2,148 research outputs found

    Spin-glass phase transition and behavior of nonlinear susceptibility in the Sherrington-Kirkpatrick model with random fields

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    The behavior of the nonlinear susceptibility χ3\chi_3 and its relation to the spin-glass transition temperature TfT_f, in the presence of random fields, are investigated. To accomplish this task, the Sherrington-Kirkpatrick model is studied through the replica formalism, within a one-step replica-symmetry-breaking procedure. In addition, the dependence of the Almeida-Thouless eigenvalue λAT\lambda_{\rm AT} (replicon) on the random fields is analyzed. Particularly, in absence of random fields, the temperature TfT_f can be traced by a divergence in the spin-glass susceptibility χSG\chi_{\rm SG}, which presents a term inversely proportional to the replicon λAT\lambda_{\rm AT}. As a result of a relation between χSG\chi_{\rm SG} and χ3\chi_3, the latter also presents a divergence at TfT_f, which comes as a direct consequence of λAT=0\lambda_{\rm AT}=0 at TfT_f. However, our results show that, in the presence of random fields, χ3\chi_3 presents a rounded maximum at a temperature T∗T^{*}, which does not coincide with the spin-glass transition temperature TfT_f (i.e., T∗>TfT^* > T_f for a given applied random field). Thus, the maximum value of χ3\chi_3 at T∗T^* reflects the effects of the random fields in the paramagnetic phase, instead of the non-trivial ergodicity breaking associated with the spin-glass phase transition. It is also shown that χ3\chi_3 still maintains a dependence on the replicon λAT\lambda_{\rm AT}, although in a more complicated way, as compared with the case without random fields. These results are discussed in view of recent observations in the LiHox_xY1−x_{1-x}F4_4 compound.Comment: accepted for publication in PR

    Procedimento de operação, manutenção e verificação de thermomixer.

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    bitstream/CENARGEN/29576/1/ct060.pd

    Procedimento de operação, manutenção e verificação da centrífuga refrigerada de bancada Eppendorf, Modelo 5810 R.

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    bitstream/CENARGEN/29583/1/ct063.pd

    Procedimento de operação, manutenção e verificação da estufa ELETROLAB modelo 112FC.

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    bitstream/CENARGEN/29586/1/ct065.pd

    Procedimento de operação, manutenção e verificação do Espectrofotômetro.

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    bitstream/CENARGEN/29588/1/ct067.pd

    Polarimetry of Li-rich giants

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    Protoplanetary nebulae typically present non-spherical envelopes. The origin of such geometry is still controversial. There are indications that it may be carried over from an earlier phase of stellar evolution, such as the AGB phase. But how early in the star's evolution does the non-spherical envelope appear? Li-rich giants show dusty circumstellar envelopes that can help answer that question. We study a sample of fourteen Li-rich giants using optical polarimetry in order to detect non-spherical envelopes around them. We used the IAGPOL imaging polarimeter to obtain optical linear polarization measurements in V band. Foreground polarization was estimated using the field stars in each CCD frame. After foreground polarization was removed, seven objects presented low intrinsic polarization (0.19 - 0.34)% and two (V859 Aql and GCSS 557) showed high intrinsic polarization values (0.87 - 1.16)%. This intrinsic polarization suggests that Li-rich giants present a non-spherical distribution of circumstellar dust. The intrinsic polarization level is probably related to the viewing angle of the envelope, with higher levels indicating objects viewed closer to edge-on. The correlation of the observed polarization with optical color excess gives additional support to the circumstellar origin of the intrinsic polarization in Li-rich giants. The intrinsic polarization correlates even better with the IRAS 25 microns far infrared emission. Analysis of spectral energy distributions for the sample show dust temperatures for the envelopes tend to be between 190 and 260 K. We suggest that dust scattering is indeed responsible for the optical intrinsic polarization in Li-rich giants. Our findings indicate that non-spherical envelopes may appear as early as the red giant phase of stellar evolution.Comment: to be published in A&A, 15 pages, 10 figures. Fig. 3 is available in ftp://astroweb.iag.usp.br/pub/antonio/4270/4270.fig3.pd

    Gestão e políticas públicas em Minas Gerais: cultura e patrimônio cultural

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    Aborda-se o papel do Estado e dos seus gestores em relação à adoção de políticas de preservação da cultura e do patrimônio cultural em Minas Gerais. O objetivo central é convidar o leitor a refletir sobre as políticas públicas de preservação do patrimônio cultural e o papel do gestor em relação às ações desenvolvidas no Estado de Minas Gerais, nos diferentes municípios que compõe esse estado

    Photoassociative ionization of Na inside a storage ring

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    Motivated by recent interest in low dimensional arrays of atoms, we experimentally investigated the way cold collisional processes are affected by the geometry of the considered atomic sample. More specifically, we studied the case of photoassociative ionization (PAI) both in a storage ring where collision is more unidirectional in character and in a trap with clear undefinition of collision axis. First, creating a ring shaped trap (atomotron) we investigated two-color PAI dependence with intensity and polarization of a probing laser. The intensity dependence of the PAI rate was also measured in a magneto-optical trap presenting equivalent temperature and density conditions. Indeed, the results show that in the ring trap, the value of the PAI rate constant is much lower and does not show evidences of saturation, unlike in the case of the 3D-MOT. Cold atomic collisions in storage ring may represent new possibilities for study.Comment: 5 pages, 5 figures; Accepted by Optics Communicatio
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