Add to ORKGAbstract We discuss the main sources of uncertainties in the calculation of the positron and antip...
In the frame work of energy dependent confinement for cosmic rays, the energy spectrum inside the so...
Recent experimental observations and results are discussed. It was found that the approximately 50 a...
It may be possible to account for a previously puzzling feature - a bump in the energy range 10 to t...
The relative merits and difficulties of the primary and secondary origin hypotheses for the observed...
Particle acceleration within turbulent region for analysis on fluctuation origin of cosmic radiatio
The possibility is investigated that the reported excess low energy antiproton component of the cosm...
The relative merits and difficulties of the primary and secondary origin hypotheses for the observed...
If antiprotons in cosmic rays are produced as secondary particles in sources, it is expected that po...
The interstellar antiproton calculations were reexamined in view of the recent progress in measureme...
The physics of the annihilation of photinos is considered as a function of mass in detail, in order ...
In the present work, the origin of antiprotons observed in cosmic rays (above the atmosphere) is ana...
Journal ArticleWe use the depth of maximum distribution as measured by the stereo Fly's Eye detector...
A balloon-borne instrument has measured the cosmic-ray antiproton flux between 130 and 320 MeV and s...
The flux of secondary antiprotons expected for the leaky-box model was calculated as well as that fo...
Abstract We discuss the main sources of uncertainties in the calculation of the positron and antip...
In the frame work of energy dependent confinement for cosmic rays, the energy spectrum inside the so...
Recent experimental observations and results are discussed. It was found that the approximately 50 a...
It may be possible to account for a previously puzzling feature - a bump in the energy range 10 to t...
The relative merits and difficulties of the primary and secondary origin hypotheses for the observed...
Particle acceleration within turbulent region for analysis on fluctuation origin of cosmic radiatio
The possibility is investigated that the reported excess low energy antiproton component of the cosm...
The relative merits and difficulties of the primary and secondary origin hypotheses for the observed...
If antiprotons in cosmic rays are produced as secondary particles in sources, it is expected that po...
The interstellar antiproton calculations were reexamined in view of the recent progress in measureme...
The physics of the annihilation of photinos is considered as a function of mass in detail, in order ...
In the present work, the origin of antiprotons observed in cosmic rays (above the atmosphere) is ana...
Journal ArticleWe use the depth of maximum distribution as measured by the stereo Fly's Eye detector...
A balloon-borne instrument has measured the cosmic-ray antiproton flux between 130 and 320 MeV and s...
The flux of secondary antiprotons expected for the leaky-box model was calculated as well as that fo...
Abstract We discuss the main sources of uncertainties in the calculation of the positron and antip...
In the frame work of energy dependent confinement for cosmic rays, the energy spectrum inside the so...
Recent experimental observations and results are discussed. It was found that the approximately 50 a...