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A hydrogenic atom consists of a single electron orbiting a nucleus with Z protons. (Z=1 would be hydrogen itself,Z=2is ionized helium ,Z=3is doubly ionized lithium, and so on.) Determine the Bohr energies En(Z), the binding energyE1(Z), the Bohr radiusa(Z), and the Rydberg constant R(Z)for a hydrogenic atom. (Express your answers as appropriate multiples of the hydrogen values.) Where in the electromagnetic spectrum would the Lyman series fall, for Z=2and Z=3? Hint: There’s nothing much to calculate here— in the potential (Equation 4.52) Ze2, so all you have to do is make the same substitution in all the final results.

V(r)=-e24πo0˙1r (4.52).

Short Answer

Expert verified

The electronic spectrum would be the Lyman seires fall, forz=2 andz=3 is at,z=2 is3.04×10-8m.

At z=3is1.35×10-8m.

Step by step solution

01

Given

The potential is given by:

V(r)=-e24πo0˙1r

02

Electronic spectrum

Consider a hydrogen, if irradiated with light it will be excited to another energy level. The energies of these photons are easily calculated from the Bohr energy formula:

En=-1n2me42h2(4ΤΤ0)2

Lyman lines range fromni=2toni=(withnf=1);

the wavelengths range from

03

Finding the electronic spectrum

1λ2=R1-14=34Rλ2=43R

Down to

role="math" localid="1658210586427" 1λ1=R1-1=RR1=1R

ForZ=2

λ1=14R=14(1.097×107)=2.28×10-8m

to

λ2=13R=3.04×10-8m,

Ultraviolet.

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Most popular questions from this chapter

(a) Use the recursion formula (Equation 4.76) to confirm that whenI=n-1 the radial wave function takes the form

Rn(n-1)=Nnrn-1e-r/na and determine the normalization constant by direct integration.

(b) Calculate 200a and <r2> for states of the form ψn(n-1)m·

(c) Show that the "uncertainty" in r(δr) is<r>/2n+1for such states. Note that the fractional spread in decreases, with increasing (in this sense the system "begins to look classical," with identifiable circular "orbits," for large ). Sketch the radial wave functions for several values of, to illustrate this point.

(a) Apply S-to|10 (Equation4.177 ), and confirm that you get 2|1-1

(b) Apply S±to[00 (Equation 4.178), and confirm that you get zero.

(c) Show that |11 and |1-1 (Equation 4.177) are eigenstates of S2, with the appropriate eigenvalue

(a) Prove that for a particle in a potential V(r)the rate of change of the expectation value of the orbital angular momentum L is equal to the expectation value of the torque:

ddt<L>=<N>

Where,

N=r×(VV)

(This is the rotational analog to Ehrenfest's theorem.)

(b) Show that d<L>/dt=0for any spherically symmetric potential. (This is one form of the quantum statement of conservation of angular momentum.)

a) Check that Arj1(kr)satisfies the radial equation with V(r)=0and I=1.

(b) Determine graphically the allowed energies for the infinite spherical well, when I=1. Show that for large n,En1(h2π2/2ma2)(n+1/2)2. Hint: First show that j1(x)=0x=tanx. Plot xandtanxon the same graph, and locate the points of intersection.

[Attempt this problem only if you are familiar with vector calculus.] Define the (three-dimensional) probability current by generalization of Problem 1.14:

J=ih2m(ψψ*-ψ*ψ)

(a) Show that satisfies the continuity equation .J=-t|ψ|2which expresses local conservation of probability. It follows (from the divergence theorem) that sJ.da=-ddtv|ψ|2d3rwhere Vis a (fixed) volume and is its boundary surface. In words: The flow of probability out through the surface is equal to the decrease in probability of finding the particle in the volume.

(b) FindJfor hydrogen in the staten=2,l=1,m=1 . Answer:

h64ma5re-r/asinθϕ^

(c) If we interpretmJas the flow of mass, the angular momentum is

L=m(r×J)d3r

Use this to calculate Lzfor the stateψ211, and comment on the result.

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