27th Symposium (International) on Combustion, Accepted for Publication
The Effects of Equivalence Ratio on the Formation of
Polycyclic Aromatic Hydrocarbons and Soot in
Premixed Methane Flames
Antonio M. Vincitore, Tyler R. Melton and Selim M. Senkan*, Department of Chemical Engineering, University of California
Los Angeles, CA 90095
* To whom correspondence should be addressed: Tel: (310) 206-4106,
Fax: (310)206-4107, e.mail:
senkan@seas.ucla.edu
ABSTRACT
The formation of polycyclic aromatic hydrocarbons (PAH)
and soot has been investigated in atmospheric pressure,
laminar, methane/oxygen/argon premixed flames as a
function of mixture equivalence ratio. Mole fraction
profiles of major products, trace aromatic, substituted
aromatic and PAH were quantified by direct gas
chromatography/mass spectrometry. In addition, soot
particle diameters, number densities and volume fractions
were determined using classical light scattering. The
dependencies of flame species on equivalence ratio, using
the expression, Ximax = Ai ni were also determined; results
reveal that the parameter (n) for stable aromatic precursors
exhibit the following rank order: C4H2 (4.39) > C3H4 (3.96)
> C4H6 (3.41) > c-C5H6 (3.30) > C4H4 (2.31) > C2H2 (1.35).
For aromatic species, the values of n were in the following
order: Phenylacetylene (10.88) > Benzene (10.21) > Indene
(7.63) > Toluene (5.43). In comparison, PAH species were
extremely sensitive to flame equivalence ratios, with the
following n values: Fluoranthene (15.1) > Acenaphthylene
(14.8) > Pyrene (13.8) > Anthracene (13.1) > Phenanthrene
(12.9) > Naphthalene (11). These results indicate that PAH
formation rates are not strongly influenced by the levels of
acetylene present in the flame under the conditions
investigated.
INTRODUCTION
Recently, we began a series of experimental studies of fuel-rich, premixed hydrocarbon flames to discern the relationships between combustion conditions and the formation of soot and polycyclic aromatic hydrocarbons (PAH) [1,2,3]. These results indicated that aromatic and PAH levels are strongly related to fuel structure and soot levels present within the flame. In earlier studies, PAH were advocated to be the precursors to soot formation [4], suggesting that an increase in soot production would be correlated to higher PAH levels. However, our recent experimental results indicate that this is not generally true [2], thus suggesting that PAH and soot formation are part of a complex chemical reaction network. Over the past years, numerous experimental studies involving premixed methane flames have been performed with a major focus on elucidating the physical and chemical processes associated with PAH and soot formation [5,6,7]. However, there still exists uncertainty with regard to reaction pathways leading to PAH production and their relationship to soot. To date, two main reaction routes have been proposed to describe the production of the first aromatic ring, i.e. benzene. The first route involves the reaction of C4 and C2 species yielding C6s, followed by the cyclization and dehydrogenation of the adduct [4]. The formation of PAH were then accounted for by the activation of the aromatic ring followed by the addition of C2H2 and other carbon moieties [4]. The second route involves the recombination of resonantly stabilized C3 species resulting in the direct formation of the aromatic ring [8]. Recently, new reaction pathways have also been proposed to account for the formation of PAH [9]. For example, the recombination of cyclopentadiene has been suggested to directly produce naphthalene, thus eliminating the need to form benzene first and expediting the PAH production process.
In this communication, we report on the detailed
chemical structures of fuel-rich, laminar premixed methane
flames as a function of mixture equivalence ratio in order
to develop insights on the relation of flame chemistry with
PAH and soot formation. The information acquired was
also analyzed to establish trends such that better models
describing PAH and soot formation can be developed. In
an earlier study, Musick et al. [10] reported the C1-C4
chemical structures of low-pressure, premixed flames of
CH4/O2/Ar over an equivalence ratio range of 0.92-1.94.
However, no information on aromatic and PAH was
provided.
EXPERIMENTAL
The experimental set-up has been described
elsewhere [1], thus only a brief description will be given
here. Atmospheric-pressure, premixed, laminar, flat-flames
of CH4/O2/Ar were stabilized over a 50 mm diameter porous
bronze burner. The burner was cooled by circulating an
ethylene glycol solution at 104.3 oC. Flames were protected
from the surrounding air by a concentric shield of Argon
gas. Gas flows were regulated using high accuracy mass
flow controllers (MKS, Burlington MA). The purities of
the gases used in this experimental study were 99.99 %.
The initial feed compositions and equivalence ratios for the
flames studied are summarized in Table 1. In all the
flames, the methane volumetric flow rate was maintained
constant at 1.88 liters per minute, while the flows of argon
and oxygen were varied. In addition, the argon mole
fractions in all flames were maintained at 0.45. This
allowed for a better control of the flame temperatures, thus
a better comparison of the concentrations as a function of
equivalence ratio. The chemical structures of five flames
with equivalence ratios ranging from 2.0 to 2.6 were
examined by withdrawing samples from within the flame
using a heated quartz microbe with a 100 µm orifice at its
tip. Samples were transported through a silica lined,
stainless steel transfer line. Flames below an equivalence
ratio of 2.0 were difficult to sample because of their close
proximity to the burner surface. Flames with equivalence
ratios above 2.6 were too unstable and sooting to sample.
A quartz wool filter was placed inside the probe to trap soot
particles. The entire sampling system was maintained at
300 oC to minimize the adsorption of large molecular
weight PAH.
Experimental Conditions of Atmospheric, Premixed Methane/Oxygen/Argon Flames a.
| Flame | YCH4 | YO2 | YAr | Vo
(cm/s) |
To
(K) | |
| 1 | 2.0 | 0.275 | 0.275 | 0.450 | 5.81 | 673 |
| 2 | 2.2 | 0.288 | 0.262 | 0.450 | 5.54 | 638 |
| 3 | 2.3 | 0.294 | 0.256 | 0.450 | 5.43 | 618 |
| 4 | 2.4 | 0.300 | 0.250 | 0.450 | 5.32 | 592 |
| 5 | 2.6 | 0.311 | 0.239 | 0.450 | 5.14 | 572 |
a Vo is defined as the cold gas velocity. To is defined as the burner surface
temperature.
Samples were immediately analyzed by a computer controlled gas chromatograph/mass spectrometer (Hewlett-Packard 5890/5972) using both capillary (0.25 mm x 60 m HP-5) and packed bed (Hayesep T and Hayesep DB) columns. Major species were analyzed using the thermal conductivity detector (TCD). Some minor and all the trace species were analyzed using the mass spectrometer. Species concentrations were determined either by direct calibration standards (Matheson Gas, Sigma Aldrich), or by the use of mass spectral ionization cross section method [11]. The accuracy of latter has been reported to be within a factor of two [11], and was verified in previous studies [1]. The accuracy of the mole fractions for species determined by direct calibration is estimated to be ±15%. Both H2 and H2O concentrations were determined from H and O atomic balances.
Concentration profiles were generated by moving the entire burner assembly vertically up or down with respect to the fixed sampling probe. Positional accuracy associated with the concentration and temperature measurements is estimated to be ± 0.25 mm. Temperature measurements were obtained with a silica coated, 0.15 mm Pt-13%Rh/Pt thermocouple. Temperature measurements reported in this work were not corrected for radiation losses.
Soot sizes, number densities and volume fractions
were determined using classical laser light scattering and
extinction measurements [12]. For this, a collimated and
focused (0.2 mm) 514.5 nm laser beam (Spectra Physics,
2037, 1.0 W) that was mechanically modulated at 1000
Hz, was passed through the flame. The light scattered by
the soot particles was collected at 90o from the incident
beam with a lens and directed through an iris onto the
cathode of a photomultiplier (PMT, Hamamatsu, R1463).
The PMT signal was amplified using a lock-in amplifier
(EG&G 5205). The transmitted light was measured with
a photodiode and recorded with an oscilloscope. Polarized
narrow band filters were placed in front of the
photomultiplier and photodiode to minimize signal
contamination from flame luminosity. The light scattering
set-up was calibrated against a known, particle free, flow
composed of argon. The calculation of the number
densities and volume fractions were accomplished by
assuming monodisperse particles having a complex
refractive index of 1.54+0.58i [13].
DISCUSSION
In Fig.1, the temperature and soot profiles for the
flames studied are presented. In this and subsequent
figures, lines have been drawn through the data points to
indicate trends. Due to crowding, Fig. 1 through Fig. 6
provide information for all flames excluding Flame 3. In
Fig. 7 and 8, we report the PAH concentration profiles for
all flames. As seen in Fig. 1, the flames based on their
temperature profiles, were positioned at various distances
from the burner surface, consistent with their equivalence
ratios. For example, Flame 1 was positioned closest to the
burner, because of its lowest equivalence ratio and thus
highest burning velocity. In contrast, Flame 5 had the
lowest burning velocity, and was positioned the farthest
from the burner surface. The flame temperatures exhibited
near linear profiles from the burner surface to the point of
maximum temperature. It is also important to note that the
maximum flame temperatures reached in all the flames
were about 1300 oC, with a 25 oC difference in peak
temperatures between the flames studied. This result is
consistent with past experimental work [14]. At distances
substantially away from the burner surface, soot deposition
on the thermocouple bead was inevitable. This led to
increased radiative heat losses from the thermocouple bead
yielding in lower temperature readings. To minimize this
effect, the thermocouple was kept in the sooting section of
the flame for a minimal amount of time, and any
accumulated soot was burned off with the aid of a small
propane torch after each measurement [1].
FIG. 1. Temperature (T), soot particle diameter (dp), number density (N)
and volume fraction (fv) measurements. Symbols used in soot measurements
correspond to the following flames : (2.0), (2.2),(2.3), (2.4),
(2.6).
In Fig. 1, the measured soot volume fraction, particle diameter and number density profiles are also reported. These properties were calculated by assuming monodisperse soot particles that were smaller than the wavelength of the light used (515.5 nm) in order to satisfy the Rayleigh scattering approximation. Although non-spherical and polydisperse soot occurs within flames to due the agglomeration of primary soot particles, the Rayleigh approximation has been demonstrated to hold to within a factor of three [15]. As evident from Fig. 1, the soot volume fraction steadily increases with increasing equivalence ratio and with distance above the burner surface. In contrast, the soot number density first increases with flame height and exhibits a maxima near the maximum flame temperature and then decreases with height above the burner. Within the flame, the decrease in soot number density can be attributed to the coagulation of elementary soot particles. As seen in Fig.1, soot particle diameters also increased with increasing equivalence ratio, closely tracking the soot volume fraction. These results were also seen in previous studies [14]. The measured maximum particle diameters ranged from 10 nm to 28 nm, for Flame 2 to Flame 5, respectively. We were not able to determine particle diameters for Flame 1.
In Fig. 2, the mole fraction profiles for the
reactants CH4 and O2 and two of the major carbon
containing products CO and CO2 are presented. As evident
from this figure, the profiles exhibit features consistent with
the relative equivalence ratios. For example, both CH4 and
O2 increasingly penetrate into the post flame zone with
increasing equivalence ratio. As expected CO was the
major combustion product in all cases.
FIG. 2. Concentration profiles of CH4, O2, CO and CO2 for Flames 1-5.
Symbols correspond to the following flames : (2.0), (2.2), (2.4),
(2.6).
FIG. 3.
The mole fraction profiles for H2, H2O, C2H2 and
C2H4 presented in Fig. 3 also exhibit features consistent
with the mixture equivalence ratio. However, the post
flame H2 and H2O levels were not sensitive to equivalence
ratio. It is also interesting to note that with the exception
the lowest equivalence ratio case , i.e. =2.0, the post flame
levels of acetylene also we re insensitive to the mixture
equivalence ratio. This is an intriguing result, because of
the significant influence equivalence ratio had on soot
volume fraction and diameter (Fig. 1) and the generally
believed notion that acetylene is an important soot growth
species [16,17].
In Fig. 4, the mole fraction profiles for ethane, 1,3 propadiene/1-propyne, diacetylene and vinylacetylene are presented. As evident from this figure, the mole fraction profiles for ethane peaked early in the flame zone, indicating the role of this species in the pre-flame reaction zone. In contrast, 1,3 propadiene/1-propyne, diacetylene and vinylacetylene penetrated well into the post flame zone suggestive of their role in PAH and soot formation.
Also evident from Fig. 4, 1,3 propadiene/1-propyne,
diacetylene and vinylacetylene appear to closely track the
mixture equivalence ratio. That is, their formation is
delayed and their peak mole fractions increased with
increasing equivalence ratio.
FIG. 4. Concentration profiles of C2H6, C3H4, C4H2 and C4H4. Symbols
correspond to the following flames : (2.0), (2.2), (2.4), (2.6).
FIG. 5. Profiles of 1,2 butadiene (a-C4H6), 1,3 butadiene (b-C4H6), 1,3
pentene-yne (C5H6) and cyclopentadiene (c-C5H6). Symbols correspond to
the following flames : (2.0), (2.2), (2.4), (2.6).
In Fig. 5, the mole fraction profiles for 1,2 butadiene, 1,3 butadiene, 3-pentene-1-yne and cyclo-pentadiene are presented. With the exception of 3-pentene-1-yne, all of these species penetrated well into the post flame zone suggesting their possible role in PAH and soot formation chemistry. These species also exhibited trends consistent with the compositions of the flames studied, with increasing levels of production with increasing equivalence ratio.
In Fig. 6, the mole fraction profiles for the
aromatic products, that include benzene, toluene, phenyl-acteylene and indene are presented. All of these species
penetrated well into the post flame zone and exhibit trends
consistent with the equivalence ratio.
FIG. 6.
The mole fraction profiles of six representative PAH measured in the flames are compared to one another in Fig.7 and Fig. 8. The structural designations of various PAH species are presented in Table 2. Although, there were many other PAH measured in the flames, space limitations prohibit the presentation of the entire set at this time. As evident from these figures, the levels of PAH produced in the flame steadily increased with flame height and generally leveled off at about 10 mm from the burner surface.
FIG. 7. Profiles of naphthalene (C10H8), acenaphthylene (C12H8) and
anthracene (a-C14H10). Symbols correspond to the following flames : (2.0),
(2.2),(2.3), (2.4), (2.6).
The dependencies of various chemical species on equivalence ratio were also analyzed using the empirical formula Ximax = Ai ni [18]. In this expression, Ximax is the maximum mole fraction of species i, Ai and ni are the correlation parameters. The parameter ni represents the sensitivity of species i on equivalence ratio, and has previously been used to explore the C1-C4 chemistry of low pressure CH4/O2/Ar flames at equivalence ratios range of 0.92-1.94 [10]. The values of Ai and ni were determined from linear regression of our experimental data. The values of Ai and ni, as well as the corresponding correlation coefficients are presented in Table 2. As evident from this table, the experimental results were well represented by the above empirical relationship with correlation coefficients higher than 0.9 for all species.
An inspection of Table 2 reveals that the mole fractions of aliphatic species produced in the flames were moderately sensitive to mixture equivalence ratio. The rank order of correlation parameter ni were: C4H2 (4.39) > C3H4 (3.96) > C4H6 (3.41) > c-C5H6 (3.3) > b-C4H4 (2.31) > C2H2 (1.35). Although this rank order is consistent with similar determinations made in low pressure flames [10], the ni values are considerably different. However, the latter is not surprising in view of the differences in equivalence ratios and pressures investigated.
FIG. 8. Profiles of phenanthrene (b-C14H10), fluoranthene (a-C16H10) and
pyrene (b-C16H10). Symbols correspond to the following flames : (2.0),
(2.2),(2.3), (2.4), (2.6).
In contrast to aliphatics, aromatics were significantly more sensitive to changes in equivalence ratio. The calculated ni values for aromatic species were: Phenylacetylene (10.88) > Benzene (10.21) > Indene (7.63) > Toluene (5.43). Furthermore, PAH species were extremely sensitive to flame equivalence ratios, exhibiting the following rank order for ni: Fluoranthene (15.1) > Acenaphthylene (14.8) > Pyrene (13.8) > Anthracene (13.1) > Phenanthrene (12.9) > Naphthalene (11).
In summary, the measurements of in-flame
concentrations of aliphatics, aromatics and PAH exhibit
different dependencies on the mixture equivalence ratio.
PAH levels were most significantly affected by equivalence
ratio followed by simple aromatics and aliphatics. The
levels of acetylene were least sensitive to equivalence ratio.
The results presented should be of considerable utility for
the development and validation of models describing the
formation of PAH and soot in flames.
Calculated values for the Ai factor and exponent ni for minor, aromatic and PAH species.
| A | n | Corr. Coeff. | |
| C2H2 | 7.0x10-3 | 1.35 | 0.935 |
| C3H4 | 2.2x10-5 | 3.96 | 0.978 |
| C4H2 | 6.2x10-5 | 4.39 | 0.971 |
| C4H4 | 2.8x10-5 | 2.31 | 0.9 |
| 1,3 butadiene (b-C4H6) | 1.1x10-6 | 3.41 | 0.943 |
| cyclopentadiene
(c-C5H5) |
7.5x10-7 | 3.3 | 0.967 |
| Benzene (C6H6) | 3.3x10-8 | 10.21 | 0.986 |
| Toluene (C7H6) | 2.5x10-8 | 5.43 | 0.972 |
| Phenylacetylene (C8H6) | 1.2x10-9 | 10.88 | 0.977 |
| Indene (C9H8) | 2.6x10-9 | 7.63 | 0.978 |
| Naphthalene (C10H8) | 4.3x10-10 | 11.04 | 0.968 |
| Acenaphthylene (C12H8) | 1.4x10-11 | 14.80 | 0.736 |
| Phenanthrene
(b-C14H10) |
2.1x10-11 | 12.87 | 0.947 |
| Anthracene (a-C14H10) | 3.7x10-12 | 13.12 | 0.854 |
| Pyrene (b-C16H10) | 7.3x10-11 | 13.81 | 0.981 |
| Fluoranthene (a-C16H10) | 8.3x10-12 | 15.09 | 0.982 |
ACKNOWLEDGMENTS
This research was supported, in part, by the US
Environmental Protection Agency, the National Science
Foundation, the UCLA Center for Clean Technology and
the Petroleum Environmental Research Forum Project.
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