Squeeze light through a narrow slit and it refuses to travel straight — it fans out into a bright band with fading fringes. That is diffraction.
Single-Slit DiffractionLive
light bending around edges
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Send light through a narrow slit and it fans out into a bright central band flanked by dimmer fringes — diffraction. The pattern follows a sinc-squared curve, with the first dark fringe where the path difference across the slit equals one wavelength. Narrower slits spread the light more, the diffraction limit that caps every lens and telescope's sharpness.
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How it works
Light passing a single slit spreads into a central bright maximum flanked by weaker fringes, following a sinc-squared intensity pattern. The first dark fringe appears where the path difference across the slit equals one wavelength, so narrower slits spread light more. This diffraction sets the ultimate resolution limit of every lens, microscope, and telescope.
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