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CR COMPOSITION AT THE BREAK AREA. Shaulov S.B. , Cherdyntceva K.V., Chubenko A.P., Kokobaev M., Kruglov A.V., Krupchatnicova J.A., Nesterova N.M., Nicolskaya N.M., Pavluchenko V.P., Piscal V.V., Vildanov N.G., Vildanova L.I. Введение. Объявите цель доклада Представьтесь. - PowerPoint PPT Presentation
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6-12 Sept., 2004, Pylos
CR COMPOSITION AT THE BREAK AREA
Shaulov S.B., Cherdyntceva K.V., Chubenko A.P., Kokobaev M., Kruglov A.V., Krupchatnicova J.A.,
Nesterova N.M., Nicolskaya N.M., Pavluchenko V.P., Piscal V.V., Vildanov N.G., Vildanova L.I.
6-12 Sept., 2004, Pylos
Введение
Объявите цель доклада Представьтесь
6-12 Sept., 2004, Pylos
HADRONHADRON(Tien-Shan, 3340m)
Emulsion chambers
EAS array
6-12 Sept., 2004, Pylos
Dependencies <Nm>-Ne are compared for two groups of
EAS:-All EAS (~400 000)-EAS with families (~1700)-one EC (~6400)-two EC (2004)
Selection criteria:-EAS in circle R 20 m, with zenith angles
30°families at EC: еEeV,1 (1 ~70%)
6-12 Sept., 2004, Pylos
<N> - Ne dependencies
6-12 Sept., 2004, Pylos
What is strange here?
1. <N> - Ne dependencies coincide for two groups up to break and differ above them.
2. EAS+ are the proton events mainly and must have relatively small muon numbers, i.e.
<N> - Ne for EAS+ must lay under one for all EAS !!!
6-12 Sept., 2004, Pylos
This discrepancy with ordinary situation don’t depends of CR composition, because…
6-12 Sept., 2004, Pylos
Mix composition <
N>
Ne
Fe
Protons
- Protons with
6-12 Sept., 2004, Pylos
Possible methodical distortions
were checked:
1. Vertical moving EAS+ curve because of muon LDF difference for EAS and EAS+ -
absent as LDFs coincide2. Horizontal moving EAS+ curve because of Ne-E0 difference for EAS
and EAS+ - difference exists, but in opposite direction…
6-12 Sept., 2004, Pylos
Model (M. Tamada) E0-Ne for EAS and EAS+
6-12 Sept., 2004, Pylos
What does it means ?
1. Primary nuclei, consisting of nucleons, can’t generate EAS which have EC -quanta and relatively large <N> simultaniousely!
2. A new EAS component arise above the EAS spectrum break.
3. This component origin is unknown. - It may be part of primary CR (SQM-?) - It may be generated by CR nuclei at atmosphere (QGM-?)4. The experimental data permit to conclude
that we deal with not-nucleus component at area above EAS spectrum break!
6-12 Sept., 2004, Pylos
Ne spectrum for EAS+
Preliminary
EAS+
6-12 Sept., 2004, Pylos
Additional conclusions … It seams that the new experimental
method EAS+EC permits to resolve the break problem, so this kind experiment necessary to develop.
If a new component has an astrophysical origin and consists of SQM particles with mass ~1 TeV, then it may explains the absence of CR spectrum cut for energy ~51019 eV (GZK-effect).
6-12 Sept., 2004, Pylos