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?

Short Answer

Expert verified

Occupancy rises gradually for smaller values of P. This shows that with cooperative binding, hemoglobin reacts with oxygen much fast in cells when P is small.

Step by step solution

01

Step 1. Formula Gibb's Factor

Gibb's Factor is given by formula:

Gibb'sFactor=e-(ε-nμ)kT

where, kis Boltzmann's constant, Tis temperature, μis chemical potential, and εis energy of state .

As, in hemoglobin molecule, oxygen can have four different states given by:

localid="1647144603783" εo=0eVε1=-0.55eV(twosinglyoccupied)ε2=-1.3eV

The average number of oxygen molecules is given by,

N=SN(S)=2e-(ε1-μ)kTZ+2e-(ε2-2μ)kTZ

02

Step 2. Formula occupancy

Occupancy of system is given by:

n=NZ=1Ze-(ε1-μ)kT+-(ε2-2μ)kT

Chemical Potential formula is :

μ=-kT×lnVZinNνQ

Substitute VN=kTPin above formula,

μ=-kT×lnkTZinPνQ

eμkT=PνQkTZin

Gibb's Factor can be written as:

e-(ε1-μ)kT=e-ε1kT×PνQkTZin=PνQkTZineε1kT=PPo

03

Step 3. Calculation

Oxygen molecule quantum volume is:

νQ=h2πmkT3

Substitute the values of the variables in above formula,

νQ=6.63×10-34J·s2π(32×1.66×10-27kg)(1.38×10-23J/K)(310K)3=5.3×10-33m3

In equation, n=1Ze-(ε1-μ)kT+-(ε2-2μ)kT

Substitute eεKT=1790 and Po=2.03barat room temperature,

n=P2.03+1790P2.0321+P2.03+1790P2.032

Occupancy in this model is nearly 100%near lungs given P=0.20bar

04

Step 4. Table and Graph

The table is created between Pressure Pand fraction of occupied sites:

P
n
0.01
0.0461
0.02
0.1554
0.03
0.2899
0.04
0.4204
0.05
0.5332
0.06
0.6257
0.07
0.7001
0.08
0.7598
0.09
0.8080

The graph between fraction of occupied sites and oxygen partial pressure is created as,

We see that the occupancy rises gradually for smaller values of P. This shows that with cooperative binding, hemoglobin reacts with oxygen much fast in cells when Pis small.

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Most popular questions from this chapter

Carry out the Sommerfeld expansion for the energy integral (7.54), to obtain equation 7.67. Then plug in the expansion for μto obtain the final answer, equation 7.68.

For a brief time in the early universe, the temperature was hot enough to produce large numbers of electron-positron pairs. These pairs then constituted a third type of "background radiation," in addition to the photons and neutrinos (see Figure 7.21). Like neutrinos, electrons and positrons are fermions. Unlike neutrinos, electrons and positrons are known to be massive (ea.ch with the same mass), and each has two independent polarization states. During the time period of interest, the densities of electrons and positrons were approximately equal, so it is a good approximation to set the chemical potentials equal to zero as in Figure 7.21. When the temperature was greater than the electron mass times c2k, the universe was filled with three types of radiation: electrons and positrons (solid arrows); neutrinos (dashed); and photons (wavy). Bathed in this radiation were a few protons and neutrons, roughly one for every billion radiation particles. the previous problem. Recall from special relativity that the energy of a massive particle is ϵ=(pc)2+mc22.

(a) Show that the energy density of electrons and positrons at temperature Tis given by

u(T)=0x2x2+mc2/kT2ex2+mc2/kT2+1dx;whereu(T)=0x2x2+mc2/kT2ex2+mc2/kT2+1dx

(b) Show that u(T)goes to zero when kTmc2, and explain why this is a

reasonable result.

( c) Evaluate u(T)in the limit kTmc2, and compare to the result of the

the previous problem for the neutrino radiation.

(d) Use a computer to calculate and plot u(T)at intermediate temperatures.

(e) Use the method of Problem 7.46, part (d), to show that the free energy

density of the electron-positron radiation is

FV=-16π(kT)4(hc)3f(T);wheref(T)=0x2ln1+e-x2+mc2/kT2dx

Evaluate f(T)in both limits, and use a computer to calculate and plot f(T)at intermediate

temperatures.

(f) Write the entropy of the electron-positron radiation in terms of the functions

uTand f(T). Evaluate the entropy explicitly in the high-T limit.

Consider a Bose gas confined in an isotropic harmonic trap, as in the previous problem. For this system, because the energy level structure is much simpler than that of a three-dimensional box, it is feasible to carry out the sum in equation 7.121 numerically, without approximating it as an integral.*

(a) Write equation 7.121 for this system as a sum over energy levels, taking degeneracy into account. Replace Tandμwith the dimensionless variables t=kT/hfandc=μ/hf.

(b) Program a computer to calculate this sum for any given values of tandc. Show that, for N=2000, equation 7.121 is satisfied at t=15provided that c=-10.534. (Hint: You'll need to include approximately the first 200 energy levels in the sum.)

(c) For the same parameters as in part (b), plot the number of particles in each energy level as a function of energy.

(d) Now reduce tto 14 , and adjust the value of cuntil the sum again equals 2000. Plot the number of particles as a function of energy.

(e) Repeat part (d) for t=13,12,11,and10. You should find that the required value of cincreases toward zero but never quite reaches it. Discuss the results in some detail.

Explain in some detail why the three graphs in Figure 7.28 all intercept the vertical axis in about the same place, whereas their slopes differ considerably.

Starting from equation 7.83, derive a formula for the density of states of a photon gas (or any other gas of ultra relativistic particles having two polarisation states). Sketch this function.

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