报告题目：The origin of Cosmic Rays and Unidentified VHE sources

报 告 人：Omar Tibolla, Institut für Theoretische Physik und Astrophysik, University of Würzburg

报告时间：2月23日（周四）16:00

报告地点：郑裕彤讲堂

报告摘要：The riddle of the origin of Cosmic Rays is open since one century and no final answer has been provided so far. Gamma ray observations above 100 MeV reveal the sites of cosmic ray acceleration to energies where they are unaffected by solar modulation. In the last years the knowledge in this field of research widely increased, however almost 50% of the TeV (> 10^12 eV) Galactic sources are still unidentified; at GeV (> 10^9 eV) energies, 67% of EGRET sources were unidentified and also with the newer generation of gamma-ray satellites we have the same result: in fact, at low Galactic latitudes (b < 10 deg), 62% of the fermi lat detected sources have no formal counterpart. hence understanding the high energy unidentified sources will be a crucial brick in solving the whole riddle of cosmic rays origin.

After the successful first VHE Galactic Plane Survey of 2004, H.E.S.S. has continued and extended that survey in 2005-2008, discovering a number of new sources, many of which are unidentified. Some of the unidentified H.E.S.S. sources have several positional counterparts and hence several different possible scenarios for the origin of the VHE gamma-ray emission; their identification remains unclear. Others have so far no counterparts at any other wavelength. Particularly, the lack of an X-ray counterpart puts serious constraints on emission models.