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  • LAOUET, N; BENRACHI, F (Université Frères Mentouri - Constantine 1, 2013-12-16)
    The consideration of the three-body monopole effects can solve the spectroscopic problems resulting from the failure of the two body realistic interactions to reproduce some nuclear properties. In the framework of studying ...
  • BETROUCHE, M (Université Frères Mentouri - Constantine 1, 2013-12-16)
    We use Feshbach-Villars formalism and time dependent unitary transformation to solve Klein-Gordon equation with time dependent linear potential. In the adiabatic approximation a geometric amplitude factor is obtained
  • ZOUIOUECHE, M; BOULJDEDRI, A (Université Frères Mentouri - Constantine 1, 2013-12-16)
    A styudy of the systematics of B(E3) values for nuclei throughout the periodic table shows clear enhancements at certain neutron numbers. These neutron numbers are in remarkably good agreement with those predicted by ...
  • FISLI, M (Université Frères Mentouri - Constantine 1, 2013-12-16)
    The production of the top quarks within the NCG approach is discussed and some new features of the cross sections and signatures are also shown
  • DIAF, A; BOUKABCHA, H (Université Frères Mentouri - Constantine 1, 2013-12-16)
    Nous calculons par la méthode variationnelle corrigée de Feynman-Kleinert, l'énergie de l'état fondamental d'un potentiel complexe à symétrie PT. La famille de potentiels étudiée contient divers ordres d'anharmonicité; ...
  • BOUHALOUF, H (Université Frères Mentouri - Constantine 1, 2013-12-16)
    A model of the Lyra universe is presented. Using the tunneling effect pproach, the Hawking radiation temperature near the black hole horizon is calculated
  • CHOUDER, B (Université Frères Mentouri - Constantine 1, 2013-12-16)
    Using the tunneling effect method near the black hole horizon and the WKB approximation for both fermionic and bosonic particles, some aspects are shown and discussed in a de Sitter-Schwarchild space-time type
  • MEBARKI, N (Université Frères Mentouri - Constantine 1, 2013-12-16)
    A model based on the ungravity proposal is presented. Some applications explaining dark energy and dark matter are discussed

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