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.
arXiv comment10 pages, 11 figures, accepted for publication in MNRAS
References in corpus (31)
- HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
- Embedded Clusters in Molecular Clouds
- Theory of Star Formation
- Characterizing interstellar filaments with Herschel in IC5146
- Scattering by Interstellar Dust Grains: Optical and Ultraviolet
- Physical Properties and Galactic Distribution of Molecular Clouds identified in the Galactic Ring Survey
- Discovery of the Interstellar Chiral Molecule Propylene Oxide (CHCHCHO)
- Millimeter-wave polarization of protoplanetary disks due to dust scattering
- Modeling UV Radiation Feedback from Massive Stars: II. Dispersal of Star-Forming Giant Molecular Clouds by Photoionization and Radiation Pressure
- 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
- Radiative grain alignment in protoplanetary disks: Implications for polarimetric observations
- 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
- Outflow-Confined H II Regions. I. First Signposts of Massive Star Formation
- Escape of Lyman-alpha and continuum photons from star-forming galaxies
- ART^2 : Coupling Lyman-alpha Line and Multi-wavelength Continuum Radiative Transfer
- Radiation hydrodynamics simulations of massive star cluster formation in giant molecular clouds
- Extended High Circular Polarization in the Orion Massive Star Forming Region: Implications for the Origin of Homochirality in the Solar System
- High resolution imaging polarimetry of HL Tau and magnetic field structure
- Star cluster formation and cloud dispersal by radiative feedback: dependence on metallicity and compactness
- Near Infrared Circular Polarization Images of NGC 6334-V
- The escape of ionizing photons from supernova-dominated primordial galaxies
- Multiple scattering of polarized radiation by non-spherical grains: first results
- 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