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

  • R. N. Boyd*
  • , T. Kajino
  • , T. Onaka
  • *Corresponding author for this work
  • Lawrence Livermore National Laboratory
  • National Astronomical Observatory of Japan
  • The University of Tokyo

Research output: Contribution to journalConference articlepeer-review

Abstract

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.

Original languageEnglish
Article number012032
JournalJournal of Physics: Conference Series
Volume403
Issue number1
DOIs
StatePublished - 2012
Externally publishedYes
EventHorizons of Innovative Theories, Experiments, and Supercomputing in Nuclear Physics, HITES 2012 - New Orleans, LA, United States
Duration: 4 Jun 20127 Jun 2012

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