15,234 research outputs found

    Curvature Inspired Cosmological Scenario

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    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

    Cosmic Evolution with Early and Late Acceleration Inspired by Dual Nature of the Ricci Scalar Curvature

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    In the present paper, it is found that dark energy emerges spontaneously from the modified gravity. According to cosmological scenario, obtained here, the universe inflates for 1037\sim 10^{-37} sec. in the beginning and late universe accelerates after 8.58 Gyrs. During the long intermediate period, it decelerates driven by radiation and subsequently by matter. Emerged gravitational dark energy mimics quintessence and its density falls by 115 orders from its initial value 2.58×1068GeV42.58\times 10^{68} {\rm GeV}^4 to its current value 2.19×1047GeV42.19\times 10^{-47} {\rm GeV}^4 .Comment: 40 pages. To appearin Int. J. Mod. Phys.

    Landau Ghosts and Anti-Ghosts in Condensed Matter and High Density Hadronic Matter

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    It is observed that the ``ghost'' (originally discovered by Landau in quantum electro-dynamics) and its counterparts in other theories are indeed ubiquitous as they occur in a one-loop approximation to any conventional (unbroken) gauge theory. The mechanism is first exposed in its generality via the Dyson equation and a simple but explicit example in condensed matter is provided through the static Clausius-Mossotti and its dynamic counterpart the Lorenz-Lorentz equation. The physical phase transition phenomenon associated with it is found to be super-radiance. We verify quantitatively that water (and many other polar liquids) are indeed super-radiant at room temperature. In quantum chromo-dynamics on the other hand, we encounter, thanks to asymptotic freedom, an ``anti-ghost'' which is closely associated with color confinement. Thus, in QCD, free quarks and glue exist in a super-radiant phase and hadronic matter in the normal one.Comment: LaTeX 12 Pages and 2 *.eps Figure

    Numerical Study of the Lowest Energy Configurations for Global String-Antistring Pairs

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    We investigate the lowest energy configurations for string - antistring pairs at fixed separations by numerically minimizing the energy. We show that for separations smaller than a critical value, a region of false vacuum develops in the middle due to large gradient energy density. Consequently, well defined string - antistring pairs do not exist for such separations. We present an example of vortex - antivortex production by vacuum bubbles where this effect seems to play a dynamical role in the annihilation of the pair. We also study the dependence of the energy of an string-antistring pair on their separation and find deviations from a simple logarithmic dependence for small separations.Comment: 14 pages, in LATEX, 7 figures (not included
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