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Suppose you could find a solutionψ(r1,r2,...,rz)to the Schrödinger equation (Equation 5.25), for the Hamiltonian in Equation 5.24. Describe how you would construct from it a completely symmetric function, and a completely anti symmetric function, which also satisfy the Schrödinger equation, with the same energy.

role="math" localid="1658219144812" H^=j=1Z-ħ22mj2-14πo,0Ze2rj+1214πo,0j1Ze2rj-rk (5.24).

role="math" localid="1658219153183" H^ψ=E (5.25).

Short Answer

Expert verified

ψ-=ψr1,r2,r3-ψr1,r2,r3-ψr1,r2,r3+ψr2,r3,r1-ψr3,r2,r1+r3,r1,r2-ψr1,r3,r2=0

Step by step solution

01

Definition of Schrodinger equation

The fundamental equation for characterizing quantum mechanical phenomena is the Schrodinger equation. It is a partial differential equation that illustrates how a physical system's wave function changes over time. The electron is a wave in the three-dimensional space surrounding the nucleus.

02

Finding a solution to Schrodinger equation

ψ±=Aψr1,r2,r3,..rz±ψr2,r1,r3,..,rz+ψr2,r3,r1,..,rz+etc.,

Where etc. runs over all permutations of the arguments,r1,r2,..,rz with a + sign for all even permutations (even number of transpositions rirjstarting from r1,r2,..,rzand ± for all odd permutations (+ for bosons, – for fermions).

At the end of the process, normalize the result to determine A. (Typically A=1/Z!, but this may not be right if the starting function is already symmetric under some interchanges.)

If ψ is symmetric in the first two arguments (or any other pair), the anti symmetric combination is zero.

For example, if Z = 3,

ψ-=ψψr1,r2,r3-ψr2,r1,r3+ψr2,r3,r1-r3,r1,r2+ψr3,r1,r2-ψr1,r3,r2=0

(They cancel in pairs).

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Most popular questions from this chapter

Derive the Stefan-Boltzmann formula for the total energy density in blackbody radiation

EV=(π2kB415ħ3C3)T4=7.57×10-16Jm-3K-4T4

Suppose we use delta function wells, instead of spikes (i.e., switch the sign ofin Equation 5.57). Analyze this case, constructing the analog to Figure 5.6. this requires no new calculation, for the positive energy solutions (except that β is now negative; use β=-1.5 for the graph), but you do need to work out the negative energy solutions (letk-2mE/handZ-ka,forE<0) and , for). How many states are there in the first allowed band?

In view ofProblem 5.1, we can correct for the motion of the nucleus in hydrogen by simply replacing the electron mass with the reduced mass.

(a) Find (to two significant digits) the percent error in the binding energy of hydrogen (Equation 4.77) introduced by our use of m instead of μ.

E1=-m2h2e24π'2=-13.6eV(4.77).

(b) Find the separation in wavelength between the red Balmer lines n=3n=2for hydrogen and deuterium (whose nucleus contains a neutron as well as the proton).

(c) Find the binding energy of positronium (in which the proton is replaced by a positron—positrons have the same mass as electrons, but opposite charge).

(d) Suppose you wanted to confirm the existence of muonic hydrogen, in which the electron is replaced by a muon (same charge, but 206.77 times heavier). Where (i.e. at what wavelength) would you look for the “Lyman-α” line n=2n=1?.

Certain cold stars (called white dwarfs) are stabilized against gravitational collapse by the degeneracy pressure of their electrons (Equation 5.57). Assuming constant density, the radius R of such an object can be calculated as follows:

P=23EtotV=23h2kF510π2m=(3π2)2/3h25mp5/3(5.57)

(a) Write the total electron energy (Equation 5.56) in terms of the radius, the number of nucleons (protons and neutrons) N, the number of electrons per nucleon d, and the mass of the electron m. Beware: In this problem we are recycling the letters N and d for a slightly different purpose than in the text.

Etot=h2V2π2m0kFK4dk=h2kF5V10π2m=h2(3π2Nd)5/310π2mV-2/3(5.56)

(b) Look up, or calculate, the gravitational energy of a uniformly dense sphere. Express your answer in terms of G (the constant of universal gravitation), R, N, and M (the mass of a nucleon). Note that the gravitational energy is negative.

(c) Find the radius for which the total energy, (a) plus (b), is a minimum.

R=(9π4)2/3h2d5/3GmM2N1/3

(Note that the radius decreases as the total mass increases!) Put in the actual numbers, for everything except , using d=1/2 (actually, decreases a bit as the atomic number increases, but this is close enough for our purposes). Answer:

(d) Determine the radius, in kilometers, of a white dwarf with the mass of the sun.

(e) Determine the Fermi energy, in electron volts, for the white dwarf in (d), and compare it with the rest energy of an electron. Note that this system is getting dangerously relativistic (seeProblem 5.36).

The ground state of dysprosium (element 66, in the 6th row of the Periodic Table)

is listed as Is5. What are the total spin, total orbital, and grand total angular

momentum quantum numbers? Suggest a likely electron configuration for

dysprosium.

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