The techniques to be used in a balloon borne experiment APEX to detect 220 MeV antiprotons are described, paying particular attention to potential sources of background. Event time history is shown to be very effective in eliminating this background. Results of laboratory tests on the timing resolution which may be achieved are presented
The PAMELA experiment is based on a satellite-borne equipment actually in the final integration phas...
The balloon-borne Isotope Matter-Antimatter Experiment (IMAX) was flown from Lynn Lake, Manitoba, Ca...
Stopped antiproton annihilation can initiate an effcient chain of reactions to produce Ξ hyperons in...
We report on the absolute antiproton flux and the antiproton to proton ratio in the energy range 0.6...
A balloon-borne instrument has measured the cosmic-ray antiproton flux between 130 and 320 MeV and s...
Most cosmic ray antiprotons observed near the Earth are secondaries produced in collisions of energe...
Recent experimental observations and results are discussed. It was found that the approximately 50 a...
A balloon-borne instrument has been used to detect cosmic-ray antiprotons. These are identified topo...
Cosmic ray antiprotons can originate from dark matter annihilating into quarks that subsequently dec...
A tracking calorimeter made of 3200 brass streamer tubes together with 3200 pick-up strips has been ...
We report new results for the cosmic-ray antiproton-to-proton ratio from 3 to 50 GeV at the top of t...
Up to one million antiprotons from a single LEAR spill have been captured in a large Penning trap. S...
Searching for cosmic antiprotons, balloon-borne experiments were performed in the last years, but wi...
This paper describes the Monte Carlo program used for the simulation of antiproton interactions at i...
This research was sponsored by the National Science Foundation Grant NSF PHY 87-1440
The PAMELA experiment is based on a satellite-borne equipment actually in the final integration phas...
The balloon-borne Isotope Matter-Antimatter Experiment (IMAX) was flown from Lynn Lake, Manitoba, Ca...
Stopped antiproton annihilation can initiate an effcient chain of reactions to produce Ξ hyperons in...
We report on the absolute antiproton flux and the antiproton to proton ratio in the energy range 0.6...
A balloon-borne instrument has measured the cosmic-ray antiproton flux between 130 and 320 MeV and s...
Most cosmic ray antiprotons observed near the Earth are secondaries produced in collisions of energe...
Recent experimental observations and results are discussed. It was found that the approximately 50 a...
A balloon-borne instrument has been used to detect cosmic-ray antiprotons. These are identified topo...
Cosmic ray antiprotons can originate from dark matter annihilating into quarks that subsequently dec...
A tracking calorimeter made of 3200 brass streamer tubes together with 3200 pick-up strips has been ...
We report new results for the cosmic-ray antiproton-to-proton ratio from 3 to 50 GeV at the top of t...
Up to one million antiprotons from a single LEAR spill have been captured in a large Penning trap. S...
Searching for cosmic antiprotons, balloon-borne experiments were performed in the last years, but wi...
This paper describes the Monte Carlo program used for the simulation of antiproton interactions at i...
This research was sponsored by the National Science Foundation Grant NSF PHY 87-1440
The PAMELA experiment is based on a satellite-borne equipment actually in the final integration phas...
The balloon-borne Isotope Matter-Antimatter Experiment (IMAX) was flown from Lynn Lake, Manitoba, Ca...
Stopped antiproton annihilation can initiate an effcient chain of reactions to produce Ξ hyperons in...