Published December 18, 2012 | Version v1
Journal article

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

  • 1. Lawrence Livermore National Laboratory, Livermore, CA 94550 (United States)
  • 2. National Astronomical Observatory of Japan, 2-21-1 Mitaka, Tokyo, 181–8588 (Japan)
  • 3. University of Tokyo, Department of Astronomy, Graduate School of Science, 7-3-1, Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan)

Description

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.

Availability note (English)

Available from http://dx.doi.org/10.1088/1742-6596/403/1/012032

Additional details

Publishing Information

Journal Title
Journal of Physics. Conference Series (Online)
Journal Volume
403
Journal Issue
1
Journal Page Range
[7 p.]
ISSN
1742-6596

Conference

Title
Conference on horizons of innovative theories, experiments, and supercomputing in nuclear physics
Acronym
HITES 2012
Dates
4-7 Jun 2012
Place
New Orleans, LA (United States)