Cosmic Rays - High Energy Physics at Wayne State
... long lifetime such that the more energetic muons reach sea level before decaying 2) Unlike electrons (which are much lighter) they do not interact with atomic fields so easily The neutrinos interact only weakly, so they easily reach sea level (and continue straight through the earth) ...
... long lifetime such that the more energetic muons reach sea level before decaying 2) Unlike electrons (which are much lighter) they do not interact with atomic fields so easily The neutrinos interact only weakly, so they easily reach sea level (and continue straight through the earth) ...
Measuring Light Neutrino Families
... The Experiment Experimental demands: The principle of the analysis: all visible channels are detected by large detectors and classified according to four categories: ...
... The Experiment Experimental demands: The principle of the analysis: all visible channels are detected by large detectors and classified according to four categories: ...
ASEPS_Poster_Ishihara1_A0
... neutrino (RMN). The product of two masses of LMN and RMN is equal to a Dirac particle mass squared. Therefore, when the mass of RMN is extremely large, the one of LMN naturally becomes very small. The LMN is considered as known neutrino weakly interacting. In the Leptogenesis scenario, heavy RMNs ha ...
... neutrino (RMN). The product of two masses of LMN and RMN is equal to a Dirac particle mass squared. Therefore, when the mass of RMN is extremely large, the one of LMN naturally becomes very small. The LMN is considered as known neutrino weakly interacting. In the Leptogenesis scenario, heavy RMNs ha ...
