Determining amino acid chirality in the supernova neutrino processing model

Michael Famiano; Richard Boyd; Toshitaka Kajino; Takashi Onaka; Katrina Koehler; Sarah Hulbert

doi:10.3390/sym6040909

Determining amino acid chirality in the supernova neutrino processing model

Michael Famiano^*
, Richard Boyd
, Toshitaka Kajino
, Takashi Onaka
, Katrina Koehler
, Sarah Hulbert

^*Corresponding author for this work

Western Michigan University
Ohio State University
National Astronomical Observatory of Japan
The University of Tokyo
Los Alamos National Laboratory

Research output: Contribution to journal › Article › peer-review

10 Scopus citations

Abstract

A model is described that can be used to estimate the bulk polarization of large rotating meteoroids in the magnetic field of a neutron star. The results of this model are applicable to the Supernova Neutrino Amino Acid Processing model, which describes one possible way in which the amino acids, known in nearly all cases to exhibit supramolecular chirality, could have become enantiomeric.

Original language	English
Pages (from-to)	909-925
Number of pages	17
Journal	Symmetry
Volume	6
Issue number	4
DOIs	https://doi.org/10.3390/sym6040909
State	Published - 2014
Externally published	Yes

Keywords

Amino acids
Chirality
Neutrinos
Weak interact

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10.3390/sym6040909

Cite this

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title = "Determining amino acid chirality in the supernova neutrino processing model",

abstract = "A model is described that can be used to estimate the bulk polarization of large rotating meteoroids in the magnetic field of a neutron star. The results of this model are applicable to the Supernova Neutrino Amino Acid Processing model, which describes one possible way in which the amino acids, known in nearly all cases to exhibit supramolecular chirality, could have become enantiomeric.",

keywords = "Amino acids, Chirality, Neutrinos, Weak interact",

author = "Michael Famiano and Richard Boyd and Toshitaka Kajino and Takashi Onaka and Katrina Koehler and Sarah Hulbert",

note = "Publisher Copyright: {\textcopyright} 2014 by the authors.",

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doi = "10.3390/sym6040909",

language = "英语",

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pages = "909--925",

journal = "Symmetry",

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AU - Famiano, Michael

AU - Boyd, Richard

AU - Kajino, Toshitaka

AU - Onaka, Takashi

AU - Koehler, Katrina

AU - Hulbert, Sarah

PY - 2014

Y1 - 2014

N2 - A model is described that can be used to estimate the bulk polarization of large rotating meteoroids in the magnetic field of a neutron star. The results of this model are applicable to the Supernova Neutrino Amino Acid Processing model, which describes one possible way in which the amino acids, known in nearly all cases to exhibit supramolecular chirality, could have become enantiomeric.

AB - A model is described that can be used to estimate the bulk polarization of large rotating meteoroids in the magnetic field of a neutron star. The results of this model are applicable to the Supernova Neutrino Amino Acid Processing model, which describes one possible way in which the amino acids, known in nearly all cases to exhibit supramolecular chirality, could have become enantiomeric.

KW - Amino acids

KW - Chirality

KW - Neutrinos

KW - Weak interact

UR - https://www.scopus.com/pages/publications/84919615349

U2 - 10.3390/sym6040909

DO - 10.3390/sym6040909

M3 - 文章

AN - SCOPUS:84919615349

SN - 2073-8994

VL - 6

SP - 909

EP - 925

JO - Symmetry

JF - Symmetry

IS - 4

ER -

Determining amino acid chirality in the supernova neutrino processing model

Abstract

Keywords

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