Add to ORKGThe physics of the annihilation of photinos is considered as a function of mass in detail, in order to obtain the energy spectra of the cosmic ray antiprotons produced under the assumption that photinos make up the missing mass in the galactic halo. The modulated spectrum is at 1 a.w. with the cosmic ray antiprotons data. A very intriguing fit is obtained to all of the present antiprotons up to 13.4 GeV data for similar to 15 GeV. A cutoff is predicted in the antiprotons spectrum at E = photino mass above which only a small flux from secondary production should remain
We examine the solar modulation of cosmic ray protons and antiprotons, and discuss the resulting ef...
Relationships between recent measurements of cosmic ray electrons, nonthermal galactic radio emissio...
High-energy collisions of cosmic-ray nuclei with interstellar gas are believed to be the mechanism p...
It may be possible to account for a previously puzzling feature - a bump in the energy range 10 to t...
Solution of Fokker-Planck diffusion equation in intensity prediction of antiproton component of prim...
The relative merits and difficulties of the primary and secondary origin hypotheses for the observed...
It is found that the measured data on the degree of anisotropy of cosmic rays are consistent with ou...
The possibility is investigated that the reported excess low energy antiproton component of the cosm...
In this paper we study the antiproton, positron and gamma-ray fluxes resulting from the annihilation...
The relative merits and difficulties of the primary and secondary origin hypotheses for the observed...
Recent experimental observations and results are discussed. It was found that the approximately 50 a...
The flux of cosmic-ray antiprotons from neutralino annihilations in the Galactic halo is computed fo...
If antiprotons in cosmic rays are produced as secondary particles in sources, it is expected that po...
We examine the transport of cosmic-ray protons and anitprotons from local interstellar space through...
The flux of cosmic ray antiprotons from neutralino annihilations in the galactic halo is computed fo...
We examine the solar modulation of cosmic ray protons and antiprotons, and discuss the resulting ef...
Relationships between recent measurements of cosmic ray electrons, nonthermal galactic radio emissio...
High-energy collisions of cosmic-ray nuclei with interstellar gas are believed to be the mechanism p...
It may be possible to account for a previously puzzling feature - a bump in the energy range 10 to t...
Solution of Fokker-Planck diffusion equation in intensity prediction of antiproton component of prim...
The relative merits and difficulties of the primary and secondary origin hypotheses for the observed...
It is found that the measured data on the degree of anisotropy of cosmic rays are consistent with ou...
The possibility is investigated that the reported excess low energy antiproton component of the cosm...
In this paper we study the antiproton, positron and gamma-ray fluxes resulting from the annihilation...
The relative merits and difficulties of the primary and secondary origin hypotheses for the observed...
Recent experimental observations and results are discussed. It was found that the approximately 50 a...
The flux of cosmic-ray antiprotons from neutralino annihilations in the Galactic halo is computed fo...
If antiprotons in cosmic rays are produced as secondary particles in sources, it is expected that po...
We examine the transport of cosmic-ray protons and anitprotons from local interstellar space through...
The flux of cosmic ray antiprotons from neutralino annihilations in the galactic halo is computed fo...
We examine the solar modulation of cosmic ray protons and antiprotons, and discuss the resulting ef...
Relationships between recent measurements of cosmic ray electrons, nonthermal galactic radio emissio...
High-energy collisions of cosmic-ray nuclei with interstellar gas are believed to be the mechanism p...
