63,610 research outputs found

    The generation of helical magnetic field in a viable scenario of Inflationary Magnetogenesis

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    We study the generation of helical magnetic fields in a model of inflationary magnetogenesis which is free from the strong coupling and back-reaction problems. To generate helical magnetic fields, we add an f2F~μνFμνf^2 \tilde{F}^{\mu\nu} F_{\mu\nu} term to the lagrangian of Ratra model. The strong coupling and back-reaction problems are avoided if we take a particular behaviour of coupling function ff, in which ff increases during inflation and decreases post inflation to reheating. The generated magnetic field is fully helical and has a blue spectrum, dρB/dlnkk4d\rho_B/d\ln k \propto k^4. This spectrum is obtained when coupling function fa2f\propto a^2 during inflation. The scale of reheating in our model has to be lower than 40004000 GeV to avoid back-reaction post inflation. The generated magnetic field spectrum satisfies the γ\gamma-ray bound for all the possible scales of reheating. The comoving magnetic field strength and its correlation length are 4×1011\sim 4 \times 10^{-11} G and 7070 kpc respectively, if reheating takes place at 100 GeV. For reheating at the QCD scales of 150150 MeV, the field strength increases to \sim nano gauss, with coherence scale of 0.60.6 Mpc.Comment: 11 pages, Submitted to PR

    Radiating spherical collapse with heat flow

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    We present here a simple model of radiative gravitational collapse with radial heat flux which describes qualitatively the stages close to the formation of a superdense cold star. Starting with a static general solution for a cold star, the model can generate solutions for the earlier evolutionary stages. The temporal evolution of the model is specified by solving the junction conditions appropriate for radiating gravitational collapse.Comment: 13 pages, including 3 figures, submitted to IJMP-
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