Stellar Explosions and the Mystery of Life's Left-Handed Molecules ✛ ✎ ✦

Original: "Supernova Neutrinos and the Origin of Biomolecular Homochirality"
arXiv:2607.12813 · 2026-07-14 · arXiv non-exclusive · independent analysis · 1 min
A neutrino breeze from supernovae, blowing for billions of years, gently nudged life's building blocks into mirror asymmetry.

All amino acids in proteins are left-handed, all sugars in DNA are right-handed. This homochirality was inherited by life from the cosmos. Schrödinger had pondered the origin of order, and Wu showed that the weak force distinguishes sides. Zwicky added that supernova explosions bombard everything with neutrinos. Now a model explains: a neutrino breeze, blowing for billions of years, gently nudged molecules toward one mirror form.

This nudge was minuscule, but chemistry amplified it: the arising imbalance accelerated its own growth, like a snowball starting an avalanche. In interstellar gas clouds at –170°C, a simulation confirmed that over 300 million years, a surplus of more than 10% left-handed molecules appears. The Murchison meteorite holds exactly this same excess.

A twist of fate: had the neutrino wind been different, DNA would have coiled the other way, and familiar enzymes wouldn't assemble — life as we know it wouldn't have happened.

This means that distant stellar explosions not only gave us our atoms but also dictated life's very architecture — across the Universe, it might turn out the same. Spectroscopes are already searching for confirmation.

Neutrinos are so ghostly they pass through the Earth without a trace, yet their age-old influence shaped the very basis of all earthly life.

In Michael Crichton's novel 'The Andromeda Strain,' alien life uses the opposite mirror form of molecules, and this becomes a threat to humanity.

\Delta E_{\mathrm{PV}} \sim G_F \Delta_{R,S}\langle \gamma^5 \rangle n_\nu
An energy shift on the order of 10^{-22} eV, creating a preference for one of the mirror isomers.
k_s \approx \frac{\Delta E_{\mathrm{PV}}}{h} \exp\left(-\frac{G_{\mathrm{rac}}}{RT}\right)
Determines the rate of chiral symmetry breaking; with typical parameters, it is 10^{-16} – 10^{-15} s^{-1}.
Scientists
Subrahmanyan ChandrasekharEnrico FermiAugustin-Louis CauchyChristiaan HuygensEmmy NoetherIsaac Newton
Concepts
black hole neutrino source solar neutrino antineutrino halo nuclei prebiotic chemistry astrochemical synthesis nucleosynthesis supernova chemical evolution stars gene expression noise methanol biomolecule chirality stellar chemical abundances kilonova helium burning photochemistry triple-alpha process (Hoyle process) neutrino dark matter interactions neutrino sources