Supernovae and the Chirality of the Amino Acids

被引:15
作者
Boyd, R. N. [1 ,2 ]
Kajino, T. [2 ,3 ]
Onaka, T. [3 ]
机构
[1] Lawrence Livermore Natl Lab, Livermore, CA 94551 USA
[2] Natl Astron Observ, Tokyo 181, Japan
[3] Univ Tokyo, Dept Astron, Grad Sch Sci, Tokyo 113, Japan
基金
美国国家科学基金会;
关键词
Amino acids; Chirality; Origin of life; Molecular clouds; Supernova neutrinos; ASYMMETRIC AUTOCATALYSIS; ENANTIOMERIC EXCESS; OPTICAL-ACTIVITY; STAR-FORMATION; AMPLIFICATION; ABSORPTION; NEUTRINOS; CHEMISTRY; REGIONS; CLOUDS;
D O I
10.1089/ast.2009.0427
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A mechanism for creating amino acid enantiomerism that always selects the same large-scale chirality is identified, and subsequent chemical replication and galactic mixing that would populate the Galaxy with the predominant species is described. This involves (1) the spin of the N-14 in the amino acids, or in precursor molecules from which amino acids might be formed, that couples to the chirality of the molecules; (2) the neutrinos emitted from the supernova, together with the magnetic field from the nascent neutron star or black hole formed from the supernova, which selectively destroy one orientation of the N-14 and thus select the chirality associated with the other N-14 orientation; (3) chemical evolution, by which the molecules replicate and evolve to more complex forms of a single chirality on a relatively short timescale; and (4) galactic mixing on a longer timescale that mixes the selected molecules throughout the Galaxy.
引用
收藏
页码:561 / 568
页数:8
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