Author/Authors :
Kalliokoski، نويسنده , , T. and Bezrukov، نويسنده , , L. and Enqvist، نويسنده , , T. and Fynbo، نويسنده , , H. and Inzhechik، نويسنده , , L. and Jones، نويسنده , , P. and Joutsenvaara، نويسنده , , Mikko J. and Karjalainen، نويسنده , , J. and Kuusiniemi، نويسنده , , P. and Loo، نويسنده , , K. and Lubsandorzhiev، نويسنده , , B. and Petkov، نويسنده , , V. and Rنihن، نويسنده , , T. and Sarkamo، نويسنده , , J. and Slupecki، نويسنده , , M. and، نويسنده ,
Abstract :
The knee is a change in the slope of the cosmic ray spectrum at approximate energy of 3 PeV. There are multiple competing models for the knee giving conflicting predictions about this change for different masses of the primary particle. Accurate mass measurements of cosmic rays spectra around 3 PeV would be able to exclude some of these models. Cosmic-ray experiment EMMA uses a new method for studying the composition of cosmic rays at the knee area. It is able to determine the multiplicity, the lateral distribution, and the arrival direction of incoming muons produced early in the shower evolution on an event-by-event basis and deduce from these measurements the mass and the energy of the primary particle. EMMA is situated at the depth of 75 m in the Pyhنsalmi mine, Finland. This rock overburden, which corresponds to 210 m of water equivalent, gives EMMA a cut-off energy of 50 GeV for vertical muons. Since the simulations using different air-shower models give similar predictions for the lateral distribution of these high energy muons, we are confident that EMMA should yield a reliable and an air-shower model independent data on the composition of cosmic rays around the knee region.
