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Make a rough estimate of this uniform energy spacing in electron volts (where 1eV=1.6×1019 J). You will need to make some rough estimates of atomic properties based on prior work. For comparison with the spacing of these vibrational energy states, note that the spacing between quantized energy levels for "electronic" states such as in atomic hydrogen is of the order of several electron volts.

(b) List several photon energies that would be emitted if a number of these vibrational energy levels were occupied due to collisional excitation. To what region of the spectrum (x-ray, visible, microwave, etc.) do these photons belong? (See Figure 8.1 at the beginning of the chapter.)

Short Answer

Expert verified

a. The uniform energy spacing is 2.12×1039 eV.

b. The several photon energies are 2.12×1039 eV,4.24×1039 eV and 6.36×1039 eVrespectively. The photons belong in the spectrum’s infrared part.

Step by step solution

01

Significance of the spring constant

The spring constant is described as the ratio of the force that is affected by the spring and the displacement caused by the spring. It mainly determines the stiffness of a spring.

02

(a) Determination of the uniform energy spacing

The equation of the uniform spacing of energy is expressed as:

E=km

Here, Eis the uniform spacing of energy, is the Planck’s constant,kis the spring constant and mis the mass of an HCl molecule.

Substitute 1.05×1034 Jsfor , 480 N/mfor kand 3×1026 kgfor min the above equation.

E=(1.05×1034 Js)480 N/m3×1026 kg=(1.05×1034 Js)1.6×1028 N/kgm=(1.05×1034 Js)1.6×1028 kgm/s2/kgm×1 kgm/s21 N=(1.05×1034 Js)1.6×1028 s-2

Hence, further as:

E=(1.05×1034 Js)1.6×1028 s-2=(1.05×1034 Js)(1.26×1014 s1)=1.3×1020 J×1.6×1019 J1 eV=2.12×1039 eV

Thus, the uniform energy spacing is 2.12×1039 eV.

03

(b) Determination of the photon energies

The equation of the photon energy in the ground state is expressed as:

E1=1×E=E

Here, E1is the photon energy in the ground state.

Substitute 2.12×1039 eVfor Ein the above equation.

E1=2.12×1039 eV

The equation of the photon energy in the first excited state is expressed as:

E2=2×E=2E

Here,E2is the photon energy in the first excited state.

Substitute 2.12×1039 eVfor Ein the above equation.

E2=2×2.12×1039 eV=4.24×1039 eV

The equation of the photon energy in the second excited state is expressed as:

E3=3×E=3E

Here,E3is the photon energy in the second excited state.

Substitute2.12×1039 eV for Ein the above equation.

E3=3×2.12×1039 eV=6.36×1039 eV

According to the diagram, it can be identified that the photons mainly belong to the spectrum’s infrared part.

Thus, the several photon energies are 2.12×1039 eV,4.24×1039 eV and6.36×1039 eV respectively. The photons belong in the spectrum’s infrared part.

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Most popular questions from this chapter

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.

If you double the amplitude, what happens to the frequency in a classical (non quantum) harmonic oscillator? In a quantum harmonic oscillator?

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.

The Frank Hertz experiment involved shooting electrons into a low density gas of mercury atoms and observing discrete amounts of kinetic energy loss by the electrons. Suppose that instead the similar experiment is done with a very cold gas of atomic hydrogen, so that all of the hydrogen atoms are initially in ground state. If the kinetic energy of an electron is 11.6 eV just before it collides with a hydrogen atom. How much kinetic energy will the electron have just after it collides with and excites the hydrogen atom?

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.)

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