49 research outputs found

    Bianchi type I space and the stability of inflationary Friedmann-Robertson-Walker space

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    Stability analysis of the Bianchi type I universe in pure gravity theory is studied in details. We first derive the non-redundant field equation of the system by introducing the generalized Bianchi type I metric. This non-redundant equation reduces to the Friedmann equation in the isotropic limit. It is shown further that any unstable mode of the isotropic perturbation with respect to a de Sitter background is also unstable with respect to anisotropic perturbations. Implications to the choice of physical theories are discussed in details in this paper.Comment: 5 pages, some comment adde

    Friedmann Equation and Stability of Inflationary Higher Derivative Gravity

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    Stability analysis on the De Sitter universe in pure gravity theory is known to be useful in many aspects. We first show how to complete the proof of an earlier argument based on a redundant field equation. It is shown further that the stability condition applies to k0k \ne 0 Friedmann-Robertson-Walker spaces based on the non-redundant Friedmann equation derived from a simple effective Lagrangian. We show how to derive this expression for the Friedmann equation of pure gravity theory. This expression is also generalized to include scalar field interactions.Comment: Revtex, 6 pages, Add two more references, some typos correcte

    A new look at the pair-production width in a strong magnetic field

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    We reexamine the process γe++e\gamma\to e^++ e^- in a background magnetic field comparable to Bcme2/eB_c\equiv m_e^2/e. This process is known to be non-perturbative in the magnetic-field strength. However, it can be shown that the {\it moments} of the above pair production width is proportional to the derivatives of photon polarization function at the zero energy, which is perturbative in BB. Hence, the pair-production width can be easily obtained from the latter by the inverse Mellin transform. The implications of our approach are discussed.Comment: 8 pages, 2 figures, Revtex, Some comments adde

    Neutrino-photon scattering and its crossed processes in a background magnetic field

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    We study the neutrino-photon processes such as γγννˉ\gamma\gamma\to \nu\bar{\nu} and νγνγ\nu\gamma\to \nu\gamma in a background magnetic field smaller than the critical magnetic field Bcme2/eB_c\equiv m_e^2/e. Using Schwinger's proper-time method, we extract leading magnetic-field contributions to the above processes. Our result is valid throughout the kinematic regime where both neutrino and photon energies are significantly smaller than mWm_W. We briefly discuss the astrophysical implications of our result.Comment: Revtex, 10 pages, 4 ps figures, to appear in Phys. Lett.

    Quenching of chlorophyll fluorescence induced by silver nanoparticles

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    The interaction between chlorophyll (Chl) and silver nanoparticles (AgNPs) was evaluated by analyzing the optical behavior of Chl molecules surrounded by different concentrations of AgNPs (10, 60, and 100 nm of diameter). UV–Vis absorption, steady state and time-resolved fluorescence measurements were performed for Chl in the presence and absence of these nanoparticles. AgNPs strongly suppressed the Chl fluorescence intensity at 678 nm. The Stern-Volmer constant (KSV) showed that fluorescence suppression is driven by the dynamic quenching process. In particular, KSV was nanoparticle size-dependent with an exponential decrease as a function of the nanoparticle diameter. Finally, changes in the Chl fluorescence lifetime in the presence of nanoparticles demonstrated that the fluorescence quenching may be induced by the excited electron transfer from the Chl molecules to the metal nanoparticles
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