10,131 research outputs found

    Density functional theory of superconductivity in doped tungsten oxides

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    We apply density functional theory for superconductors (SCDFT) to doped tungsten oxide in three forms: electrostatically doped WO3, perovskite WO3−xFx, and hexagonal CsxWO3. We achieve a consistent picture in which the experimental superconducting transition temperature Tc is reproduced, and superconductivity is understood as a weak-coupling state sustained by soft vibrational modes of the WO6 octahedra. SCDFT simulations of CsxWO3 allow us to explain the anomalous Tc behavior observed in most tungsten bronzes, where Tc decreases with increasing carrier density. Here, the opening of structural channels to host Cs atoms induces a softening of strongly coupled W-O modes. By increasing the Cs content, these modes are screened and Tc is strongly reduced

    Stochastic Schr\"odinger equations with coloured noise

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    A natural non-Markovian extension of the theory of white noise quantum trajectories is presented. In order to introduce memory effects in the formalism an Ornstein-Uhlenbeck coloured noise is considered as the output driving process. Under certain conditions a random Hamiltonian evolution is recovered. Moreover, non-Markovian stochastic Schr\"odinger equations which unravel non-Markovian master equations are derived.Comment: 4pages, revte

    Star formation in early-type galaxies: the role of stellar winds and kinematics

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    Early-type galaxies (ETGs) host a hot ISM produced mainly by stellar winds, and heated by Type Ia supernovae and the thermalization of stellar motions. High resolution 2D hydrodynamical simulations showed that ordered rotation in the stellar component results in the formation of a centrifugally supported cold equatorial disc. In a recent numerical investigation we found that subsequent generations of stars are formed in this cold disc; this process consumes most of the cold gas, leaving at the present epoch cold masses comparable to those observed. Most of the new stellar mass formed a few Gyrs ago, and resides in a disc.Comment: 2 pages, 1 figure, to appear in proceedings of IAU Symposium 315, "From Interstellar Clouds to Star-Forming Galaxies: Universal Processes?", P. Jablonka, F. Van der Tak & P. Andre', ed

    On the (2,3)-generation of the finite symplectic groups

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    This paper is a new important step towards the complete classification of the finite simple groups which are (2,3)(2,3)-generated. In fact, we prove that the symplectic groups Sp2n(q)Sp_{2n}(q) are (2,3)(2,3)-generated for all n≥4n\geq 4. Because of the existing literature, this result implies that the groups PSp2n(q)PSp_{2n}(q) are (2,3)(2,3)-generated for all n≥2n\geq 2, with the exception of PSp4(2f)PSp_4(2^f) and PSp4(3f)PSp_4(3^f)

    More on regular subgroups of the affine group

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    This paper is a new contribution to the study of regular subgroups of the affine group AGLn(F)AGL_n(F), for any field FF. In particular we associate to any partition λ≠(1n+1)\lambda\neq (1^{n+1}) of n+1n+1 abelian regular subgroups in such a way that different partitions define non-conjugate subgroups. Moreover, we classify the regular subgroups of certain natural types for n≤4n\leq 4. Our classification is equivalent to the classification of split local algebras of dimension n+1n+1 over FF. Our methods, based on classical results of linear algebra, are computer free

    The simple classical groups of dimension less than 6 which are (2,3)-generated

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    In this paper we determine the classical simple groups of dimension r=3,5 which are (2,3)-generated (the cases r = 2, 4 are known). If r = 3, they are PSL_3(q), q 4, and PSU_3(q^2), q^2 9, 25. If r = 5 they are PSL_5(q), for all q, and PSU_5(q^2), q^2 >= 9. Also, the soluble group PSU_3(4) is not (2,3)-generated. We give explicit (2,3)-generators of the linear preimages, in the special linear groups, of the (2,3)-generated simple groups.Comment: 12 page

    The (2,3)(2,3)-generation of the finite unitary groups

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    In this paper we prove that the unitary groups SUn(q2)SU_n(q^2) are (2,3)(2,3)-generated for any prime power qq and any integer n≥8n\geq 8. By previous results this implies that, if n≥3n\geq 3, the groups SUn(q2)SU_n(q^2) and PSUn(q2)PSU_n(q^2) are (2,3)(2,3)-generated, except when (n,q)∈{(3,2),(3,3),(3,5),(4,2),(4,3),(5,2)}(n,q)\in\{(3,2),(3,3),(3,5),(4,2), (4,3),(5,2)\}.Comment: In this version, we obtained a complete classification of the finite simple unitary groups which are (2,3)-generated; some proofs have been semplifie
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