NEUTRINO ODYSSEY
... Although they hardly interact at all, they helped forge the elements in the early Universe, they tell us how the Sun shines, and they may even cause the titanic explosion of a dying star. They may well be the reason we live in a Universe filled with matter – in other words, a reason for our being he ...
... Although they hardly interact at all, they helped forge the elements in the early Universe, they tell us how the Sun shines, and they may even cause the titanic explosion of a dying star. They may well be the reason we live in a Universe filled with matter – in other words, a reason for our being he ...
n - IN2P3
... http://library.lanl.gov/cgibin/getfile?00326606.pdf#search='delayed%20coincidence%20cadmium%20neutrino' ...
... http://library.lanl.gov/cgibin/getfile?00326606.pdf#search='delayed%20coincidence%20cadmium%20neutrino' ...
Neutrinos and our Sun
... where G is the gravitational constant. EG is clearly a factor of 100, too small compared to E 0 . ...
... where G is the gravitational constant. EG is clearly a factor of 100, too small compared to E 0 . ...
Detecting sterile neutrinos with KATRIN
... Prospects for the detection of sterile neutrinos with KATRIN-like experiments Anna Sejersen Riis, Steen Hannestad “Detecting sterile neutrinos with KATRIN like experiments” JCAP02(2011)011 ...
... Prospects for the detection of sterile neutrinos with KATRIN-like experiments Anna Sejersen Riis, Steen Hannestad “Detecting sterile neutrinos with KATRIN like experiments” JCAP02(2011)011 ...
PHY313 - CEI544 The Mystery of Matter From Quarks to the
... • This process continues until the elements that are produced reach the peak of the nuclear binding energy, at Fe/Ni. • Then the star cools (Red Giant). Gravitation takes over compressing the star. The heaviest elements accumulate at the core in layers of density. Compression reheats the star & it e ...
... • This process continues until the elements that are produced reach the peak of the nuclear binding energy, at Fe/Ni. • Then the star cools (Red Giant). Gravitation takes over compressing the star. The heaviest elements accumulate at the core in layers of density. Compression reheats the star & it e ...
Common problem against B and L genesis and its possible resolution
... from nucleosynthesis, including hadronic decay n3 / 2 2 TRH O[10 ] s m pl TRH 106 108 GeV Possible to produce heavy ...
... from nucleosynthesis, including hadronic decay n3 / 2 2 TRH O[10 ] s m pl TRH 106 108 GeV Possible to produce heavy ...
Student Seminar Subatomic Physics, blok 1+2 2002/03
... interest. We aim to select a menu that is highly relevant for the various research groups at the KVI and educative also for masters students not (yet) affiliated to the KVI. The literature will consist mostly of actual research overview articles supported by chapters from textbooks. The selection of ...
... interest. We aim to select a menu that is highly relevant for the various research groups at the KVI and educative also for masters students not (yet) affiliated to the KVI. The literature will consist mostly of actual research overview articles supported by chapters from textbooks. The selection of ...
The Standard Model of Particle Physics Piet Mulders
... symmetry of the world • CP is almost a good symmetry • Thus also time reversal is almost a good symmetry, but not exact! • This symmetry breaking allows for the surplus of matter over antimatter in the universe (even if this is only 1 : 109) Number of baryons 0,25 x 1079 (~ 0,25 per m3) But the nu ...
... symmetry of the world • CP is almost a good symmetry • Thus also time reversal is almost a good symmetry, but not exact! • This symmetry breaking allows for the surplus of matter over antimatter in the universe (even if this is only 1 : 109) Number of baryons 0,25 x 1079 (~ 0,25 per m3) But the nu ...
International Journal of High-Energy Physics CERN Courier Volume
... Igor Tkachev, of the Institute for Nuclear Research (INR) of the Russian Academy of Sciences (RAS), Moscow, and Alexander Dolgov, of the Alikhanov Institute for Theoretical and Experimental Physics, Moscow, and INFN, have been awarded the 2014 Markov Prize. They received the award at the 2014 Markov ...
... Igor Tkachev, of the Institute for Nuclear Research (INR) of the Russian Academy of Sciences (RAS), Moscow, and Alexander Dolgov, of the Alikhanov Institute for Theoretical and Experimental Physics, Moscow, and INFN, have been awarded the 2014 Markov Prize. They received the award at the 2014 Markov ...
OscSNS: Precision Neutrino Measurements at
... The flagship cross section analyses of OscSNS are the elastic scattering νee-→ νee- (NC and CC), NC νµe-→ νµe-, NC anti-νµe-→ antiνµe-, NC νµC→ νµC, and the CC νe12C→e-12N interactions. The current world's best measurement of the νee-→ νee- interaction arises in a sample of only 191 events [6], and ...
... The flagship cross section analyses of OscSNS are the elastic scattering νee-→ νee- (NC and CC), NC νµe-→ νµe-, NC anti-νµe-→ antiνµe-, NC νµC→ νµC, and the CC νe12C→e-12N interactions. The current world's best measurement of the νee-→ νee- interaction arises in a sample of only 191 events [6], and ...
Icarus – wire production - Faculty of Physics University of Warsaw
... • All the equipment has been constructed, purchased or borrowed from Pavia with many improvements as compared to the original Pavia setup for the wire production of T600. • Common work of the experimental groups from Warsaw, Katowice and Cracow, in close collaboration with the Pavia group. • Laborat ...
... • All the equipment has been constructed, purchased or borrowed from Pavia with many improvements as compared to the original Pavia setup for the wire production of T600. • Common work of the experimental groups from Warsaw, Katowice and Cracow, in close collaboration with the Pavia group. • Laborat ...
The Birth, Life, and Death of Stars
... collaboration of more than 350 scientists from five countries has proposed to build a world-leading neutrino experiment that would involve construction at both Fermi National Accelerator Laboratory (Fermilab), located in Batavia, Illinois, and the Sanford Underground Research Facility (Sanford Lab) ...
... collaboration of more than 350 scientists from five countries has proposed to build a world-leading neutrino experiment that would involve construction at both Fermi National Accelerator Laboratory (Fermilab), located in Batavia, Illinois, and the Sanford Underground Research Facility (Sanford Lab) ...
Bruno Pontecorvo
Bruno Pontecorvo (Russian: Бру́но Макси́мович Понтеко́рво, Bruno Maksimovich Pontekorvo; 22 August 1913 – 24 September 1993) was an Italian nuclear physicist, an early assistant of Enrico Fermi and then the author of numerous studies in high energy physics, especially on neutrinos. According to Oleg Gordievsky (the highest-ranking KGB officer ever to defect) and Pavel Sudoplatov (former deputy director of Foreign Intelligence for the Soviet Union), Pontecorvo was also a Soviet agent. Convinced communist, he defected to the Soviet Union in 1950, where he continued his research on the decay of the muon and on neutrinos. The prestigious Pontecorvo Prize was instituted in his memory in 1995.