Parabolic light rays in a reciprocal-square-root speed profile
ID: parabolic-light-rays-in-a-reciprocal-square-root-speed-profile
For speed , with , the elapsed-time integrand is . The Beltrami identity gives , where is the turning height. Integration yields the displayed parabola. If the endpoints are , symmetry gives and . Hence , and the two algebraic turning heights are . Only heights lying within the specified optical layer are admissible.
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