Suppose a particle with mass m1 and speed v1i undergoes an elastic collision with stationary particle of mass m2. After the collision, particle of mass m1 moves with speed v1f in a direction of angle θ above the line it was moving previously. Particle with mass m2 moves with speed v2f in a direction of angle ϕ below the line which particle with mass m1 was moving previously. Using equations for conservation of momentum and kinetic energy, how can we prove these two equations
v1fv1i=m1m1+m2[cosθ±√cos2θ−m21−m22m21]
and
tan(θ+ϕ)tan(ϕ)=m1+m2m1−m2 ?
EDIT. Here is what I've done:
For the first one, set the xy coordinate system so that the positive direction of the x axis points toward the original path of the particle with mass m1. So we have three equations:
m1v1i=m1v1fcosθ+m2v2fcosϕ
0=m1v1fsinθ−m2v2fsinϕ
m1v21i=m1v21f+m2v22f.
From the second one, we get:
v2f=m1v1fsinθm2sinϕ
Plotting this into third equation, we get
v21i=v21f(1+m1sin2θm2sin2ϕ) (1)
From the first equation, we have
cosϕ=m1(v1i−v1fcosθ)m2v2f
which after applying the equation we have for v2f becomes
sin2ϕ=11+(v1i−v1fcosθ)2sin2θ×v1f2
Plotting this into equation (1), gives us an equation in terms of m1, m2, v1f, v1i and θ, but it is too far from what I expected.
For the second one, assigning the xy coordinate in a way that the positive direction of the x axis points toward the final path of the particle m2, will give us three equations (two for conservation of linear momentum and one for conservation of kinetic energy), but I don't know what to do next.
Answer
Since this is a homework problem, I will only provide a sketch of the solution. From the conservation laws, we have the three equations
m1v1i−m1v1fcosθ=m2v2fcosϕ,m1v1fsinθ=m2v2fsinϕ,m1v21i−m1v21f=m2v22f.
Summing the squares of (1) and (2) eliminates ϕ. The RHS of the resultant equation contains v22f which can be eliminated using (3). Then, one would obtain a quadratic equation in terms of v1fv1i, which can be solved to obtain the desired equation
v1fv1i=m1m1+m2[cosθ±√cos2θ−m21−m22m21].
For the next equation, we rotate the axes to obtain the angle θ+ϕ more easily. Here, the conservation laws are
m1v1icosϕ−m1v1fcos(θ+ϕ)=m2v2f,m1v1isinϕ=m1v1fsin(θ+ϕ),m1v21i−m1v21f=m2v22f. First, we square (4) and use (6) to eliminate v2f. Then, we use (5) to eliminate v1i,vif from the resultant equation, obtaining an equation in terms of ϕ and θ+ϕ. Using trigonometric identities, we get an equation in terms of tanϕ and tan(θ+ϕ) only. Then, this equation can be rewritten as a quadratic equation in tanϕtan(θ+ϕ): [1−tanϕtan(θ+ϕ)]2=m2m1[1−tan2ϕtan2(θ+ϕ)], which can be solved to obtain the desired equation
tan(θ+ϕ)tan(ϕ)=m1+m2m1−m2.
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