On the Cosmic Ray-Induced Ionization Rate in Molecular Clouds

الملخص EN

The transformation of the energy dependence of the cosmic ray proton flux in the keV to GeV region is investigated theoretically when penetrating inside molecular clouds (Av>5 mag).

The computations suggest that energy losses of the cosmic ray particles by interaction with the matter of the molecular cloud are principally caused by the inelastic (electronic) interaction potential; the transformed energy distribution of energetic protons is determined mainly by the column density of the absorbing medium.

A cutoff of the cosmic ray spectrum inside clouds by their magnetic fields is also phenomenologically taken into account.

This procedure allows a determination of environment-dependent ionization rates of molecular clouds.

The theoretically predicted ionization rates are in good agreement with those derived from astronomical observations of H3+ absorption lines in the spectrum of the cloud connected with the Herbig Be star LkHα 101.