EBK AN INTRODUCTION TO MODERN ASTROPHYS
EBK AN INTRODUCTION TO MODERN ASTROPHYS
2nd Edition
ISBN: 9781108390248
Author: Carroll
Publisher: YUZU
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Chapter 8, Problem 8.10P

(a)

To determine

To compare the ratios NII/NI and NIII/NII for the temperatures of 5000K, 15,000K, and 25,000K.

(a)

Expert Solution
Check Mark

Answer to Problem 8.10P

For all the given temperatures, (NII/NI)(NIII/NII).

Explanation of Solution

In the case under consideration, the subscript I stands for neutral helium, II stands for singly ionized helium, and III sands for the completely ionized helium atom.

Given that the ionization energies χI=24.6eV, χII=54.4eV and the partition functions are ZI=1, ZII=2, and ZIII=1. The electron pressure is given as Pe=20Nm2.

Write the expression for the Saha equation in terms of the electron pressure.

  Ni+1Ni=2kTZi+1PeZi(2πmekTh2)3/2eχi/kT        (I)

Here, k is the Boltzmann constant, Pe is the electron pressure, T is the absolute temperature, me is the mass of electron, and h is the Planck’s constant.

Rewrite equation (I) for determining the required ratios.

  NIINI=2kTZIIPeZI(2πmekTh2)3/2eχI/kT        (II)

  NIIINII=2kTZIIIPeZII(2πmekTh2)3/2eχII/kT        (III)

Conclusion:

Substitute 1.38×1023JK1 for k, 5000K for T, 1 for ZI, 2 for ZII, 20Nm2 for Pe, 9.1×1031kg for me, 6.626×1034Js for h, and 24.6eV for χI in equation (II) to find the ratio NII/NI corresponding to temperature 5000K.

NIINI=2(1.38×1023JK1)(5000K)(2)(20Nm2)(1)(2π(9.1×1031kg)(1.38×1023JK1)(5000K)(6.626×1034Js)2)3/2e(24.6eV)(1.38×1023JK1)(5000K)=(1.38 ×1020)(8.518266682 ×1026)e(24.6eV×1.6×1019J1eV)(1.38×1023JK1)(5000K)=1.9×1018

Similarly the values of the ratios NII/NI and NIII/NII can be calculated for different temperatures and the results are tabulated below.

T(K)NII/NINIII/NII
50001.9×10184.3×1049
15,0009.9×1012.4×1011
25,0007.2×1031.8×103

From the table it is clear that the ratio (NII/NI)(NIII/NII) for all the given temperatures.

Therefore, for all the given temperatures, (NII/NI)(NIII/NII).

(b)

To determine

To show that NII/Ntotal=NII(NI+NII+NIII) can be expressed in terms of the ratios NII/NI and NIII/NII.

(b)

Expert Solution
Check Mark

Answer to Problem 8.10P

The ratio NIINtotal=NII(NI+NII+NIII) can be expressed in terms of the ratios NII/NI and NIII/NII as NIINtotal=NII/NI(1+(NII/NI)+(NIII/NII)(NII/NI)).

Explanation of Solution

Given ratio expression is;

  NIINtotal=NII(NI+NII+NIII) (IV)

Take NI as a common factor from the denominator in equation (IV).

  NIINtotal=NIINI(1+NIINI+NIIINI)NIINtotal=(NIINI)(1+NIINI+NIIINI)        (V)

Multiply and divide the third term in the denominator in equation (V) with NII.

  NIINtotal=(NIINI)(1+NIINI+NIIINI×NIINII)NIINtotal=(NIINI)(1+NIINI+(NIIINII)(NIINI))        (VI)

Equation (VI) is the form of the equation (IV) written in terms of the ratios NII/NI and NIII/NII.

Conclusion:

Therefore, the ratio NIINtotal=NII(NI+NII+NIII) can be expressed in terms of the ratios NII/NI and NIII/NII as NIINtotal=NII/NI(1+(NII/NI)+(NIII/NII)(NII/NI)).

(c)

To determine

To plot the graph of NII/Ntotal.

(c)

Expert Solution
Check Mark

Answer to Problem 8.10P

The plot the graph of NII/Ntotal is shown in Figure 1.

Explanation of Solution

The expression for NII/Ntotal written in terms of NII/NI and NIII/NII is given in equation (VI).

  NIINtotal=(NIINI)(1+NIINI+(NIIINII)(NIINI))

From the obtained values of NII/NI and NIII/NII from part (a), the term (NIIINII)(NIINI) can be neglected since they does not contribute significant change to the value of NII/Ntotal for the temperature range 5000K to 25,000K. Thus, equation (VI) becomes;

  NIINtotal=(NIINI)(1+NIINI)        (VII)

With the given values of electron pressure, ionization energies and partition functions for the neutral helium atom and singly ionized helium atom, the ratio NII/NI can be determined for a range of temperatures in between 5000K to 25,000K as shown in part (a). These values can be plugged in to equation (VII) and hence the plot of NII/Ntotal will be obtained.

Conclusion:

The graph of NII/Ntotal is shown in Figure 1 below.

EBK AN INTRODUCTION TO MODERN ASTROPHYS, Chapter 8, Problem 8.10P

From the graph it can be noted that when the temperature corresponding to the partial ionization of the neutral helium is about 15,000K or 1.5×104K.

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