Warning: foreach() argument must be of type array|object, bool given in /var/www/html/web/app/themes/studypress-core-theme/template-parts/header/mobile-offcanvas.php on line 20

A hypothetical atom has energy levels uniformly separated by 1.2 eV . At a temperature of 2000 K, what is the ratio of the number of atoms in the 13thexcited state to the number in the11thexcited state?

Short Answer

Expert verified

The ratio of the number of atoms in the 13thexcited state to the number of atoms in the 11thexcited state is 9ร—10-7.

Step by step solution

01

The given data:

The energy difference between two atomic levels of an atom,โˆ†E=1.2eV

The temperature of the states,T=2000K

Number of atoms in the higher-energy state,N1=6.1ร—1013/cm3

Number of atoms in the lower-energy state, N2=2.5ร—1015/cm3

02

Understanding the concept of Boltzmann distribution equation

The Boltzmann distribution is a probability function used in statistical physics to define the state of a particle system in terms of temperature and energy.

Using the Boltzmann-distribution equation which is the expression for the probability for stimulated emission of radiation to the probability for spontaneous emission of radiation under thermal equilibrium, we can get the required ratio of the number of atoms present in the excited state to that present in the excited state.

Formula:

The Boltzmann energy distribution equation,

N1N2=e-E2-E2/kT โ€ฆ.. (1)

Here, Boltzmann constant,k=8.625ร—10-5eV/K

03

Calculation of the ratio of number of atoms in the given states:

The energy difference between any two levels is,

E13-E11=21.2eV=2.4eV

So, the energy difference between the13th excited state and the 11th excited state is given as:

Now, using this energy difference value in the equation (i) with the given data, we can get the ratio of the number of atoms in the 13th excited state to the number of atoms in the 11th excited state as follows:

N1N2=e-2.4eV8.625ร—10-5eV/K2000K=e-13.91=9ร—10-7

Hence, the value of the required ratio is 9ร—10-7.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

Comet stimulated emission.When a comet approaches the Sun, the increased warmth evaporates water from the ice on the surface of the comet nucleus, producing a thin atmosphere of water vapor around the nucleus. Sunlight can then dissociate H2Omolecules in the vapor to H atoms and OH molecules. The sunlight can also excite the OH molecules to higher energy levels.

When the comet is still relatively far from the Sun, the sunlight causes equal excitation to the E2and E1levels (Fig. 40-28a). Hence, there is no population inversion between the two levels. However, as the comet approaches the Sun, the excitation to theE1level decreases and population inversion occurs. The reason has to do with one of the many wavelengthsโ€”said to be Fraunhofer linesโ€”that are missing in sunlight because, as the light travels outward through the Sunโ€™s atmosphere, those particular wavelengths are absorbed by the atmosphere.

As a comet approaches the Sun, the Doppler Effect due to the cometโ€™s speed relative to the Sun shifts the Fraunhofer lines in wavelength, apparently overlapping one of them with the wavelength required for excitation to the E1level in OH molecules. Population inversion then occurs in those molecules, and they radiate stimulated emission (Fig. 40 28b). For example, as comet Kouhoutek approached the Sun in December 1973 and January 1974, it radiated stimulated emission at about during mid-January. (a) What was the energy difference E2-E1for that emission? (b) In what region of the electromagnetic spectrum was the emission?

Show that if the 63 electrons in an atom of europium were assigned to shells according to the โ€œlogicalโ€ sequence of quantum numbers, this element would be chemically similar to sodium.

Consider the elements krypton and Rubidium.

(a) Which is more suitable for use in a Sternโ€“Gerlach experiment of the kind described in connection with Fig. 40-8?

(b) Which, if either, would not work at all?

Figure 40-21 shows partial energy-level diagrams for the helium and neon atoms that are involved in the operation of a heliumโ€“neon laser. It is said that a helium atom in stateE3 can collide with a neon atom in its ground state and raise the neon atom to state E2. The energy of helium state E3(20.61eV)is close to, but not exactly equal to, the energy of neon state role="math" localid="1661494292758" E2(20.66eV). How can the energy transfer take place if these energies are not exactly equal?

The mirrors in the laser of Fig. 40-20, which are separated by 8.0 cm, form an optical cavity in which standing waves of laser light can be set up. Each standing wave has an integral number n of half wavelengths in the 8.0 cm length, where n is large and the waves differ slightly in wavelength. Near ฮป=533nm, how far apart in wavelength are the standing waves?

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free