The Sunyaev-Zeldovich Effect in The Case of The 1-5μm Infrared Background

In this paper, we propose a new method intended to measure the 1-5 μm IR background. This new method is based on the measurement of a peculiar frequency-dependent anisotropy of the 1-5 μm IR background(if it exist). Which is produced by the Compton interaction of the 1-5 μm IR background photons with hot gases in rich cluster of galaxies (electron temperature T_e-10⁸ K).This method automatically cancels the galactic and zodiacal background.