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Photoelectron spectroscopy

Key points

  • Photoelectron spectroscopy (PES) is an experimental technique used to determine the relative energies of electrons in atoms and molecules.
  • Photoelectron spectrometers work by ionizing samples using high-energy radiation (such as UV or x-rays) and then measuring the kinetic energies (KE) of the ejected electrons.
  • Given the energy of the incident radiation (hν) and the KE of the photoelectrons, the binding energy (BE) of each ejected electron can be calculated using the following equation: BE=hνKEelectron
  • A PES spectrum is a graph of photoelectron count vs. binding energy.
  • The peaks in a PES spectrum correspond to electrons in different subshells of an atom. The peaks with the lowest binding energies correspond to valence electrons, while the peaks with higher binding energies correspond to core electrons.

Introduction: What is photoelectron spectroscopy?

Photoelectron spectroscopy (PES) is an experimental technique that measures the relative energies of electrons in atoms and molecules. Scientists often use PES to study the elemental composition of materials or to characterize bonding in molecules. In this article, however, we’re going to use PES to deepen our understanding of atomic structure: by looking at PES data for pure samples of elements, we’ll see how photoelectron spectroscopy provides direct support for the concepts of electron shells and subshells, electron configurations, and more.

The basics of photoelectron spectroscopy

Photoelectron spectroscopy is based on the photoelectric effect, a physical phenomenon first characterized by Albert Einstein in 1905. The photoelectric effect is as follows: when electrons in a metal are exposed to light of sufficient radiation, the electrons are ejected from the metal surface. If we know the kinetic energy of the ejected electrons (known as photoelectrons) and the energy of the incident radiation, we can calculate the energy of the electrons in the solid metal. (For more details, check out this article on the photoelectric effect.)
Photoelectron spectroscopy simply applies the photoelectric effect to free atoms or molecules instead of metals. In PES, a sample is bombarded with high-energy radiation, usually UV or X-ray, which causes electrons to be ejected from the sample. The ejected electrons travel from the sample to an energy analyzer, where their kinetic energies are recorded, and then to a detector, which counts the number of photoelectrons at various kinetic energies. A simplified diagram of this process is shown below.
A photoelectron spectrometer.
A diagram of a photoelectron spectrometer. UV or X-ray radiation is used to ionize a sample, and the kinetic energies of the ejected electrons are recorded by the energy analyzer. Image credit: "ARPESgeneral" by Saiht on Wikimedia Commons, CCO 1.0.
The energy required to eject an electron from the sample is known as the electron’s ionization energy or binding energy. We know the energy of the radiation (hν) used to eject the electron. So, by measuring the kinetic energy of the photoelectron (KEelectron), we can calculate the binding energy (BE) of the electron in the sample:
BE=hνKEelectron
The binding energy of an electron in an atom depends on its location around the nucleus. Electrons in the outermost shell (valence electrons) are more shielded and farther from the nucleus on average, so they have the lowest binding energies of all of the electrons in an atom. In contrast, electrons in inner shells (core electrons) are less shielded and closer to the nucleus on average, so they have higher binding energies. As we’ll see in the next section, understanding the relationship between an electron's binding energy and its location is essential for the interpretation of PES data.

Analyzing PES spectra

Data from PES experiments is obtained as plots of photoelectron count vs. binding energy, with binding energy usually expressed in units of electron volts (eV) or megajoules (MJ) per mole. To help with data interpretation, PES data for elements is often plotted so that binding energy decreases as you move right along the horizontal axis, allowing us to think of the origin as representing the nucleus of the atom.
A typical PES spectrum features peaks at different binding energies. Because electrons in a particular subshell of an atom have the same binding energy, each of these peaks corresponds to electrons in a different subshell. The binding energy of a peak tells us how much energy is required to remove an electron from the subshell, and the intensity of the peak tells us the relative number of electrons in the subshell.
To illustrate, let's look at some PES data. Real PES data is messy and often difficult to interpret by non-experts, so we're going to be examining idealized spectra in which the data has been simplified so as to be more understandable.

PES spectrum of lithium

Let's start with the idealized PES spectrum for lithium, Li. For reference, the ground-state electron configuration for lithium is 1s22s1.
The idealized PES spectrum of lithium. The spectrum shows two peaks, one with a binding energy between 10 and 1 MJ/mol and another with a binding energy between 1 and 0 MJ/mol. The peak with the higher binding energy is twice as intense as the peak with the lower binding energy.
The idealized PES spectrum of lithium.
The PES spectrum shows two peaks, which represent electrons in the 2 different subshells of lithium (1s and 2s). The peak that is closer to the origin is twice as intense as the farther peak. The 1s subshell of lithium contains twice as many electrons as the 2s subshell (2 vs. 1), so the peak closer to the origin must correspond to lithium's 1s subshell.
This also makes sense in terms of binding energies: We know that the electrons in the 1s subshell of lithium are closer to the nucleus and less shielded than the electron in the 2s subshell. As a result, the 1s electrons require more energy to remove. This is consistent with the fact that the 1s peak in the PES spectrum is at a higher binding energy.
Note that the binding energy of lithium's 2s peak is equal to the first ionization energy of lithium–that is, the amount of energy is required to remove the outermost or least bound electron from a lithium atom. However, the binding energy of the 1s peak is not equal to the second ionization energy of lithium. Once the first electron is removed from lithium, the 1s electrons will be held even more tightly by the nucleus, increasing the binding energy of these electrons.

PES spectrum of oxygen

Next, let's consider an element with more electrons. Below is the idealized PES spectrum for oxygen, O. For reference, oxygen's ground-state electron configuration is 1s22s22p4.
The idealized PES spectrum of oxygen. The spectrum shows three peaks, one with a binding energy between 100 and 10 MJ/mol and two with binding energies between 10 and 1 MJ/mol. The peak with the lowest binding energy is twice as intense as the other two peaks.
The idealized PES spectrum of oxygen.
In this spectrum, there are three peaks, each representing electrons in a different subshell of oxygen (either 1s, 2s, or 2p). In terms of binding energy, we would expect the peak with the highest binding energy (the leftmost peak) to correspond to the electrons in the 1s subshell, since these electrons are closer to the nucleus and less shielded than those in the 2s or 2p subshells. The peak with the next highest binding energy must correspond to the 2s subshell, and the peak with the lowest binding energy (the rightmost peak) to the 2p subshell.
We can double-check our peak assignments by considering the intensities of the three peaks: Oxygen's 2p subshell contains twice as many electrons as either the 1s or 2s subshell (4 vs. 2). As a result, we would expect the 2p peak to be twice as intense as either the 1s or 2s peak, which is what we see in the spectrum.
Finally, notice that the peaks corresponding to the 2s and 2p electrons have fairly similar binding energies (both between 1 and 10 MJ/mol), while the peak corresponding to the 1s electrons has a much higher binding energy (closer to 100 MJ/mol). Electrons in the same electron shell have similar energies, so we'd expect to see the peaks representing electrons in the same shell to be grouped together in a PES spectrum. Keeping an eye out for these "groups" can help you distinguish between valence and core electrons in a PES spectrum.
Concept check: How many peaks would you expect in the PES spectrum of neutral calcium?

Identifying an element based on its PES spectrum

A pure sample of an unknown element was analyzed using a photoelectron spectrometer, producing the spectrum shown below. What is the identity of our mystery element?
The idealized PES spectrum of an unknown element. The spectrum shows five peaks, one with a binding energy near 100 MJ/mol, two with binding energies near 10 MJ/mol, two with binding energies near 1 MJ/mol. From left to right, the relative intensities of the peaks are 2x, 2x, 6x, 2x, and 1x.
The idealized PES spectrum of a mystery element!
The PES spectrum shows five peaks, which we would expect to correspond to electrons in the five subshells that are closest to the nucleus: 1s, 2s, 2p, 3s, and 3p. The peak with the highest binding energy (the leftmost peak) must correspond to the 1s subshell, while the peak with the lowest binding energy (the rightmost peak) must correspond to the 3p subshell. Note that the 3p peak is half the height of the 1s, 2s, and 3s peaks, which suggests that there is only 1 electron in the 3p subshell of our mystery element.
Which element has only one electron in its 3p subshell? Looking at the periodic table, the first element in the third row of the p-block is aluminum (Al). So, this must be our mystery element! To be sure, let's check that the peaks in the spectrum are consistent with the electron configuration of Al, which is 1s22s22p63s23p1.
As we already know, there are five peaks in the spectrum, which nicely corresponds to the five occupied subshells indicated in aluminum's electron configuration. The intensities of the peaks are consistent with the fact that the 2p subshell contains three times as many electrons as the 1s, 2s, and 3s subshells and six times as many electrons as the 3p subshell. Finally, we see that there are three regions or groups of peaks in the spectrum, which makes sense considering there are three occupied electron shells in Al. Overall, we can be confident that this spectrum actually does represent aluminum!

Summary

  • Photoelectron spectroscopy (PES) is an experimental technique used to determine the relative energies of electrons in atoms and molecules.
  • Photoelectron spectrometers work by ionizing samples using high-energy radiation (such as UV or x-rays) and then measuring the kinetic energies (KE) of the ejected electrons.
  • Given the energy of the incident radiation (hν) and the KE of the photoelectrons, the binding energy (BE) of each ejected electron can be calculated using the following equation: BE=hνKEelectron
  • A PES spectrum is a graph of photoelectron count vs. binding energy.
  • The peaks in a PES spectrum correspond to electrons in different subshells of an atom. The peaks with the lowest binding energies correspond to valence electrons, while the peaks with higher binding energies correspond to core electrons.

Want to join the conversation?

  • blobby green style avatar for user Chuck Finley
    Is there a substantive reason for the distinction in terminology between the work function and the binding energy? Does the difference simply exist to dinstinguish between contexts?
    (22 votes)
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    • leafers ultimate style avatar for user yunhu987
      The distinction between work function and binding energy exists primarily to distinguish between different contexts and conceptual frameworks.

      The work function refers specifically to the minimum energy required to emit an electron from the surface of a material into vacuum. It is considered in the context of electrons interacting with a material surface.

      Binding energy, on the other hand, refers more generally to the energy required to separate constituents that are bound together. It is used in a variety of contexts beyond just electrons and material surfaces.

      So the work function deals specifically with the energy required to remove an electron from the surface of a material, while binding energy is a more general term that can refer to the energy required to separate any kind of bound particles or entities.

      Though numerically these values may be similar for a given system, the work function and binding energy terminology serve to clarify the conceptual framework being considered:

      • Work function - focusing on electrons interacting with a material surface

      • Binding energy - considering a more general interaction between any type of bound particles

      So in summary, while the numerical values may coincide in some cases, the work function and binding energy concepts originate from different frameworks and serve different purposes. The distinction in terminology helps clarify whether we are focusing specifically on electron emission from a material surface or considering a more general separation of bound particles. The difference is primarily one of context and emphasis rather than substantive numerical difference.
      (5 votes)
  • leafers tree style avatar for user Vô Ảnh Cước
    In the third paragraph, how the energy analyzer "count" number of electrons correspond with one determined ionization energy ? Are there any proportion of energy to that number !
    (7 votes)
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    • starky ultimate style avatar for user t r
      I don't think there can be a simple proportion of ionization energies from element to element. Remember, the Bohr model [E=(1/n^2)*13.6eV] fails beyond H and He+ so the ionization tables that this article refers to are empirical.
      (9 votes)
  • blobby green style avatar for user Kristen Whitmer
    When analyzing the binding energy of an element, does it matter what type of ionizing energy is first used to eject the electron(s) from a sample?

    For example if you first bombarded a sample with XPS (according to the description under the subtitle "The basics of photoelectron spectroscopy" this would in theory eject the core electrons) would this alter the binding energy data? If the core electrons were ejected prior to the valence electrons, wouldn't shielding effects be attenuated and consequently, the binding energy of the outer-shell electrons would be increased?
    (5 votes)
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  • male robot hal style avatar for user Bohdan D. Jacklitsch
    The PES spectra show all electrons in a given shell to have the same binding energy. But that leads me to two questions on the same topic. If it were because other electrons were blocking it, than wouldn't further ionizing an already ionized sample make it easier? Or, if it had to do with the fact that protons are positive and electrons are negative, and therefore it takes more energy to remove more electrons to counteract the unequal charge, wouldn't the positive charge increase even more the moment one electron in a shell is removed, therefore increasing the binding energy for every electron rather than for every shell?
    (5 votes)
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  • male robot donald style avatar for user Johnson Zhou
    I thought an electron has a huge amount of kinetic energy in the atom, I heard that it is moving at a third of the speed of light. Why is this not taken into account?
    (5 votes)
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    • leafers ultimate style avatar for user yunhu987
      Electrons do have a significant amount of kinetic energy in atoms due to their high velocity. However, this kinetic energy is generally not taken into account when calculating work functions and binding energies for a few reasons:

      The kinetic energy of electrons in atoms is not well-defined. Due to the Heisenberg uncertainty principle, we cannot precisely know both the position and momentum of an electron at the same time. So while we know electrons move fast, we can't pinpoint their exact location and velocity.

      The important energy for work function and binding energy calculations is the potential energy, not the kinetic energy. The potential energy determines how strongly the electron is bound to the atom and how much energy is required to remove it. The kinetic energy, while large, does not reflect the strength of this binding.

      When an electron is removed from an atom, its initial kinetic energy is lost and it gains new kinetic energy based on the work function or binding energy. So its final kinetic energy depends on the difference in potential energies, not its initial kinetic energy within the atom.

      Work functions and binding energies are measured experimentally by seeing how much energy is required to remove an electron. This measures the change in potential energy, not any initial kinetic energy the electron may have had.

      So in summary, while electrons do have significant kinetic energy due to their fast motion within atoms, this kinetic energy is generally ignored when calculating work functions and binding energies. The important factor is the change in potential energy, which determines how strongly the electron is bound and how much energy is required to remove it from the atom. The initial kinetic energy is lost during this process.
      (3 votes)
  • marcimus pink style avatar for user sachi.sharma
    can you have the PES graph of an ion like Li+? If so, how would you be bale to tell the difference from the graph of an element that looks the same like He in this case?
    (4 votes)
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    • piceratops ultimate style avatar for user Struggle is the key.
      I don't know the answer but from what I have read so for in this article once you eject an electron from one of its shell the binding energy changes. Lets say you would eject an the valence electron in this case the 2s electron from Li. Since the nucleus of Li has three protons and Helium has two 1s^2 electrons the binding energy for the remaining 1s^2 for Li+ would be different compared to the binding energy of the 1s^2 from He. I would belive this to be the case since the effective charge of the nucleus is not the same as for He. So I would believe if one could have a PES graph for ion like Li+ it would be different from the graph of He.
      Could it be so that the the binding energy would by shifted by som factor for the two peaks compared with the peaks of He? Lets say He has it 1s^2 peak at 100 MJ/mol would it be the case then that Li+ (assuming that the 2s electron was ejected) would have it lets say a PES graph of peak of 130 MJ/mol. The 130 is just arbitrary I'm thinkin of som factor a>1 => 100*a is the new peak.
      (4 votes)
  • female robot amelia style avatar for user Lionel Powers
    I'm curious - is there a way that a travelling electron can further increase its kinetic energy? For instance, if it was hit by another photon or traveled next to a negative charge. Or will it maintain the energy once got knocked off, until affected by other charges..
    (3 votes)
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    • piceratops seed style avatar for user RogerP
      You can increase the kinetic energy of charged subatomic particles by accelerating them through an electric field. This is the basis of particle accelerators.

      I don't think a travelling electron can absorb energy from a photon - at least, I've never heard of that happening but it might be a question better answered by a physicist.
      (3 votes)
  • blobby green style avatar for user Ali, Mir
    I have a question that's been bothering me for a while...

    We know that ionization energy on each peak is the energy needed to remove an electron from a particular subshell. Bearing this in mind, do all electrons on a subshell eject when you exposed it to the ionization energy? For example, would all 4 of Oxygen's valence electrons eject if you expose it to 1.31 MJ/mol?
    (4 votes)
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  • starky ultimate style avatar for user MagicMoney
    It states that, "However, the binding energy of the
    1s peak is not equal to the second ionization energy of lithium. Once the first electron is removed from lithium, the 1s, electrons will be held even more tightly by the nucleus, increasing the binding energy of these electrons."

    So it's saying that the second ionization energy is not equal to the second binding energy, in the sense that when you ionize it initially it changes the electron configuration making the electrons closer to the nucleus less shielded by the outer electrons. However, I don't see the difference between sequentially removing an electron from an atom and measuring the electron ionization energy to photoelectron spectroscopy's binding energy.

    Both of those methods remove electrons sequentially and measure their energies, so why can't you determine the second ionization energy from a photoelectron spectroscopy chart?
    (2 votes)
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    • leafers ultimate style avatar for user yunhu987
      at first glance, it may seem like photoelectron spectroscopy binding energies should correspond directly to ionization energies. However, there are a few key differences:

      Ionization energies measure the energy required to remove an electron from a neutral atom, leaving an ion. Binding energies, on the other hand, measure the energy of electrons within an already ionized atom.

      As you noted, removing the first electron changes the electron configuration, pulling the remaining electrons closer to the nucleus and increasing their binding energy. This effect is not accounted for in ionization energy measurements, which consider the removal of each electron independently from the neutral atom.

      Ionization energies refer specifically to the process of electron removal - ejecting an electron into vacuum. Binding energies, however, reflect the energy of the remaining electrons within the ionized atom, not just the energy required to remove them.

      Experimental measurements of ionization energies and binding energies involve different processes. Ionization energies are measured by exposing atoms to radiation or electric fields and detecting the ejected electrons. Binding energies are determined from the kinetic energies of photoelectrons ejected from ionized atoms.
      (4 votes)
  • piceratops ultimate style avatar for user wanglx123456789
    what is first ionization energy and second ionization energy ?
    (1 vote)
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    • leaf red style avatar for user Richard
      Ionization energy is energy required to remove the outer most electron from an atom. The first ionization energy would be the energy required to remove the first electron, the second ionization energy would be the energy to remove the second electron, and so on. The reason it's called ionization is that when you remove an electron from a neutral atom, it becomes a positively charged ion, or cation, having lost a negatively charged electron. Hope that helps.
      (4 votes)