13,485 research outputs found

    Chemical evolution models with a new stellar nucleosynthesis

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    Numerical models for the chemical evolution of the Galaxy have been computed with the new stellar yields published by Maeder (1992). These metallicity dependent yields represent an important improvement in the chemical evolution of galaxies but there are still uncertainties in the stellar evolution which prevent completely satisfactory results. {}From the comparison of the model predictions with the corresponding observational constraints we find that Maeder's nucleosynthesis reproduces the oxygen and carbon abundances and provides consistent Δ\DeltaY/Δ\Delta(O/H) ratios if a significant amount of gas is accreted by the galactic disc during its whole lifetime. The lower mass limit for the black hole formation (Mbh_{bh}) must be larger than 22.5 M_{\odot} to avoid oxygen underproduction.Comment: 6 pages, MNRAS LaTex style, figures available on request from [email protected]

    Nonequilibrium transport through magnetic vibrating molecules

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    We calculate the nonequilibrium conductance through a molecule or a quantum dot in which the occupation of the relevant electronic level is coupled with intensity λ\lambda to a phonon mode, and also to two conducting leads. The system is described by the Anderson-Holstein Hamiltonian. We solve the problem using the Keldysh formalism and the non-crossing approximation (NCA) for both, the electron-electron and the electron-phonon interactions. We obtain a moderate decrease of the Kondo temperature TKT_K with λ\lambda for fixed renormalized energy of the localized level Ed~\tilde{E_d}. The meaning and value of Ed~\tilde{E_d} are discussed. The spectral density of localized electrons shows in addition to the Kondo peak of width 2TK2 T_K, satellites of this peak shifted by multiples of the phonon frequency ω0 \omega_0. The nonequilibrium conductance as a function of bias voltage VbV_b at small temperatures, also displays peaks at multiples of ω0\omega_0 in addition to the central dominant Kondo peak near Vb=0V_b=0.Comment: 11 pages, 13 figures, accepted in Phys. Rev.

    Replicas of the Kondo peak due to electron-vibration interaction in molecular transport properties

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    The low temperature properties of single level molecular quantum dots including both, electron-electron and electron-vibration interactions, are theoretically investigated. The calculated differential conductance in the Kondo regime exhibits not only the zero bias anomaly but also side peaks located at bias voltages which coincide with multiples of the energy of vibronic mode VΩ/eV \sim \hbar\Omega/e. We obtain that the evolution with temperature of the two main satellite conductance peaks follows the corresponding one of the Kondo peak when ΩkBTK\hbar\Omega \gg k_B T_K, being TK T_K the Kondo temperature, in agreement with recent transport measurements in molecular junctions. However, we find that this is no longer valid when Ω \hbar\Omega is of the order of a few times kBTKk_B T_K.Comment: 6 pages, 4 figures. Accepted for publication in Physical Review

    Restoring the SU(4) Kondo regime in a double quantum dot system

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    We calculate the spectral density and occupations of a system of two capacitively coupled quantum dots, each one connected to its own pair of conducting leads, in a regime of parameters in which the total coupling to the leads for each dot Γi\Gamma_i are different. The system has been used recently to perform pseudospin spectroscopy by controlling independently the voltages of the four leads. For an odd number of electrons in the system, Γ1=Γ2\Gamma_1=\Gamma_2, equal dot levels E1=E2E_1=E_2 and sufficiently large interdot repulsion U12U_{12} the system lies in the SU(4) symmetric point of spin and pseudospin degeneracy in the Kondo regime. In the more realistic case Γ1Γ2\Gamma_1 \neq \Gamma_2, pseudospin degeneracy is broken and the symmetry is reduced to SU(2). Nevertheless we find that the essential features of the SU(4) symmetric case are recovered by appropriately tuning the level difference δ=E2E1\delta=E_2-E_1. The system behaves as an SU(4) Kondo one at low energies. Our results are relevant for experiments which look for signatures of SU(4) symmetry in the Kondo regime of similar systems.Comment: 9 pages, 10 figure

    Orbital Kondo spectroscopy in a double quantum dot system

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    We calculate the nonequilibrium conductance of a system of two capacitively coupled quantum dots, each one connected to its own pair of conducting leads. The system has been used recently to perform pseudospin spectroscopy by controlling independently the voltages of the four leads. The pseudospin is defined by the orbital occupation of one or the other dot. Starting from the SU(4) symmetric point of spin and pseudospin degeneracy in the Kondo regime, for an odd number of electrons in the system, we show how the conductance through each dot varies as the symmetry is reduced to SU(2) by a pseudo-Zeeman splitting, and as bias voltages are applied to any of the dots. We analize the expected behavior of the system in general, and predict characteristic fingerprint features of the SU(4) to SU(2) crossover that have not been observed so far.Comment: 5 pages, 6 figures, submitted to Phys. Rev.

    The intermediate age open cluster NGC 2660

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    We present CCD UBVI photometry of the intermediate old open cluster NGC2660, covering from the red giants region to about seven magnitudes below the main sequence turn-off. Using the synthetic Colour - Magnitude Diagram method, we estimate in a self-consistent way values for distance modulus ((m-M)0 ~= 12.2), reddening (E(B-V) ~= 0.40), metallicity ([Fe/H] about solar), and age (age ~ 1 Gyr). A 30% population of binary stars turns out to be probably present.Comment: 12 pages, 8 (encapsulated) figures, to be published on MNRA
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