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Stardust, supernovae, neutrinos and the chirality of the amino acids

  • R. N. Boyd*
  • , T. Kajino
  • , T. Onaka
  • *此作品的通讯作者
  • Lawrence Livermore National Laboratory
  • National Astronomical Observatory of Japan
  • The University of Tokyo

科研成果: 期刊稿件会议文章同行评审

摘要

A mechanism for creating amino acid enantiomerism that involves selection of one chirality by interactions with the neutrinos from a core-collapse supernova is defined. This selection mechanism involves the alignment between the spins of the neutrinos and of the 14N nuclei in the amino acids, or in precursor molecules, which in turn couple to the molecular chirality. Details of the chiral selection, as well as the subsequent chemical evolution and galactic mixing that would ultimately populate the Galaxy with the selected species are discussed. The resulting amino acids could either be the source thereof on Earth or could have produced the chirality that was ultimately achieved for Earthly amino acids.

源语言英语
文章编号012032
期刊Journal of Physics: Conference Series
403
1
DOI
出版状态已出版 - 2012
已对外发布
活动Horizons of Innovative Theories, Experiments, and Supercomputing in Nuclear Physics, HITES 2012 - New Orleans, LA, 美国
期限: 4 6月 20127 6月 2012

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