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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...
Lokajíček Tomáš Ing. CSc.
Kohout Pavel Mgr. Ph.D.
Solar Michael RNDr. CSc.
Liščuk Josef Ing.
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MINISTR ŠKOLSTVÍ KE SPOLUPRÁCI ČR S SÚJV
Ministr školství ke spolupráci ČR s SÚJV
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Investigation in nuclear physics, solid state physics and biophysics by beams of electrons, pozitrons and high-frequency radiation
Investigation in nuclear physics, solid state physics and biophysics by beams of electrons, pozitrons and high-frequency radiation
Publications More...
Interpolating formula for the 0 nu beta beta-decay half-life in the case of light and heavy neutrino mass mechanisms
We revisit the "interpolating formula" proposed in our previous publication. It allows one to calculate the 0 nu beta beta-decay half-life for arbitrary neutrino mass without the involvement of the complicated results for nuclear matrix elements (NMEs)