7,748 research outputs found

    Generation of Closed Timelike Curves with Rotating Superconductors

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    The spacetime metric around a rotating SuperConductive Ring (SCR) is deduced from the gravitomagnetic London moment in rotating superconductors. It is shown that theoretically it is possible to generate Closed Timelike Curves (CTC) with rotating SCRs. The possibility to use these CTC's to travel in time as initially idealized by G\"{o}del is investigated. It is shown however, that from a technology and experimental point of view these ideas are impossible to implement in the present context.Comment: 9 pages. Submitted to Classical and Quantum Gravit

    Gravitoelectromagnetism and Dark Energy in Superconductors

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    A gravitomagnetic analogue of the London moment in superconductors can explain the anomalous Cooper pair mass excess reported by Janet Tate. Ultimately the gravitomagnetic London moment is attributed to the breaking of the principle of general covariance in superconductors. This naturally implies non-conservation of classical energy-momentum. Possible relation with the manifestation of dark energy in superconductors is questioned.Comment: 10 pages. Poster presented at "From Quantum to Cosmos - Fundamental Physics Research in Space" 22-24 May 2006, To Appear in Int. J. Mod. Phys.

    Single observable concurrence measurement without simultaneous copies

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    We present a protocol that allows us to obtain the concurrence of any two qubit pure state by performing a minimal and optimal tomography of one of the subsystems through measuring a single observable of an ancillary four dimensional qudit. An implementation for a system of trapped ions is also proposed, which can be achieved with present day experimental techniques.Comment: 4 pages, 1 figur

    Pastejo precoce de bezerros de raca leiteira nascidos em duas estacoes do ano.

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    Quintessence and Scalar Dark Matter in the Universe

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    Continuing with previous works, we present a cosmological model in which dark matter and dark energy are modeled by scalar fields Φ\Phi and Ψ\Psi, respectively, endowed with the scalar potentials V(Φ)=Vo[cosh(λκoΦ)1]V(\Phi)=V_{o}[ \cosh {(\lambda \sqrt{\kappa_{o}}\Phi)}-1] and V~(Ψ)=Vo~[sinh(ακoΨ)]β\tilde{V}(\Psi)=\tilde{V_{o}}[ \sinh {(\alpha \sqrt{\kappa_{o}}\Psi)}] ^{\beta}. This model contains 95% of scalar field. We obtain that the scalar dark matter mass is mΦ1026eV.m_{\Phi}\sim 10^{-26}eV. The solution obtained allows us to recover the success of the standard CDM. The implications on the formation of structure are reviewed. We obtain that the minimal cutoff radio for this model is rc1.2kpc.r_{c}\sim 1.2 kpc.Comment: 4 pages REVTeX, 3 eps color figures. Minor changes and references updated. To appear in Classical and Quantum Gravity as a Letter to the Editor. More information at http://www.fis.cinvestav.mx/~siddh/PHI

    Entropic Entanglement Criteria for Continuous Variables

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    We derive several entanglement criteria for bipartite continuous variable quantum systems based on the Shannon entropy. These criteria are more sensitive than those involving only second-order moments, and are equivalent to well-known variance product tests in the case of Gaussian states. Furthermore, they involve only a pair of quadrature measurements, and will thus should prove extremely useful the experimental identification of entanglement.Comment: 4 pages, 2 figure

    Decoherence and the quantum-classical limit in the presence of chaos

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    We investigate how decoherence affects the short-time separation between quantum and classical dynamics for classically chaotic systems, within the framework of a specific model. For a wide range of parameters, the distance between the corresponding phase-space distributions depends on a single parameter χ\chi that relates an effective Planck constant eff\hbar_{\rm eff}, the Lyapunov coeffficient, and the diffusion constant. This distance peaks at a time that depends logarithmically on eff\hbar_{\rm eff}, in agreement with previous estimations of the separation time for Hamiltonian systems. However, for χ1\chi\lesssim 1, the separation remains small, going down with eff2\hbar_{\rm eff}^2, so the concept of separation time loses its meaning.Comment: 5 pages, 4 figures (in 6 postscript files) two of them are color figure
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