9,074 research outputs found

    Structure and growth process of vapor-grown carbon fibers

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    The structure, effect of heat, and growth process of vapor-grown carbon fibers are investigated. The growth process of the carbon fibers could be divided into three stages; nucleation, elongation, and thickening processes. Also, a multi-layered structure can be produced as well as graphitization

    Universality of massive scalar field late-time tails in black-hole spacetimes

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    The late-time tails of a massive scalar field in the spacetime of black holes are studied numerically. Previous analytical results for a Schwarzschild black hole are confirmed: The late-time behavior of the field as recorded by a static observer is given by ψ(t)t5/6sin[ω(t)×t]\psi(t)\sim t^{-5/6}\sin [\omega (t)\times t], where ω(t)\omega(t) depends weakly on time. This result is carried over to the case of a Kerr black hole. In particular, it is found that the power-law index of -5/6 depends on neither the multipole mode \ell nor on the spin rate of the black hole a/Ma/M. In all black hole spacetimes, massive scalar fields have the same late-time behavior irrespective of their initial data (i.e., angular distribution). Their late-time behavior is universal.Comment: 11 pages, 14 figures, published versio

    Theory for Photon-Assisted Macroscopic Quantum Tunneling in a Stack of Intrinsic Josephson Junctions

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    We propose a theory for photon-assisted macroscopic quantum tunneling (MQT) in a stack of capacitively-coupled intrinsic Josephson junctions in which the longitudinal Josephson plasma, i.e., longitudinal collective phase oscillation modes, is excited. The scheme of energy-level quantization in the collective oscillatory states is clarified in the NN-junction system. When the MQT occurs from the single-plasmon states excited by microwave irradiation in the multi-photon process to the uniform voltage state, our theory predicts that the escape rate is proportional to N2N^2. This result is consistent with the recent observation in Bi-2212 intrinsic Josephson junctions.Comment: 5 pages, 2 figure

    Voltage-biased I-V characteristics in the multi-Josephson junction model of high Tc_c superconductor

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    By use of the multi-Josephson junction model, we investigate voltage-biased I-V characteristics. Differently from the case of the single junction, I-V characteristics show a complicated behavior due to inter-layer couplings among superconducting phase differences mediated by the charging effect. We show that there exist three characteristic regions, which are identified by jumps and cusps in the I-V curve. In the low voltage region, the total current is periodic with trigonometric functional increases and rapid drops. Then a kind of chaotic region is followed. Above certain voltage, the total current behaves with a simple harmonic oscillation and the I-V characteristics form a multi-branch structure as in the current-biased case. The above behavior is the result of the inter-layer coupling, and may be used to confirm the inter-layer coupling mechanism of the formation of hysteresis branches.Comment: 12 pages, Latex, 4 figure

    Inflaton perturbations in brane-world cosmology with induced gravity

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    We study cosmological perturbations in the brane models with an induced Einstein-Hilbert term on a brane. We consider an inflaton confined to a de Sitter brane in a five-dimensional Minkowski spacetime. Inflaton fluctuations excite Kaluza-Klein modes of bulk metric perturbations with mass m2=2(21)(+1)H2m^2 = -2(2\ell-1) (\ell +1) H^2 and m2=2(2+3)H2m^2 = -2\ell(2\ell+3) H^2 where \ell is an integer. There are two branches (±\pm branches) of solutions for the background spacetime. In the ++ branch, which includes the self-accelerating universe, a resonance appears for a mode with m2=2H2m^2 = 2 H^2 due to a spin-0 perturbation with m2=2H2m^2 = 2H^2. The self-accelerating universe has a distinct feature because there is also a helicity-0 mode of spin-2 perturbations with m2=2H2m^2 = 2H^2. In the - branch, which can be thought as the Randall-Sundrum type brane-world with the high energy quantum corrections, there is no resonance. At high energies, we analytically confirm that four-dimensional Einstein gravity is recovered, which is related to the disappearance of van Dam-Veltman-Zakharov discontinuity in de Sitter spacetime. On sufficiently small scales, we confirm that the lineariaed gravity on the brane is well described by the Brans-Dicke theory with ω=3Hrc\omega=3Hr_c in - branch and ω=3Hrc\omega = -3H r_c in ++ branch, respectively, which confirms the existence of the ghost in ++ branch. We also study large scale perturbations. In ++ branch, the resonance induces a non-trivial anisotropic stress on the brane via the projection of Weyl tensor in the bulk, but no instability is shown to exist on the brane.Comment: 20 pages, 4 figure

    f(R) brane cosmology

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    Despite the nice features of the Dvali, Gabadadze and Porrati (DGP) model to explain the late-time acceleration of the universe, it suffers from some theoretical problems like the ghost issue. We present a way to self-accelerate the normal DGP branch, which is known to be free of the ghost problem, by means of an f(R) term on the brane action. We obtain the de Sitter self-accelerating solutions of the model and study their stability under homogeneous perturbations.Comment: 4 pages, 2 figures. Contribution to the proceedings of Spanish Relativity Meeting 2009, Bilbao, Spain, 7-11 September 200
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