๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Neutrino induced charm production in the CHORUS experiment

โœ Scribed by Oliver Melzer


Publisher
Elsevier Science
Year
1999
Tongue
English
Weight
343 KB
Volume
75
Category
Article
ISSN
0920-5632

No coin nor oath required. For personal study only.

โœฆ Synopsis


The CHORUS experiment has been designed to detect decays of r leptons coming from v~ ---* v~ neutrino oscillation using nuclear emulsion as primary neutrino target. The ability for detecting decays of short-lived particles can be used to search for charm particles produced via deep inelastic and diffractive neutrino interactions. Detection techniques and first observations of charm particle decays will be reported.


๐Ÿ“œ SIMILAR VOLUMES


Status of the CHORUS neutrino oscillatio
โœ Erhan Pesen ๐Ÿ“‚ Article ๐Ÿ“… 1999 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 378 KB

The CHORUS experiment is designed to search for v,, + v, oscillation with a hybrid detector system containing 800 kg nuclear emulsions as target and vertex detector. Run I (320 000 recorded u,,CC in 1!394/5) and more than haIf of the run II (460 000 u,,CC in 1996/7) data taking have been successfull

Prediction of neutrino fluxes in the NOM
โœ P Astier; D Autiero; A Baldisseri; M Baldo-Ceolin; M Banner; G Bassompierre; K B ๐Ÿ“‚ Article ๐Ÿ“… 2003 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 547 KB
The search for possible time variations
โœ H. J. Haubold; E. Gerth ๐Ÿ“‚ Article ๐Ÿ“… 1985 ๐Ÿ› John Wiley and Sons ๐ŸŒ English โš– 736 KB

With thc graclu:il accumulation of experimental data in the solar ncutrino experimcnt of DAVIS and collaborators (runs 18 -74 for 1970r g R ~) , the question, whttthcr there arc time variations of the solar neutrino flux, is of rcnewcd intcrcst. \Vc discuss tlic matliematical-numerical methods appli