Chlorine has two naturally occurring isotopes,CI35and CI37. Show that

the vibrational spectrum of HCIshould consist of closely spaced doublets,

with a splitting given by v=7.51×10-4v, where v is the frequency of the

emitted photon. Hint: Think of it as a harmonic oscillator, with ω=k/μ, where

μis the reduced mass (Equation 5.8 ) and k is presumably the same for both isotopes.

Short Answer

Expert verified

It will identified a difference in HCL's vibrational spectrum using a harmonic oscillator

model.

Show the vibrational spectrum of HCL consist of closely spaced doublets, with a

splitting v=7.51×10-4v,

Step by step solution

01

Definition of harmonic oscillator

  • A model for molecular vibration is the simple harmonic oscillator. It denotes the relative motion of atoms in a diatomic molecule or
  • The simultaneous motion of atoms in a polyatomic molecule along a vibrational "normal mode."
02

Determine the photon energy in a vibrational   state

A photon's energy in a vibrational state n is:

EY=12+n

The amount of energy required for a photon to go from its initial state nito its final

state nfis:

EY=Ef=Ei-12+nf-12+ni-nhωn-nf-ni

The photon's frequency is:

v=Eyh=nω2π

For oscillation frequency, we can use the harmonic oscillator formula:

ω=Kμv=n2πKμv=nK2πμ-1/2

03

Determine the reduced mass

Take absolute value (because frequency must be positive) with respect to reduced

mass μ:

v=nK2π×-12μ3/2μ=μ2μnK2πμ-1/2=μ2μvμ=mhmCImH+mCI=11mCI+1mLIμ=-11mCI+1mμI=μmCI2mCI

04

Determine the value of∆v

For mCI=36, it use the average value. It goes like this:

v=v2μmCImCI2=v2mCI/mC1+mCmUmCImCI=236-118=mCImH-361v=121/181+36v=v36×37v=7.51×10-4v

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

Suppose you had three particles, one in stateψa(x), one in stateψb(x), and one in stateψc(x). Assuming ψa,ψb, andψc are orthonormal, construct the three-particle states (analogous to Equations 5.15,5.16, and 5.17) representing

(a) distinguishable particles,

(b) identical bosons, and

(c) identical fermions.

Keep in mind that (b) must be completely symmetric, under interchange of any pair of particles, and (c) must be completely antisymmetric, in the same sense. Comment: There's a cute trick for constructing completely antisymmetric wave functions: Form the Slater determinant, whose first row isψa(x1),ψb(x1),ψc(x1) , etc., whese second row isψa(x2),ψb(x2),ψc(x2) , etc., and so on (this device works for any number of particles).

Certain cold stars (called white dwarfs) are stabilized against gravitational collapse by the degeneracy pressure of their electrons (Equation 5.57). Assuming constant density, the radius R of such an object can be calculated as follows:

P=23EtotV=23h2kF510π2m=(3π2)2/3h25mp5/3(5.57)

(a) Write the total electron energy (Equation 5.56) in terms of the radius, the number of nucleons (protons and neutrons) N, the number of electrons per nucleon d, and the mass of the electron m. Beware: In this problem we are recycling the letters N and d for a slightly different purpose than in the text.

Etot=h2V2π2m0kFK4dk=h2kF5V10π2m=h2(3π2Nd)5/310π2mV-2/3(5.56)

(b) Look up, or calculate, the gravitational energy of a uniformly dense sphere. Express your answer in terms of G (the constant of universal gravitation), R, N, and M (the mass of a nucleon). Note that the gravitational energy is negative.

(c) Find the radius for which the total energy, (a) plus (b), is a minimum.

R=(9π4)2/3h2d5/3GmM2N1/3

(Note that the radius decreases as the total mass increases!) Put in the actual numbers, for everything except , using d=1/2 (actually, decreases a bit as the atomic number increases, but this is close enough for our purposes). Answer:

(d) Determine the radius, in kilometers, of a white dwarf with the mass of the sun.

(e) Determine the Fermi energy, in electron volts, for the white dwarf in (d), and compare it with the rest energy of an electron. Note that this system is getting dangerously relativistic (seeProblem 5.36).

(a)Use Equation5.113 to determine the energy density in the wavelength rangedλ. Hint: setρ(ω)=ρ-(λ), and solve forρ(λ)-

(b)Derive the Wien displacement law for the wavelength at which the blackbody energy density is a maximum
λmax=2.90×10-3mKT

You'll need to solve the transcendental equation(5×x)=5e-x, using a calculator (or a computer); get the numerical answer accurate to three significant digits.

Obtain equation 5.76 by induction. The combinatorial question is this: How many different ways you can put N identical balls into d baskets (never mind the subscriptfor this problem). You could stick all of them into the third basket, or all but one in the second basket and one in the fifth, or two in the first and three in the third and all the rest in the seventh, etc. Work it out explicitly for the casesN=1,N=2,N=3andN=4; by that stage you should be able to deduce the general formula.

Imagine two non interacting particles, each of mass , in the one dimensional harmonic oscillator potential (Equation 2.43). If one is in the ground state, and the other is in the first excited state, calculate (x1-x2)2assuming
(a) they are distinguishable particles, (b) they are identical bosons, and (c) they are identical fermions. Ignore spin (if this bothers you, just assume they are both in the same spin state.)

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