An impact model of Newton's law of gravitation

被引：9

作者：

Wilhelm, Klaus ^{[1
]}

Wilhelm, Horst ^{[2
]}

Dwivedi, Bhola N. ^{[3
]}

机构：

[1] Max Planck Inst Sonnensyst Forsch MPS, D-37191 Katlenburg Lindau, Germany

[2] Cephalos Gesell Automatisierung mbH, D-26871 Papenburg, Germany

[3] Banaras Hindu Univ, Indian Inst Technol, Dept Appl Phys, Varanasi 221005, Uttar Pradesh, India

来源：

ASTROPHYSICS AND SPACE SCIENCE | 2013年 / 343卷 / 01期

关键词：

Gravitation; Impact model; Secular mass increase; TUNNELING TIME; QUANTUM-THEORY; DARK ENERGY; SPEED; UNIVERSE;

D O I：

10.1007/s10509-012-1206-3

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The far-reaching gravitational force-in the approximation of Newton's law of gravitation-is described by a heuristic model with hypothetical massless particles propagating at the speed of light in vacuum and transferring momentum and energy between physical entities through interactions on a local basis. The model has some similarities with the impact theory presented by Nicolas Fatio de Duillier to the Royal Society in 1690. Objections raised against this idea are dispelled by invoking the Special Theory of Relativity, considering non-local interactions, and replacing the shielding concept by a secular mass increase of massive bodies. Some consequences and applications of the model are discussed.

引用

页码：135 / 144

页数：10

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