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    2.

    The wavelength of radiation emitted is Ξ»0{\lambda _0} when an electron jumps from the third to second orbit of hydrogen atom. For the electron jump from fourth to the second orbit of the hydrogen atom, the wavelength of radiation emitted will be

    A

    (1625)Ξ»0\left( {\frac{{16}}{{25}}} \right){\lambda _0}

    B

    (2027)Ξ»0\left( {\frac{{20}}{{27}}} \right){\lambda _0}

    C

    (2720)Ξ»0\left( {\frac{{27}}{{20}}} \right){\lambda _0}

    D

    (2516)Ξ»0\left( {\frac{{25}}{{16}}} \right){\lambda _0}

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    3.

    The energy of electron in the nth orbit of hydrogen atom is expressed asEn=βˆ’13.6n2eV{E_n} = \frac{{ - 13.6}}{{{n^2}}}eV. The shortest and longest wavelength of Lyman series will be

    A

    910  A0,  1213  A0910\,\,{A^0},\,\,1213\,\,{A^0}

    B

    5463  A0,  7858  A05463\,\,{A^0},\,\,7858\,\,{A^0}

    C

    1315  A0,  1530  A01315\,\,{A^0},\,\,1530\,\,{A^0}

    D

    None of these

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    6.

    The wavelength of the first line of Balmer series is 6563  A06563\,\,{A^0}. The Rydberg constant for hydrogen is about

    A

    1.09{\mkern 1mu} {\mkern 1mu}  imes {10^7}{\mkern 1mu}\;{m^{ - 1}}

    B

    1.09{\mkern 1mu} {\mkern 1mu}  imes {10^8}{\mkern 1mu} per\;m

    C

    1.09{\mkern 1mu} {\mkern 1mu}  imes {10^9}{\mkern 1mu} per\;m

    D

    1.09{\mkern 1mu} {\mkern 1mu}  imes {10^5}{\mkern 1mu} {\mkern 1mu} per\;m

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    8.

    The ratio of speed of an electron in ground state in Bohrs first orbit of hydrogen atom to velocity of light in air is

    A

    e22 Ρ0hc\frac{{{e^2}}}{{2\,{\varepsilon _0}hc}}

    B

    2 e2Ξ΅0hc\frac{{2\,{e^2}{\varepsilon _0}}}{{hc}}

    C

    e32 Ρ0hc\frac{{{e^3}}}{{2\,{\varepsilon _0}hc}}

    D

    2 Ρ0hce2\frac{{2\,{\varepsilon _0}hc}}{{{e^2}}}

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