Show that|ψ|2=|ψ|2 , with related as in Eq. 38-14. That is, show that the probability density does not depend on the time variable.

Short Answer

Expert verified

The value 1 is does not depend on the time variable that shows that the probability density does not depend on the time variable.

Step by step solution

01

Determine the concept and the formula

In the year 1900, derived a formula that shows the relationship between all the wavelength and all the temperatures and that is given as Equation 38-14 in book and also known as the Planck’s radiation law

Sλ=2πc2hλ51ehcλKt-1

Here, h is the Planck constant, k is the Boltzmann constant, and T is the temperature of the radiating surface (in kelvins), λis wavelength S is thermal radiation.

02

Determine the derivation as:

By referring the equation number 38-14 solve for the derivation as:

ψ2=eikx2ψ2=eikx*eikx=e-ikxeikxψ2=e0=1ψ2=ψ2

The value 1 is does not depend on the time variable that shows that the probability density does not depend on the time variable.

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Most popular questions from this chapter

A metal plate is illuminated with light of a certain frequency. Which of the following determine whether or not electrons are ejected: (a) the intensity of the light, (b) how long the plate is exposed to the light, (c) the thermal conductivity of the plate, (d) the area of the plate, (e) the material of which the plate is made?

Figure 38-24 shows an electron moving through several regions where uniform electric potentials V have been set up. Rank the three regions according to the de Broglie wavelength of the electron there, greatest first.

The wavelength associated with the cutoff frequency for silver is 325nm. Find the maximum kinetic energy of electrons ejected from a silver surface by ultraviolet light of wavelength 254nm.

For the thermal radiation from an ideal blackbody radiator with a surface temperature of 2000 K, let Icrepresent the intensity per unit wavelength according to the classical expression for the spectral radiancy and Iprepresent the corresponding intensity per unit wavelength according to the Planck expression. What is the ratio Ic/Ipfor a wavelength of

(a) 400 nm (at the blue end of the visible spectrum) and

(b) 200 μm(in the far infrared)?

(c) Does the classical expression agree with the Planck expression in the shorter wavelength range or the longer wavelength range?

Show that ΔE/E, the fractional loss of energy of a photon during a collision with a particle of mass m, is given by

ΔEE=hf'mc2(1-cosϕ)
where E is the energy of the incident photon, f'is the frequency of the scattered photon, and ϕis defined as in Fig. 38-5.

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