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Study of hadron bundles observed in chacaltaya two-story emulsion chamber
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Aoki, H. |
| Copyright Year | 1985 |
| Description | The existence of hadron-rich families associated with few gamma-ray emission named Centauro and Mini-Centauro phemonena was reported. It was investigated whether these are produced by the special type of interaction different from the ordinary pion multiple production or not. The experimental results are compared with simulation calculation based on ordinary multiple pion production model. Both hadron multiplicity distribution, obtained from the present observation and the simulation calculation, show almost the same distribution which means that hadron bundles of such smaller multiplicities are considered to originate from successive interactions of surviving nucleon with the nature of multiple production during passage through the atmosphere. |
| File Size | 174832 |
| Page Count | 4 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19850027609 |
| Archival Resource Key | ark:/13960/t72v7dx6k |
| Language | English |
| Publisher Date | 1985-08-01 |
| Access Restriction | Open |
| Subject Keyword | Space Radiation Hadrons Gamma Rays Particle Beams Energy Spectra Particle Emission Pion Beams Radiation Measurement Mathematical Models Nuclear Emulsions Bundles Nuclear Interactions Centaurus Constellation Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
