منابع مشابه
Galactic cosmic rays & gamma rays : a synthesis
We have developed a model which aims to reproduce observational data of many kinds related to cosmic-ray origin and propagation: direct measurements of nuclei, antiprotons, electrons and positrons, γ-rays, and synchrotron radiation. Our main results include evaluation of diffusion/convection and reacceleration models, estimates of the halo size, calculations of the interstellar positron and ant...
متن کاملGamma rays from the Galactic bulge and large extra dimensions.
An intriguing feature of extra dimensions is the possible production of Kaluza-Klein gravitons by nucleon-nucleon bremsstrahlung, in the course of core collapse of massive stars, with gravitons then being trapped around the newly born neutron stars and decaying into two gamma rays, making neutron stars gamma-ray sources. We strengthen the limits on the radius of compactification of extra dimens...
متن کاملDark Matter and Gamma Rays from the Galactic Halo
The nature of the dark matter in the halo of our Galaxy is still largely unknown. The microlensing events found so far towards the Large Magellanic Cloud suggest that at most about 20% of the halo dark matter is in the form of MACHOs (Massive Astrophysical Compact Halo Objects). The dark matter could also, at least partially, consist of cold molecular clouds (mainly H2). Another possibility is ...
متن کاملHigh Energy Diffuse Gamma-Rays from Galactic Plane
The dominant part of the diffuse gamma rays beyond 1 TeV from the Galactic plane has been thought as due to the inverse Compton scattering of interstellar photons with high-energy cosmic-ray electrons. In these energy regions, diffuse gamma-ray observations give us unique information on the energy spectrum of high-energy electron in the interstellar space, since we cannot observe those electron...
متن کاملEvidence for Dark Matter Annihilation from Galactic Gamma Rays?
The diffuse galactic EGRET gamma ray data show a clear excess for energies above 1 GeV in comparison with the expectations from conventional galactic models. The excess is seen with the same spectrum in all sky directions, as expected for Dark Matter (DM) annihilation. This hypothesis is investigated in detail. The energy spectrum of the excess is used to limit the WIMP mass to the 50-100 GeV r...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Journal of Physics G: Nuclear and Particle Physics
سال: 2007
ISSN: 0954-3899,1361-6471
DOI: 10.1088/0954-3899/34/7/019