Fasten your belts

Suppose you're in a spaceship leaving the earth. Half of your trip, that has a total distance of L L , you're accelerated by a constant force of F = m a 0 F = ma_{0} , where m m is the mass of the spaceship. The other half of the trip, the force changes direction until the end of the trip, reaching your destination with velocity 0. The time you took to reach your destination, as seen by someone from the earth, can be written as t = A c a 0 ( ( a 0 L B c 2 + C ) 2 + D ) 1 2 , t = \frac{Ac}{a_{0}} \left ( \left ( \frac{a_{0}L}{Bc^{2}} + C \right )^{2} + D \right )^{\frac12} , where A A , B B , C , C, and D D are all integers.

What is the value of A + B + C + D ? A + B + C + D?


The answer is 4.

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1 solution

According to Newton (and that does not change in relativity):

p ˙ = F = m a 0 . \dot{p} = F = ma_{0}.

But, of course, the momentum for Einstein is a little bit different than it is for Newton: p = γ m v p = \gamma m v , where

γ = 1 1 ( v c ) 2 . \gamma = \frac{1}{\sqrt{1 - \left ( \frac{v}{c} \right )^{2}}}.

Then it is easy to see that p ˙ = γ 3 m v ˙ = m a 0 \dot{p} = \gamma^{3} m \dot{v} = ma_{0} from which we find

d v ( 1 ( v c ) 2 ) 3 / 2 = a 0 d t . \frac{dv}{\left ( 1 - \left ( \frac{v}{c} \right )^{2} \right )^{3/2}} = a_{0} dt.

Integrating and isolating the velocity we'll find:

v ( t ) = a 0 t 1 + ( a 0 t c ) 2 . v(t) = \frac{a_{0}t}{\sqrt{1 + \left ( \frac{a_{0}t}{c} \right )^{2}}}.

As we know the total length of the trip, it would be nice if we could find a relation between time and position. It is easy to find, since d x = v ( t ) d t dx = v(t) dt . Therefore

L = 0 L d x = 2 0 t f / 2 a 0 t 1 + ( a 0 t c ) 2 d t = 2 c 2 a 0 ( ( ( a 0 t f 2 c ) 2 + 1 ) 1 / 2 1 ) . L = \int_{0}^{L} dx = 2 \int_{0}^{t_f/2} \frac{a_{0}t}{\sqrt{1 + \left ( \frac{a_{0}t}{c} \right )^{2}}} \, dt = \frac{2c^{2}}{a_{0}} \left ( \left ( \left ( \frac{a_{0}t_f}{2c} \right )^{2} + 1 \right )^{1/2} - 1 \right ).

The integration on t t is bounded in the interval [ 0 , t f / 2 ] \left [ 0, t_f/2 \right ] because the force changes direction exactly at x = L / 2 x = L/2 . But, as this is a symmetrical configuration, the total time integral is just twice the value we get (therefore the "2" before the integral). Isolating for t f t_f :

t f = 2 c a 0 ( ( a 0 L 2 c 2 + 1 ) 2 1 ) 1 / 2 . t_f = \frac{2c}{a_{0}} \left ( \left ( \frac{a_{0}L}{2c^{2}} + 1 \right )^{2} - 1 \right )^{1/2}.

So A = 2 A = 2 , B = 2 B = 2 , C = 1 C = 1 and D = 1 D = - 1 . The sum is 4 4 .

I loved your solution, it is very clearly written! I am a novice in relativity, and still I found it very easy to understand how you found solved this problem, how you found out the distance as a function of time.

I tried to compare this result with the result we would get using classical mechanics, for fun. If we use classical mechanics, we obtain t f = 2 L a 0 t_f = 2 \sqrt{\dfrac{L}{a_0}} . If we use relativity, we get t f = 2 L a 0 + L 2 4 c 2 t_f = 2 \sqrt{\dfrac{L}{a_0} + \dfrac{L^2}{4c^2}} . Indeed, if L a 0 \dfrac{L}{a_0} is much greater than L 2 4 c 2 \dfrac{L^2}{4c^2} , then both times become closer in value to each other.

PS. There is a typo in the final equation. There is a power of 1 / 2 1/2 missing in the expression for t f t_f .

Pranshu Gaba - 4 years, 3 months ago

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Hey there! I'm glad to hear you're learning relativity and I'm also glad that my problem kinda of helped you, hehe. I'll be posting some relativity problems in the near future, hope I can keep helping ya. xD Also, thanks for pointing out the typo. :)

A Former Brilliant Member - 4 years, 3 months ago

I found a similar problem in Griffith's Electrodynamics, so I just applied the results of that problem to this problem. Constant force motion in Special Relativity results to position being a hyperbolic function of time, thus this is also known as hyperbolic motion, as opposed to parabolic motion in Classical Mechanics. Hyperbolic motion arises when a charged particle is in a uniform electric field.

Ramon Vicente Marquez - 4 years, 3 months ago

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