Toward General Theories and Extensions I

In these next few posts we want to try and salvage some sort of a general statement about acceleration.

What we will discover is that we can discuss the nature of spacetime, if we start from these basic ideas, without cluttering the discussion with unnecessary mathematical machinery.

We will of-course, GOD willing, discuss that same machinery later on. But notice that we haven't explicitly touched upon aspects of symplectic geometry as yet. This by no means makes our discussions meaningless or exceedingly simplistic. In the meantime, we sacrifice mathematical machinery for a clear understanding of the spacetime events.

On Acceleration III

On Acceleration II

  

   

On Acceleration

In these next postings, what we try to do, we extend the usual standard classical models. In particular, we ape the notion of a coordinate acceleration. That which is equivalent to the difference between the proper acceleration and the acceleration in a frame in which a particle/entity is undergoing constant acceleration.

 The link to this rather tenous example has been provided above.

Imagine that the force/acceleration exerted by a particle M^ (M hat) onto another particle U (mu) changes as M^ approaches U.

In the next frame, imagine that M^ is as a result of the breakdown of a much larger particle. That M^ is the difference between the larger mass M1 and the smaller mass M*.

What we try to develop is a classical theory of how the change in acceleration experienced by U may develop. Essentially, by replacing the mass M^ by its equality. The reason why we may want to do this is so that we explore how generalisations can be made.