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THE COSMOLOGICAL IMPLICATIONS OF NONLOCAL GRAVITY

机译：非局部引力的宇宙学意义

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Here, we present a review of the possible impact of a theory of nonlocal gravity, proposed by the author, on some aspects of cosmology. The maximal failure of the quantum prediction of the 'cosmological constant' creates difficulties for a quantum theory of gravity, and for gravity as a local force. The attractive nature of the gravitational force and the negative sign of its energy may be indications that it is intrinsically nonlocal and not limited to speed of light transfer. A new set of equations are needed to reconcile the effects with those observed under local measuring conditions. The cosmological redshift, microwave background radiation and arrow of time now become purely physical phenomena suggesting a totally different cosmology from the one currently generally accepted. The 'cosmological constant', as a consequence, was predicted by this method long before it was experimentally discovered. The calculations also provide values for astronomical constants and predictions in particle physics such as the masses of the lightest neutrinos. Cosmology becomes a result of fundamental physical laws and not a merely historical record of arbitrary events that just happened to take place in some inexplicable sequence.
机译：在这里，我们提出了作者提出的非局部引力理论对宇宙学某些方面可能产生的影响的综述。 “宇宙常数”的量子预测的最大失败给引力量子论和引力作为局部力带来了困难。引力的吸引力及其能量的负号可能表明它本质上是非局部的，并且不限于光传输的速度。需要一套新的方程式来协调这些影响与在局部测量条件下观察到的影响。宇宙学的红移，微波背景辐射和时间箭头现在变成纯粹的物理现象，表明与目前普遍接受的宇宙学完全不同的宇宙学。结果，很早就通过实验发现了“宇宙常数”。这些计算还提供了天文学常数的值以及粒子物理学中的预测，例如最轻的中微子的质量。宇宙学成为基本物理定律的结果，而不仅仅是偶然地以某种莫名其妙的顺序发生的任意事件的历史记录。

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