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Spherically Symmetric Inflation

机译:球对称膨胀

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摘要

Abstract—It is shown in this letter that in the framework of an inhomogeneous geometry and a massive non-self-interacting scalar field with spherical symmetry, one needs a homogeneous patch bigger than a dizain of horizons in order to start inflation. The results are completely independent of initial conditions on the spatial distribution of the scalar field. The initial condition on the metric parameters are also justified. This is a generalization of the results obtained by E. Calzetta and M. Sakellariadou [1]: Phys. Rev. D 45, 2802 (1992), showing that their conclusions are rather robust.
机译:摘要—在这封信中表明,在一个不均匀的几何结构和一个具有球对称性的巨大的非自相互作用标量场的框架中,为了开始膨胀,需要一个比地层大的均匀斑块。结果完全独立于标量场空间分布的初始条件。度量参数的初始条件也是合理的。这是对E. Calzetta和M. Sakellariadou [1]:物理学的结果的概括。 Rev 45,2802(1992),表明他们的结论是相当可靠的。

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