Generation of high circular polarization of interstellar Lyman radiation triggering biological homochirality
arXiv:2306.12101 · doi:10.1093/mnras/stad1899
Abstract
The homochirality of biological molecules on the Earth is a long-standing mystery regarding the origin of life. Circularly polarized ultraviolet (UV) light could induce the enantiomeric excess of biological molecules in the interstellar medium, leading to the homochirality on the earth. By performing 3D radiation transfer simulations with multiple scattering processes in interstellar dusty slabs, we study the generation of circular polarization (CP) of ultraviolet light at Lyman () as well as in the near-infrared (NIR, ) wavelengths. Our simulations show that the distributions of CP exhibit a symmetric quadrupole pattern, regardless of wavelength and viewing angle. The CP degree of scattered light from a dusty slab composed of aligned grains is percent for Ly and percent at NIR wavelengths in the case of oblate grains with an MRN size distribution. We find that the CP degree of Ly is well correlated with that in the NIR regardless of viewing angles, whilst being a factor of higher. Thus, high CP of Ly is expected in sites where NIR CP is detected. We suggest that such circularly polarized Ly may initiate the enantiomeric excess of biological molecules in space.
10 pages, 11 figures, accepted for publication in MNRAS
References in corpus (15)
- Theory of Star Formation
- Discovery of the Interstellar Chiral Molecule Propylene Oxide (CHCHCHO)
- Observations of the Lyman- Universe
- The Astrodust+PAH Model: A Unified Description of the Extinction, Emission, and Polarization from Dust in the Diffuse Interstellar Medium
- Star Formation Efficiency and Dispersal of Giant Molecular Clouds with UV Radiation Feedback: Dependence on Gravitational Boundedness and Magnetic Fields
- The Dielectric Function of "Astrodust" and Predictions for Polarization in the 3.4m and 10m Features
- Radiation hydrodynamics simulations of massive star cluster formation in giant molecular clouds
- Star cluster formation and cloud dispersal by radiative feedback: dependence on metallicity and compactness
- Upper stellar mass limit by radiative feedback at low-metallicities: metallicity and accretion rate dependence
- Near-Infrared Circular Polarization Survey in Star-Forming Regions: Correlations and Trends
- Far and extreme UV radiation feedback in molecular clouds and its influence on the mass and size of star clusters
- Ly-alpha Radiative Transfer: A Stokes Vector Approach to Ly-alpha Polarization
- High circular polarization of near infrared light induced by micron-size dust grains
- On Far-Infrared and Submm Circular Polarization
- SEURAT: SPH scheme extended with ultraviolet line radiative transfer