Molybdenum metal must absorb radiation with an energy higher than $7.22 \times 10^{-19} \mathrm{~J}$ ( "energy threshold") before it can eject an electron from its surface via the photoelectric effect. (a) What is the frequency threshold for emission of electrons? (b) What wavelength of radiation will provide a photon of this energy? (c) If molybdenum is irradiated with light of wavelength of \(240 \mathrm{nm}\), what is the maximum possible velocity of the emitted electrons?

Short Answer

Expert verified
The frequency threshold for emission of electrons is \(1.09 \times 10^{15} \mathrm{Hz}\). The wavelength of radiation that provides a photon of this energy is \(275 \mathrm{nm}\). The maximum possible velocity of the emitted electrons when molybdenum is irradiated with light of wavelength \(240 \mathrm{nm}\) is \(4.38 \times 10^5 \mathrm{m/s}\).

Step by step solution

01

a) Frequency threshold for emission of electrons#

Using the energy of a photon equation, we can solve for the frequency threshold: \(E_{threshold} = h\nu_{threshold}\) Solving for \(\nu_{threshold}\): \(\nu_{threshold} = \frac{E_{threshold}}{h}\) Given \(E_{threshold} = 7.22 \times 10^{-19} J\) and \(h = 6.63 \times 10^{-34} Js\), we can calculate the frequency threshold: \(\nu_{threshold} = \frac{7.22 \times 10^{-19}}{6.63 \times 10^{-34}} = 1.09 \times 10^{15} \mathrm{Hz}\) The frequency threshold for emission of electrons is \(1.09 \times 10^{15} \mathrm{Hz}\).
02

b) Wavelength of radiation for the given photon energy#

Using the wavelength and frequency relationship, we can solve for the wavelength of radiation that provides the given photon energy: \(c = \lambda\nu\) Solving for \(\lambda\): \(\lambda = \frac{c}{\nu}\) Given \(c = 3 \times 10^8 \mathrm{m/s}\) and \(\nu_{threshold} = 1.09 \times 10^{15} \mathrm{Hz}\), we can calculate the wavelength of radiation: \(\lambda = \frac{3 \times 10^8}{1.09 \times 10^{15}} = 2.75 \times 10^{-7} \mathrm{m} = 275 \mathrm{nm}\) The wavelength of radiation that provides a photon of this energy is \(275 \mathrm{nm}\).
03

c) Maximum possible velocity of emitted electrons#

Given the wavelength of irradiated light, we can first calculate the energy of a photon at \(240 \mathrm{nm} \): \(E_{photon} = h\nu = \frac{hc}{\lambda}\) Using \(h = 6.63 \times 10^{-34} Js\), \(c = 3 \times 10^8 \mathrm{m/s}\) and \(\lambda = 240 \times 10^{-9} \mathrm{m}\), we can determine the energy of a photon: \(E_{photon} = \frac{(6.63 \times 10^{-34})(3 \times 10^8)}{240 \times 10^{-9}} = 8.29 \times 10^{-19} J\) Now we can calculate the kinetic energy of emitted electrons: \(KE_{max} = E_{photon} - E_{threshold}\) Using \(E_{photon} = 8.29 \times 10^{-19} J\) and \(E_{threshold} = 7.22 \times 10^{-19} J\): \(KE_{max} = 8.29 \times 10^{-19} - 7.22 \times 10^{-19} = 1.07 \times 10^{-19} J\) Finally, we can find the maximum possible velocity of emitted electrons using the kinetic energy equation: \(KE_{max} = \frac{1}{2}mv^2\) Solving for \(v_{max}\): \(v_{max} = \sqrt{\frac{2KE_{max}}{m}}\) Assuming the mass of an electron is \(m = 9.11 \times 10^{-31} \mathrm{kg}\): \(v_{max} = \sqrt{\frac{2(1.07 \times 10^{-19})}{9.11 \times 10^{-31}}} = 4.38 \times 10^5 \mathrm{m/s}\) The maximum possible velocity of the emitted electrons is \(4.38 \times 10^5 \mathrm{m/s}\).

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

As discussed in the A Closer Look box on "Measurement and the Uncertainty Principle," the essence of the uncertainty principle is that we can't make a measurement without disturbing the system that we are measuring. (a) Why can't we measure the position of a subatomic particle without disturbing it? (b) How is this concept related to the paradox discussed in the Closer Look box on "Thought Experiments and Schrödinger's Cat"?

The rays of the Sun that cause tanning and burning are in the ultraviolet portion of the electromagnetic spectrum. These rays are categorized by wavelength. So-called UV-A radiation has wavelengths in the range of $320-380 \mathrm{nm},\( whereas UV-B radiation has wavelengths in the range of \)290-320 \mathrm{nm}$. (a) Calculate the frequency of light that has a wavelength of \(380 \mathrm{nm} .\) (b) Calculate the energy of a mole of \(380-\mathrm{nm}\) photons. (c) Which are more energetic, photons of UV-A radiation or photons of UV-B radiation? (d) The UV-B radiation from the Sun is considered a more important cause of sunburn in humans than UV-A radiation. Is this observation consistent with your answer to part (c)?

Give the values for \(n, l,\) and \(m_{l}\) for \((\mathbf{a})\) each orbital in the \(3 p\) subshell, (b) each orbital in the \(4 f\) subshell.

Determine whether each of the following sets of quantum numbers for the hydrogen atom are valid. If a set is not valid, indicate which of the quantum numbers has a value that is not valid: (a) \(n=3, l=3, m_{l}=2, m_{5}=+\frac{1}{2}\) (b) \(n=4, l=3, m_{l}=-3, m_{\mathrm{s}}=+\frac{1}{2}\) (c) \(n=3, l=1, m_{l}=2, m_{s}=+\frac{1}{2}\) (d) \(n=5, l=0, m_{l}=0, m_{\mathrm{s}}=0\) (e) \(n=2, l=1, m_{l}=1, m_{s}=-\frac{1}{2}\)

The wavenumber \(\bar{\lambda}\) is the number of waves that exist over a specified distance, very often \(1 \mathrm{~cm}\). The wavenumber can easily be calculated by taking the reciprocal of the wavelength. Give typical wavenumbers for (a) X-rays \((\lambda=1 \mathrm{nm})\) (b) visible light \((\lambda=500 \mathrm{nm})\) (c) microwaves $(\lambda=1 \mathrm{~mm})$.

See all solutions

Recommended explanations on Chemistry Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free