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Action-at-a-distance electrodynamics in quasi-steady-state cosmology

机译:准稳态宇宙学中的远距离动作电动力学

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Action-at-a-distance electrodynamics a€“ alternative approach to field theory a€“ can be extended to cosmological models using conformal symmetry. An advantage of this is that, the origin of arrow of time in electromagnetism can be attributed to the cosmological structure. Different cosmological models can be investigated, based on Wheelera€“Feynman absorber theory, and only those models can be considered viable for our Universe which have net full retarded electromagnetic interactions, i.e., forward direction of time. This work evaluates the quasi-steady-state model and demonstrates that it admits full retarded and not advanced solution. Thus, quasi-steady-state cosmology (QSSC) satisfies this necessary condition for a correct cosmological model, based on action-at-a-distance formulation.
机译:距离作用电动力学是场论的一种替代方法,可以使用共形对称性扩展到宇宙学模型。这样做的一个优点是,电磁中时间箭头的起源可以归因于宇宙学结构。可以根据Wheelera的“费曼吸收器”理论研究不同的宇宙学模型,并且只有那些模型具有完全完全延迟的电磁相互作用(即时间的正向)才能被认为对我们的宇宙是可行的。这项工作评估了准稳态模型,并证明它接受了完全滞后而不是高级的解决方案。因此,基于远距离作用公式,准稳态宇宙论(QSSC)满足了正确的宇宙学模型的这一必要条件。

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