29,486 research outputs found

    Polydispersity Effects in the Dynamics and Stability of Bubbling Flows

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    The occurrence of swarms of small bubbles in a variety of industrial systems enhances their performance. However, the effects that size polydispersity may produce on the stability of kinematic waves, the gain factor, mean bubble velocity, kinematic and dynamic wave velocities is, to our knowledge, not yet well established. We found that size polydispersity enhances the stability of a bubble column by a factor of about 23% as a function of frequency and for a particular type of bubble column. In this way our model predicts effects that might be verified experimentally but this, however, remain to be assessed. Our results reinforce the point of view advocated in this work in the sense that a description of a bubble column based on the concept of randomness of a bubble cloud and average properties of the fluid motion, may be a useful approach that has not been exploited in engineering systems.Comment: 11 pages, 2 figures, presented at the 3rd NEXT-SigmaPhi International Conference, 13-18 August, 2005, Kolymbari, Cret

    Interplay between Zeeman interaction and spin-orbit coupling in a two-dimensional semiconductor system

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    We analyse the interplay between Dresselhaus, Bychkov-Rashba, and Zeeman interactions in a two-dimensional semiconductor quantum system under the action of a magnetic field. When a vertical magnetic field is considered, we predict that the interplay results in an effective cyclotron frequency that depends on a spin-dependent contribution. For in-plane magnetic fields, we found that the interplay induces an anisotropic effective gyromagnetic factor that depends on the orientation of the applied field as well as on the orientation of the electron momentum.Comment: 5 page

    Radiative capture reaction for 17^{17}Ne formation within a full three-body model

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    Background: The breakout from the hot Carbon-Nitrogen-Oxigen (CNO) cycles can trigger the rp-process in type I x-ray bursts. In this environment, a competition between 15O(α,γ)19Ne^{15}\text{O}(\alpha,\gamma){^{19}\text{Ne}} and the two-proton capture reaction 15O(2p,γ)17Ne^{15}\text{O}(2p,\gamma){^{17}\text{Ne}} is expected. Purpose: Determine the three-body radiative capture reaction rate for 17Ne{^{17}\text{Ne}} formation including sequential and direct, resonant and non-resonant contributions on an equal footing. Method: Two different discretization methods have been applied to generate 17^{17}Ne states in a full three-body model: the analytical transformed harmonic oscillator method and the hyperspherical adiabatic expansion method. The binary pp--15^{15}O interaction has been adjusted to reproduce the known spectrum of the unbound 16^{16}F nucleus. The dominant E1E1 contributions to the 15O(2p,γ)17Ne^{15}\text{O}(2p,\gamma){^{17}\text{Ne}} reaction rate have been calculated from the inverse photodissociation process. Results: Three-body calculations provide a reliable description of 17^{17}Ne states. The agreement with the available experimental data on 17^{17}Ne is discussed. It is shown that the 15O(2p,γ)17Ne^{15}\text{O}(2p,\gamma){^{17}\text{Ne}} reaction rates computed within the two methods agree in a broad range of temperatures. The present calculations are compared with a previous theoretical estimation of the reaction rate. Conclusions: It is found that the full three-body model provides a reaction rate several orders of magnitude larger than the only previous estimation. The implications for the rp-process in type I x-ray bursts should be investigated.Comment: 10 pages, 10 figures. Corrected versio

    Anomalous quartic WWγγWW\gamma\gamma couplings in epep collisions at the LHeC and the FCC-he

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    We conducted a study on measuring W+W−W^+W^- production and on the sensitivity limits at 95%95\% Confidence Level on thirteen anomalous couplings obtained by dimension-8 operators which are related to the anomalous quartic WWγγWW\gamma\gamma couplings. We consider the main e−p→e−γ∗γ∗p→e−W+W−pe^-p \to e^-\gamma^*\gamma^*p \to e^-W^+W^-p reaction with the sub-process γ∗γ∗→W+W−\gamma^*\gamma^* \to W^+W^- at the Large Hadron electron Collider (LHeC) and the Future Circular Collider-hadron electron (FCC-he). For the LHeC, energies of the e−e^- beams are taken to be Ee=60E_e =60 and 140 GeV and the energy of the pp beams is taken to be Ep=7E_p = 7 TeV. For the FCC-he, energies of the e−e^- beams are taken to be Ee=60E_e =60 and 140 GeV and the energy of the pp beams is taken to be Ep=50E_p = 50 TeV, respectively. It is interesting to notice that the LHeC and the FCC-he will lead to model-independent limits on the anomalous quartic WWγγWW\gamma\gamma couplings which are one order of magnitude stringent than the CMS Collaboration limits, in addition to being competitive with other limits reported in the literature.Comment: 28 pages, 10 Figures and 13 Table

    Chern-Simons and Born-Infeld gravity theories and Maxwell algebras type

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    Recently was shown that standard odd and even-dimensional General Relativity can be obtained from a (2n+1)(2n+1)-dimensional Chern-Simons Lagrangian invariant under the B2n+1B_{2n+1} algebra and from a (2n)(2n)-dimensional Born-Infeld Lagrangian invariant under a subalgebra LB2n+1\cal{L}^{B_{2n+1}} respectively. Very Recently, it was shown that the generalized In\"on\"u-Wigner contraction of the generalized AdS-Maxwell algebras provides Maxwell algebras types Mm\cal{M}_{m} which correspond to the so called BmB_{m} Lie algebras. In this article we report on a simple model that suggests a mechanism by which standard odd-dimensional General Relativity may emerge as a weak coupling constant limit of a (2p+1)(2p+1)-dimensional Chern-Simons Lagrangian invariant under the Maxwell algebra type M2m+1\cal{M}_{2m+1}, if and only if m≥pm\geq p. Similarly, we show that standard even-dimensional General Relativity emerges as a weak coupling constant limit of a (2p)(2p)-dimensional Born-Infeld type Lagrangian invariant under a subalgebra LM2m\cal{L}^{\cal{M}_{2m}} of the Maxwell algebra type, if and only if m≥pm\geq p. It is shown that when m<pm<p this is not possible for a (2p+1)(2p+1)-dimensional Chern-Simons Lagrangian invariant under the M2m+1\cal{M}_{2m+1} and for a (2p)(2p)-dimensional Born-Infeld type Lagrangian invariant under LM2m\cal{L}^{\cal{M}_{2m}} algebra.Comment: 30 pages, accepted for publication in Eur.Phys.J.C. arXiv admin note: text overlap with arXiv:1309.006
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