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Consider the earth鈥搒un system as a gravitational analog to the hydrogen atom.

(a) What is the potential energy function (replacing Equation 4.52)? (Let be the mass of the earth, and M the mass of the sun.)

V(r)=-e2400,1r

(b) What is the 鈥淏ohr radius,鈥ag,for this system? Work out the actual number.

(c) Write down the gravitational 鈥淏ohr formula,鈥 and, by equating Ento the classical energy of a planet in a circular orbit of radius r0, show that n=r0/ag.From this, estimate the quantum number n of the earth.

(d) Suppose the earth made a transition to the next lower level(n-1) . How much energy (in Joules) would be released? What would the wavelength of the emitted photon (or, more likely, gravitation) be? (Express your answer in light years-is the remarkable answer a coincidence?).

Short Answer

Expert verified

(a)The potential energy function isV(r)=-GMmr

(b)The actual number isa=2.3410-138)m

(c)By the quantum number of the earthn=r0ag

(d) The wave length emitted by photons=1ly

Step by step solution

01

Given:

A potential function is a function of the position of an object. It can be defined only for conservative forces. A forces is conservative if the work it does on n object only on the initial and final position of the object and net on the path. The gravitational force is a conservative force.

The potential is given by:

V(r)=-e2401r

02

The potential energy function

Consdier the Earth-sun system as a gravitational analog to the hydrogen atom. The potential is:

V(r)=-GMmrm/r.

Where G is the gravitational constant, G=6.67310-11m3kg-1s-2

translates hydrogen results to the gravitational analogs.

03

(b) The “Bohr radius” is

The Bohr radius for the Earth can be found by replacinge2 bymM and1/4蟺蔚0 by G ,so we get:

ag=2GMm2

Substitute with the numerical values to get:

ag=1.054610-34Js26.672610-11m/kg.s21.98921030kg5.981024kg2ag=2.3410-138m

04

Step 4:(c) Finding the formula

Equation 4.70 (the allowed energies) is given by:

En=-m22(GMm)21n2

There are many items that could be altered to test the recreation of another. These changing quantities are called variables. A variables is any factor, trait, or condition that can exist in differing amounts or types. An experiment usually amounts or types, An experiment usually has three kinds of variables: independent, dependent, and controlled.

Ec=12mv2-GMmroGMmro2=mv2ro12mv2=GMm2ro

So,

cEc=-GMm2ro

=-m22(GMm)21n2n2=GMm22ro=roag

n=roag.

ro=earth-sundistance=1.4961011mn=1.49610112.3410-138=2.531074r0=earth-sundistance=1m.

05

(d) Wavelength of the emitted photon

The wavelength of the emitted photon

E=-G2M2m3221n+12-1n2.1n+12=1n21+1/n21n21-2n

So,

role="math" localid="1658389122151" 1(n+1)2-1n21n21-2n-1=-2n3;E=G2M2m32n3E=6.6710-1121.99103025.98102431.05510-3422.53743=2.0910-41J

Ep=E=hv=hc=31086.6310-34/2.0910-41=9.521015m

But1ly=9.461015m.that1ly,n2=GMm2ro/2=chE=c2蟺魔2n3G2M2m3=c2蟺魔2G2M2m3GMm2r023/2=c2r03GM

But(from(c))

v=GM/ro=2ro, where T is the period of the orbit (in this case one year),

so T=2ro3/GMand hence =cT(one light year).

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Most popular questions from this chapter

(a) Construct the spatial wave function ()for hydrogen in the state n=3,I=2,m=1.Express your answer as a function of r,,,anda(the Bohr radius) only鈥攏o other variables (p,z,etc.) or functions (p,v,etc.), or constants (A,c0,etc.), or derivatives, allowed (蟺 is okay, and e, and 2, etc.).

(b) Check that this wave function is properly normalized, by carrying out the appropriate integrals over, ,and.

(c) Find the expectation value of rsin this state. For what range of s (positive and negative) is the result finite?

A hydrogen atom starts out in the following linear combination of the stationary states n=2, l=1, m=1 and n=2, l=1, m=-1.

(r,0)=12(211+21-1)

(a) Construct(r,t)Simplify it as much as you can.

(b) Find the expectation value of the potential energy,<V>. (Does it depend on t?) Give both the formula and the actual number, in electron volts.

[Refer to. Problem 4.59for background.] Suppose A=B02(X^-yI^) and=Kz2, where B0 and Kare constants.

(a) Find the fields E and B.

(b) Find the allowed energies, for a particle of mass m and charge q , in these fields, Answer: E(n1,n2)=(n1+12)1+(n2+12)2,(n1,n2=0,1,2,...)where1qB0/mand22qK/m. Comment: If K=0this is the quantum analog to cyclotron motion;1 is the classical cyclotron frequency, and it's a free particle in the z direction. The allowed energies,(n1+12)1, are called Landau Levels.

Use separation of variables in Cartesian coordinates to solve infinite cubical well

V(x,y,z)=0if x,y,z are all between 0 to a;

V(x,y,z)=Otherwise

a) Find the stationary states and the corresponding energies

b) Call the distinct energies E1,E2,E3,..in the order of increasing energy. Findlocalid="1658127758806" E1,E2,E3,E4,E5,E6determine their degeneracies (that is, the number of different states that share the same energy). Comment: In one dimension degenerate bound states do not occur but in three dimensions they are very common.

c) What is the degeneracy of E14 and why is this case interesting?

(a)Derive Equation 4.131 from Equation 4.130. Hint: Use a test function; otherwise you're likely to drop some terms.

(b)Derive Equation 4.132 from Equations 4.129 and 4.131 .Hint : Use Equation 4.112.

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