Step 1: Detector Calibration
The detector signal in a TPD experiment is calibrated by injecting a known volume of the probe gas as a pulse into an inert gas stream that flows directly to the detector, bypassing the sample. This is accomplished using a GC valve equipped with a calibrated GC loop of known volume, as shown schematically in Figure 2 of the source document.
The calibration pulse establishes a reference: a detector signal of X counts corresponds to a volume Y of chemisorbing gas. This gas volume is then converted to micromoles using the ideal gas law. The calibration factor allows the TPD desorption signal, once integrated over time, to be expressed as gas uptake in micromoles per gram of catalyst.
Step 2: Calculating Metal Dispersion
With the uptake in micromoles per gram of catalyst established, metal dispersion is calculated from Equation 1:
Dispersion (%) = [Gas Uptake (micromol/g) x (10^-6 mol/micromol) x Stoichiometric Factor (SF) x Molecular Weight (g/mol)] / Metal Loading (wt%) x 100%
The stoichiometric factor (SF) is defined as the number of adsorbed species per binding site. For CO adsorbing in a linear geometry on one site, SF = 1. For CO in a bridging geometry spanning two sites, SF = 0.5.
Dispersion is the fraction of total metal atoms that are surface-exposed. A catalyst with 100 percent dispersion has every metal atom accessible for chemisorptive bonding. A catalyst with lower dispersion has metal atoms buried within crystallites or agglomerated in larger particles where they are inaccessible to reactant molecules. Higher dispersion means more efficient use of the metal in a catalytic reaction.
Step 3: Converting Dispersion to Specific Surface Area
Dispersion alone does not give a surface area in physical units. The conversion requires knowledge of the surface area of a single metal atom, which allows calculation of the maximum theoretical surface area on a per-gram-of-metal basis. This quantity is called Sg.
The specific surface area (Asp) of the catalyst sample is then:
Asp = Sg x D (Equation 3)
Where D is the dispersion measured in Equation 1. This gives the actual surface area per gram of metal present in the catalyst, accounting for the fraction of atoms that are surface-exposed.
Step 4: The Spherical Crystallite Model
To convert surface area into a physical crystallite diameter, a crystallite geometry must be assumed. The most common assumption is a sphere with volume V = (pi/6)d^3 and surface area A = pi d^2. Dividing volume by surface area gives:
V/A = d/6 (Equation 2)
The specific volume of the metal sample is the inverse of its bulk density (Vsp = 1/rho). Dividing Vsp by Asp gives the volume-to-surface-area ratio for the sample:
Vsp/Asp = V/A (Equation 4)
Setting this equal to d/6 from the spherical model and solving for crystallite diameter gives the final expression:
d = 6 / (rho x Sg x D) (Equation 6)
Where rho is the metal density, Sg is the maximum surface area per gram of metal, and D is the measured dispersion.
Step 5: Worked Numerical Example for Nickel
For a supported nickel catalyst with a measured dispersion of 33 percent (D = 0.33), the average crystallite diameter is calculated using the physical constants for nickel from Table 1:
Nickel density (rho): 8.9 g/cm3, converted to atomic scale units: rho = 8.9 x (cm3 / 10^8 Angstrom)^3 = 8.9 x 10^-24 g/Angstrom^3
Maximum surface area of Ni (Sg): 667 m2/g, converted: Sg = 667 m2/g x (10^10 Angstrom/m)^2 = 6.67 x 10^22 Angstrom^2/g
Crystallite diameter (Equation 9): d = (6 x Angstrom^3 x g) / [(8.9 x 10^-24 g) x (6.67 x 10^22 Angstrom^2) x 0.33]
Therefore, d = 31 Angstroms.
This result means that a nickel catalyst with 33 percent dispersion has average crystallite diameters of approximately 31 Angstroms (3.1 nm), calculated directly from the TPD uptake and the physical properties of nickel.