1. Introduction
Industrial nitric acid (HNO
) production utilises the Ostwald process, where ammonia is mainly oxidised by air over a Pt-Rh gauze catalyst into NO and H
O (Equation
1), followed by homogeneous gas phase oxidation of NO to NO
(Equation
2) and further absorption of NO
by water to produce nitric acid (Equation
3).
The Ostwald process is a mature, extensively studied and highly optimised process for commercial nitric acid production. A typical gas composition after the ammonia combustor (Equation
1) contains 10% of NO, along with 6% O
and 15% H
O at 800
C [
1,
2,
3]. The gas further travels through heat exchangers with short residence times to attain a temperature range of 350-400
C. From this point onwards to the NO
absorption column, the NO
concentration in the gas stream increases due to the gas phase conversion of NO. Nitric oxide (NO) is a free radical with an unpaired electron and its oxidation can also be assumed to take place in two steps as follows [
1]:
According to Honti [
1], the first dimerization reaction of NO is instantaneous with an equilibrium constant (K
) that increases with temperature like any other exothermic reaction. If the overall rate of the NO oxidation reaction is
r, then it depends on the rate of reaction of Eq.
5 and K
as follows:
Hence, as K
increases with temperature, the overall rate of the NO oxidation reaction
r is decreasing, giving rise to an inverse Arrhenius behaviour. Homogeneous NO to NO
conversion (%) is calculated as follows:
Figure 1 presents NO to NO
equilibrium conversion (%) variation with temperature and pressure. That is, NO oxidation to NO
follows an inverse Arrhenius behaviour, but is proportional to pressure which is in line with Le Chatelier’s principle.
Heterogeneously catalysing this bulky homogeneous gas phase oxidation of NO to NO
has several advantages: (1) it decreases capital expenditure (CAPEX) of new nitric acid plants, (2) thus reducing industrial footprint, and (3) significant heat recovery [
4]. Grande et al.[
4] evaluated the kinetics of catalytic oxidation of NO to NO
using a Pt/alumina catalyst at 4-5 bar pressure and found that with a stable heterogeneous catalyst that can oxidise NO to NO
in the range of 250-350
C, the process can be intensified by 10% in terms of energy consumed. A catalyst for NO oxidation faces two main challenges, (i) gas-phase conversion of NO to NO
(presented in
Figure 1) and (ii) presence of strong oxidisers in the feed (NO, O
, NO
, HNO
and HNO
). A direct result of the gas-phase conversion of NO to NO
is that the oxygen available for catalytic reaction becomes limited in the feed. There have been numerous studies on the oxygen storage capacities of ceria (CeO
) and ceria-supported catalysts which enhance the activity for CO and hydrocarbon oxidation of three-way converters[
5,
6,
7]. Cerium being one of the most versatile rare earth elements does not really fall into the "critical rare earth" category and has been a popular catalyst and support material since 1994 [
8]. In literature, several base metal oxides such as Co oxides, Mn oxides and various perovskites have been investigated for NO oxidation at low concentrations of NO [
9,
10,
11,
12,
13]. More than base metals, noble metals and particularly Pt have been studied for their NO oxidation capacity at low concentrations of NO[
14,
15,
16,
17,
18]. Apart from the earlier publications from our group at high NO concentrations (with and without water in the feed) [
12,
19,
20,
21] and Grande et al.[
4], only a few other early patents talk about catalytic oxidation of NO to NO
at conditions relevant to industrial nitric acid production [
22,
23,
24]. Unlike base metals, noble metals can resist oxidation in moist air and from certain acids [
25]. However, the cost of noble metals is 10-50 times higher than base metals [
25,
26] and almost all of the platinum group metals (PGM) are at supply risk globally [
27]. Hence, designing a suitable catalyst for NO oxidation at industrial nitric acid conditions should account for not just catalytic activity but also cost, availability and global supply. However, insufficient data exist regarding the catalytic NO to NO
oxidation activity of various metals under industrially relevant conditions.
In this work we report the low-temperature activity of a series of ceria (CeO) based catalysts to attain NO-NO equilibrium at industrial nitric acid production conditions. This research can assist in the optimisation and better design of a catalyst to oxidise NO at high concentrations and also serve as a starting point for catalytic activity-related research on NO oxidation at industrial nitric acid production conditions. We mainly compare transition metals, two post-transition metals and three rare earth metals. Except for osmium, all other noble metals are tested for their NO oxidation activity for comparison.
3. Results and Discussion
20 monometallic and 4 bimetallic catalysts were successfully prepared and tested for their capacity to oxidise NO in the presence and absence of NO
as a function of temperature (150-400
C).
Table 2 presents catalyst surface areas, metal dispersion for the different catalysts, and apparent activation energies in the presence and absence of NO
. The catalyst surface area decreased slightly with metal impregnation. The major drop in surface area was seen when bimetallic ruthenium-manganese catalysts were prepared with manganese loading larger than 10wt.%.
Table S1 details metal dispersion programme and
Table 2 presents dispersion results. The dispersion analysis programme and probe specie were adjusted for different metal catalysts, and it was not possible to calculate dispersion for the Cr
, Mn
, Y
, Zr
, Nb
, Pd
, Sn
, Re
, Pb
, Gd
and Er
catalysts. Among monometallic catalysts, the decreasing order of catalyst metal dispersion was Pt
> Rh
> Ir
> Ru
> Ag
> Fe
≈ Co
> Ni
≈ Au
. The bimetallic catalyst dispersion analysis was also challenging due to the presence of Mn, however, CO chemisorption was performed on these bimetallic catalysts, assuming exclusive adsorption of CO on Ru. Similar to the surface area of bimetallic catalysts, the dispersion was also reduced with increased manganese loading.
Comparison plots for apparent activation energy for all monometallic and bimetallic catalysts are presented in
Figure 3 and
Figure 4 respectively. The apparent activation energy calculations proved to be difficult for Sn
, Gd
, Er
and Re
in feed(i) and few of the monometallic catalysts have been omitted for apparent activation energy calculations due to low catalytic activity in the actual temperature range (presented in (d)-(f) of Figure S3). Figures S5 and S6 present the Arrhenius plot fit for all monometallic catalysts in feed (i) and (ii), respectively. Table S2 presents goodness-of-fit R
parameter for the Arrhenius plots and respective activation energies. From
Figure 3 and Table S2, in feed(i) apparent activation energy of Period 4 metal-containing catalysts and Pt
catalyst were the lowest with good Arrhenius plot fit. The bimetallic catalysts had reasonable activation energies when compared to monometallic Ru and Mn catalysts in feed (i) (see
Figure 3 and
Figure 4). The activation energy for bimetallic RuMn first decreased to 39.4kJ/mol with 10wt.% manganese loading and then increased two-fold for the Ru
catalyst in feed (i) (see
Figure 4 and Table S2).
Figure 5 presents X-ray diffractograms for all as-prepared bimetallic catalysts, Mn
and Ru
catalysts, diffractograms for all other monometallic catalysts are presented in Figure S4. From diffractograms of all monometallic catalysts (presented in Figure S4), the fluorite cubic structure of CeO
is maintained upon doping with different elements. Only Ru
and Mn
catalysts had other distinct diffraction peaks than from that of CeO
, which corresponds to RuO
(presented as * in Figure S4) and MnO
(presented as
▵ in Figure S4) respectively, indicating larger RuO
particles for these catalysts. The bimetallic Ru-Mn catalysts (Ru
, Ru
, Ru
and Ru
), had RuO
peaks in their respective diffractograms ( presented in
Figure 5). However, the presence of MnO
peaks was more evident when the Mn loading was 10wt.% and above. As for the monometallic catalysts, the fluorite structure of ceria was maintained also in the bimetallic catalysts.
Figures S3, S5 and S6 presents catalytic NO conversions with respect to temperature and activation energy (in the temperature range of 340-350
C) of different monometallic ceria-supported catalysts in feed (i) and (ii) grouped and presented by periods in the periodic table for comparison. Among the monometallic catalysts, Period 4 metal-containing catalysts were more active than the rest of the monometallic catalysts at temperatures below 320
C. Out of all monometallic catalysts, only Ru
and Ir
attained NO-NO
equilibrium in the measured temperature range for feed (i) and only Ru
for feed (ii). The majority of monometallic catalysts had activity in feed (ii) similar to that of gas-phase conversion with only CeO
, indicating NO
as an activity inhibitor as discussed by Mulla et al. [
15] for platinum catalysts.
Figure 6 presents average catalytic conversion at 380
C for all monometallic catalysts and the CeO
support in feed (i) and (ii) during temperature scan (150-400
C) at WHSV= 24,000 Ncm
/g
at ambient pressure. The addition of NO
in feed(ii) reduced the catalytic activity of all monometallic catalysts (presented in (d)-(f) Figures S3 and
Figure 6). Mn
, Fe
, Ru
and Ir
catalysts were the most promising monometallic catalysts in terms of catalytic activity in both feed compositions (i) and (ii).
Catalyst selection rules dictate for active, cost-effective, versatile, selective, and stable catalysts [
39,
40]. Ru
and Ir
are the most active catalysts, but lower cost efficiency in comparison with Mn
and Fe
catalysts [
27]. Ruthenium is more known for its versatility in catalysis compared to iridium due to its lower ionisation energy and more accessible range of oxidation states (-2 to +8)[
41]. Manganese-based catalysts are used for low-temperature NO oxidation reactions at lower concentrations of NO [
42,
43,
44] and our previous research portrayed that the 72hr isothermal activity of manganese on zirconia catalysts for NO oxidation at industrial nitric acid conditions can be improved by doping with Ag [
20]. The highest achievable oxidation state in the first row of d-block elements increases up to manganese and decreases towards zinc. Manganese has multiple stable oxidation states (+2 to +7) and thus higher redox potential than the neighbouring element iron [
45].
From the above literature and results presented in Figures S3 and
Figure 6 and
Table 2, manganese-based catalysts can participate in oxygen activation and transfer processes, whereas the presence of ruthenium can contribute to catalytic activity and stability [
42,
43,
44,
46,
47]. A combination of Ru-Mn bimetallic catalysts suggests a pathway for producing catalysts for NO to NO
oxidation with significant low-temperature activity and lower activation energy. The Ru
, Ru
, Ru
and Ru
catalysts are four Ru-Mn bimetallic catalysts on ceria support with increasing loading of manganese.
Figure 7 and
Figure 8 presents NO to NO
conversion for Mn
, Ru
, Ru
, Ru
, Ru
and Ru
catalysts in feed (i) and (ii). Similar to conversions of monometallic catalysts, the NO conversion of bimetallic catalysts were severely inhibited by the presence of NO
in the feed due to competitive adsorption of NO
on the catalyst surface. The addition of 5wt.% manganese to the Ru
catalyst improved low-temperature catalytic activity in feed(i), whereas catalytic activity in feed (ii) remained similar to that of the Ru
catalyst. Increasing manganese loading higher than 10wt.% resulted in a decrease in catalytic activity for Ru
and Ru
catalysts in both feed (i) and (ii). The apparent activation energy in feed (i) and (ii) for the bimetallic catalysts are presented in
Table 2 and respective Arrhenius plots are presented in Figures S7 and S8. The Ru
catalyst proved to be the most active catalyst with an apparent activation energy of 39.4 kJ/mol and 85.4 kJ/mol in feed (i) and (ii) respectively.
Figure 9 presents 45hrs isothermal runs for Mn
, Ru
, Ru
and the CeO
support at 320
C in 10% NO, 6% O
, 15% H
O and rest Ar at WHSV= 24,000 Ncm
/g
at ambient pressure. The isothermal activity of the Ru
and Ru
catalyst stabilised after 10hrs of the experimental run. However, NO conversion for Mn
decreased over time and eventually resembling the NO conversion obtained over the CeO
support, thus indicating deactivation. This deactivation of manganese can be due to MnO
reducing to Mn
O
as previously seen for Mn/ZrO
catalysts [
20]. The addition of 10wt.% manganese clearly enhanced the low-temperature activity of the Ru
catalyst and the catalyst was stable throughout 45hrs of an isothermal run at 320
C at ambient pressure.
Author Contributions
Jithin Gopakumar: Conceptualization, Methodology, Validation, Formal analysis, Investigation, Writing – Original Draft, Writing – Review & Editing, Visualization Albert Miro i Rovira: Investigation, Formal analysis, Validation Bjørn Christian Enger: Conceptualization, Validation, Writing – Review & Editing, Supervision, Funding acquisition David Waller: Conceptualization, Validation, Writing – Review & Editing, Supervision, Funding acquisition Magnus Rønning: Conceptualization, Validation, Writing – Review & Editing, Supervision, Project Administration, Funding acquisition.
Figure 1.
Homogeneous equilibrium conversion of NO to NO as a function of temperature at 1 and 4 barg pressures.
Figure 1.
Homogeneous equilibrium conversion of NO to NO as a function of temperature at 1 and 4 barg pressures.
Figure 2.
Experimental setup used of catalytic testing and in-situ production of NO. All (- - -) dashed lines are heated to 200C to avoid cold spots and acid condensation. The dashed lines a-b (- - -) represent a coiled line section immersed in cooling water for in-situ conversion of NO to NO.
Figure 2.
Experimental setup used of catalytic testing and in-situ production of NO. All (- - -) dashed lines are heated to 200C to avoid cold spots and acid condensation. The dashed lines a-b (- - -) represent a coiled line section immersed in cooling water for in-situ conversion of NO to NO.
Figure 3.
Apparent activation energy (E kJ/mol) in two different feeds; (a) Feed (i) 10% NO, 6% O, 15% HO and rest Ar and (b) Feed (ii) 8% NO, 2% NO 5% O, 15% HO and rest Ar, with a space velocity of 24,000 Ncm/g for different monometallic catalysts.
Figure 3.
Apparent activation energy (E kJ/mol) in two different feeds; (a) Feed (i) 10% NO, 6% O, 15% HO and rest Ar and (b) Feed (ii) 8% NO, 2% NO 5% O, 15% HO and rest Ar, with a space velocity of 24,000 Ncm/g for different monometallic catalysts.
Figure 4.
Apparent activation energy (E kJ/mol) in two different feeds; (a) Feed (i) 10% NO, 6% O, 15% HO and rest Ar and (b) Feed (ii) 8% NO, 2% NO 5% O, 15% HO and rest Ar, with a space velocity of 24,000 Ncm/g for different bimetallic catalysts.
Figure 4.
Apparent activation energy (E kJ/mol) in two different feeds; (a) Feed (i) 10% NO, 6% O, 15% HO and rest Ar and (b) Feed (ii) 8% NO, 2% NO 5% O, 15% HO and rest Ar, with a space velocity of 24,000 Ncm/g for different bimetallic catalysts.
Figure 5.
X-ray diffraction (XRD) patterns recorded for the CeO support (PDF-00-034-0394), with Mn, Ru, Ru, Ru, Ru and Ru catalyst samples in the 2 range 5-75 with Cu K radiation (1.54060Å). Diffraction peaks of RuO (PDF-04-003-2008) are represented as * and MnO (PDF-04-007-3893) are presented as Δ
Figure 5.
X-ray diffraction (XRD) patterns recorded for the CeO support (PDF-00-034-0394), with Mn, Ru, Ru, Ru, Ru and Ru catalyst samples in the 2 range 5-75 with Cu K radiation (1.54060Å). Diffraction peaks of RuO (PDF-04-003-2008) are represented as * and MnO (PDF-04-007-3893) are presented as Δ
Figure 6.
NO conversion (%) over various monometallic catalysts at 380C during temperature scan (150-400C) at WHSV= 24,000 Ncm/g at ambient pressure in Feed (i): 10% NO, 6% O, 15% HO and rest Ar and Feed (ii) 8% NO, 2% NO 5% O, 15% HO and rest Ar. Period 4 (from the Periodic table) metal catalysts are: Cr, Mn, Fe, Co and Ni, Period 5 metal catalysts are: Y, Zr, Nb, Ru, Rh, Pd, Ag and Sn, and Period 6 metal catalysts are Gd, Er, Re, Ir, Pt, Au and Pb. NO conversion (%) at 380C presented above for all catalysts are average conversions of three parallel temperature scans (150-400C) in feed (i) and (ii).
Figure 6.
NO conversion (%) over various monometallic catalysts at 380C during temperature scan (150-400C) at WHSV= 24,000 Ncm/g at ambient pressure in Feed (i): 10% NO, 6% O, 15% HO and rest Ar and Feed (ii) 8% NO, 2% NO 5% O, 15% HO and rest Ar. Period 4 (from the Periodic table) metal catalysts are: Cr, Mn, Fe, Co and Ni, Period 5 metal catalysts are: Y, Zr, Nb, Ru, Rh, Pd, Ag and Sn, and Period 6 metal catalysts are Gd, Er, Re, Ir, Pt, Au and Pb. NO conversion (%) at 380C presented above for all catalysts are average conversions of three parallel temperature scans (150-400C) in feed (i) and (ii).
Figure 7.
NO conversion (%) of Mn, Ru, Ru, Ru, Ru and Ru catalysts as a function of temperature with Feed (i): 10% NO, 6% O, 15% HO and rest Ar, heated at a rate of 5C/min at WHSV= 24,000 Ncm/g at ambient pressure.
Figure 7.
NO conversion (%) of Mn, Ru, Ru, Ru, Ru and Ru catalysts as a function of temperature with Feed (i): 10% NO, 6% O, 15% HO and rest Ar, heated at a rate of 5C/min at WHSV= 24,000 Ncm/g at ambient pressure.
Figure 8.
NO conversion (%) of Mn, Ru, Ru, Ru, Ru and Ru catalysts as a function of temperature with Feed (ii): 8% NO, 2% NO, 5% O, 15% HO and rest Ar, heated at a rate of 5C/min at WHSV= 24,000 Ncm/g at ambient pressure.
Figure 8.
NO conversion (%) of Mn, Ru, Ru, Ru, Ru and Ru catalysts as a function of temperature with Feed (ii): 8% NO, 2% NO, 5% O, 15% HO and rest Ar, heated at a rate of 5C/min at WHSV= 24,000 Ncm/g at ambient pressure.
Figure 9.
NO conversion (%) of Mn, Ru, Ru and the CeO support at 320C in 10% NO, 6% O, 15% HO and rest Ar at WHSV= 24,000 Ncm/g at ambient pressure for 45hrs.
Figure 9.
NO conversion (%) of Mn, Ru, Ru and the CeO support at 320C in 10% NO, 6% O, 15% HO and rest Ar at WHSV= 24,000 Ncm/g at ambient pressure for 45hrs.
Table 1.
Designations of all ceria-based catalysts and impregnated metal precursor details.
Table 1.
Designations of all ceria-based catalysts and impregnated metal precursor details.
Catalyst Name |
Metal Precursor |
Commercial Supplier |
Cr
|
Cr(NO).9HO |
Sigma Aldrich |
Mn
|
Mn(NO).4HO |
Sigma Aldrich |
Fe
|
FeCl
|
Sigma Aldrich |
Co
|
Co(NO).6HO |
Sigma Aldrich |
Ni
|
Ni(NO).6HO |
Sigma Aldrich |
Y
|
Y(NO).6HO |
Sigma Aldrich |
Zr
|
ZrO(NO).xHO |
Sigma Aldrich |
Nb
|
NbCl
|
Sigma Aldrich |
Ru
|
RuCl.xHO |
Sigma Aldrich |
Ru
|
RuCl.xHO,Mn(NO).4HO |
Sigma Aldrich |
Ru
|
RuCl.xHO,Mn(NO).4HO |
Sigma Aldrich |
Ru
|
RuCl.xHO,Mn(NO).4HO |
Sigma Aldrich |
Ru
|
RuCl.xHO,Mn(NO).4HO |
Sigma Aldrich |
Rh
|
RhCl
|
Sigma Aldrich |
Pd
|
PdCl
|
Sigma Aldrich |
Ag
|
AgNO
|
Alfa Aesar |
Sn
|
SnCl
|
Sigma Aldrich |
Re
|
ReCl
|
Sigma Aldrich |
Ir
|
IrCl
|
Merck |
Pt
|
(Pt(NO))
|
Alfa Aesar |
Au
|
(HAuCl)
|
Sigma Aldrich |
Pb
|
PbCl
|
Sigma Aldrich |
Gd
|
Gd(NO).6HO |
Alfa Aesar |
Er
|
ClEr.6HO |
Sigma Aldrich |
Table 2.
BET surface areas (N physisorption) and respective total metal dispersion (%) from chemisorption measurements for the different catalysts.
Table 2.
BET surface areas (N physisorption) and respective total metal dispersion (%) from chemisorption measurements for the different catalysts.
Catalyst |
Surface
|
Dispersion |
Metal:Probe |
Probe Gas |
|
Area [m/g] |
[%] |
Specie |
Uptake [mol g] |
CeO
|
92 |
− |
− |
− |
Cr
|
78 |
− |
− |
− |
Mn
|
82 |
− |
− |
− |
Fe
|
82 |
3% |
1:1 - Fe:H [29] |
2 |
Co
|
80 |
10% |
1:1 - Co:H [30,31] |
27 |
Ni
|
79 |
11% |
1:1 - Ni:H [32] |
33 |
Y
|
85 |
− |
− |
− |
Zr
|
86 |
− |
− |
− |
Nb
|
79 |
− |
− |
− |
Ru
|
72 |
41% |
1:1 - Ru:CO [33,34] |
39 |
Ru
|
71 |
39% |
1:1 - Ru:CO [33,34] |
35 |
Ru
|
65 |
32% |
1:1 - Ru:CO [33,34] |
31 |
Ru
|
55 |
19% |
1:1 - Ru:CO [33,34] |
18 |
Ru
|
48 |
13% |
1:1 - Ru:CO [33,34] |
12 |
Rh
|
74 |
38% |
1:1 - Rh:H [35] |
39 |
Pd
|
72 |
− |
− |
− |
Ag
|
70 |
29% |
1:1 - Ag:H [36] |
24 |
Sn
|
80 |
− |
− |
− |
Re
|
75 |
− |
− |
− |
Ir
|
76 |
37% |
1:1 - Ir:CO [37] |
35 |
Pt
|
75 |
43% |
1:1 - Pt:CO [21] |
42 |
Au
|
72 |
2% |
1:1 - Au:H [38] |
2 |
Pb
|
70 |
− |
− |
− |
Gd
|
81 |
− |
− |
− |
Er
|
77 |
− |
− |
− |