When applying quantum mechanics, we often concentrate on states that qualify as “orthonormal”, The main point is this. If we evaluate a probability integral over all space of ϕ1*ϕ1or of ϕ2*ϕ2, we get 1 (unsurprisingly), but if we evaluate such an integral forϕ1*ϕ2orϕ2*ϕ1 we get 0. This happens to be true for all systems where we have tabulated or actually derived sets of wave functions (e.g., the particle in a box, the harmonic oscillator, and the hydrogen atom). By integrating overall space, show that expression (7-44) is not normalized unless a factor of 1/2is included with the probability.

Short Answer

Expert verified

By integrating overall space, you get that, a factor of ½ will be required to be included with the probability.

Step by step solution

01

Used formula:

The wave function transitional state can be represented by the following equation:

Ψtransition(r,t)=Ψi(r,t)+Ψf(r,t)Ψtransition(r,t)=Ψi(r)e-iEit/h+Ψf(r)e-iEft/h..(7-44)

Where, Ψ isWave function, Ψi is the Wave function of initial state, Ψf is the Wave function of final state, r is the radius, t is time, Ei is the initial energy, Ef is final energy, h is Planck’s constant.
02

Integrating overall space:

Consider the given data as below.

Ψ.ΨdV=1

Now, if you introduce a factor A which can be adjusted to give probability equal to 1.

A.Ψi*re+iEit/h+A.Ψf*re+e+iEit/hA.Ψire-iEit/h+A.Ψfre+e-iEit/hdV=1A2Ψir2dV+e+i(Ei+Ef)t/hΨi*rΨfrdV+e-i(Ei-Ef)t/hΨf*rΨirdV+Ψfr2dV=1A21+0+0+1=1

A=12

Hence, the factor12must be included with each wave function.

As you know that probability density is the square of wave function.

Hence, a factor of 12 will be required to be included with the probability.

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

A spherical infinite well has potential energy

U(r)={0r<a+r>a

Since this is a central force, we may use the Schrodinger equation in the form (7-30)-that is, just before the specific hydrogen atom potential energy is inserted. Show that the following is a solution

R(r)=Asinbrr

Now apply the appropriate boundary conditions. and in so doing, find the allowed angular momenta and energies for solutions of this form.

In general, we might say that the wavelengths allowed a bound particle are those of a typical standing wave,λ=2L/n , where is the length of its home. Given that λ=h/p, we would have p=nh/2L, and the kinetic energy, p2/2m, would thus be n2h2/8mL2. These are actually the correct infinite well energies, for the argumentis perfectly valid when the potential energy is 0 (inside the well) and is strictly constant. But it is a pretty good guide to how the energies should go in other cases. The length allowed the wave should be roughly the region classically allowed to the particle, which depends on the “height” of the total energy E relative to the potential energy (cf. Figure 4). The “wall” is the classical turning point, where there is nokinetic energy left: E=U. Treating it as essentially a one-dimensional (radial) problem, apply these arguments to the hydrogen atom potential energy (10). Find the location of the classical turning point in terms of E , use twice this distance for (the electron can be on both on sides of the origin), and from this obtain an expression for the expected average kinetic energies in terms of E . For the average potential, use its value at half the distance from the origin to the turning point, again in terms of . Then write out the expected average total energy and solve for E . What do you obtain

for the quantized energies?

Question: A particle is trapped in a spherical infinite well. The potential energy is 0for r < a and infinite for r > a . Which, if any, quantization conditions would you expect it to share with hydrogen, and why?

To conserve momentum, an atom emitting a photon must recoil, meaning that not all of the energy made available in the downward jump goes to the photon. (a) Find a hydrogen atom's recoil energy when it emits a photon in a n = 2 to n = 1 transition. (Note: The calculation is easiest to carry out if it is assumed that the photon carries essentially all the transition energy, which thus determines its momentum. The result justifies the assumption.) (b) What fraction of the transition energy is the recoil energy?

Can the transition 2s1s in the hydrogen atom occur by electric dipole radiation? The lifetime of the 2 s is known to be unusual. Is it unusually short or long?

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