290,624 research outputs found

    Pyrite oxidation under initially neutral pH conditions and in the presence of Acidithiobacillus ferrooxidans and micromolar hydrogen peroxide

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    Hydrogen peroxide (H2O2) at a micromolar level played a role in the microbial surface oxidation of pyrite crystals under initially neutral pH. When the mineral-bacteria system was cyclically exposed to 50 μM H2O2, the colonization of Acidithiobacillus ferrooxidans onto the mineral surface was markedly enhanced, as compared to the control(no added H2O2). This can be attributed to the effects of H2O2 on increasing the roughness of the mineral surfaces, as well as the acidity and Fe2+ concentration at the mineral-solution interfaces. All of these effects tended to create more favourable nanoto micro-scale environments in the mineral surfaces for the cell adsorption. However, higher H2O2 levels inhibited the attachment of cells onto the mineral surfaces, possibly due to the oxidative stress in the bacteria when they approached the mineral surfaces where high levels of free radicals are present as a result of Fenton-like reactions. The more aggressive nature of H2O2 as an oxidant caused marked surface flaking of the mineral surface. The XPS results suggest that H2O2 accelerated the oxidation of pyrite-S and consequently facilitated the overall corrosion cycle of pyrite surfaces. This was accompanied by pH drop in the solution in contact with the pyrite cubes

    Scaling of Anisotropic Flows and Nuclear Equation of State in Intermediate Energy Heavy Ion Collisions

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    Elliptic flow (v2v_2) and hexadecupole flow (v4v_4) of light clusters have been studied in details for 25 MeV/nucleon 86^{86}Kr + 124^{124}Sn at large impact parameters by Quantum Molecular Dynamics model with different potential parameters. Four parameter sets which include soft or hard equation of state (EOS) with/without symmetry energy term are used. Both number-of-nucleon (AA) scaling of the elliptic flow versus transverse momentum (ptp_t) and the scaling of v4/A2v_4/A^{2} versus (pt/A)2(p_t/A)^2 have been demonstrated for the light clusters in all above calculation conditions. It was also found that the ratio of v4/v22v_4/{v_2}^2 keeps a constant of 1/2 which is independent of ptp_t for all the light fragments. By comparisons among different combinations of EOS and symmetry potential term, the results show that the above scaling behaviors are solid which do not depend the details of potential, while the strength of flows is sensitive to EOS and symmetry potential term.Comment: 5 pages, 5 figure

    A Remark on Soliton Equation of Mean Curvature Flow

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    In this short note, we consider self-similar immersions F:RnRn+kF: \mathbb{R}^n \to \mathbb{R}^{n+k} of the Graphic Mean Curvature Flow of higher co-dimension. We show that the following is true: Let F(x)=(x,f(x)),xRnF(x) = (x,f(x)), x \in \mathbb{R}^{n} be a graph solution to the soliton equation Hˉ(x)+F(x)=0. \bar{H}(x) + F^{\bot}(x) = 0. Assume supRnDf(x)C0<+\sup_{\mathbb{R}^{n}}|Df(x)| \le C_{0} < + \infty. Then there exists a unique smooth function f:RnRkf_{\infty}: \mathbb{R}^{n}\to \mathbb{R}^k such that f(x)=limλfλ(x) f_{\infty}(x) = \lim_{\lambda \to \infty}f_{\lambda}(x) and f(rx)=rf(x) f_{\infty}(r x)=r f_{\infty}(x) for any real number r0r\not= 0, where fλ(x)=λ1f(λx). f_{\lambda}(x) = \lambda^{-1}f(\lambda x). Comment: 6 page

    Degenerate Metric Phase Boundaries

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    The structure of boundaries between degenerate and nondegenerate solutions of Ashtekar's canonical reformulation of Einstein's equations is studied. Several examples are given of such "phase boundaries" in which the metric is degenerate on one side of a null hypersurface and non-degenerate on the other side. These include portions of flat space, Schwarzschild, and plane wave solutions joined to degenerate regions. In the last case, the wave collides with a planar phase boundary and continues on with the same curvature but degenerate triad, while the phase boundary continues in the opposite direction. We conjecture that degenerate phase boundaries are always null.Comment: 16 pages, 2 figures; erratum included in separate file: errors in section 4, degenerate phase boundary is null without imposing field equation

    Energy-Dependent GRB Pulse Width due to the Curvature Effect and Intrinsic Band Spectrum

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    Previous studies have found that the width of gamma-ray burst (GRB) pulse is energy dependent and that it decreases as a power-law function with increasing photon energy. In this work we have investigated the relation between the energy dependence of pulse and the so-called Band spectrum by using a sample including 51 well-separated fast rise and exponential decay long-duration GRB pulses observed by BATSE (Burst and Transient Source Experiment on the Compton Gamma Ray Observatory). We first decompose these pulses into rise, and decay phases and find the rise widths, and the decay widths also behavior as a power-law function with photon energy. Then we investigate statistically the relations between the three power-law indices of the rise, decay and total width of pulse (denoted as δr\delta_r, δd\delta_d and δw\delta_w, respectively) and the three Band spectral parameters, high-energy index (α\alpha), low-energy index (β\beta) and peak energy (EpE_p). It is found that (1)α\alpha is strongly correlated with δw\delta_w and δd\delta_d but seems uncorrelated with δr\delta_r; (2)β\beta is weakly correlated with the three power-law indices and (3)EpE_p does not show evident correlations with the three power-law indices. We further investigate the origin of δdα\delta_d-\alpha and δwα\delta_w-\alpha. We show that the curvature effect and the intrinsic Band spectrum could naturally lead to the energy dependence of GRB pulse width and also the δdα\delta_d-\alpha and δwα\delta_w-\alpha correlations. Our results would hold so long as the shell emitting gamma rays has a curve surface and the intrinsic spectrum is a Band spectrum or broken power law. The strong δdα\delta_d-\alpha correlation and inapparent correlations between δr\delta_r and three Band spectral parameters also suggest that the rise and decay phases of GRB pulses have different origins.Comment: 29 pages, 9 figures, 4 tables. Accepted for publication in The Astrophysical Journa
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