18,021 research outputs found

    The CWKB approach to non-reflecting potential and cosmological implications

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    We discuss the method of calculating the reflection coefficient using complex trajectory WKB (CWKB) approximation. This enables us to give an interpretation of non-reflecting nature of the potential under certain conditions and clarify some points, reported incorrectly elsewhere [vs:ejp] for the potential U(x)=−U0cosh2(x/a)U(x)=-U_0cosh^2(x/a). We show that the repeated reflectios between the turning points are essential, which most authors overlooked, in obtaining the non-reflecting c ondition. We find that the considered repeated reflection paths are in conformity with Bogolubov transformation technique. We discuss the implications of the results when applied to the particle production scenario, considering xx as a time variable and also stress the cosmological implications of the result with reference to radiation domonated and de Sitter spacetime.Comment: 9 pages, late

    Secrecy versus patents: process innovations and the role of uncertainty

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    Whilst firms often prefer secrecy to patents and process innovations particu- larly lend themselves to secrecy, we establish a rationale for process innovators who patent. Using a simple two-period model, we show that under myopic op- timisation, the incentive to patent rather than pursue secrecy increases as the probability that the rival firm attaches to it being low-cost falls and as the pro- portion of the cost reduction due to the innovation, secured by the rival firm in the period after the patent has expired, falls. However, the gain to the innovating firm from patenting rather than secrecy strictly increases if the cost reduction due to the innovation is sufficiently small that the high-cost firm could profitably bluff that it is low-cost. Finally, allowing the low-cost firm the option of using an output signal in such cases, may make the patent strategy more or less attractive relative to the case of myopic optimisation

    Measuring the Balance of Intra-Regional Trade

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    We introduce an original method of measuring the extent of the overall balance of migration among countries within a region which allows comparisons of the balance over time as well as between regions and various possible sub-regions

    Effect of realistic interatomic interactions and two-body correlation on the heat capacity of a trapped BEC

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    An approximate many-body theory has been used to calculate the heat capacity and the condensate fraction of a BEC with effective repulsive interaction. The effect of interactions has been analyzed and compared with the non-interacting case. It has been found that the repulsive interaction lowers the critical temperature from the value found in the non-interacting case. The difference between the critical temperatures increases with the increase in the total number of atoms in the trap.Comment: 15 pages, 5 figure

    Monodromy group for a strongly semistable principal bundle over a curve, II

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    Let XX be a geometrically irreducible smooth projective curve defined over a field kk. Assume that XX has a kk-rational point; fix a kk-rational point x∈Xx\in X. From these data we construct an affine group scheme GX{\mathcal G}_X defined over the field kk as well as a principal GX{\mathcal G}_X-bundle EGXE_{{\mathcal G}_X} over the curve XX. The group scheme GX{\mathcal G}_X is given by a Q{\mathbb Q}--graded neutral Tannakian category built out of all strongly semistable vector bundles over XX. The principal bundle EGXE_{{\mathcal G}_X} is tautological. Let GG be a linear algebraic group, defined over kk, that does not admit any nontrivial character which is trivial on the connected component, containing the identity element, of the reduced center of GG. Let EGE_G be a strongly semistable principal GG-bundle over XX. We associate to EGE_G a group scheme MM defined over kk, which we call the monodromy group scheme of EGE_G, and a principal MM-bundle EME_M over XX, which we call the monodromy bundle of EGE_G. The group scheme MM is canonically a quotient of GX{\mathcal G}_X, and EME_M is the extension of structure group of EGXE_{{\mathcal G}_X}. The group scheme MM is also canonically embedded in the fiber Ad(EG)x{\rm Ad}(E_G)_{x} over xx of the adjoint bundle.Comment: This final version includes strengthening of the result by referee's comments. K-Theory (to appear

    The Holography Hypothesis in Pre-Big-Bang Cosmology with String Sources

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    The holographic ratio in Pre-big bang string cosmology is obtained in the presence string sources. An iterative procedure is adopted to solve the equations of motion and derive the ratio in four dimensional world. First the zeroth order ratio is computed in the remote past, i.e. at t=−∞t=-\infty, then the holographic ratio is obtained taking into account the evolution of the backgrounds following the iterative procedure. The corrections to the zeroth order value of the ratio depends on the form of the initial number distribution of the strings chosen. Moreover, we estimate the holographic ratio in the recent past (i.e. when γ=−1d\gamma=-\frac{1}{d}) and in the remote past (i.e. when γ=0\gamma= 0), γ≡pϱ\gamma\equiv\frac{p}{\varrho}, in different dimensions in the Einstein frame and in the string frame. We find that in the first case it has similar time dependences in both the frames, especially in four dimensions the ratio is explicitly computed to be the same in the two cases, whereas for γ=0\gamma=0 case the time dependence is different.Comment: 33 pages, latex, five figure
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