58,299 research outputs found

    Correlation of the orbach relaxation coefficient with optical linewidths- laf3-er3 plus

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    Correlation of Orbach coefficient of spin-lattice relaxation with optical transition linewidths for trivalent erbium in lanthanum fluorid

    3-manifolds with(out) metrics of nonpositive curvature

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    In the context of Thurstons geometrisation program we address the question which compact aspherical 3-manifolds admit Riemannian metrics of nonpositive curvature. We show that non-geometric Haken manifolds generically, but not always, admit such metrics. More precisely, we prove that a Haken manifold with, possibly empty, boundary of zero Euler characteristic admits metrics of nonpositive curvature if the boundary is non-empty or if at least one atoroidal component occurs in its canonical topological decomposition. Our arguments are based on Thurstons Hyperbolisation Theorem. We give examples of closed graph-manifolds with linear gluing graph and arbitrarily many Seifert components which do not admit metrics of nonpositive curvature.Comment: 16 page

    Fully Constrained Majorana Neutrino Mass Matrices Using Σ(72×3)\Sigma(72\times 3)

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    In 2002, two neutrino mixing ansatze having trimaximally-mixed middle (ν2\nu_2) columns, namely tri-chi-maximal mixing (TχM\text{T}\chi\text{M}) and tri-phi-maximal mixing (TϕM\text{T}\phi\text{M}), were proposed. In 2012, it was shown that TχM\text{T}\chi\text{M} with χ=±π16\chi=\pm \frac{\pi}{16} as well as TϕM\text{T}\phi\text{M} with ϕ=±π16\phi = \pm \frac{\pi}{16} leads to the solution, sin2θ13=23sin2π16\sin^2 \theta_{13} = \frac{2}{3} \sin^2 \frac{\pi}{16}, consistent with the latest measurements of the reactor mixing angle, θ13\theta_{13}. To obtain TχM(χ=±π16)\text{T}\chi\text{M}_{(\chi=\pm \frac{\pi}{16})} and TϕM(ϕ=±π16)\text{T}\phi\text{M}_{(\phi=\pm \frac{\pi}{16})}, the type~I see-saw framework with fully constrained Majorana neutrino mass matrices was utilised. These mass matrices also resulted in the neutrino mass ratios, m1:m2:m3=(2+2)1+2(2+2):1:(2+2)1+2(2+2)m_1:m_2:m_3=\frac{\left(2+\sqrt{2}\right)}{1+\sqrt{2(2+\sqrt{2})}}:1:\frac{\left(2+\sqrt{2}\right)}{-1+\sqrt{2(2+\sqrt{2})}}. In this paper we construct a flavour model based on the discrete group Σ(72×3)\Sigma(72\times 3) and obtain the aforementioned results. A Majorana neutrino mass matrix (a symmetric 3×33\times 3 matrix with 6 complex degrees of freedom) is conveniently mapped into a flavon field transforming as the complex 6 dimensional representation of Σ(72×3)\Sigma(72\times 3). Specific vacuum alignments of the flavons are used to arrive at the desired mass matrices.Comment: 20 pages, 1 figure. arXiv admin note: substantial text overlap with arXiv:1402.085

    Deviations from Tribimaximal Neutrino Mixing using a Model with Δ(27)\Delta(27) Symmetry

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    We present a model of neutrino mixing based on the flavour group Δ(27)\Delta(27) in order to account for the observation of a non-zero reactor mixing angle (θ13\theta_{13}). The model provides a common flavour structure for the charged-lepton and the neutrino sectors, giving their mass matrices a `circulant-plus-diagonal' form. Mass matrices of this form readily lead to mixing patterns with realistic deviations from tribimaximal mixing, including non-zero θ13\theta_{13}. With the parameters constrained by existing measurements, our model predicts an inverted neutrino mass hierarchy. We obtain two distinct sets of solutions in which the atmospheric mixing angle lies in the first and the second octants. The first (second) octant solution predicts the lightest neutrino mass, m329 meVm_3 \sim 29~\text{meV} (m365 meVm_3 \sim 65~\text{meV}) and the CPCP phase, δCPπ4\delta_{CP} \sim -\frac{\pi}{4} (δCPπ2\delta_{CP} \sim \frac{\pi}{2}), offering the possibility of large observable CPCP violating effects in future experiments.Comment: 9 pages, 3 figure

    Understanding entanglement as resource: locally distinguishing unextendible product bases

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    It is known that the states in an unextendible product basis (UPB) cannot be distinguished perfectly when the parties are restricted to local operations and classical communication (LOCC). Previous discussions of such bases have left open the following question: What entanglement resources are necessary and/or sufficient for this task to be possible with LOCC? In this paper, I present protocols which use entanglement more efficiently than teleportation to distinguish certain classes of UPB's. The ideas underlying my approach to this problem offer rather general insight into why entanglement is useful for such tasks.Comment: Final, published version. Many revisions following very useful suggestions of the referee have been added. In particular, Appendix A has been completely rewritte

    Viscous Hydrodynamics and Relativistic Heavy Ion Collisions

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    The matter created in relativistic heavy ion collisions is fairly well described by ideal hydrodynamics, and somewhat better described by viscous hydrodynamics. To this point, most viscous calculations have been two-dimensional, based on an assumption of Bjorken boost invariance along the beam axis. Here, first results are presented for a fully three-dimensional viscous model. The model is described and tests of the numerical accuracy of the code are presented. Two- and three-dimensional runs are compared, and modest changes are observed for mid-rapidity observables at the highest RHIC (Relativistic Heavy Ion Collider) energies.Comment: 23 pages, 7 figure

    16S rRNA gene-based profiling of the human infant gut microbiota is strongly influenced by sample processing and PCR primer choice

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    Acknowledgements The authors acknowledge the assistance of Grietje Holtrop (RINH-BioSS) with the statistical analysis of the data and the Wellcome Trust Sanger Institute’s 454 pyrosequencing team for generating 16S rRNA gene data. AWW, PS and JP received core funding support from the Wellcome Trust [grant number 098051]. AWW, JCM, HJF and KPS are funded by the Scottish Government (SG-RESAS).Peer reviewedPublisher PD

    On the Electronic Spectroscopy of Closed Shell Cations Derived From Resonance Stabilized Radicals: Insights From Theory and Franck-Condon Analysis

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    Context. Recent attention has been directed on closed-shell aromatic cations as potential carriers of the diffuse interstellar bands. The spectra of mass-selected, matrix-isolated benzylium, and tropylium cations were recently reported. The visible spectrum of benzylium exhibits a large Franck-Condon (FC) envelope, inconsistent with diffuse interstellar band carriers. Aims. We perform a computational analysis of the experimentally studied benzylium spectrum before extending the methods to a range of larger, closed-shell aromatic cations to determine the potential for this class of systems as diffuse interstellar band carriers. Methods. Density functional theory (DFT), time-dependant ((TD)DFT), and multi-configurational self-consistent field second-order perturbation theory (MRPT2) methods in concert with multidimensional FC analysis is used to model the benzylium spectrum. These methods are extended to larger closed-shell aromatic hydrocarbon cations derived from resonance-stabilized radicals, which are predicted to show strong S0 → Sn transitions in the visible region. The ionization energies of a range of these systems are also calculated by DFT. Results. The simulated benzylium spectrum was found to yield excellent agreement with the experimental spectrum showing an extended progression in a low frequency (510 cm-1) ring distortion mode. The FC progression was found to be significantly quenched in the larger species: 1-indanylium, 1-naphthylmethylium, and fluorenium. Excitation and ionization energies of the closed-shell cations were found to be consistent with diffuse interstellar band carriers, with the former lying in the visible range and the latter straddling the Lyman limit in the 13−14 eV range. Conclusions. Large closed-shell polycyclic aromatic hydrocarbon cations remain viable candidate carriers of the diffuse interstellar bands
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