For wavelength of visible radiation of Hydrogen spectrum, Balmer gave an equation as \(λ = \frac{xm^2}{m^2-4}\), where m is the integer value. The value of x in terms of Rydberg's constant R is
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Start from \(\dfrac1\lambda=R\left(\dfrac1{2^2}-\dfrac1{m^2}\right)\) and invert.