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Committee for cooperation of the Czech Republic with Joint Institute for Nuclear Research Login
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COMMITTEE
The main task of the Committee is organization of scientific cooperation between czech research and academic institutions and JINR.

Members of the Committee:

Bartova Eva (IBP ASCR)
Burdik Cestmir (FNSPE CTU)
Davidkova Marie (INP ASCR)
Dobes Jan (INP ASCR, Chairman of the Committee for cooperation of the Czech Republic with JINR)
Hedbavny Pavel (Czech Vacuum Society)
Chudoba Vratislav (Head of the national group of the CR in JINR)
Jancik Petr (FMST VSB-TUO)
Janosec Jiri (TC ASCR)
Jirak Zdenek (IP ASCR)
Katovsky Karel (FEEC BUT)
Kvasil Jan (FMP CU)
Leitner Rupert (MFF CUNI,Chairman of the Committee for cooperation of the Czech Republic with CERN)
Lidl Vaclav (MPO CR)
Maslan Miroslav (FoS UP)
Pospisil Stanislav (IEAP CTU, Member of the JINR Scientific Council)
Prasil Jan (MPO CR)
Rod Frantisek (MF CR)
Skoda Radek (FEE UWB)
Stekl Ivan (IEAP CTU, Vice-chairman of the Committee for cooperation of the Czech Republic with JINR)
Tursunov Arman (FPS SUO)
Vratislav Stanislav (FNSPE CTU)
Vysinka Marek (Plenipotentiary of the Government of the Czech Republic in JINR)
Wagner Vladimir (INP ASCR)
Wilhelm Ivan (Member of the JINR Scientific Council)
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ADDRESS
Committee for cooperation of CR with JINR
secretariat
NPI AS CR
Na Truhlářce 39/64
180 00 Prague
Czech Republic

Tel.: +420 266 177 235
E-mail: dubna@ujf.cas.cz
Peoples More...
Kubančák Jan Ing.
Třebický Ferdinand MUDr.
Svoboda Josef Ing. Ph.D.
Kučeráková Monika Ing. Ph.D.
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MINISTR ŠKOLSTVÍ KE SPOLUPRÁCI ČR S SÚJV
Ministr školství ke spolupráci ČR s SÚJV
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Educational programme
Educational programme
Publications More...
Transverse momentum and centrality dependence of dihadron correlations in Au plus Au collisions at root s(NN)=200 GeV: Jet quenching and the response of partonic matter
Azimuthal angle (Delta phi) correlations are presented for charged hadrons from dijets for 0.4 < p(T)< 10 GeV/c in Au+Au collisions at root s(NN)=200 GeV. With increasing p(T), the away-side distribution evolves from a broad and relatively flat shape to a