A hot bar of iron glows a dull red. Using our simple ball-spring model of a solid (Figure 8.23), answer the following questions,explaining in detail the processes involved. You will need to make some rough estimates of atomic properties based on prior work. (a) What is the approximate energy of the lowest-energy spectral emission line? Give a numerical value. (b) What is the approximate energy of the highest-energy spectral emission line? Give a numerical value. (c) What is the quantum number of the highest-energy occupied state? (d) Predict the energies of two other lines in the emission spectrum of the glowing iron bar. (Note: Our simple model is too simple-the actual spectrum is more complicated. However, this simple analysis gets at some important aspects of the phenomenon.)

Short Answer

Expert verified

(a) The approximate energy of the lowest-energy spectral emission line is2.5×1020 J .

(b) The approximate energy of the highest-energy spectral emission line is 2.88×1019 J.

(c) The quantum number of the highest energy occupied state is about 12.

(d) The energies of two other lines in the emission spectrum are5×1020 J and7.5×1020 J respectively.

Step by step solution

01

Significance of the energy

The energy is referred to as a qualitative property which is transferred from one object to another object. It can also not be destroyed nor created.

02

(a) Determination of the approximate energy of the lowest energy line

The lowest energy emission spectrum line mainly represents the jump from one to another vibrational energy. The energy required for melting the iron is the energy of the lowest energy emission spectrum line.

The equation of the lowest energy emission spectrum line is expressed as:

E=kT

Here,E is the lowest energy emission spectrum line,k is the Boltzmann constant andT is the iron’s melting point.

Substitute 1.38×1023J/Kfork and1811 K forT in the above equation.

E=(1.38×1023J/K)(1811 K)=2.5×1020 J

Thus, the approximate energy of the lowest-energy spectral emission line is 2.5×1020 J.

03

(b) Determination of the approximate energy of the highest energy line 

The red colour line from the diagram given in the question is the highest energy emission spectral line.

The equation of the energy of the highest emission spectral line is expressed as:

E1=hf

Here,E1 is the energy of the highest emission spectral line,h is the Planck’s constant andf is the red light’s frequency.

Substitute6.626×1034​Js forh and 435×1012 s-1forf in the above equation.

E1=(6.626×1034​Js)(435×1012 s-1)=2.88×1019 J

Thus, the approximate energy of the highest-energy spectral emission line is 2.88×1019 J.

04

(c) Determination of the quantum number 

The equation of the quantum number is expressed as:

N=E1E

Here,N is the quantum number.

Substitute the values in the above equation.

N=2.88×1019 J2.5×1020 J=11.5212

Thus, the quantum number of the highest energy occupied state is about 12.

05

(d) Determination of the prediction of energies

The equation of the energy of the first line in the emission spectrum is expressed as:

U1=E+E=2E

Here,U1 is the energy of the first line in the emission spectrum.

Substitute the values in the above equation.

U1=2×2.5×1020 J=5×1020 J

The equation of the energy of the second line in the emission spectrum is expressed as:

U2=E+2E=3E

Here,U2 is the energy of the second line in the emission spectrum.

Substitute the values in the above equation.

U2=3×2.5×1020 J=7.5×1020 J

Here, these calculations are accurate and also wild.

Thus, the energies of two other lines in the emission spectrum are5×1020 J and7.5×1020 J respectively.

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Most popular questions from this chapter

The photon energy for green light lies between the values for red and violet light. What is the approximate energy of the photons in green light? The intensity of sunlight above the Earth’s atmosphere is about 1400 W (J/s) per square meter. That is, when sunlight hits perpendicular to a square meter of area, about 1400 W of energy can be absorbed. Using the photon energy of green light, about how many photons per second strike an area of one square meter? (This is why the lumpiness of light was not noticed for so long.)

Match the description of a process with the corresponding arrow in figure 8.38: (a) Absorption of a photon whose energy is E1-E0. (b) Absorption from an excited state (a rare event at ordinary temperatures). (c) Emission of a photon whose energy isE3-E1 . (d) Emission of a photon whose energy isE2-E0 . (e) In drawing arrows to represent energy transitions, which of the following statement are correct. (1) it doesn’t matter in which direction you draw the arrow as long as it connects the initial and final states. (2) For emission, the arrow points down. (3) For absorption, the arrow points up. (4) The tail of the arrow is drawn on the initial state. (5) The head of the arrow is drawn on the final state. (6) It is not necessary to draw and arrowhead.

Some material consisting of a collection of microscopic objects is kept at a high temperature. A photon detector capable of detecting photon energies from infrared through ultraviolet observes photons emitted with energies of0.3eV,0.5eV,0.8eV,2,0eV,2.5eV,and2.8eV. These are the only photon energies observed. (a) Draw and label a possible energy-level diagram for one of the microscopic objects, which has four bound states. On the diagram, indicate the transitions corresponding to the emitted photons. Explain briefly. (b) Would a spring–mass model be a good model for these microscopic objects? Why or why not? (c) The material is now cooled down to a very low temperature, and the photon detector stops detecting photon emissions. Next, a beam of light with a continuous range of energies from infrared through ultraviolet shines on the material, and the photon detector observes the beam of light after it passes through the material. What photon energies in this beam of light are observed to be significantly reduced in intensity (“dark absorption lines”)? Explain briefly.

Summarize the differences and similarities between different energy levels in a quantum oscillator. Specifically for the first two levels in figure 8.26, compare the angular frequency Ks/m, the amplitude , and the kinetic energyk at the same value of . ( In a quantum-mechanical analysis the concepts of angular frequency and amplitude require reinterpretation. Nevertheless, there remain elements of the classical picture. For example, larger amplitude corresponds to a higher probability of observing a large stretch.)

Suppose we have a reason to suspect that a certain quantum object has only three quantum states.When we excite a collection of such objects we observe that they emit electromagnetic radiation of three different energies: 0.3eV(infrared), 2.0eV(visible), and 2.3eV(visible).

(a) Draw a possible energy-level diagram for one of the quantum objects, which has three bound states. On the diagram, indicate the transitions corresponding to the emitted photons, and check that the possible transitions produce the observed photons and no others. The energyK+U of the ground state is -4eV. Label the energies of each level ( K+U, which is negative).

(b) The material is now cooled down to a very low temperature, and the photon detector stops detecting photon emissions. Next a beam of light with a continuous range of energies from infrared through ultraviolet shines on the material, and the photon detector observes the beam of light after it passes through the material. What photon energies in this beam of light are observed to be significantly reduced in intensity ("dark absorption lines")? Energy of highest-energy dark line: eV Energy of lowest-energy dark line: eV

(c) There exists another possible set of energy levels for these objects which produces the same photon emission spectrum. On an alternative energy-level diagram, different from the one you drew in part (a), indicate the transitions corresponding to the emitted photons, and check that the possible transitions produce the observed photons and no others. When you are sure that your alternative energy-level diagram is consistent with the observed photon energies, enter the energies of each level (K+U, which is negative).

(d) For your second proposed energy-level scheme, what photon energies would be observed to be significantly reduced in intensity in an absorption experiment ("dark absorption lines")? (Given the differences from part (b), you can see that an absorption measurement can be used to tell which of your two energy-level schemes is correct).

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