At the beginning of the scientific era, scientists described the world using classical mechanics. The energy of the particles at the macroscopic or microscopic level was assumed to be able to take any value. After discovering quantum mechanics, a new understanding of energy came about across the world. According to quantum mechanics, the energy of the particles at the macroscopic or microscopic level exists at discrete levels instead of taking a continuum of values. But, of course, the difference between the discrete values is so small at the macroscopic level that energy seems to be a continuum. Also, we cannot see the discrete behavior of microscopic phenomena. So, then, how do scientists become so sure about quantum mechanics?
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Jetzt kostenlos anmeldenAt the beginning of the scientific era, scientists described the world using classical mechanics. The energy of the particles at the macroscopic or microscopic level was assumed to be able to take any value. After discovering quantum mechanics, a new understanding of energy came about across the world. According to quantum mechanics, the energy of the particles at the macroscopic or microscopic level exists at discrete levels instead of taking a continuum of values. But, of course, the difference between the discrete values is so small at the macroscopic level that energy seems to be a continuum. Also, we cannot see the discrete behavior of microscopic phenomena. So, then, how do scientists become so sure about quantum mechanics?
The solar cells we use these days to get electricity from sun rays is one of the most significant modern applications of quantum mechanics in terms of its effects and implications for broader society. The photoelectric effect, black body radiation, double slit experiment, and Bohr atomic model are famous phenomena explained with quantum mechanics. Without quantum mechanics, macroscopic observations are easy to predict, but the microscopic world becomes mysterious. You might be wondering, if the energy was seen almost as continuous at the macroscopic level, how did scientists discover energy quantization? The answer to this question is explored in this article!
First, let's define what exactly is energy quantization!
The phenomenon in which the amount of energy emitted or absorbed by a body is an integral multiple of a constant amount is called energy quantization.
These discrete energy packets are known as quanta. To explain the photoelectric effect, the energy absorbed by the metal surface from the incident ray is modeled as consisting of quanta. The photoelectric effect is therefore a demonstration of the quantization of energy.
Planck defines energy quantization in terms of the quantization of electromagnetic waves.
Quantum mechanics describes electromagnetic waves as a collection of small energy packets known as photons. The energy of each of these photons in terms of the frequency of the wave is \[E=h\nu,\]
where \(h=6.626\times 10^{-34}\,\mathrm{J\,s}\,\left(\mathrm{joule\,second}\right)\) is Planck's constant, and \(\nu\) is the frequency of the wave.
This equation shows that the energy of each photon increases with an increase in the wave's frequency!
The frequency of visible lights varies as \[\nu_{\mathrm{violet}} > \nu_{\mathrm{indigo}} > \nu_{\mathrm{blue}} > \nu_{\mathrm{green}} > \nu_{\mathrm{yellow}} > \nu_{\mathrm{orange}} > \nu_{\mathrm{red}}.\] From the relation between the energy of each quantum of wave in terms of the frequency, the energy varies as \[E_{\mathrm{violet}} > E_{\mathrm{indigo}} > E_{\mathrm{blue}} > E_{\mathrm{green}}>E_{\mathrm{yellow}}>E_{\mathrm{orange}}>E_{\mathrm{red}}.\]
The speed of an electromagnetic wave in a vacuum is \(c=3\times10^{8}\,\mathrm{m\,s^{-1}}\). The relation between the speed \(\left(c\right)\), wavelength \(\left(\lambda\right)\), and frequency \(\left(\nu\right)\) of the ray is
\[c=\nu\lambda.\]
Using this relation, the energy of each quantum in terms of the wavelength is
\[E=h\frac{c}{\lambda}.\]
The above equation describes the energy of each photon, but electromagnetic waves consist of many photons. The amount of energy emitted or absorbed by the body due to the incidence of electromagnetic waves on the body is,
\[E=nh\nu,\]
where \(n\) is the number of the incident photons (integers) i.e. \(n=\pm1,\pm2,\pm3,...\)
In other words, the amount of energy absorbed or emitted will be in the form of \(E=\pm h\nu,\pm1h\nu,\pm2h\nu,...\) instead of in the form of \(E=\pm1.1h\nu,\pm1.2h\nu,\pm1.3h\nu,...\) or any other real number multiple of \(h\nu\).
Some examples of energy quantization are the vibrations on the harp (only specific musical notes are possible), speed boat waves (waves formed are discrete instead of in a continuum), etc.
The cause of energy quantization is the wave nature of the matter. With the dual nature of matter by De Broglie, Bohr explained the electron revolution around the nucleus in the form of its wave nature. Bohr postulated that the electrons only revolve in the orbit where their waves interfere constructively.
The Bohr model is the structural atomic model in which the electrons revolve around the nucleus in distinct circular orbits(or shells).
Before explaining the quantization of energy with the Bohr model, we need to know about the postulates of the Bohr model of atoms.
In the Figure above, let \(n_\mathrm{i}\) and \(n_\mathrm{f}\) be an initial and a final energy orbit of the electron. Then the energy of the electromagnetic wave emitted is \(\Delta E=\left(n_{\mathrm{f}}-n_{\mathrm{i}}\right)h\nu\). Substituting the known values of the quantum number \(n_\mathrm{f}\) and \(n_\mathrm{i}\) in the equation, gives\[\begin{align*}\Delta E&=\left(3-2\right)h\nu \\&=h\nu.\end{align*}\]
This shows that the amount of energy emitted from the atom is quantized. Thus, the Bohr model proves energy quantization.
An important modern example of energy quantization is the solar cell based on a well-known phenomenon, i.e. the photoelectric effect. So, let's start with the photoelectric effect.
After five years of the discovery of energy quantization by Planck, Albert Einstein explained the mysterious interaction of light and matter called the photoelectric phenomena discovered by Heinrich Rudolf Hertz. According to Albert Einstein, an incident ray of light on a metal surface behaves like a collection of small energy packets called photons. The energy of each photon is equivalent to the energy of each quantum, i.e., \(E=h\nu\), where \(\nu\) is the frequency of the incident ray.
Einstein postulated that each electron is bound to the metal with a characteristic energy associated with this binding called the work function \(\left(E_\circ=h\nu_\circ\right)\). Therefore, to remove the electron from the surface of the metal, the frequency of the incident ray must be equal to or greater than the threshold frequency \(\left(\nu_\circ\right)\). The maximum kinetic energy of the emitted electron in terms of the frequency of the incident ray is
\[E_\mathrm{max}=h\nu-h\nu_\circ.\]
These emitted electrons are known as photoelectrons.
So, how is this phenomenon used in solar cells? First, let's think about what we can do with the emitted electron from the metal surface. If we provide a potential difference in the setup such that all the emitted electrons start moving from one point to another, this can generate an electric current. Well, scientists use a similar process in solar cells to generate electricity from solar rays.
Energy quantization explains many phenomena that classical mechanics cannot explain. Some of these examples are listed below.
Bohr explained the discrete lines in the spectrum of a hydrogen atom as being caused by the transition of electrons between fixed energy orbits due to energy quantization. The energy emitted by electrons in the hydrogen atom is quantized. Thus, the spectrum of hydrogen consists of discrete lines instead of a continuum.
Energy quantization explains the photoelectric phenomenon, which cannot be explained by classical physics. Also, it helps in determining the maximum kinetic energy of the emitted electrons from the surface of the metal.
Energy quantization provides evidence for wave-particle duality; like the incident ray as a collection of photons or the wave nature of electrons revolving around the nucleus.
In conclusion, energy quantization throws light on several physical phenomena which couldn't be previously explained using classic physics theories.
The phenomenon in which the amount of energy emitted or absorbed by a body is an integral multiple of a constant amount is called energy quantization.
An example of energy quantization is in the discrete energy levels that electrons can occupy in the orbitals of atoms. These discrete energy levels give rise to discrete emission and absorption spectra with narrow defined bands corresponding to each possible transition between energy levels.
Energy quantization is a consequence of the theory of quantum mechanics. Ultimately this phenomenon can be traced back to solutions of the Schrodinger equation.
Energy quantization is important because it explains the spectrum of the hydrogen atom amongst a whole host of other fundamental physical phenomena.
The amount of energy emitted or absorbed by the body due to the incidence of electromagnetic waves on the body is E=nhν, where n is the number of the photons incident (an integer value). This discrete value of energy demonstrates energy quantization.
The energy of a photon is directly proportional to its _____.
frequency.
The energy of the photon is inversely proportional to ____.
wavelength.
The quantization of energy explains the photoelectric effect.
True.
The quantization of energy is can be used to explain which physical phenomena?
Blackbody radiation.
What is the energy of the photon of electromagnetic wave with wavelength \(3\,\mathrm{m}\) incident on the metal surface?
\(6.626\times10^{-26}\,\mathrm{J}\)
What is the energy of the photon of electromagnetic wave with the frequency of \(10^{25}\,\mathrm{s^{-1}}\) incident on the metal surface?
\(6.626\times10^{-9}\,\mathrm{J}\)
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