Disclaimer: The following is a non-rigorous, high-school mathematics "compatible" derivation that aims to provide quick proof of equations presented in Blackett's landmark paper. The concepts I used are based on elementary conservation rules in physics taught in many pre-university physics courses.
BACKGROUND
In 1923, Blackett published a study of "forked" alpha particle tracks observed in a cloud chamber. In the paper, he interpreted those occasional Y-shaped tracks as a consequence of elastic nuclear collision between alpha particles and nucleus of atoms present in the atmosphere. To aid his discussion, he described a convenient way to determine the masses of the target nuclei by measuring the scattering angle of the particles from the initial trajectory of the incident particle. (see the actual equation below circled in red)
The paper provide no mathematical derivation probably because it was considered trivial to the readers then. Since another form of this equation was cited once again in his 1948 Nobel lecture, this post attempts to show how this important equation came to be using physics concepts found in high-school texts.
DERIVATION
First, this equation concerns a situation where two rigid particles are colliding: A rigid incident particle of mass m1 (interpreted as the alpha particle) with initial velocity u is to collide elastically with a rigid stationary target particle of mass m2 (interpreted as the nucleus of atoms present in the atmosphere) in a classical 2-dimension Cartesian reference frame.
The collision result in change of velocity (thus momentum) for both particles where the direction of incident velocity is taken as the "reference axis" and the scattering angle of both particles is the angle it subtends to the "reference axis" respectively. I provide a diagram below illustrating the system before and after collision;
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