In Young's double-slit, the m-th bright fringe sits at y_m = m * lambda * L / d, where d is the slit spacing and L the screen distance. The formula comes straight from the path-difference condition, delta = m * lambda, paired with the small-angle approximation. The exact position holds only for coherent monochromatic light, a known wavelength, and aligned slits; real fringes blur with bandwidth, finite slit width, screen calibration, and detector noise.
The paraxial screen position is source-bound to a checked bright path difference. Exact arithmetic here means exact results for the stated model inputs; measured inputs still carry uncertainty and significant-figure limits.
highlighted = computed this step
The screen row starts from a bright path source
The Young-fringe helper does not invent a screen position by itself. It cites an accepted bright path-difference source, then uses the slit spacing and screen distance.
path source accepted=1
Fringe position scales with order
Hold wavelength, screen distance, and slit spacing fixed. The screen position grows in the same ratio as the order.
m123λ2m2m2mL6m6m6md3m3m3my4m8m12m
The first Young fringe cites a path source
The fringe position is accepted only after the Young check cites the bright path-difference source.