Predicció dels períodes de les seques

En aquest article es fa una predicció teòrica dels períodes de les seques externes i internes de l'estany de Banyoles utilitzant el mètode proposat per Mortimer (1979) i que es basa en un model unidimensional i iteratiu d'integració de les equacions de continuïtat i de moviment. La poca profunditat del llac fa que per a les seques internes s'hagin de considerar 4 zones diferents d'oscil·lació. El període de l'harmònic fonamental per a les seques externes és de 6,9 min. Els harmònics fonamentals per a les seques internes a les quatre diferents zones valen: 2,7 hores, 1,89 hores, 1 hora i 35 min

A new efficient approach to the direct restricted active space self-consistent field method

An implicitly parallel method for integral-block driven restricted active space self-consistent field (RASSCF) algorithms is presented. The approach is based on a model space representation of the RAS active orbitals with an efficient expansion of the model subspaces. The applicability of the method is demonstrated with a RASSCF investigation of the first two excited states of indole

Determination of the direct band-gap energy of InAlAs matched to InP by photoluminescence excitation spectroscopy

A series of InxAl1-xAs samples (0.51≪x≪0.55)coherently grown on InP was studied in order to measure the band-gap energy of the lattice matched composition. As the substrate is opaque to the relevant photon energies, a method is developed to calculate the optical absorption coefficient from the photoluminescence excitation spectra. The effect of strain on the band-gap energy has been taken into account. For x=0.532, at 14 K we have obtained Eg0=1549±6 meV