CPL - Chalmers Publication Library
| Utbildning | Forskning | Styrkeområden | Om Chalmers | In English In English Ej inloggad.

Cosmic-Ray-Induced Ionization in Molecular Clouds Adjacent to Supernova Remnants

F. Schuppan ; Julia K. Becker ; John H. Black (Institutionen för rymd- och geovetenskap, Radioastronomi och astrofysik) ; S. Casanova ; M. Mandelartz
Cosmic Rays in Star-Forming Environments, Astrophysics and Space Science Proceedings Vol. 34 (2013), p. 317.
[Konferensbidrag, övrigt]

Energetic gamma rays (GeV to TeV photon energy) have been detected toward several supernova remnants (SNR) that are associated with molecular clouds. If the gamma rays are produced mainly by hadronic processes rather than leptonic processes like bremsstrahlung, then the flux of energetic cosmic ray nuclei (>1GeV) required to produce the gamma rays can be inferred at the site where the particles are accelerated in SNR shocks. It is of great interest to understand the acceleration of the cosmic rays of lower energy (<1GeV) that accompany the energetic component. These particles of lower energy are most effective in ionizing interstellar gas, which leaves an observable imprint on the interstellar ion chemistry. A correlation of energetic gamma radiation with enhanced interstellar ionization can thus be used to support the hadronic origin of the gamma rays and to constrain the acceleration of ionizing cosmic rays in SNR. Using observational gamma ray data, the primary cosmic ray proton spectrum can be modeled for E>1GeV, and careful extrapolation of the spectrum to lower energies offers a method to calculate the ionization rate of the molecular cloud.

Nyckelord: cosmic rays, gamma rays, molecular clouds

Denna post skapades 2013-12-09. Senast ändrad 2015-03-12.
CPL Pubid: 188678


Läs direkt!

Lokal fulltext (fritt tillgänglig)

Länk till annan sajt (kan kräva inloggning)