Galactic Arm Structure and Gamma Ray Astronomy

In an attempt to explain the observed unexpectedly high energy gamma radiation over a broad region of the galactic plane in the general direction of the galactic center, a model is proposed wherein the galactic cosmic rays are preferentially located in the high matter density regions of galactic arm segments, as a result of the weight of the matter in these arms tieing the magnetic fields and hence the cosmic rays to these regions. The presently observed galactic gamma ray longitudinal distribution can be explained with the current estimate of the average galactic matter density, if the average arm to interarm matter ratio is five to one for the major arm segments toward the galactic center from the sun, and if the cosmic ray density normalized to its local value is assumed to be directly proportional to the matter density.