Double Chooz (DC) is a reactor neutrino oscillation experiment whose purpose is the measurement of the last unknown mixing angle θ13 . It inherits from the past CHOOZ experiment which was limited by the statistical and systematic errors at the same extent of about 2.8%. To lower the statistical error, the DC detector target mass has been increased and a longer exposure is foreseen while the lowering of the systematic error is ensured by the use of two identical detectors. One will be located in the vicinity of the reactor cores to monitor the flux and spectrum of the anti-νe emitted whereas the other one will be located where the effect of the oscillation is expected to be maximal. They are respectively so-called 'near' and 'far' detectors....
In this thesis, we studied low temperature silicon devices of nanometer size. In these devices, an e...
The study of the energy spectrum of ultra-high energy cosmic rays (E > 1020 eV) requires to determin...
The study of the energy spectrum of ultra-high energy cosmic rays (E > 1020 eV) requires to determin...
Double Chooz (DC) is a reactor neutrino oscillation experiment whose purpose is the measurement of t...
Double Chooz (DC) is a reactor neutrino oscillation experiment whose purpose is the measurement of t...
Double Chooz (DC) is a reactor neutrino oscillation experiment whose purpose is the measurement of t...
Double Chooz (DC) is a reactor neutrino oscillation experiment whose purpose is the measurement of t...
Double Chooz (DC) is a reactor neutrino oscillation experiment whose purpose is the measurement of t...
Double Chooz (DC) is a reactor neutrino oscillation experiment whose purpose is the measurement of t...
Two high energy particle physics analyses are presented in this PhD report using events with two lep...
Two high energy particle physics analyses are presented in this PhD report using events with two lep...
Two high energy particle physics analyses are presented in this PhD report using events with two lep...
Since the start of proton-proton collisions at LHC in 2009, the ATLAS and CMS experiments have recor...
Since the start of proton-proton collisions at LHC in 2009, the ATLAS and CMS experiments have recor...
In this thesis, we studied low temperature silicon devices of nanometer size. In these devices, an e...
In this thesis, we studied low temperature silicon devices of nanometer size. In these devices, an e...
The study of the energy spectrum of ultra-high energy cosmic rays (E > 1020 eV) requires to determin...
The study of the energy spectrum of ultra-high energy cosmic rays (E > 1020 eV) requires to determin...
Double Chooz (DC) is a reactor neutrino oscillation experiment whose purpose is the measurement of t...
Double Chooz (DC) is a reactor neutrino oscillation experiment whose purpose is the measurement of t...
Double Chooz (DC) is a reactor neutrino oscillation experiment whose purpose is the measurement of t...
Double Chooz (DC) is a reactor neutrino oscillation experiment whose purpose is the measurement of t...
Double Chooz (DC) is a reactor neutrino oscillation experiment whose purpose is the measurement of t...
Double Chooz (DC) is a reactor neutrino oscillation experiment whose purpose is the measurement of t...
Two high energy particle physics analyses are presented in this PhD report using events with two lep...
Two high energy particle physics analyses are presented in this PhD report using events with two lep...
Two high energy particle physics analyses are presented in this PhD report using events with two lep...
Since the start of proton-proton collisions at LHC in 2009, the ATLAS and CMS experiments have recor...
Since the start of proton-proton collisions at LHC in 2009, the ATLAS and CMS experiments have recor...
In this thesis, we studied low temperature silicon devices of nanometer size. In these devices, an e...
In this thesis, we studied low temperature silicon devices of nanometer size. In these devices, an e...
The study of the energy spectrum of ultra-high energy cosmic rays (E > 1020 eV) requires to determin...
The study of the energy spectrum of ultra-high energy cosmic rays (E > 1020 eV) requires to determin...