- ✓$510\, KeV$
- B$931\, KeV$
- C$510 \,MeV$
- D$931\, MeV$
Here ${m_e} = 9.1 \times {10^{ - 31}}kg$ and $c =$ velocity of light
$\therefore $Rest energy $ = 9.1 \times {10^{ - 31}} \times {(3 \times {10^8})^2}joule$
$ = \frac{{9.1 \times {{10}^{ - 31}} \times {{(3 \times {{10}^8})}^2}}}{{1.6 \times {{10}^{ - 19}}}}eV = 510\;keV$
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$( R _{\text {out }}=200 \Omega, R _{\text {in }}=100 k \Omega,$$ V _{ cC }=3 volt , V _{ BE }=0.7 volt ,V _{ GE }=0, \beta=200 )$
$(A)$ the cut-off wavelength will reduce to half, and the wavelengths of the characteristic $X$-rays will remain the same
$(B)$ the cut-off wavelength as well as the wavelengths of the characteristic $X$-rays will remain the same
$(C)$ the cut-off wavelength will reduce to half, and the intensities of all the $X$-rays will decrease
$(D)$ the cut-off wavelength will become two times larger, and the intensity of all the $X$-rays will decrease