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The results of the MACRO experiment on atmospheric neutrino oscillations arepresented and discussed. The data concern different event topologies withaverage neutrino energies of ~ 4 and ~ 50 GeV. The Multiple Coulomb Scatteringof muons in the MACRO absorbers was used to estimate the neutrino energy ofeach event of the higher energy sample. The angular distributions, the absolutefluxes and the L/E distribution favour nu_mu <--> nu_tau oscillations withmaximal mixing and Delta m^2=0.0025 eV^2. Results are presented on the searchesfor astrophysical sources of high energy muon neutrinos, for bursts of electronantineutrinos from stellar gravitational collapses and on indirect searches forWIMPs from the Earth and from the Sun.

Neutrino physics and astrophysics with the MACRO experiment at the Gran Sasso lab