Here we investigate the link between nand l, reflected in equation (7-33). (a) Show that if a classical point charge were held in a circular orbit about a fixed point charge by the Coulomb force, its kinetic energy would be given by KE=e2/8πε0r (b) According to equation (7-30), the rotational kinetic energy in hydrogen is h2l(l+1)/2mr2. Of course, ris not well defined for a “cloud”, but by usingr=n2a0argue that the condition that l not exceed n is reasonable.

Short Answer

Expert verified

(a) Kinetic energy of the point charge KE=e28πε0r.

(b) Here, should not exceed because sum of kinetic and rotational energy will be greater than the total energy.

Step by step solution

01

Given equations (Equation 7.33):

The azimuthal quantum number specifies the angular momentum as well as the shape of the atomic orbital.

|L|=l(l+1)×h;l=0,1,2,3..............(n-1)L=l(l+1)×h;I=0,1,2,3..............(n-1)

Where, nis the principal quantum number, Iis the Azimuthal quantum number, his Planck’s constant, Lis the Orbital angular momentum.

02

(a) Kinetic energy of the point charge:

As you know that, Coulomb force is,
F=q24πε0r2

Where, q is the charge on the objects, r is the distance,ε0

is the Permitivity of free space.

The acceleration of the charge is given by,

a=v2r

Where, v is the speed of the object and r is the radius of curvature

Write the equation for Newton’s second law of motion as given below.

F=ma

Where, F is the force, m is the mass, and a is the acceleration.

e24πε0r2=mv2re28πε0r=12mv2

Where, e is the charge on an electron.

The kinetic energy is

KE=12mv2KE=e28πε0r......(1)

03

(b) Rotational energy of the particle:

Rotational energy of the particle is,

E=l(l+1)h22mr2

Where, h is Planck’s constant.

E=I(I+1)h22mr1a01n2=I(I+1)h22mrme24πε0h21n2E=e22(4πεo)rI(I+1)n2

04

Conclusion:

From equations (1) and (2), you get, if I exceeds n, the rotational energy would exceed kinetic energy in circular orbit and the sum of the energies will be more than the ‘total energy’.

Hence, the argue that the condition thatI not exceed n is reasonable.

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Most popular questions from this chapter

Question: The 2D Infinite Well: In two dimensions the Schrödinger equation is

(2x2+2y2)ψ(x,y)=-2m(E-U)h2ψ(x,y)

(a) Given that U is a constant, separate variables by trying a solution of the form ψ(x,y)=f(x)g(y), then dividing byf(x)g(y) . Call the separation constants CX and CY .

(b) For an infinite well

role="math" localid="1659942086972" U={00<x<L,0<y<Lotherwise

What should f(x) and g(y) be outside the well? What functions should be acceptable standing wave solutions f(x) for g(y) and inside the well? Are CX and CY positive, negative or zero? Imposing appropriate conditions find the allowed values of CX and CY .

(c) How many independent quantum numbers are there?

(d) Find the allowed energies E .

(e)Are there energies for which there is not a unique corresponding wave function?

A supersonic: - plane travels al 420m/s. As this plane passes two markers a distance of 4.2km apart on the ground, how will the time interval registered on a very precise clock onboard me plane differ from 10s?

Supposea barrier qualifies as wide, and width are such that 2L2mU0h=5 ,

(a) Calculate the transmission probabilities whenEU0is 0.4and when it is0.6

(b) Repeat part (a), but for the case where 2L2mU0his50 instead of 5.

(C) Repeat part (a) but for 2L2mU0h=500.

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  1. Calculate the probability that an electron in such a state would be in the +z-hemisphere.(Note: Here, the cross terms so not integrate to 0 )
  2. What value of𝛕leads to the maximum probability, and what is the corresponding ratio ofψ2.0.0 andψ2.0.0 ?
  3. Using a computer , make a density (Shading) plot of the probability density-density versus r and𝛉- for the𝛕-value found in part (b).

Herewetake direct approach to calculate reflection probability for tunneling mean while obtaining relationship applying in further exercise.

  1. Write out thesmoothness condition oftheboundaries between regions for the E<U0barrier from them. Show that the coefficient H of reflected wave is given by,
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