Electron's emission in Sn atom

In summary, the problem is asking for the construction of a scheme for the core levels of Sn and their corresponding excitations energies. The Kα and Kβ lines represent the wavelengths of the X-ray photons emitted when electrons are ejected from the K-shell and the L-shell, respectively. The excitation energies can be calculated by subtracting the respective binding energies from the K-shell binding energy.
  • #1
pollo93
1
0
Good morning everybody, here's a problem about excitations energy of the core level of a Sn atom.
It says to construct the scheme of the core levels of Sn indicating the excitations energies. Now the K edge (the problem doesn't say we are necessarily talking about X-rays, but I think we are because of this notation) is at λ=0.425 A and the first two lines are Kα=0.517 A and Kβ=0.437 A. (A is for "angstrom": 10^-10 m)

Now shouldn't the excitations energies be just hc/λ ? Probably I actually didn't understand what Kα and Kβ are. I think they are the wavelengths of the emissed photoelectrons due to X-ray, but I'm probably wrong.

Who can help me? Thanks.
 
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  • #2
The excitation energies of a core level are typically described in terms of the binding energy, which is the energy required to remove an electron from the core level. The Kα and Kβ lines correspond to the wavelengths of the X-ray photons that are emitted when an electron is ejected from the core level. The excitation energy for a given core level is equal to the difference between the binding energy of that level and the binding energy of the next lower level. For example, in the case of a Sn atom, the binding energy of the K-shell is 54.8 eV and the binding energy of the L-shell is 19.2 eV. Therefore, the excitation energy of the K-shell would be the difference between these two values, which is 35.6 eV. This corresponds to a wavelength of 0.425 Å. The Kα and Kβ lines correspond to the emission of X-ray photons when electrons are ejected from the K-shell and the L-shell, respectively. The energy of these photons (i.e. the excitation energies) can be calculated by subtracting the respective binding energies from the K-shell binding energy:Kα: 54.8 eV - 46.3 eV = 8.5 eV (wavelength = 0.517 Å)Kβ: 54.8 eV - 32.2 eV = 22.6 eV (wavelength = 0.437 Å)Therefore, the scheme of the core levels of Sn indicating the excitation energies would look like this:K-Shell: 54.8 eV (λ = 0.425 Å)Kα: 8.5 eV (λ = 0.517 Å)Kβ: 22.6 eV (λ = 0.437 Å)L-Shell: 19.2 eV
 

1. How does an electron get emitted in a Sn atom?

The emission of an electron in a Sn atom is a result of energy being absorbed by the atom. This energy can come from various sources such as heat, light, or collisions with other particles. When an electron gains enough energy, it can overcome the attractive force of the atom's nucleus and become free, resulting in emission.

2. What is the significance of an electron's emission in Sn atom?

The emission of an electron in a Sn atom is important as it can provide information about the energy levels and structure of the atom. It can also be used in various applications such as electron microscopy and spectroscopy.

3. Can an electron be emitted from any energy level in a Sn atom?

No, an electron can only be emitted from certain energy levels in a Sn atom. This is because each energy level has a specific amount of energy associated with it, and the electron must gain enough energy to overcome the attractive force of the nucleus. This is known as the ionization energy.

4. What happens to the Sn atom after an electron is emitted?

After an electron is emitted from a Sn atom, the atom becomes positively charged as it has lost one of its negatively charged particles. This can affect the chemical properties of the atom and how it interacts with other atoms.

5. Can the emission of electrons in a Sn atom be controlled?

Yes, the emission of electrons in a Sn atom can be controlled through various methods such as applying a magnetic field or using a laser to excite the atoms. This can allow scientists to study the properties of the emitted electrons and manipulate their behavior for different applications.

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