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تابع مقال الدكتور هالتون ارب
علم الكونيات والفيزياء

Proper time for local physics

Led by investigations of Tepper Gill and Hans Montanus (1999), among others, a new way of treating classical physics problems is evolving. It is called proper time physics because there are two time scales, t, the universal time and the different τ time scales for many different objects. It takes place in flat (Euclidean) space with a preferred reference frame. As the summary Table 1 shows, these essential properties are exactly the same as in the Narlikar-Arp variable mass cosmological solution. The m(t) properties do not come into the traditional local physics problems because the creation epoch of the dominant material is the same. But on the cosmological scale the effects of different creation epochs are enormous (and lead to the reductio ad absurdum of the Big Bang). It is very attractive, some might even say mandatory, to have at present the same physics applied to phenomena on all scales.