Saturday, 18 July 2015

homework and exercises - Velocity of an object undergoing homogenous acceleration


So I was considering the following problem within the context of Special Relativity:


Given an object O, with initial velocity v, undergoing constant acceleration at a rate of a, I want to express the velocity as a function of time.


So from newtonian mechanics:


velocity (S) = initial-velocity (v) + acceleration*time (a*t)



However this makes no sense in context of special relativity since it suggests that given a particular acceleration and enough time it is possible to exceed the speed of light.


What I realized I needed was a mapping from newtonian velocity to its special relativistic equivalent. Which I derived as follows:


Kinetic Erel = m0c2/(1v2rel/c2)1/2m0c2


Kinetic Enewt = 1/2m0v2newt


Where vrel = relativistic velocity, vnewt = newtonian velocity, m0 = rest mass, c = speed of light.


Setting both equal to each other and dividing by m0 I find that: c2(1v2relc2)12c2=12v2newt


Adding c2 to both sides and raising to the power -1 I find: (1vrel2c2)12c2=1c2+1/2v2newt


multiplying both sides by c^2, squaring both sides, subtracting 1, multiplying by -1, and taking the square root I now have: vrel=c(1c2c2+1/2v2newt)12


So given a velocity from a newtonian problem ex: 5 m/s I can convert to its energy equivalent in special relativity via this formula. Note that as newtonian velocity goes to infintiy relativistic velocity approaches c and at 0 both quantities are 0.


Given this framework I know for fact from earlier that newtonian velocity is given as:



v(initial) + at or using our previously defined units: v + at.


Therefore the relativistic velocity can be expressed as: vrel=c(1c2c2+1/2(v+at)2)12


Is this correct?



Answer



In special relativity, proper acceleration is defined as a=dudt,

where u=dxdτ=vdtdτ
is the proper velocity, and dτ=dt1v2/c2
is the proper time. So ddt(v1v2/c2)=a.
If we integrate this over a time interval [0,t], we get, if a is constant, v1v2/c2v01v20/c2=at,
with v0 the initial velocity. If we define the constant w0=v01v20/c2,
then v2=(1v2/c2)(at+w0)2,
so that we finally get v(t)=at+w01+(at+w0)2/c2.


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