19,072 research outputs found

    Curvature Inspired Cosmological Scenario

    Full text link
    Using modified gravity with non-linear terms of curvature, R2R^2 and R(r+2)R^{(r +2)} (with rr being the positive real number and RR being the scalar curvature), cosmological scenario,beginning at the Planck scale, is obtained. Here, a unified picture of cosmology is obtained from f(R)f(R)- gravity. In this scenario, universe begins with power-law inflation, followed by deceleration and acceleration in the late universe as well as possible collapse of the universe in future. It is different from f(R)f(R)- dark energy models with non-linear curvature terms assumed as dark energy. Here, dark energy terms are induced by linear as well as non-linear terms of curvature in Friedmann equation being derived from modified gravity.It is also interesting to see that, in this model, dark radiation and dark matter terms emerge spontaneously from the gravitational sector. It is found that dark energy, obtained here, behaves as quintessence in the early universe and phantom in the late universe. Moreover, analogous to brane-tension in brane-gravity inspired Friedmann equation, a tension term λ\lambda arises here being called as cosmic tension. It is found that, in the late universe, Friedmann equation (obtained here) contains a term ρ2/2λ- \rho^2/2\lambda (ρ\rho being the phantom energy density) analogous to a similar term in Friedmann equation with loop quantum effects, if λ>0\lambda > 0 and brane-gravity correction when λ<0.\lambda < 0.Comment: 19 Pages. To appear in Int. J. Thro. Phy

    Simulation of unsteady rotational flow over propfan configuration

    Get PDF
    During the past decade, aircraft engine manufacturers and scientists at NASA have worked on extending the high propulsive efficiency of a classical propeller to higher cruise Mach numbers. The resulting configurations use highly swept twisted and very thin blades to delay the drag divergence Mach number. Unfortunately, these blades are also susceptible to aeroelastic instabilities. This was observed for some advanced propeller configurations in wind tunnel tests at NASA Lewis Research Center, where the blades fluttered at cruise speeds. To address this problem and to understand the flow phenomena and the solid fluid interaction involved, a research effort was initiated at Georgia Institute of Technology in 1986, under the support of the Structural Dynamics Branch of the NASA Lewis Research Center. The objectives of this study are: (1) the development of solution procedures and computer codes capable of predicting the aeroelastic characteristics of modern single and counter-rotation propellers; and (2) the use of these solution procedures to understand physical phenomena such as stall flutter, transonic flutter, and divergence
    corecore