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De-Broglie wavelength of particle moving at a (1/4) th of speed of light having rest mass \(\mathrm{m}_{0}\) is \(\ldots \ldots \ldots\) (A) $\left\\{(3.87 \mathrm{~h}) /\left(\mathrm{m}_{0} \mathrm{C}\right)\right\\}$ (B) $\left\\{(4.92 \mathrm{~h}) /\left(\mathrm{m}_{0} \mathrm{C}\right)\right\\}$ (C) $\left\\{(7.57 \mathrm{~h}) /\left(\mathrm{m}_{0} \mathrm{C}\right)\right\\}$ (D) $\left\\{(9.46 \mathrm{~h}) /\left(\mathrm{m}_{\circ} \mathrm{C}\right)\right\\}$

Short Answer

Expert verified
The correct De-Broglie wavelength for the given problem is: \[\lambda \approx \frac{1.62\times 10^{-33}\mathrm{Js}}{m_0c}\]

Step by step solution

01

De-Broglie wavelength formula

The De-Broglie wavelength formula is given by: \[\lambda =\frac{h}{p}\] where \(h\) represents the Planck's constant and \(p\) represents the momentum of the particle.
02

Calculate the momentum of the particle

The momentum of the particle is given by: \[p = mv\] where \(m\) is the relativistic mass of the particle and \(v\) is the velocity. For a particle moving at a quarter of the speed of light, we have \(v = \frac{1}{4}c\), where \(c\) is the speed of light.
03

Relativistic mass

The relativistic mass \(m\) is given by the following formula: \[m = \frac{m_0}{\sqrt{1-\frac{v^2}{c^2}}}\] where \(m_0\) is the rest mass and \(v\) is the velocity. In this case, \(v = \frac{1}{4}c\), so we can substitute this into the formula to find the relativistic mass: \[m = \frac{m_0}{\sqrt{1-\frac{(\frac{1}{4}c)^2}{c^2}}}\]
04

Simplify the relativistic mass equation

Simplifying the relativistic mass equation, we get: \[m = \frac{m_0}{\sqrt{1-\frac{1}{16}}}\] \[m = \frac{m_0}{\sqrt{\frac{15}{16}}}\] \[m = \frac{4m_0}{\sqrt{15}}\]
05

Calculate the momentum

Now we can calculate the momentum using the relativistic mass and velocity (\(v = \frac{1}{4}c\)): \[p = mv = \frac{4m_0}{\sqrt{15}} \cdot \frac{1}{4}c = \frac{m_0c}{\sqrt{15}}\]
06

Calculate the De-Broglie wavelength

Now we can use the De-Broglie wavelength formula with the calculated momentum: \[\lambda = \frac{h}{p} = \frac{h}{\frac{m_0c}{\sqrt{15}}}\] \[\lambda = \frac{h\sqrt{15}}{m_0c}\] Now, we know that Planck's constant (\(h\)) is approximately 6.626 x 10^{-34} Js. Multiplying this by the square root of 15 and simplifying: \[\lambda = \frac{(6.626 \times 10^{-34} \mathrm{Js})\sqrt{15}}{m_0c}\] \[\lambda = \frac{1.6175\times10^{-33}\mathrm{Js}}{m_0c}\] Since the given options have 2 decimal places for the coefficient, we can round the value to match that level of precision: \[\lambda \approx \frac{1.62\times 10^{-33}\mathrm{Js}}{m_0c}\]
07

Compare with given options

Comparing this result with the given options, we notice that none of the options matches the correct answer. This means that there might be a mistake in the given options, or the exercise needs to be revised. However, the correct De-Broglie wavelength for the given problem is: \[\lambda \approx \frac{1.62\times 10^{-33}\mathrm{Js}}{m_0c}\]

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Most popular questions from this chapter

If \(\propto\) -particle and proton are accelerated through the same potential difference, then the ratio of de Brogile wavelength of \(\propto\) -particle and proton is \(\ldots \ldots \ldots\) (A) \((1 / \sqrt{2})\) (B) \(\sqrt{2}\) (C) \(\\{1 /(2 \sqrt{2})\\}\) (D) \(2 \sqrt{2}\)

Find the velocity at which mass of a proton becomes \(1.1\) times its rest mass, \(\mathrm{m}_{\mathrm{g}}=1.6 \times 10^{-27} \mathrm{~kg}\) Also, calculate corresponding temperature. For simplicity, consider a proton as non- interacting ideal-gas particle at \(1 \mathrm{~atm}\) pressure. $\left(1 \mathrm{eV}=1.6 \times 10^{-19} \mathrm{~J} \cdot \mathrm{h}=6.63 \times 10^{-34} \mathrm{~J} . \mathrm{s}, \mathrm{c}=3 \times 10^{8} \mathrm{~ms}^{-1}\right)$ (A) $\mathrm{V}=1.28 \times 10^{8}(\mathrm{~m} / \mathrm{s}), \mathrm{T}=7.65 \times 10^{12} \mathrm{~K}$ (B) $\mathrm{V}=12.6 \times 10^{8}(\mathrm{~m} / \mathrm{s}), \mathrm{T}=7.65 \times 10^{11} \mathrm{~K}$ (C) $\mathrm{V}=1.26 \times 10^{7}(\mathrm{~m} / \mathrm{s}), \mathrm{T}=5.76 \times 10^{11} \mathrm{~K}$ (D) $\mathrm{V}=12.6 \times 10^{7}(\mathrm{~m} / \mathrm{s}), \mathrm{T}=7.56 \times 10^{11} \mathrm{~K}$

In which of the following phenomena the photon picture is required? (A) Energy distribution in black body radiation (B) Compton scattering (C) Photoelectric effect (D) all of the above

The work function of a metal is \(1 \mathrm{eV}\). Light of wavelength $3000 \AA$ is incident on this metal surface. The maximum velocity of emitted photoelectron will be \(\ldots \ldots .\) (A) \(10 \mathrm{~ms}^{-1}\) (B) \(10^{3} \mathrm{~ms}^{-1}\) (C) \(10^{4} \mathrm{~ms}^{-1}\) (D) \(10^{6} \mathrm{~ms}^{-1}\)

de-Broglie wavelength of atom at T \(\mathrm{K}\) absolute temperature will be \(\ldots \ldots \ldots\) (A) \([\mathrm{h} /\\{\mathrm{mkT}\\}]\) (B) \([\mathrm{h} /\\{\sqrt{3} \mathrm{mKT}\\}]\) (C) \([\\{\sqrt{2} \mathrm{mKT}\\} / \mathrm{h}]\) (D) \(\sqrt{(2 \mathrm{mKT})}\)

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