Assume that a hypothetical object has just four quantum states, with the energies shown in Figure 8.43.

(a) Suppose that the temperature is high enough that in a material containing many such objects, at any instant some objects are found in all of these states. What are all the energies of photons that could be strongly emitted by the material? (In actual quantum objects there are often “selection rules” that forbid certain emissions even though there is enough energy; assume that there are no such restrictions here.) (b) If the temperature is very low and electromagnetic radiation with a wide range of energies is passed through the material, what will be the energies of photons corresponding to missing (“dark”) lines in the spectrum? (Assume that the detector is sensitive to a wide range of photon energies, not just energies in the visible region.)

Short Answer

Expert verified

(a) 1.9eV, 2.5eV, 3eV, 0.6eV, 1.1eVand 0.5eV

(b) 1.9eV, 2.5eVand 3eV

Step by step solution

01

Identification of the given data

The given data is listed below as-

  • The energy at the ground state is, E0
  • The energy at the first excited state is, E1=1.9eV+E0
  • The energy at the second excited state is,E2=2.5eV+E0
  • The energy at the third excited state is, E3=3.0eV+E0
02

Significance of the change in the energy of the photon

The change in the energy of the photon equals the difference between the energy at the higher and the energy at the lower state.

The equation of the photon energies can be expressed as,

ΔE=Ef-E0 …(1)

Here, ΔE is the emitted energy of photon, Ef is the energy in excited state and E0 is energy in the ground state.

03

Determination of the energies of the photons emitted by the material 

E1=1.9eV(a)

As there is no energy at the ground state, then the energy at the ground state is zero that is E0=0.

For the electrons going from the ground state to the first excited state,

For Ef=E1=1.9eVand E0=0eVin equation (1).

E=1.9eV-(0eV)=1.9eV

For the electrons going from the ground state to the second excited state,

For Ef=E2=2.5eVand E0=0eVin equation (1).

E=2.5eV-(0eV)=2.5eV

For the electrons going from the ground state to the third excited state,

For Ef=E3=3.0eVand E0=0eVin equation (1).

E=3.0eV-(0eV)=3.0eV

For the electrons going from the first excited state to the second excited state, the equation becomes,

ΔE=Ef-E1 …(2)

Here, ΔEis the energy emitted by the photon, Efis the energy of the other excited state and E1is the energy of the first excited state

For the electrons going from the first excited state to the second excited state

For Ef=E2=2.5eVand E1=1.9eVin equation (2),

E=2.5eV-(1.9eV)=0.6eV

For the electrons going from the first excited state to the third excited state,

For Ef=E3=3eVand E1=1.9eVin equation (2),

E=3eV-(1.9eV)=1.1eV

For the electrons going from the second excited state to the third excited state, the equation becomes,

ΔE=Ef-E2 …(3)

Here, ΔEis the energy emitted by the photon, Efis the energy of the other excited state and E2is the energy of the second excited state.

For Ef=E3=3.0eVand E2=2.5eVin equation (3).

E=3.0eV-(2.5eV)=0.5eV

Thus, the energies of photon that could be strongly emitted by the material are 1.9eV, 2.5eV, 3eV, 0.6eV, 1.1eVand 0.5eV.

04

Determination of the dark lines in the spectrum

(b)

The electrons move from the ground to the higher excited state and gain energy. Hence, due to low temperature and the electromagnetic radiation, wide energy range has been passed through the material. So, energy of the photon that is corresponding to the dark lines is from the ground to the higher excited states.

Thus, the energies of the photons that corresponds to the missing lines in the spectrum are1.9eV, 2.5eVand 3eVrespectively.

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Most popular questions from this chapter

The first excited state of a mercury atom is 4.9eV above the ground state. A moving electron collides with a mercury atom and excites the mercury atom to its first excited state. Immediately after the collision the kinetic energy of the electron is 0.3eV. What was the kinetic energy of the electron just before the collision?

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