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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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HOW TO GET THERE
Tram 3, 10, 24 - Bulovka stop
Bus 201 - Vychovatelna stop
Bus 166 - Nemocnice Bulovka gynekologie stop

MAP
Peoples More...
Vacík Jiří promovaný fyzik CSc.
Katovský Karel doc. Ing. Ph.D.
Babič Andrej Mgr.
Rod František Ing. Mgr.
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MINISTR ŠKOLSTVÍ KE SPOLUPRÁCI ČR S SÚJV
Ministr školství ke spolupráci ČR s SÚJV
Grants More...
Study of few-nucleon system using polarised deuteron target and development of highly polarized neutron beam
Study of few-nucleon system using polarised deuteron target and development of highly polarized neutron beam
Publications More...
Exact Solution for a Black Hole Embedded in a Nonstatic Dust-filled Universe
An exact solution of the Lemaitre-Tolman-Bondi class is investigated as a possible model of the Schwarzschild-like black hole embedded in a nonstatic dust-filled universe for the three types of spatial curvature. The solution is obtained in comoving coord