Read The Nature of Mathematics Online

by Geeky Nigeria

60 THE NATURE OF MATHEMATICS 

We have met this difficulty when considering the method of 
indivisibles, and will meet it again when considering the in- 
finitesimal calculus, and will only see how it is overcome when 
we have become familiar with the conception of a " limit." 

This new notion of velocity includes that of uniform velocity 
as a particular case. In fact, the rules of the infinitesimal 

calculus allow us to conclude, from the equation =a, where 

dt 



a is some constant, the equation 8 = at + b, where b is another 
constant. We must remember that all this was not expressly 
formulated until about fifty years after Galileo had published 
his investigations on the motion of falling. 

If we consider the curve of velocities, uniformly accelerated 
motion occupies in it exactly the same place as uniform velocity 
does in the curve of spaces. If we denote by v the numerical 
measure of the velocity at the end of t units of time, the 
acceleration, in the notation of the differential calculus, is 

measured by , and the equation = ft, where h is some 
dt dt 

constant, is the equation of uniformly accelerated motion. In 
Newtonian dynamics, we have to consider variably accelerated 
motions, and this is where the infinitesimal calculus or some 
practically equivalent calculus such as Newton's " method of 
fluxions " becomes so necessary in theoretical mechanics. 

We will now consider the curve of spaces for uniformly 
accelerated motion. On this diagram the arcs being t and s 
we will draw the curve 



where g denotes a constant. Of course, this is the same thing 

CJOC 

as drawing the curve y = y in a plane divided up by the 

m 

a;-axis and the y-axis of Descartes. This curve is a parabola 
passing through the origin. An interesting thing about this 
curve is that it is the curve that would be described by a body 
projected obliquely near the surface of the earth if the air did 
not resist, and is very nearly the path of such a projectile in the 
resisting atmosphere. A free body, according to Galileo's view, 
always falls towards the earth with a uniform vertical accelera- 
tion measured by the above number g. If we project a body 
vertically upwards with the initial velocity of c units, its velocity 

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