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Physics Test - 23

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Physics Test - 23
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  • Question 1
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    The three stable isotopes of neon: \({ }^{20} \mathrm{Ne}_{10},{ }^{21} \mathrm{Ne}_{10}\) and \({ }^{22} \mathrm{Ne}_{10}\) have respective abundances of \(90.51 \%, 0.27 \%\) and \(9.22 \%\). The atomic masses of the three isotopes are \(19.99 \mathrm{~u}, 20.99 \mathrm{~u}\) and \(21.99 \mathrm{~u}\), respectively. Obtain the average atomic mass of neon.

    Solution

    Given,

    Atomic mass of \({ }^{20} \mathrm{Ne}_{10}, \mathrm{~m}_{1}=19.99 \mathrm{~u}\)

    Abundance of \({ }^{20} \mathrm{Ne}_{10}, \eta_{1}=90.51 \%\)

    Atomic mass of \({ }^{21} \mathrm{Ne}_{10}, \mathrm{~m}_{2}=20.99 \mathrm{~u}\)

    Abundance of \({ }^{21} \mathrm{Ne}_{10}, \eta_{2}=0.27 \%\)

    Atomic mass of \({ }^{22} \mathrm{Ne}_{10}, \mathrm{~m}_{3}=21.99 \mathrm{~u}\)

    Abundance of \({ }^{22} \mathrm{Ne}_{10}, \eta_{3}=9.22 \%\)

    The average atomic mass of neon is given as:

    \(m=\frac{m_{1} \eta_{1}+m_{2} \eta_{2}+m_{3} \eta_{3}}{\eta_{1}+\eta_{2}+\eta_{3}}\)

    \(=\frac{19.99 \times 90.51+20.99 \times 0.27+21.99 \times 9.22}{90.51+0.27+9.22}\)

    \(=20.1771 \mathrm{~u}\)

     

  • Question 2
    1 / -0

    The temperature determines the direction of net change of:

    Solution

    The temperature determines the direction of net change of intermolecular kinetic energy.

    On heating, the temperature rises, particles gain energy. As the kinetic energy increases, intermolecular space increases as they get separated from each other and the force of attraction decreases as the particles go far away from each other.

  • Question 3
    1 / -0

    Displacement of a particle executing simple harmonic motion is represented by \(\mathrm{Y}=\) \(0.08 \sin \left(3 \pi \mathrm{t}+\frac{\pi}{4}\right)\) metre. Then calculate:

    (a) Time period.

    (b) Initial phase

    (c) Displacement from mean position at \(\mathrm{t}=\frac{7}{36}\) sec.

    Solution

    Given:

    Displacement equation is given as \(\mathrm{Y}=0.08 \sin \left(3 \pi \mathrm{t}+\frac{\pi}{4}\right)\)

    On comparing with \(\mathrm{Y}=\mathrm{A} \sin (\mathrm{\omega t}+\pi)\)

    We get, \(\mathrm{\omega}=3 \pi\) and \(\phi=\frac{\pi}{4}\)

    Time period \(\mathrm{T}=\frac{2 \pi}{\mathrm{\omega}}\)

    \(=\frac{2 \pi}{3 \pi}\)

    \(=\frac{2}{3} \mathrm{~s}\)

    Initial phase \(\phi=\frac{\pi}{4}\)

    \(\text { At } \mathrm{t}=\frac{7}{36} \mathrm{~s} \)

    \( \mathrm{Y}=0.08 \sin \left(3 \pi \times \frac{7}{36}+\frac{\pi}{4}\right)\)

    \(=0.08 \sin (\frac{5 \pi }{ 6}) \)

    \(\Rightarrow \mathrm{Y}=0.08 \times 0.5\)

    \(=0.04 \mathrm{~m}\)

  • Question 4
    1 / -0

    A non monochromatic light is used in an experiment on photoelectric effect. The stopping potential: 

    Solution

    For photoelectric effect to be observed, wavelength of the incident light \((\lambda)\) should be less than the threshold wavelength \(\left(\lambda_{0}\right)\) of the metal.

    Einstein's photoelectric equation:

    \(\mathrm{eV}_{0}=\frac{\mathrm{hc}}{\lambda}-\phi_{0}\)

    Here, \(V_{0}=\) stopping potential, \(\lambda_{0}=\) threshold wavelength,

    \(h\) = Planck"s constant, \(\phi_{0}=\) work-function of metal.

    So, the stopping potential is related to the shortest wavelength.

  • Question 5
    1 / -0

    Two stable isotopes of lithium \(^6 Li_3\) and \(^7 Li_3\) have respective abundances of \(7.5 \%\) and \(92.5 \%\). These isotopes have masses \(6.01512 \mathrm{~u}\) and \(7.01600 \mathrm{u}\), respectively. Find the atomic mass of lithium.

    Solution

    Given,

    Mass of \({ }^{6} \mathrm{Li}_{3}\), lithium isotope, \(\mathrm{m} _{1}=6.01512 \mathrm{u}\)

    Mass of \({ }^{7} \mathrm{Li}_{3}\), lithium isotope, \(\mathrm{m_2}=7.01600 \mathrm{u}\)

    Abundance of \({ }^{6} \mathrm{Li}_{3}, \eta_{1}=7.5 \%\)

    Abundance of \({ }^{7} \mathrm{Li}_{3}, \eta_{2}=92.5 \%\)

    The atomic mass of lithium atom is given as:

    \(m=\frac{m_{1} \eta_{1}+m_{2} \eta_{2}}{\eta_{1}+\eta_{2}}\)

    \(=\frac{6.01512 \times 7.5+7.01600 \times 92.5}{92.5+7.5}\)

    \(=6.940934 \mathrm{u}\)

  • Question 6
    1 / -0

    The farther away a planet is from the Sun:

    Solution

    According to Kepler's second law of planetary motion, the planets move faster near the Sun and move slowly away from the Sun to cover equal areas in equal intervals of time.

    Therefore, as the distance of the planet increases from the Sun, it will orbit the Sun slower and hence, takes a longer time.

    Hence, the farther away a planet is from the Sun, the longer it takes to orbit the Sun once.

  • Question 7
    1 / -0

    Light rays from an object fall on a surface and get reflected in a completely diffused manner. What can you say about the nature of image of the object?

    Solution

    An image is a copy of an object that is formed by reflected (or refracted) light. Regular reflection occurs when light reflects off a very smooth surface and forms a clear image.

    Diffuse reflection occurs when light reflects off a rough surface and forms a blurry image or no image at all.

    ​So, Light rays from an object fall on a surface and get reflected in a completely diffused manner; No image will be formed.

  • Question 8
    1 / -0

    Which of the following pairs has the same dimensions?

    Solution

    Impulse is defined as the change in momentum.

    Impulse I \(=\Delta \mathrm{p}=\mathrm{mv}-\mathrm{mu}\)

    So, both Impulse and momentum have the same units/dimensions.

  • Question 9
    1 / -0

    A Carnot engine, whose efficiency is 40%, takes in heat from a source maintained at a temperature of 500K. It is desired to have an engine of efficiency 60%. Then, the intake temperature for the same exhaust (sink) temperature must be :

    Solution

    The efficiency of the carnot's heat engine is given as

    \(\eta=\left(1-\frac{T_2}{T_1}\right) \times 100\)

    When efficiency is \(40 \%\),

    \(\mathrm{T}_1=500 \mathrm{~K} ; \eta=40 \)

    \(40=\left(1-\frac{\mathrm{T}_2}{500}\right) \times 100 \)

    \(\Rightarrow \frac{40}{100}=1-\frac{\mathrm{T}_2}{500} \)

    \(\Rightarrow \frac{\mathrm{T}_2}{500}=\frac{60}{100} \Rightarrow \mathrm{T}_2=300 \mathrm{~K}\)

    When efficiency is \(60 \%\), then

    \(\frac{60}{100}=\left(1-\frac{300}{\mathrm{~T}_2}\right) \Rightarrow \frac{300}{\mathrm{~T}_2}=\frac{40}{100} \)

    \(\Rightarrow \mathrm{T}_2=\frac{100 \times 300}{40} \Rightarrow \mathrm{T}_2=750 \mathrm{~K}\)

  • Question 10
    1 / -0

    A p-n junction has acceptor impurity concentration of \(10^{17} \mathrm{~cm}^{-3}\) in the \(P\) side and donor impurity concentration of \(10^{16}\) \(\mathrm{cm}^{-3}\) in the \(N\) side. What is the contact potential at the junction?

    \((k T=\) thermal energy, intrinsic carrier concentration \(\left.n_{\mathrm{i}}=1.6 \times 10^{10} \mathrm{~cm}^{-3}\right)\)

    Solution

    Given,

    Acceptor impurity concentration, \(n_a = 10^{17}  \mathrm{~cm}^{-3}\)

    Donor impurity concentration, \(n_a = 10^{16}  \mathrm{~cm}^{-3}\)

    Intrinsic carrier concentration \(n_{\mathrm{i}}=1.6 \times 10^{10} \mathrm{~cm}^{-3}\)

    Contact potential at the junction,

    \(V=\frac{k T}{e}\) ln \((\frac{n_{a} n_{d}}{n_{i}^{2}})\)

    \(\Rightarrow V=\frac{k T}{e}\) ln \(\frac{10^{17} \times 10^{16}}{(1.6 \times 10^{10})^{2}}\)

    \(\Rightarrow V=\frac{k T}{e}\) ln \((4 \times 10^{12})\)

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