Exclusion of cosmic rays from molecular clouds by self-generated electric fields
arXiv:2009.14208 · doi:10.3847/2041-8213/abbc20
Abstract
It was recently discovered that in some regions of the Galaxy, the cosmic ray (CR) abundance is several orders of magnitude higher than previously thought. Additionally, there is evidence that in molecular cloud envelopes, the CR ionization may be dominated by electrons. We show that for regions with high, electron-dominated ionization, the penetration of CR electrons into molecular clouds is modulated by the electric field that develops as a result of the charge they deposit. We evaluate the significance of this novel mechanism of self-modulation and show that the CR penetration can be reduced by a factor of a few to a few hundred in high-ionization environments, such as those found near the Galactic center.
arXiv commentAccepted by ApJ Letters
References in corpus (24)
- Our astrochemical heritage
- Cosmic-ray ionization of molecular clouds
- Investigating the Cosmic-Ray Ionization Rate in the Galactic Diffuse Interstellar Medium through Observations of H3+
- Simultaneous Acceleration of Protons and Electrons at Nonrelativistic Quasiparallel Collisionless Shocks
- Cosmic-ray ionisation in circumstellar discs
- The cosmic ray ionization rate in the Galactic disk, as determined from observations of molecular ions
- Protostellar Disk Formation Enabled by Removal of Small Dust Grains
- Effective destruction of CO by cosmic rays: implications for tracing H gas in the Universe
- The structure and stability of molecular cloud cores in external radiation fields
- The Different Structures of the Two Classes of Starless Cores
- The Origin of Diffuse X-ray and -ray Emission from the Galactic Center Region: Cosmic Ray Particles
- Impact of low-energy cosmic rays on star formation
- Decoupling of Magnetic Fields in Collapsing Protostellar Envelopes and Disk Formation and Fragmentation
- Cosmic-ray and X-ray Heating of Interstellar Clouds and Protoplanetary Disks
- Physical conditions in the central molecular zone inferred by H3+
- The Central 300 pc of the Galaxy probed by infrared spectra of H and CO: part I. Predominance of warm and diffuse gas and high H ionization rate
- Chemistry and Radiative Transfer of Water in Cold, Dense Clouds
- Penetration of cosmic rays into dense molecular clouds: role of diffuse envelope
- Cosmic ray penetration in diffuse clouds
- Parallel electric field generation by Alfven wave turbulence
- Tentative Evidence for Relativistic Electrons Generated by the Jet of the Young Sun-like Star DG Tau
- Diffusive Versus Free-Streaming Cosmic Ray Transport in Molecular Clouds
- Gas and dust temperature in pre-stellar cores revisited: New limits on cosmic-ray ionization rate
- Magnetic Mirroring and Focusing of Cosmic Rays