Thermal desorption spectroscopy

Thermal desorption spectroscopy (TDS), also known as temperature programmed desorption (TPD) is the method of observing desorbed molecules from a surface when the surface temperature is increased. Many researchers prefer the name TPD because it is not a spectroscopic method.

Desorption

When molecules or atoms come in contact with a surface, they adsorb onto it, minimizing their energy by forming a bond with the surface. The binding energy varies with the combination of the adsorbate and surface. If the surface is heated, at one point, the energy transferred to the adsorbed species will cause it to desorb. The temperature at which this happens is known as the desorption temperature. Thus TDS shows information on the binding energy.

Measurement

Since TDS observes the mass of desorbed molecules, it shows what molecules are adsorbed on the surface. Moreover, TDS recognizes the different adsorption conditions of the same molecule from the differences between the desorption temperatures of molecules desorbing different sites at the surface, e.g. terraces vs. steps. TDS also obtains the amounts of adsorbed molecules on the surface from the intensity of the peaks of the TDS spectrum, and the total amount of adsorbed species is shown by the integral of the spectrum.

To measure TDS, one needs a mass spectrometer, such as a quadrupole mass spectrometer or a time-of-flight (TOF) mass spectrometer, under ultrahigh vacuum (UHV) conditions. The amount of adsorbed molecules is measured by increasing the temperature at a heating rate of typically 2 K/s to 10 K/s. Several masses may be simultaneously measured by the mass spectrometer, and the intensity of each mass as a function of temperature is obtained as a TDS spectrum.

The heating procedure is often controlled by the PID control algorithm, with the controller being either a computer or specialised equipment such as a Eurotherm.

Other methods of measuring desorption are Thermal Gravimetric Analysis (TGA) or using infrared detectors, thermal conductivity detectors etc.

Quantitative Interpretation of TDS data

TDS Spectrum 1 A Thermal Desorption Spectrum of NO absorbed on Platinum-Rhodium (100) single crystal. The unit of the x-axis is temperature in Kelvin, the unit of the y-axis is an arbitrary unit, in fact the intensity of a mass spectrometer measurement.
TDS Spectrum 2 A Thermal Desorption Spectrum of NO absorbed on Platinum-Rhodium (100) single crystal. The spectra of several NO coverages are combined in one spectrum. The unit of the x-axis is temperature in Kelvin, the unit of the y-axis is an arbitrary unit, in fact the intensity of a mass spectrometer measurement.

TDS spectrum 1 and 2 are typical examples of a TDS measurement. Both TDS are examples of NO desorbing from a single crystal in high vacuum. The crystal was mounted on a titanium filament and heated with current. The desorbing NO was measured using a mass spectrometer monitoring the atomic mass of 30.

Before 1990 analysis of a TDS spectrum was usually done using a so-called simplified method; the "Redhead" method,[1] assuming the exponential prefactor and the desorption energy to be independent of the surface coverage. After 1990 and with use of computer algorithms TDS spectra were analyzed using the "complete analysis method" [2] or the "leading edge method".[3] These methods assume the exponential prefactor and the desorption energy to be dependent of the surface coverage. Several available methods of analyzing TDS are described and compared in an article by A.M. de JONG and J.W. NIEMANTSVERDRIET [4]

Theoretical Introduction

Thermal desorption is described based on the Arrhenius equation.


r(\sigma) = -\frac{\mathrm{d}\sigma}{\mathrm{d}t} = v(\sigma) \sigma^n * e^{-E_{\mathrm{act}}(\sigma)/RT}


where

 r(\sigma) the desorption rate [mol/cm2 sec] as a function of  \sigma
 n order of desorption
 \sigma surface coverage
 v(\sigma) pre-exponential factor [Hz] as a function of  \sigma
 E_{\mathrm{act}}(\sigma) activation energy of desorption [kJ/mol] as a function of  \sigma
 R gas constant [J K−1 mol−1]
 T temperature [K]

This equation is difficult in daily practice while several variables are a function of the coverage and influence each other.[5] The “complete analysis method” calculates the pre-exponential factor and the activation energy at several coverages. This calculation can be simplified. First we assume the pre-exponential factor and the activation energy to be independent of the coverage.

We also assume a linear heating rate:
(equation 1)


\begin{align}
 T(t) = T_0 + (\beta *t)
\end{align}

where:

	\beta the heating rate in [K/s]
T_0 the start temperature in [K]
t the time in [s]

We assume that the pump rate of the system is indefinitely large, thus no gasses will absorb during the desorption. The change in pressure during desorption is described as:
(equation 2)


\frac{\mathrm{d}P}{\mathrm{d}t} + P/\alpha = \frac{\mathrm{d}(a*r(t))}{\mathrm{d}t}

where:

 P the pressure in the system
 t the time in [s]

where:

 a = A/KV

where:

 A the sample surface [m2]
 K  a constant
 V volume of the system [m3]

where:

 r(t) the desorption rate [mol/cm2 sec]

where:

 \alpha = V/S

where:

 S the pump rate
 V volume of the system [m3]

We assume that S is indefinitely large so molecules do not re-adsorp during desorption process and we assume that 
P/\alpha is indefinitely small compared to  \frac{\mathrm{d}P}{\mathrm{d}t} and thus:
(equation 3)

 a*r(t) = \frac{\mathrm{d}P}{\mathrm{d}t}

Equation 2 en 3 lead to conclude that the desorption rate is a function of the change in pressure. One can use data in an experiment, which are a function of the pressure like the intensity of a mass spectrometer, to determine the desorption rate.

Since we assumed the pre-exponential factor and the activation energy to be independent of the coverage. Thermal desorption is described with a simplified Arrhenius equation:
(equation 4)


r(t) = -\frac{\mathrm{d}\sigma}{\mathrm{d}t} = v_n \sigma^n * e^{-E_{\mathrm{act}}/RT}

where:

 r(t) the desorption rate[mol/cm2 sec]
 n order of desorption
\sigma surface coverage
 v_n pre-exponential factor [Hz]
 E_{\mathrm{act}} activation energy of desorption [kJ/mol]
 R gas constant
 T temperature [K]

Using the before mentioned Redhead method (a method less precise as the "complete analysis" or the "leading edge" method) and the temperature maximum T_m one can determine the activation energy:
(equation 5)
for n=1

 
E_{\mathrm{act}} /{RT_m}^2 = v_1/\beta* e^{-E_{\mathrm{act}}/RT}


(equation 6)
for n=2

 
E_{\mathrm{act}} /{RT_m}^2 = \sigma_0 v_2/\beta* e^{-E_{\mathrm{act}}/RT}

M. Ehasi en K. Christmann [6] have described a simple method to determine the activation energy of the second order. Equation 6 can be changed into:
(equation 6a)

 
\ln({\sigma_0 {T_m}^2}) = {-E_{\mathrm{act}}/RT} + \ln({\beta* -E_{\mathrm{act}}/v_2R})

where:  \sigma_0 is the surface area of a TDS or TPD peak.

A graph of  \ln({\sigma_0 T_m}) versus  1/T_m results in a straight line with a slope equal to -E_{\mathrm{act}}/R.

Thus in a first order reaction the T_m is independent of the surface coverage. Changing the surface coverage one can determine n. Usually a fixed value of the pre-exponential factor is used and is \beta known, with these values one can derive the  E_{\mathrm{act}} iteratively from T_m.

See also

References

  1. Redhead, P. A. "Thermal desorption of gases" Vacuum 12 (1962) p.203-211
  2. D.A. King, Surface Science 47 (1975) p 384.
  3. E. Habenschaden and J. Küppers, Surface Science 138 (1984) 147
  4. A.M. de JONG and J.W. NIEMANTSVERDRIET, Surface Science 233 (1990) 355-365
  5. J.W. Niemantsverdriet, K. Markert and K. Wandelt, Applied Surface Science 31 (1988) 211
  6. M. Ehasi, K. Christmann, Surface Science 172 (1988)

External links

This article is issued from Wikipedia - version of the Thursday, May 05, 2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.