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Evaluate the integral in equation N=2π2πmh23/2V0ϵdϵeϵ/kT-1numerically, to confirm the value quoted in the text.

Short Answer

Expert verified

The integral in equationN=2π2πmh23/2V0ϵdϵeϵ/kT-1is evaluated in simpler form.

Step by step solution

01

Step 1. Given information 

The total number of atoms, Nin Bose-Einstein distribution over all the states is given as:

N=2π2πmh232V0εdεeεkT-1

=2π2πmkTh232V0xex-1dx

Where,

h= Planck's constant,

k= Boltzmann's constant,

V= volume of the box,

ε= energy of the atom for higher energy level,

T= temperature,

m= mass of the atom,

x=εkTis a new variable

02

Step 2. Calculating the integral ∫0∞xdxex-1

Now,

0xdxex-1=0xe-x1-e-xdx

=0x12e-x1-e-x-1

=0x12e-x1+e-x+e-2x+e-3x+dx

=0x12e-x+e-2x+e-3x+e-4x+dx

=0x12k=0e-(k+1)xdx

=k=00x12e-(k+1)xdx

03

Step 3. Solving the integral ∫0∞x12e-(k+1)xdx using the formula  ∫0∞xne-axdx=(n!)a-(n+1)

Therefore,

0x12e-(k+1)x=12!(k+1)-12+1

As we know 12!=Γ12+1, and also Γ12=π

Now,

Γ12+1=12Γ12

=12π

Substituting the value of 12!=12πin the equation 0x12e-(k+1)x=12!(k+1)-12+1we get,

0x12e-(k+1)x=π2(k+1)-32

04

Step 4.  Substituting the value of π2(k+1)-32=∫012x-(k+1)x in the equation

we get,

0xex-1dx=k=0π2(k+1)-32

=π2k=0(k+1)-32

=π21+1232+1332+1432+..

=π2ζ32

05

Step 5. Substitute the value of  ζ32=∑k=1∞1k32=2.612 in the equation 

we get,

0xex-1dx=π2(2.612)

06

Step 6.  Substituting the value of π2(2.612)=∫0∞x12ex-1dx in the equation N=2π2πmkTh232V∫0∞xex-1dx

N=2π2πmkTh232Vπ2(2.612)

=2.6122πmkTh232V

The equation N=2π2πmh23/2V0ϵdϵeϵ/kT-1is evaluated in simpler form.

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Most popular questions from this chapter

The heat capacity of liquid H4ebelow 0.6Kis proportional to T3, with the measured valueCV/Nk=(T/4.67K)3. This behavior suggests that the dominant excitations at low temperature are long-wavelength photons. The only important difference between photons in a liquid and photons in a solid is that a liquid cannot transmit transversely polarized waves-sound waves must be longitudinal. The speed of sound in liquid He4is 238m/s, and the density is 0.145g/cm3. From these numbers, calculate the photon contribution to the heat capacity ofHe4in the low-temperature limit, and compare to the measured value.

(a) As usual when solving a problem on a computer, it's best to start by putting everything in terms of dimensionless variables. So define t=T/Tcc=μ/kTc,andx=ϵ/kTc. Express the integral that defines μ, equation 7.122, in terms of these variables. You should obtain the equation

(b) According to Figure 7.33, the correct value of cwhen T=2Tcis approximately -0.8. Plug in these values and check that the equation above is approximately satisfied.

(c) Now vary μ, holding Tfixed, to find the precise value of μfor . Repeat for values of T/Tcranging from 1.2up to 3.0, in increments of 0.2. Plot a graph of μas a function of temperature.

Each atom in a chunk of copper contributes one conduction electron. Look up the density and atomic mass of copper, and calculate the Fermi energy, the Fermi temperature, the degeneracy pressure, and the contribution of the degeneracy pressure to the bulk modulus. Is room temperature sufficiently low to treat this system as a degenerate electron gas?

In a real hemoglobin molecule, the tendency of oxygen to bind to a heme site increases as the other three heme sites become occupied. To model this effect in a simple way, imagine that a hemoglobin molecule has just two sites, either or both of which can be occupied. This system has four possible states (with only oxygen present). Take the energy of the unoccupied state to be zero, the energies of the two singly occupied states to be -0.55eV, and the energy of the doubly occupied state to be -1.3eV(so the change in energy upon binding the second oxygen is -0.75eV). As in the previous problem, calculate and plot the fraction of occupied sites as a function of the effective partial pressure of oxygen. Compare to the graph from the previous problem (for independent sites). Can you think of why this behavior is preferable for the function of hemoglobin?

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