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

When starlight passes through a cold cloud of hydrogen gas, some hydrogen atoms absorb energy, then reradiate it in all directions. As a result, spectrum of the star shows dark absorption lines at the energies for which less energy from the star reaches us. How does the spectrum of dark absorption lines for very cold hydrogen differs from the spectrum of bright emission lines from very hot hydrogen?

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.)

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?

Suppose we have reason to suspect that a certain quantum object has only three quantum states. When we excite such an object we observe that it emits electromagnetic radiation of three different energies: 2.48eV(green), 1.91eV(orange), and 0.57eV(infrared). (a) Propose two possible energy-level schemes for this system. (b) Explain how to use an absorption measurement to distinguish between the two proposed schemes.

The mean lifetime of a certain excited atomic state is 5 ns. What is the probability of the atom staying in this excited state for t=10 ns or more?

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