Skip to main navigation Skip to search Skip to main content

An accelerator search at 900 GeV CM energy for the Centauro phenomenon

  • G. J. Alner
  • , R. E. Ansorge
  • , B. Åsman
  • , C. N. Booth
  • , L. Burow
  • , P. Carlson
  • , R. S. Dewolf
  • , A. Drees
  • , B. Eckart
  • , G. Ekspong
  • , I. Evangelou
  • , A. Eyring
  • , J. P. Fabre
  • , L. Fröbel
  • , C. Fuglesang
  • , J. Gaudaen
  • , C. Geich-Gimbel
  • , B. Holl
  • , R. Hospes
  • , D. P. Johnson
  • K. Jon-And, Th Kokott, F. Lotse, N. Manthos, R. Meinke, D. J. Munday, J. E.V. Ovens, W. Pelzer, J. J. Reidy, J. G. Rushbrooke, H. Schmickler, F. Triantis, W. Pelzer, J. J. Reidy, J. G. Rushbrooke, H. Schmickler, F. Triantis, L. Van Hamme, Ch Walck, C. P. Ward, D. R. Ward, C. J.S. Webber, T. O. White, G. Wilquet, N. Yamdagni

Research output: Contribution to journalArticlepeer-review

32 Scopus citations

Abstract

A search for the Centauro phenomenon has been made at s = 900 GeV using the UA5 detector at the SPS pp collider operated in a pulsed mode. Possible interpretations of the cosmic ray data are discussed leading to various analyses of our data which exploit the distinctive features of the Centauro events: high multiplicity, high pT and absence of produced photons. No indication of Centauro production is observed. Upper limits on the production of Centauros at the level of a few per thousand inelastic events are obtained.

Original languageEnglish
Pages (from-to)415-422
Number of pages8
JournalPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Volume180
Issue number4
DOIs
StatePublished - Nov 20 1986

Fingerprint

Dive into the research topics of 'An accelerator search at 900 GeV CM energy for the Centauro phenomenon'. Together they form a unique fingerprint.

Cite this