MODERN COSMOLOGY

Investigation of the WIMP annual modulation signature 287 Figure 9.1.Model-independent residual rate in the 2–6 keV cumulative e ...

288 Signature for signals from the dark universe 3 and DAMA/NaI-4 running periods, which have been recently released [9]; a devo ...

Investigation of the WIMP annual modulation signature 289 in our experiment is given by PMT fast single photoelectrons with deca ...

290 Signature for signals from the dark universe lowest energy region in [7–9]; in fact, if it were otherwise—considering theR 9 ...

Investigation of the WIMP annual modulation signature 291 lower bound accounted for results achieved in accelerators. The calcul ...

292 Signature for signals from the dark universe Figure 9.2. Regions allowed at 3σC.L. in the planeξσp(ξ = 0 .3 GeV cmρWIMP− 3 a ...

DAMA annual modulation result versus CDMS exclusion plot 293 Ta b l e 9. 2 .Several numbers on the DAMA and CDMS experiments as ...

294 Signature for signals from the dark universe gives in [33] about 30 expected neutrons to be compared with the 13 quoted reco ...

References 295 In [35] a possible heavy neutrino of the fourth family has been considered instead. Further studies on model fram ...

Chapter 10 Neutrino oscillations: a phenomenological overview GianLuigi Fogli Dipartimento di Fisica e INFN, Sezione di Bari, Vi ...

Three-neutrino mixing and oscillations 297 In this chapter we analyse atmospheric and solar data in a common 3ν oscillation fram ...

298 Neutrino oscillations: a phenomenological overview Figure 10.1. Parameter spaces of solar and atmospheric neutrinos in the l ...

Analysis of the atmospheric data 299 Figure 10.2.Three-flavour analysis in the triangle plot, for five representative values of ...

300 Neutrino oscillations: a phenomenological overview Figure 10.3.90% C.L. bounds on the mass parameterm^2 from atmospheric dat ...

Analysis of the atmospheric data 301 Figure 10.4.Bounds onUe3^2 as a function ofm^2 from SK data (52 kTy), with and without the ...

302 Neutrino oscillations: a phenomenological overview Figure 10.5.SK zenith distributions of leptons at best fit (broken lines) ...

Analysis of the solar data 303 Figure 10.6.Double ratio ofμ/e events (data/theory) for SG and MG events in SK: full curve, predi ...

304 Neutrino oscillations: a phenomenological overview Figure 10.7. The solar neutrino deficit, shown as a discrepancy between d ...

Analysis of the solar data 305 Figure 10.8. Two-generation vacuum solutions to the solar neutrino problem (all data included). U ...

306 Neutrino oscillations: a phenomenological overview Figure 10.9. Two-generation MSW solutions to the solar neutrino problem. ...