Question
[Question Context: Consider the motion of a test particle of (constant) mass m inside the gravitational field produced by the Sun in the context of special relativity.
In addition, consider the equations of motion for the test particle, which can be written as d(mγc)dt=→vc⋅→F
OR
d(mγ→v)dt=→F,
where →v is the speed of the test particle, c is the (constant) speed of light, and by definition, γ≡1√1−→v2c2.
In addition, the gravitational force is given by →F≡−GMmr2ˆer
where ˆer is the unit vector in the direction between the Sun (of mass M) and the test particle (of mass m).]
The Question Itself
Solve the previously found differential equation d2udθ2+u(1−G2M2ℓ2c2)−GMdℓ2=0
Source: [NOT APPLICABLE]
Personal Comment
Perhaps it's just me, however, I can't seem to solve this differential equation in a clean manner. For some reason, I always get a ton of constants and I feel like I am doing something wrong. With that in mind, any assistance, hints, or comments to help me toward the right answer would be much appreciated. Thank you for reading!
Answer
Re-write for legibility: u″(θ)+αu(θ)−β=0
Which is the classic ODE of the SHM. Solve and back-substitute. Don't neglect the BCs!
No comments:
Post a Comment