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Dual Nature of Radiation question

2012 · Shift 1 · Q58
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Dual Nature of Radiation question

2012 · Shift 1 · Q58

JEE AdvancedPhysicsDual Nature of RadiationNumerical+4 / −1
A proton is fired from very far away towards a nucleus with charge Q = 120e, where e is the electronic charge. It makes a closest approach of 10 fm to the nucleus. The de Broglie wavelength (in units of fm) of the proton at its start is ‾\underline{\hspace{2cm}}​. (Take the proton mass, mp=(5×3)×10−27{m_p} = (5 \times 3) \times {10^{ - 27}}mp​=(5×3)×10−27 kg; h/e=4.2×10−15h/e = 4.2 \times {10^{ - 15}}h/e=4.2×10−15 J.s/C; 14πε0=9×109{1 \over {4\pi {\varepsilon _0}}} = 9 \times {10^9}4πε0​1​=9×109 m/F; 1 fm = 1015 m.)
Numerical answer
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Correct answer: 7

Step-by-step Derivation

  1. Analyze the Physical Scenario and Apply Conservation of Energy

    A proton with charge e is fired from a very large distance towards a nucleus with charge Q = 120e. Initially, the proton has kinetic energy KiK_iKi​ and its potential energy UiU_iUi​ is negligible, so Ui≈0U_i ≈ 0Ui​≈0. The total initial energy is Ei=KiE_i = K_iEi​=Ki​.

    The proton travels towards the nucleus and its kinetic energy is converted into electrostatic potential energy due to repulsion. At the point of closest approach, rminr_minrm​in, the proton momentarily stops before being repelled. At this point, its kinetic energy Kf=0K_f = 0Kf​=0. The potential energy UfU_fUf​ is given by Coulomb's law: Uf=14πε0(e)(Q)rmin=k(e)(120e)rmin=120ke2rminU_f = \frac{1}{4\pi \varepsilon_0} \frac{(e)(Q)}{r_{min}} = \frac{k(e)(120e)}{r_{min}} = \frac{120 k e^2}{r_{min}}Uf​=4πε0​1​rmin​(e)(Q)​=rmin​k(e)(120e)​=rmin​120ke2​

    According to the principle of conservation of energy, the total initial energy equals the total final energy: Ei=EfE_i = E_fEi​=Ef​ Ki=Uf=120ke2rminK_i = U_f = \frac{120 k e^2}{r_{min}}Ki​=Uf​=rmin​120ke2​

  2. Relate Kinetic Energy to de Broglie Wavelength

    The de Broglie wavelength λ of a particle is related to its momentum p by the equation λ = h/p. The kinetic energy K is related to momentum p and mass mpm_pmp​ by K=p2/(2mp)K = p^2 / (2m_p)K=p2/(2mp​). Therefore, p=2mpKp = \sqrt{2m_p K}p=2mp​K​.

    Substituting this into the de Broglie wavelength formula, we get the initial wavelength λ of the proton: λ=h2mpKi\lambda = \frac{h}{\sqrt{2m_p K_i}}λ=2mp​Ki​​h​

  3. Combine Formulas and Solve for Wavelength

    Substitute the expression for KiK_iKi​ from Step 1 into the wavelength equation: λ=h2mp(120ke2rmin)=h240mpke2rmin\lambda = \frac{h}{\sqrt{2m_p \left( \frac{120 k e^2}{r_{min}} \right)}} = \frac{h}{\sqrt{\frac{240 m_p k e^2}{r_{min}}}}λ=2mp​(rmin​120ke2​)​h​=rmin​240mp​ke2​​h​

    To make use of the given constant h/e, we can rearrange the expression: λ=h/e240mpkrmin\lambda = \frac{h/e}{\sqrt{\frac{240 m_p k}{r_{min}}}}λ=rmin​240mp​k​​h/e​

  4. Address the Proton Mass Value and Perform Calculations

    The problem states the proton mass as mp=(5×3)×10−27m_p = (5 × 3) × 10^{−27}mp​=(5×3)×10−27 kg, which is 15×10−2715 × 10^{−27}15×10−27 kg. This value is nearly 9 times the actual proton mass and leads to a non-integer answer, which is unlikely for an integer-type question. It is highly probable that this is a typo and the intended value was mp=(5/3)×10−27m_p = (5/3) × 10^{−27}mp​=(5/3)×10−27 kg, which is a common approximation for the proton mass (1.67×10−271.67 × 10^{−27}1.67×10−27 kg). Using this corrected value leads to a clean integer answer.

    Let's proceed with the calculation using mp=(5/3)×10−27m_p = (5/3) × 10^{−27}mp​=(5/3)×10−27 kg.

    Given values:

    • rmin=10r_{min} = 10rmin​=10 fm =10×10−15= 10 × 10^{−15}=10×10−15 m
    • mp=(5/3)×10−27m_p = (5/3) × 10^{−27}mp​=(5/3)×10−27 kg
    • h/e=4.2×10−15h/e = 4.2 × 10^{−15}h/e=4.2×10−15 J.s/C
    • k=1/(4πε0)=9×109k = 1 / (4πε_0) = 9 × 10^9k=1/(4πε0​)=9×109 N m²/C²

    First, calculate the term under the square root: 240mpkrmin=240×(53×10−27)×(9×109)10×10−15\frac{240 m_p k}{r_{min}} = \frac{240 \times (\frac{5}{3} \times 10^{-27}) \times (9 \times 10^9)}{10 \times 10^{-15}}rmin​240mp​k​=10×10−15240×(35​×10−27)×(9×109)​ =240×5×93×10×10−27+9+15=(80×5×3)×10−3=1200×10−3=1.2= \frac{240 \times 5 \times 9}{3 \times 10} \times 10^{-27+9+15} = (80 \times 5 \times 3) \times 10^{-3} = 1200 \times 10^{-3} = 1.2=3×10240×5×9​×10−27+9+15=(80×5×3)×10−3=1200×10−3=1.2 Let me re-calculate that part: =240×5×93×10×10−3=(80×5×3/10)imes10−3=(24×5×3)×10−3=360×10−3=0.36= \frac{240 \times 5 \times 9}{3 \times 10} \times 10^{-3} = (80 \times 5 \times 3 / 10) imes 10^{-3} = (24 \times 5 \times 3) \times 10^{-3} = 360 \times 10^{-3} = 0.36=3×10240×5×9​×10−3=(80×5×3/10)imes10−3=(24×5×3)×10−3=360×10−3=0.36

    Now, take the square root of this value: 0.36=0.6\sqrt{0.36} = 0.60.36​=0.6

    Finally, calculate the de Broglie wavelength λ: λ=h/e240mpkrmin=4.2×10−150.6\lambda = \frac{h/e}{\sqrt{\frac{240 m_p k}{r_{min}}}} = \frac{4.2 \times 10^{-15}}{0.6}λ=rmin​240mp​k​​h/e​=0.64.2×10−15​ λ=7×10−15 m\lambda = 7 \times 10^{-15} \text{ m}λ=7×10−15 m

  5. State the Final Answer in Required Units

    The question asks for the answer in units of femtometers (fm). Since 1fm=10−151 fm = 10^{−15}1fm=10−15 m: λ=7 fm\lambda = 7 \text{ fm}λ=7 fm

    The integer value is 7.

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