By Howard E. Haber, ann E. Nelson
This e-book comprises the lecture classes carried out on the institution of the Theoretical complex learn Institute (TASI, Colorado, united states) on trouble-free Particle Physics in 2002. during this college, 3 sequence of lectures are awarded in parallel within the sector of phenomenology, TeV-scale physics, and astroparticles physics. The phenomenology lecture sequence coated a huge spectrum of ordinary study innovations used to interpret brand new and destiny collider info. The TeV-scale physics lecture sequence desirous about smooth speculations approximately physics past the traditional version, with an emphasis on supersymmetry and extra-dimensional theories. The lecture sequence on astroparticle physics handled fresh advancements in theories of darkish topic and darkish strength, the cosmic microwave history, and customers for the impending period of gravitational wave astronomy.
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Additional info for Particle Physics And Cosmology: The Quest For Physics Beyond The Standard Model(s) : Tasi 2002 Boulder, Colorado, USA3 2- 28 June 2002
This is particularly interesting since the KamLAND setup is such that it is sensitive to the region of the parameter space indicated by the LMA solution to the solar neutrino anomaly. 37 Recently, the KamLAND experiment announced their first result . 041 (62) NMC where N0bs is the number of observed events and NMc is the expected number. 0. (63) These values are very close to the ones indicated by the solar neutrino data, see eq. (56). The importance of this result is twofold. First, it provides a completely solar model independent test for the neutrino oscillation solutions of the solar neutrino problem.
In the more general case, corrections to the adiabatic limit are taken into account. In particular, transitions between the effective mass eigenstates are important in the vicinity of the resonance. ] , (37) where 9m is the effective mixing angle at the production point. In this general case, the flavor transition probabilities become a rather involved function of the neutrino and medium parameters. It is this richness that makes the flavor composition of the solar neutrinos a complicated and not a monotonic function of their energies.
59). 5 f* i 1 cosG Figure 7. The low energy electron and muon neutrino fluxes compared to the MC predictions as observed by SuperKamiokande. The solid lines are the expected fluxes assuming no oscillations. The dashed lines are the best fits to neutrino oscillation. The solid circles are the data points. ) experiment also measured the zenith angle dependence of the neutrino flux. The data indicate that the preferred explanation is that of muon neutrino disappearance. For example, fig. 7 shows that the low energy ve flux agrees while the v^ flux disagrees with the MC prediction.
Particle Physics And Cosmology: The Quest For Physics Beyond The Standard Model(s) : Tasi 2002 Boulder, Colorado, USA3 2- 28 June 2002 by Howard E. Haber, ann E. Nelson