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Polyatomic Ideal Gases “Borrowed” from various sources on the web!

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Presentation on theme: "Polyatomic Ideal Gases “Borrowed” from various sources on the web!"— Presentation transcript:

1 Polyatomic Ideal Gases “Borrowed” from various sources on the web!

2 Energy level and its degeneracy
Energy levels are said to be degenerate, if the same energy level is obtained by more than one quantum mechanical state. They are then called degenerate energy levels. The number of quantum states at the same energy level is called the degree of degeneracy.

3 A molecular energy state is the sum of an electronic (e), nuclear (n), vibrational (v), rotational (r) and translational (t) component, such that:

4 The degree of freedom of movement
Translation: x,y,z F=3

5 Rotation For linear molecules, F=2 For non-linear molecules, F=3

6 Vibration A polyatomic molecule containing n atoms has 3n degrees of freedom totally. Three of these degrees of freedom can be assigned to translational motion of the center of mass, two or three to rotational motion. 3n-5 for a linear molecule; 3n-6 for a nonlinear molecule

7 CO2 has 3×3-5 = 4 degrees of freedom of vibration; nonlinear molecule of H2O has 3×3-6 = 3 degrees of freedom of vibration.

8 Translational particle
The expression for the allowed translational energy levels of a particle of mass m confined within a 3-dimensional box with sides of length a, b, c is Where h=6.626×10-34J·s,nx, ny, nz are integrals called quantum numbers. The number of them is 1,2,…∞ . If a=b=c, equation becomes

9 all energy levels except ground energy level are degenerate.
Example At 300K, kPa, 1 mol of H2 was added into a cubic box. Calculate the energy level εt,0 at ground state, and the energy difference between the first excited state and ground state.

10 Solution Take the H2 at the condition as an ideal gas, then the volume of it is
The mass of hydrogen molecule is

11 the energy difference is so small that the translational particles are excited easily to populate on different excited states, and that the energy changes of different energy levels can be think of as a continuous change approximately.

12 Rigid rotator (diatomic)
The equation for rotational energy level of diatomic molecules is : where J is rotational quantum number, I is the moment of inertia (转动惯量) μ is the reduced mass (折合质量), The degree of degeneracy is

13 One-dimensional harmonic oscillator
Where v quantum number,when v=0,the energy is called zero point energy. One dimensional harmonic vibration is non-degenerate.

14 Electron and atomic nucleus
The differences between energy levels of electron motion and nucleus motion are big enough to keep the electrons and nuclei stay at their ground states. Both degree of degeneracy, ge,0, for electron motion at ground state and degree of degeneracy, gn,0, for nucleus motion at ground state are different for different substances, but they are constant for a given substance.

15 Computations of the partition function
Some features of partition functions (1) at T=0, the partition function is equal to the degeneracy of the ground state. (2) When T is so high that for each term εi/kT=0, (3) factorization property If the energy is a sum of those from independent modes of motion, then

16 The partition functions for 5 mode motions are expressed as

17

18 Zero-point energy zero-point energy is the energy at ground state or the energy as the temperature is lowered to absolute zero. Suppose some energy level of ground state is ε0, and the value of energy at level i is εi, the energy value of level i relative to ground state is Taking the energy value at ground state as zero, we can denote the partition function as q0.

19 Since εt,0≈0, εr,0=0, at ordinary temperatures.

20 The vibrational energy at ground state is
therefore the number of distribution in any levels does not depend on the selection of zero-point energy.

21 Translational partition function
Energy level for translation The partition function

22

23 Take qt,x as an example For a gas at ordinary temperature α2<<1, the summation converts into an integral.

24 From mathematic relations in Appendix
In like manner,

25 Example Calculate the molecular partition function q for He in a cubical box with sides 10cm at 298K. Solution The volume of the box is V=0.001m3. The mass of the He molecule is 0.004/(6.022×1023)=6.6466×10-27kg. Substituting these numbers and the proper natural constants, we have

26 For ideal gas,

27 Rotational partition function
The rotational energy of a linear molecule is given by εr = J(J+1)h2/8π2I and each J level is 2J+1 degenerate. define the characteristic rotational temperature

28 Θr<<T at ordinary temperature, The summation can be approximated by an integral
Let J(J+1)=x, hence J(2J+1)dJ=dx, then

29 For a homonuclear diatomic molecule, such as O2, it comes back to the same state after only 180o rotation. where σ is called the symmetry number. σ is the number of indistinguishable orientations that a molecule can exhibit by being rotated around symmetry axis. It is equal to unity for heteronuclear diatomic molecules and is equal to 2 for mononuclear diatomic molecules. For HCl, σ = 1; and for Cl2, σ = 2.

30 Vibrational partition function
Vibrational energies for one dimensional oscillator are Vibration is non-degenerate, g=1. The partition function is

31 Define the characteristic vibrational temperature

32 Characteristic vibrational temperatures are usually several thousands of Kelvins except for very low frequency vibrational modes. we cannot use integral instead of summation in the calculation of vibrational partition function.

33 At low T, , ,according to mathematics

34 take the ground energy level as zero,
For NO, the characteristic vibrational temperature is 2690K. At room temperature Θv/T is about 9; the , indicating that the vibration is almost in the ground state.

35 Electronic and nuclear partition function
Energy difference is large, so electrons are generally at ground state, all terms except first one in the summation expression is negligible.

36 If the quantum number of total angular momentum for electronic motion is j, the degeneracy is (2j+1). Then the electronic partition function can be written as A rare exception is halide atoms and NO molecule. The difference between the ground state and the first excited state of them are not so large, the second term in the summation has to be considered.

37 Nuclear motion Nuclear motion is always in the ground state at ordinary chemical and physical process because of large energy difference between ground and first excited state. Its partition function has the form of where I is a quantum number of nuclear spin.

38 Thermodynamic energy and partition function

39 Thermodynamic energy and partition function
Substitute this equation into equation (8.48), we have

40 Substitute the factorization of partition function for q
Only qt is the function of volume, therefore

41 If the ground energy is specified to be zero, then

42 It tells us that the thermodynamic energy depends on the zero point energy. Nε0 is the total energy of system when all particles are localized in ground state. It (denoted as U0) can also be thought of as the energy of system at 0K. Then,

43 U0 can be expressed as the sum of different energies

44 The calculation of (1) The calculation of

45 The calculation of The degree of freedom of rotation for diatomic or linear molecules is 2, the contribution to the energy of every degree is also ½ RT for a mole substance.

46 The calculation of Usually, Θv is far greater than T, the quantum effect of vibration is very obvious. When Θv/T>>1, Showing that the vibration does not have contribution to thermodynamic energy relative to ground state.

47 If the temperature is very high or theΘv is very small, thenΘv/T<<1, the exponential function can be expressed as

48 For monatomic gaseous molecules we do not need to consider the rotation and vibration, and the electronic and nuclear motions are supposed to be in their ground states. The molar thermodynamic energy is

49 For diatomic gaseous molecules vibration and rotation must be considered. If only lowest vibrational levels are occupied, the molar thermodynamic energy is

50 If all vibrational energies are equally accessible, the molar thermodynamic energy for vibration is
The molar thermodynamic energy for diatomic molecules is then

51 Heat capacity and partition function
The molar heat capacity, CV,m, can be derived from the partition function. Replace q with We can see from above equations that heat capacity does not depends on the selection of zero point of energy.

52 Electrons and nucleus are in ground state

53 The calculation of CV,t, CV,r and CV,v

54 (2) The calculation of CV,r
If the temperature is very low, only the lowest rotation state is occupied and then rotation does not contribute to the heat capacity.

55 The calculation of CV,v

56 Generally, Θv/T>>1, equation becomes
It shows that under general conditions, the contribution to heat capacity of vibration is approximately zero.

57 When temperature is high enough,

58 In gases, all three translational modes are active and their contribution to molar heat capacity is
The number of active rotational modes for most linear molecules at normal temperature is 2 In most cases, vibration has no contribution to the heat capacity,

59 Entropy and partition function
8.8.1 Entropy and microstate Boltzmann formula k = ×10-23 J K-1 As the temperature is lowered, the Ω, and hence the S of the system decreases. In the limit T→0, Ω=1, so lnΩ=0, because only one configuration is compatible with E=0. It follows that S→0 as T→0, which is compatible with the third law of thermodynamics.

60 For example When N approaches infinity,

61 Entropy and partition function
For a non-localized system, the most probable distribution number is Using Stirling equation ln N!=N ln N - N and Boltzmann distribution expression

62 We have,

63 For localized system Entropy does not depend on the selection of zero point energy .

64 Factorizing the partition function into different modes of motions and using
We can give

65 For identical particle system, entropies for every mode of motion can be expressed as

66 Calculation of statistical entropy
At normal condition electronic and nuclear motions are in ground state, and in general physical and chemical process the contribution to the entropy by two modes of motion keeps constant. Therefore only translational, rotational and vibrational entropies are involved in computation of statistical entropy.

67 (1) Calculation of St

68 For ideal gases, the Sackur–Tetrode equation is used to calculate the molar translational entropy.

69 (2) Calculation of Sr For linear molecules
When all rotational energy levels are accessible We obtain

70 (3) Calculation of Sv Substitute Into the following equation

71 residual entropy in some the experimental entropy is less than the calculated value. One explanation to this discrepancy is that the experimental system does not reach a real state of equilibrium. In other words, some disorder is present in the solid even at T = 0 K. In this case, the entropy at T = 0 is then greater than zero. This difference in entropy is called the residual entropy.

72 Other thermodynamic functions and partition functions
A, G, H and q

73


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