子的丰度和寿命的影响.
- 模拟分子丰度的化学年龄依赖.
主要成果:
- 与氨的质子转移反应显著减少了COMs的丰度和寿命,其质子亲和度大于氨.
- 氨充当质子穿器,通过分裂性重组导致甲基胺和尿素等分子的破坏.
- 源的化学年龄极大地影响了这些含物种的检测能力.
结论:
- 涉及氨的气相破坏途径限制了关键的含星际分子的丰富性和可检测性.
- 观察到的氨基的稀缺性可以通过这些质子转移反应的快速破坏来解释.
- 未来检测像甘氨酸这样的分子可能比预期的更具挑战性,因为气相破坏速度快.
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