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Newton’s second law establishes a relationship between the force F
acting on a body of mass m and the acceleration a caused by this force.
The acceleration a of a body is directly proportional to the acting force F and inversely proportional to its mass m, that is a=Fm
or
F=ma=md2rdt2.
This formulation is valid for systems with constant mass. When the mass changes (for example, in the case of relativistic motion), Newton’s second law takes the form
F=dpdt,
where p is the impulse (momentum) of the body.
In general, the force F can depend on the coordinates of the body, i.e., the radius vector r , its velocity v , and time t :
F=F(r,v,t).
Below we consider the special cases where the force
F
depends only on one of these variables.
Force Depends on Time:
F=F(t)
Assuming that the motion is one-dimensional, Newton’s second law is written as the second order differential equation:
md2xdt2=F(t).
Integrating once, we find the velocity of the body v(t):
v(t)=v0+1mt∫0 F(τ)dτ.
Here we assume that the body begins to move at time
t=0 with the initial velocity
v(t=0)=v0.
Integrating again, we get the law of motion
x(t):x(t)=x0+t∫0 v(τ)dτ , where
x0 is the initial coordinate of the body,
τ is the variable of integration.