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机构地区:[1]Department of Nuclear and Energy Engineering, Cheju National University
出 处:《Communications in Theoretical Physics》2010年第5期869-881,共13页理论物理通讯(英文版)
摘 要:We discuss a new class of RSII braneworld cosmology exhibiting accelerated expansion and dominated by quintessence. It is explicitly demonstrated that the universe expansion history (transition from inflation to deceleration epoch to acceleration and effective quintessence era) may naturally occur in such unified theory for some classes of inverse scalar potentials. Besides a decaying effective cosmological constant, the model incorporates an increasing black hole mass, an increasing Maxwellian electrical charge with cosmic time and a time-dependent brahe tension. The cosmological model exhibits several features of cosmological and astrophysical interest for both the early and late universe consistent with recent observations, in particular the ones concerned with the gravitational constants, black holes masses and charges and variation of the gauge coupling parameters with cosmic time. One interesting mark of the constructed model concerns the fact that a black hole mass surrounded by quintessence energy may increase with time even if the horizon disappears.
关 键 词:brane world RSII cosmology higher order curvature corrections black hole black strings effective cosmological constant Maxwellian charge QUINTESSENCE accelerated expansion
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