PhD Thesis
Manuel Fiolhais Centre for Computational Physics (CFC-UC) University of Coimbra, Portugal Some highlights of Nuclear Physics at The University of Coimbra.
1 Trieste 23-25 Sept. 2002. 2 Standard and non-standard solar models Success of stellar evolutionary theory Basic inputs of the theory Standard solar.
Primordial Black Holes and Dark Matter? John Miller (Oxford) Collaborators: Ilia Musco (Oslo) Antonella Garzilli (SISSA)
Stellar Formation
Manuel Fiolhais Centre for Computational Physics (CFC-UC) University of Coimbra, Portugal
Inter Stellar Matter with a high enough density, and a low enough temperature for proto-stars to form. Protostars form in cold dark nebulae Star Formation.
Neutrino2002 Poster Session L arge V olume D etector at LNGS a nd n eutrino oscillation
Vali Huseynov a,b , Rasmiyya Gasimova a , Nurida Akbarova a and Billura Hajiyeva a
