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An electron is accelerated through an electric potential to a kinetic energy of \(2.15 \times 10^{-15} \mathrm{J}\) . What is its characteristic wavelength? [Hint: Recall that the kinetic energy of a moving object is \(E=\frac{1}{2} m v^{2},\) where \(m\) is the mass of the object and \(\nu\) is the speed of the object.

Short Answer

Expert verified
The characteristic wavelength of the electron is approximately \(3.34 \times 10^{-10}\) meters.

Step by step solution

01

We are given the kinetic energy of the electron: \(E = 2.15 \times 10^{-15} J\). Using the formula for kinetic energy, \(E = \frac{1}{2}mv^2\), we can solve for the speed of the electron (v). Rearrange the formula to isolate v: \(v^2 = \frac{2E}{m}\) Note that the mass of an electron is approximately \(9.11 \times 10^{-31} kg\). Now, we substitute the given values and find the square root to find the speed of the electron: \begin{aligned} v &= \sqrt{\frac{2(2.15 \times 10^{-15})}{9.11 \times 10^{-31}}} \\ v &= \sqrt{4.72 \times 10^{14}} \\ v &= 2.17 \times 10^7 m/s \end{aligned} #Step 2: Find the characteristic wavelength#

Now that we have the speed of the electron, we can use the de Broglie wavelength formula \(\lambda = \frac{h}{mv}\) to find the characteristic wavelength. The Planck constant (h) has a value of \(6.63 \times 10^{-34} Js\). Plug in the values of mass, speed, and the Planck constant: \(\lambda = \frac{6.63 \times 10^{-34}}{(9.11 \times 10^{-31})(2.17 \times 10^7)}\) Calculate the wavelength: \(\lambda = 3.34 \times 10^{-10} m\) The characteristic wavelength of the electron is approximately \(3.34 \times 10^{-10}\) meters.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Kinetic Energy
Kinetic energy is the energy that an object possesses due to its motion. It's a fundamental concept in physics that helps us understand how objects move and interact. You can calculate kinetic energy using the formula \(E = \frac{1}{2}mv^2\), where \(E\) is the kinetic energy, \(m\) is the mass of the object, and \(v\) is its velocity.
For an electron, knowing its kinetic energy is crucial to determine other properties like its speed. By rearranging the formula, you can solve for the velocity by finding that \(v = \sqrt{\frac{2E}{m}}\).
This approach makes it possible to calculate other physical characteristics, such as the de Broglie wavelength, which is essential in understanding quantum behavior.
Electron Mass
The mass of an electron is a fundamental constant in physics. It's very tiny—about \(9.11 \times 10^{-31} \text{ kg}\). Given its small size, the mass of an electron is significant in calculations involving atomic and subatomic particles.
Using accurate values for the electron mass is crucial in equations like kinetic energy and de Broglie wavelength. These calculations allow us to predict and explain the behavior of electrons in different contexts.
For example, when determining the speed or wavelength of an electron accelerated by a known energy, precise knowledge of its mass is required to obtain correct results. Such calculations underpin key discoveries and applications in quantum mechanics.
Planck Constant
The Planck constant \(h\) is a crucial part of quantum mechanics. It connects the energy of a photon to its frequency via the equation \(E = hf\), where \(f\) is the frequency of the photon.
In the context of de Broglie wavelength, the Planck constant helps relate particle-like and wave-like properties of subatomic particles through \(\lambda = \frac{h}{mv}\). Here, \(\lambda\) is the wavelength, \(m\) is mass, and \(v\) is velocity.
The constant \(h\) is a tiny value, approximately \(6.63 \times 10^{-34} \text{ Js}\). Its smallness corresponds to the equally minuscule scales at which quantum effects become significant, allowing us to explore and understand phenomena that are inaccessible at larger scales.
The Planck constant thus serves as a bridge between the classical and quantum worlds, playing an essential role in calculations of energy and motion at the microscopic level.

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Most popular questions from this chapter

A certain orbital of the hydrogen atom has \(n=4\) and \(l=2 .\) (a) What are the possible values of \(m_{l}\) for this orbital? (b) What are the possible values of \(m_{s}\) for the orbital?

How many unique combinations of the quantum numbers \(l\) and \(m_{l}\) are there when (a) \(n=3,\) (b) \(n=4 ?\)

One type of sunburn occurs on exposure to UV light of wavelength in the vicinity of 325 \(\mathrm{nm} .\) (a) What is the energy of a photon of this wavelength? (b) What is the energy of a mole of these photons? (c) How many photons are in a 1.00 \(\mathrm{mJ}\) burst of this radiation? (d) These UV photons can break chemical bonds in your skin to cause sunburn-a form of radiation damage. If the 325 -nm radiation provides exactly the energy to break an average chemical bond in the skin, estimate the average energy of these bonds in kJ/mol.

(a) A green laser pointer emits light with a wavelength of 532 nm. What is the frequency of this light? (b) What is the energy of one of these photons? (c) The laser pointer emits light because electrons in the material are excited (by a battery) from their ground state to an upper excited state. When the electrons return to the ground state, they lose the excess energy in the form of 532 -nm photons. What is the energy gap between the ground state and excited state in the laser material?

Identify the specific element that corresponds to each of the following electron configurations and indicate the number of unpaired electrons for each: (a) \(1 s^{2} 2 s^{2},(\mathbf{b}) 1 s^{2} 2 s^{2} 2 p^{4}\) (c) \([\operatorname{Ar}] 4 s^{1} 3 d^{5},(\mathbf{d})[\mathrm{Kr}] 5 s^{2} 4 d^{10} 5 p^{4}\)

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