Open Access
CC BY 4.0 · Sustainability & Circularity NOW 2026; 03: a27913831
DOI: 10.1055/a-2791-3831
Original Article

Complete Oxidation of CO, Propene, and Toluene as Model Components of Diesel Engine Exhaust and VOC using Ceria-modified Cu/Hydroxyapatite: Effect of Preparation Methods and Ce Concentration

Authors

  • Rahul More

  • Kajal Pawar

  • Rushikesh Pagare

  • Pavan More


SERB provide financial support for project sanction order No. EEQ/2016/000264. The support received from the BANRF Fellowship (BARTI/Fellowship/BANRF-2021/2135 & 21/06/2023), Pune, as a senior research fellow is gratefully acknowledged.
Supported by: Science and Engineering Research Board EEQ/2016/000264
 


Graphical Abstract

Abstract

The Ce-modified Cu/HAp catalyst was prepared by successive deposition and coprecipitation methods and was investigated for propene oxidation serving as a model component of diesel engine exhaust and volatile organic components (VOCs). The Cu0.4/Ce0.1/HAp catalyst prepared by successive deposition showed better performance than the Cu0.4–Ce0.1/HAp catalyst prepared by the coprecipitation method. Furthermore, the Ce concentration has been optimized using successive deposition methods. The catalyst was modified with 0.4 mol Cu and 0.1 mol Ce deposited on HAp and tested for CO, propene, and toluene oxidation. Complete conversion is attained by the Cu0.4/Ce0.1/HAp catalyst at approximately 339 °C, highlighting its superior low-temperature activity compared with the remaining Ce-modified Cu/HAp catalyst series. All catalysts were characterized by P-XRD, BET, Raman, XPS, ATR-FTIR, H2-TPR, FESEM, and HR-TEM techniques. The formation of facile CuO x species with more Ce3+ and adsorbed oxygen was observed in the Cu0.4/Ce0.1/HAp catalyst. These species are responsible for the oxidation of propene at lower temperatures compared to the remaining catalyst.


1

Introduction

Volatile organic components (VOCs) and CO are very harmful components in automobile engine exhaust gases.[1] [2] [3] [4] VOCs are produced from biogenic, pyrogenic, and anthropogenic sources. These sources are responsible for the direct and indirect hazards to both the atmosphere and human health.[5] [6] However, very stringent exhaust regulations have been imposed worldwide in recent years to curb the negative effects of diesel engines and VOC emissions on human health and the environment. Therefore, the complete oxidation of CO and VOC has been studied by many researchers.[1] [4] [6] [7] [8] Noble metals like platinum and or platinum supported on alumina are used commercially for total oxidation of diesel engine exhaust and VOC.[9] [10] [11] However, high cost, higher light temperature, and low stability restrict the use of these catalysts.[12] [13] [14] To overcome these problems, metal/metal oxides supported on different metal oxides like CeO2, Al2O3, TiO2, hydroxyapatite, etc., had been previously reported for the total oxidation of diesel engine exhaust.[7] [9] [10] [15] [16] [17] [18] Thus, metal oxides like Al2O3, TiO2, CeO2, and hydroxyapatite (HAp) are used as a support for Cu, Mn, and oxides and have been reported for the total oxidation of diesel engine exhaust and VOCs.[3] [15] HAp is known for its very flexible hydrotalcite structure with good thermal stability. HAp is also known for its surface acidity and basicity, exchangeable Ca abilities, and strong adsorption properties.[19] Moreover, ceria has been used in three-way catalysts due to its high oxygen-storage capacity, metal dispersion, and facile redox cycle between the Ce3+/Ce4+.[20] [21] [22] [23] Furthermore, copper has shown facile redox properties between Cu+/Cu2+ in the presence of ceria and has been studied for the oxidation of diesel engine exhaust and VOC.[20] [22] [24] [25] Thus, Cu and Ce showed facile synergistic redox properties and were responsible for the formation of interfacial active sites, which oxidize the CO, propene, and toluene into CO2.[26] [27] The copper–ceria catalyst showed formation of more Ce3+ species, oxygen vacancies, and adsorbed oxygen, responsible for the low-temperature oxidation.[26] [27] [28] [29] However, the effect of Ce on the properties and catalytic activity of Cu supported on HAp is ambiguous and needs to be understood in detail.

The addition of Ce in the Cu/HAp catalyst could improve the low-temperature activation of oxygen by forming a higher oxygen vacancy. The Ce doping could stabilize the structure and improve the redox properties of Cu. The present study deals with the effect of Ce concentration and the preparation methods on the oxidation activity of Cu/HAp with respect to CO, propene, and toluene as a model component of diesel engine exhaust and VOC. The catalyst’s characterizations were studied in detail and correlated to the oxidation activity.


2

Results and Discussion

2.1

Characterization of Ce-promoted Cu/HAp Prepared by Successive Deposition

2.1.1

Powder X-ray Diffraction

The XRD patterns of the Cu/HAp and Ce-promoted Cu/HAp catalysts prepared by the successive deposition methods are shown in [Fig. 1]. The XRD peaks of Ce-promoted Cu/HAp correspond to the HAp (JCPDS no. 09-0432). However, the peaks centered at 2θ = 32.53°, 35.38°, 38.78°, 58.14°, 62.0°, 66.18°, 67.18°, and 67.94° correspond to the CuO (JCPDS no. 48-1548) having a monoclinic structure. HAp peaks at 25.82°, 31.98°, 33.97°, 43.88°, 46.74°, 49.54°, and 53.16° have shifted to a lower angle after deposition of Cu on HAp.[30] The XRD peaks of CuO are observed at 35.3°, 38.2°, and 62.0°. The CuO phase was observed in the Cu/Hap catalyst. However, low intensity of the same peaks was observed in Ce-modified Cu/HAp catalysts. In the case of successive deposition of Ce on HAp followed by Cu (0.1–0.4 mol), no separate peak of Ce was observed due to the overlapping with the peaks of HAp and CuO at 28.34°, 32.86°, 47.34°, and 56.27°. The reduced intensity could be attributed to the dispersion of Cu and Ce species on the surface of HAp. Furthermore, the increase in Cu deposition on Ce/HAp shows the shifting of the HAp peak toward a lower angle. The shifting indicates the interaction of Ce with Cu and HAp, which may lead to the formation of Ce3+ species. The successive deposition of Cu2+ and Ce on HAp could create the oxygen vacancies (VÖ) responsible for the formation of more Ce3+ (2 Ce4+ ↔ 2Ce3+ + VÖ2+) ions. The formation of more Ce3+ species could be responsible for the activation of gaseous oxygen at lower temperatures. The activation of oxygen leads to the oxidation of propene at lower temperatures.

Zoom
Fig. 1 Powder X-ray diffraction patterns of HAp, Cu/HAp, and Cu x /Ce0.5−x /HAp.

2.1.2

Surface Area Study

The BET surface area was measured by N2 adsorption and is shown in [Table 1]. The surface area of the catalysts increases with an increase in ceria concentration. The interaction between Cu and Ce reduces the agglomeration and could sustain the active sites beneficial for propene oxidation at lower temperatures.

Table 1

Surface and bulk properties of HAp and Ce-modified Cu/HAp.

Catalyst

2θ°

S BET (m2/g)

HAp

31.98

28.8

Cu0.5/HAp

31.76

40.1

Cu0.1/Ce0.4/HAp

31.82

64.4

Cu0.2/Ce0.3/HAp

31.82

63.6

Cu0.3/Ce0.2/HAp

31.84

62.3

Cu0.4/Ce0.1/HAp

31.88

65.4


2.1.3

ATR-FTIR Study of Ce-promoted Cu/HAp Prepared by the Successive Deposition Method

The attenuated total reflectance Fourier transform infrared spectra are shown in [Fig. 2]. The fundamental vibrational modes for (PO4)3− in hydroxyapatite were observed at 565, 602, 962, 1030, and 1090 cm−1.[30] [31] The strong bands at 602 and 565 cm−1 are assigned to ʋ4 vibrational modes of O–P–O, whereas 962 cm−1 ʋ1 stretching vibrations are associated with a P–O bond. The larger peak at 1030 cm−1 and the smaller peak located at 1090 cm−1 correspond to the vibrational modes of the (PO4)3− group.

Zoom
Fig. 2 ATR-FTIR spectra of HAp and Ce-modified Cu/HAp.

The deposition of Cu on the HAp support leads to the shifting of the HAp peaks 562, 1025, and 1088 cm−1 toward a higher wavenumber 564, 1032, and 1090 cm−1, respectively. This shifting indicates the strong interaction of Cu with the O–P–O and P–O bonds of Hap, which is responsible for the increase in strength of the O–P–O and P–O bonds. Whereas, after the addition of ceria by the successive deposition method, catalysts (Cu0.4/Ce0.1/HAp) showed bands at 563, 1030, and 1089 cm−1. These results indicate that the IR bands shifted to a lower wavenumber after the addition of Ce in Cu/HAp. The observed shifts in the bands may be attributed to the interaction between Cu and Ce with HAp, leading to the weakening of the O–P–O and P–O bonds.


2.1.4

Raman Spectroscopy Study

Raman spectroscopy can be useful to elucidate the formation of defective sites and the influence of Ce on the structure of Cu/HAp. The Raman scattering spectra of HAp and Ce-modified Cu/HAp are shown in [Fig. 3]. The Raman scattering spectra showed characteristic bands of the HAp phase with vibrational modes of the phosphate group,[32] and the surface defects with the Ce–O band correspond to the Ce-modified HAp catalyst. The prominent band at 962 cm−1 is attributed to the symmetrical stretching of the P–O bonds.[33] Additionally, the distinctive band observed at approximately 456 cm−1, corresponding to the F2g vibrational mode, is indicative of CeO2 and is absent in Cu/HAp, confirming the presence of CeO2 in the sample.[34]

Zoom
Fig. 3 Raman spectra of Cu/HAp, Ce/Hap, and Ce-modified Cu/HAp.

In the case of Cu/HAp, the shifting of the band was observed from 962 to 954 cm−1. However, Cu0.4/Ce0.1/HAp showed the same band at 951 cm−1. The maximum decrease in the frequency of P–O bonds was observed in Cu0.4/Ce0.1/HAp. Furthermore, the characteristic F2g band of CeO2 has shifted toward the higher frequency (from 440 to 446 cm−1) with an increase in Cu concentration from 0.1 to 0.3 mol (Cu0.1 to Cu0.3). However, a further increase in Cu concentration to 0.4 mol (Cu0.4) leads to the shifting of the F2g peak of CeO2 to the lower frequency (from 446 to 433 cm−1) with broadening. Similarly, the B2g vibrational peak of CuO at 648 cm−1 shifted to 640 cm−1. The decrease in frequencies indicates the weakening of the P–O and Cu–O bonds with the formation of more labile oxygen required for the low-temperature oxidation of propene. Thus, an increase in asymmetry, oxygen vacancy, and distortion in the Ce results in Raman band shifting. The Cu0.4/Ce0.1/HAp showed the maximum shifting, indicating the formation of more oxygen vacancies and more labile oxygen, which eventually results in improvement in activity toward propene oxidation at a lower temperature. These results are in good agreement with FTIR and XRD results.


2.1.5

H2-Temperature Programmed Reduction Study of Ce-modified Cu/HAp Prepared by Successive Deposition

The temperature-programmed reduction (TPR) profiles of both Cu/HAp and Ce-modified Cu/HAp are illustrated in [Fig. 4]. The TPR peaks, evident in the temperature range of 150–300 °C, signify the reduction process of Cu2+ to Cu0 through Cu1+. The Cu/HAp catalyst modified with 0.1 mol Ce showed a reduction of Cu2+ to Cu0 at 194 °C. However, the catalyst with increasing concentration of Ce (0.2–0.4 mol) showed a reduction of Cu2+ to Cu0 above 203 °C. The Cu/HAp catalyst showed a reduction of larger CuO species at 485 °C, which is absent in Ce-modified Cu/HAp. These results indicate that the Ce-modified Cu/HAp showed the formation of smaller CuO particles/clusters compared to the Cu/HAp. The Cu/HAp catalyst modified with an optimum concentration of Ce showed a reduction of CuO and Cu2O to Cu at lower temperatures compared to the remaining catalyst.

Zoom
Fig. 4 H2-TPR spectra of Cu/HAp and Ce-modified Cu/HAp.

The H2-TPR peaks of Cu0.4/Ce0.1/HAp prepared by the successive deposition method showed a reduction of Cu and Ce at lower temperatures and indicated the improvement in redox properties of the catalyst after Ce modification. The tendency of lower reduction temperature indicates that the presence of Ce promotes surface reducibility, which could be due to strong interaction with well-dispersed CuO x . The Cu0.4/Ce0.1/HAp showed a weakening of Cu–O bond strength through the strong synergetic interaction between CuO x and Ce species. The synergistic interaction could enhance the facile redox property of the catalyst, which was responsible for the low-temperature propene oxidation.


2.1.6

X-ray Photoelectron Spectroscopy Study

The XPS spectra of Cu/HAp and Cu0.4/Ce0.1/HAp are shown in [Fig. 5]. [Table 2] shows the semiquantitative analysis of the catalysts. The deconvoluted spectra of Cu 2p showed peaks at 932.5 and 954.3 eV, corresponding to Cu1+ and Cu2+, respectively ([Fig. 5A]). However, the deconvoluted XPS peaks at 952.15 and 654.28 eV correspond to the Cu 2p1/2.[1] The four satellite peaks at 940.6, 943.2, 961.6, and 963.1 eV were observed due to the presence of CuO. The shake-up satellite peaks correspond to the major characteristics of Cu2+ species, indicating the predominant nature of Cu2+ in Cu/HAp and Cu0.4/Ce0.1/HAp catalysts. The percentage concentration of Cu2+ and Cu1+ is calculated ([Table 5]) by deconvoluted spectra using the following formula

% Cu I = A 2 / A + B × 100
% Cu II = B + A 1 / A + B × 100

where the main emission line A in [Fig. 6]. 9A contains both the Cu (II) (A1) and Cu (I) (A2) contributions. However, the satellite intensity (B) is entirely from Cu (II). A is the sum of A1 and A2, whereas B is the sum of satellite peaks.[35]

Zoom
Fig. 5 XPS spectra of Cu/HAp and Cu0.4/Ce0.1/HAp (A) Cu 2p (B) Ce 3d (C) O 1.
Table 2

Semiquantitative analysis of catalyst species with their binding energy.

Catalyst

Binding energy (eV)

Ratio Cu2+/Cu

Relative area of OL/Oa/Os (%)

Cu+1

Cu+2

OL

Oa

Os

Cu/HAp

932.5

934.3

529.6

531.0

532.2

56.1

13.4/65.9/20.7

Cu0.4/Ce0.1/HAp

932.7

934.5

529.6

530.9

532.2

58.5

13.2/68.5/18.4

Zoom
Fig. 6 FESEM and HRTEM images of (a, c, e) Cu/HAp and (b, d, f) Cu0.4/Ce0.1/HAp.

The ratio of Cu2+/Cu (Cu2+ + Cu1+) for Cu/HAp and Cu0.4/Ce0.1/HAp is 56.1 and 58.1, respectively. The addition of Ce in Cu/HAp leads to an increase in the concentration of Cu2+. Ce 3d spectra were deconvoluted into three pairs of spin-orbit doublets ([Fig. 5B]). The characteristic peaks are denoted in the range of 877-898 eV and 900-922 eV and assigned as v, v′, v″, v″′ and u, u′, u″, u″′, respectively. The v, v″′, u, and u″′ belong to Ce4+. However, the peaks assigned as v′/u′ and v″/u″ belong to Ce3+ and oxygen vacancies, respectively.[36] [37] The Cu/HAp and Cu0.4/Ce0.1/HAp showed an area ratio of Ce3+/(Ce3+ + Ce4+) 22.46% and 31.47% respectively, which indicates the presence of more Ce3+ species in Cu0.4/Ce0.1/HAp. The formation of more Cu2+ species indicates the improvement in the redox cycle between Cu and Ce. The facile redox cycle between Cu+ and Cu2+ depends on the redox cycle of Ce3+ ↔ Ce4+. These results indicate the redox equilibrium of Cu2+ + Ce3+ ↔ Cu+ + Ce4+, which could be responsible for the lower temperature oxidation of propene.

The XPS deconvoluted spectra of oxygen are shown in [Fig. 5C]. The XPS peaks observed at B.E. at 529.00–530.5, 530–531.5, and 531.5–532.5 eV correspond to the surface lattice oxygen (OL, OLattice, O2−), adsorbed oxygen (OA, O2−, O2 2−, or O), and adsorbed OH groups or molecular water on the surface of the catalysts (OS, Osurface).[38] [39] [40] The O absorbed peak ratios were quantified by integrating the peak area of all oxygen. The Cu/HAp and Cu0.4/Ce0.1/HAp showed 65.90 and 68.46% of OA, respectively. The adsorbed oxygen is reported to be active for the facile redox reaction.[41] The OA peak was observed at a lower binding energy in Cu0.4/Ce0.1/HAp. A higher concentration of adsorbed oxygen on the Cu0.4/Ce0.1/HAp catalyst surface was observed compared to the Cu/HAp, which suggested the formation of more labile oxygen after the addition of Ce. The adsorbed oxygen (OA) and improved redox cycle of Cu and Ce were responsible for the improvement in low-temperature oxidation of propene.


2.1.7

HR-TEM and SEM Study

The particle size and surface morphology of the Cu/HAp and Cu0.4/Ce0.1/HAp catalysts were observed by HRTEM and FESEM. Cu/HAp catalyst shows uniform distribution, quasi-spherical morphology, and clusters. Cu0.4/Ce0.1/HAp shows the formation of ceria nanorods along with spherical particles and clusters ([Fig. 6a, b]). The formation of nanorods favors the improvement in the redox cycle of Ce.[42] [43] [44] The results indicate that the Cu0.4/Ce0.1/HAp showed the formation of highly dispersed CuO x species with Ce nanorods, which was responsible for the low-temperature propene oxidation. The Cu/HAp showed quasi-spherical and flaky HAp particles. The quasi-spherical HAp could be due to CuO and flakes, or HAp could be due to the HAp support ([Fig. 6c]). Whereas Cu0.4/Ce0.1/HAp exhibits quasi-spherical and flake-like HAp particle formation along with Ce nanorods ([Fig. 6d]). The presence of nanorods suggests the interaction of Cu with Ce and HAp. The particle size of Cu/HAp ranges from 15 to 35 nm, whereas Cu0.4/Ce0.1/HAp exhibits a decrease in particle size within the range of 3-30 nm (see [Fig. 6c, d]). Additionally, the HR-TEM analysis of Cu/HAp reveals d-spacing values of 0.27 nm (200) and 0.25 nm (200), corresponding to HAp and CuO, respectively (see [Fig. 6e, f]). Whereas, Cu0.4/Ce0.1/HAp shows d-spacing of 0.27 nm (200), 0.23 nm (111), and 0.32 nm (111), which corresponds to HAp, CuO, and the presence of Ce rod, respectively. These results indicate that the Cu0.4/Ce0.1/HAp showed the formation of highly dispersed, smaller CuOx species with Ce nanorods, which were responsible for the low-temperature propene oxidation.



2.2

Catalytic Activity

2.2.1

Propene Oxidation

2.2.1.1

Activity of Cu/HAp and Ce-promoted Cu/HAp Catalyst Prepared by the Successive Deposition Method (Bimetallic)

The Ce-modified Cu/HAp prepared by the successive deposition method (Cu0.4/Ce0.1/HAp) showed maximum propene conversion compared to the catalyst prepared by the coprecipitation method (Cu0.4/Ce0.1/HAp). Furthermore, the concentration of Ce in Cu/HAp prepared by successive deposition methods has been optimized for the complete oxidation of propene. The results of catalyst optimization are shown in [Fig. 7] and [Table 3]. The Cu/HAp catalyst modified with 0.1 mol Ce (Cu0.4/Ce0.1/HAp) showed T light–off, T 50, and T 100 for propene oxidation to CO2 at 158, 267, and 339 °C, respectively. However, further increase in the concentration of Ce (0.2–0.4 mol), T light–off, T 50, and T 100 shifted toward higher temperature. Feng Pan et al.[45] reported that the LaFe0.8Co0.2O3 catalyst reached about 90% propene conversion at roughly 345 °C. In contrast, the catalyst developed in the present study achieves full propene oxidation at a slightly lower temperature of 339 °C, highlighting its stronger low-temperature activity.

Zoom
Fig. 7 Propene oxidation activity of Cu/HAp and Ce-promoted Cu/HAp catalyst prepared by the successive deposition method. Reaction feed: −300 ppm propene, 5% O2, He balance, GHSV = 50,000 mL g−1 h−1.
Table 3

T Light–off, T 50, and T 100 comparisons of Cu/HAp and Ce-modified Cu/HAp on propene oxidation.

Catalyst

T Light–off Temp. (°C)

T 50 (°C)

T 100 (°C)

Cu/HAp

204

290

368

Cu0.1/Ce0.4/HAp

171

291

384

Cu0.2/Ce0.3/HAp

165

282

370

Cu0.3/Ce0.2/HAp

160

277

352

Cu0.4/Ce0.1/HAp

158

267

339

The catalyst Cu-modified Ce/HAp (Ce0.3/Cu0.2/HAp) demonstrated the highest propene conversion. Additionally, the mole of Cu in the Ce/HAp made using the successive deposition approach has been adjusted to investigate the optimal Cu loading for propene oxidation. [Fig. 8] and [Table 4] display the oxidation activity of propene on various molar amounts of Cu and Ce on HAp. The Ce/HAp catalyst modified with Cu displayed T100 for the oxidation of propene by the following order, Ce/HAp (>400) > Ce0.4/Cu0.1/HAp (398 °C) > Ce0.1/Cu0.4/HAp (391 °C) > Ce0.2/Cu0.3/HAp (370 °C) > Cu/HAp (368 °C) > Ce0.3/Cu0.2/HAp (363 °C). Hence, Cu-modified Ce/HAp shows higher-temperature propene oxidation activity than Ce-modified Cu/HAp due to the more facile redox behavior of Ce and Cu.

Zoom
Fig. 8 Propene oxidation activity of Cu/HAp and Cu-promoted Ce/HAp catalysts prepared by the successive deposition method. Reaction feed: 300 ppm propene, 5% O2, He balance, GHSV = 50,000 mL g−1 h−1.
Table 4

Propene oxidation activity of Cu/HAp and Cu-promoted Ce/HAp catalysts prepared by the successive deposition method. Reaction feed: −300 ppm propene, 5% O2, He balance, GHSV = 50,000 mL g−1 h−1.

Catalyst

T Light–off Temp. (°C)

T 50 (°C)

T 100 (°C)

Cu/HAp

204

290

368

Ce/HAp

292

>400

>400

Ce0.1/Cu0.4/HAp

216

294

391

Ce0.2/Cu0.3/HAp

164

273

370

Ce0.3/Cu0.2/HAp

168

265

363

Ce0.4/Cu0.1/HAp

222

322

398

Table 5

T Light–off, T 50, and T 100 comparison of Cu/HAp and Ce-modified Cu/HAp with and without H2O.

Catalyst

T Light–off (°C)

T 50 (°C)

T 100 (°C)

Cu/HAp

204

290

368

Cu/HAp + H2O

200

277

375

Cu0.4/Ce0.1/HAp

158

267

339

Cu0.4/Ce0.1/HAp + H2O

160

302

340


2.2.1.2

Effect of H2O Addition

[Fig. 9] depicts the impact of water on Cu/HAp and Cu0.4/Ce0.1/Hap catalysts. After adding H2O to the reaction feed, the activity of propene oxidation continues to decline. Propene was converted by 50% in Cu0.4/Ce0.1/HAp at 268 °C, and with the addition of water, it shifted at 302 °C. This temperature rise is caused by water molecules obstructing the catalysts’ active sites. The FTIR spectra of the catalyst after water addition are shown in [Fig. 10]. The (PO4)3− vibrations (560 and 1028 cm−1) are shifted toward a lower frequency as a result of the adsorption of water molecules.

Zoom
Fig. 9 Propene oxidation activity of Cu/HAp and Ce-promoted Cu/HAp catalyst with and without H2O. Reaction feed: 300 ppm Propene, 0.5% H2O, 5%O2, He balance, GHSV = 50,000 mL g−1 h−1.
Zoom
Fig. 10 ATR-FTIR spectra of HAp, Cu/HAp, and Cu0.4/Ce0.1/HAp with and without H2O.

2.2.1.3

Effect of SO2 Addition

[Fig. 11] illustrates how SO2 affects Cu/HAp and Cu0.4/Ce0.1/HAp. With the addition of SO2 to the reaction feed, the activity of propene oxidation keeps declining. In Cu0.4/Ce0.1/HAp, complete (T 100) of the propene was seen at 339 °C, and with the addition of SO2, it moved to 360 °C ([Table 6]). This temperature rise is caused by SO2 molecules poisoning the catalysts’ active sites. As a result, the oxidation activity of the Cu/HAp and Cu0.4/Ce0.1/HAp catalysts decreases due to the deterioration of their active centers.

Zoom
Fig. 11 Propene oxidation activity of Cu/HAp and Ce-promoted Cu/HAp catalyst with and without SO2. Reaction feed: 300 ppm Propene, 0.5% SO2, 5% O2, He balance, GHSV = 50,000 mL g−1 h−1.
Table 6

T Light–off, T 50, and T 100 comparison of Cu/HAp and Ce-modified Cu/HAp with and without SO2.

Catalyst

T Light–off (°C)

T 50 (°C)

T 100 (°C)

Cu/HAp

204

290

368

Cu/HAp + SO2

210

340

390

Cu0.4/Ce0.1/HAp

158

268

339

Cu0.4/Ce0.1/HAp + SO2

170

315

360



2.2.2

CO Oxidation

[Fig. 12] depicts the toluene oxidation of Cu/HAp and Cu0.4/Ce0.1/HAp. The T light–off, T 50, and T 100 for Cu/HAp are recorded at 65, 158, and 200 °C, respectively. After promotion with Ce in Cu/HAp (Cu0.4/Ce0.1/HAp), the T light–off, T 50, and T 100 were measured at 50, 140, and 175 °C, respectively ([Table 7]). This low-temperature activity was noticed as a result of the synergistic interaction between Cu and Ce, which generates more labile oxygen and encourages oxidation. In addition, more labile and facile oxygen and Cu species were observed, which move CO oxidation toward low temperature. Waikar et al.[46] reported that their 0.5MnO x /0.05Ce–0.45Al2O3 catalyst achieved full CO conversion around 200 °C. Kim et al.[47] evaluated CO oxidation performance for Mn/Al2O3 and Mn–Ce/Al2O3 catalysts prepared through impregnation, reporting that the material reached 50% conversion at about 170 °C and complete conversion near 300 °C. In comparison, the catalyst developed in the present study reaches complete oxidation at a lower temperature of 175 °C, indicating a more efficient low-temperature activity.

Zoom
Fig. 12 The CO oxidation activity of Cu0.5/HAp and Cu0.4/Ce0.1/HAp. Reaction condition: −300 ppm CO, 5% O2, He balance, GHSV-50,000 mL g−1 h−1.
Table 7

T Light–off, T 50, and T 100 comparison of Cu0.5/HAp and Cu0.4/Ce0.1/HAp on CO oxidation.

Catalyst

T Light–off (°C)

T 50 (°C)

T 100 (°C)

Cu0.5/HAp

65

158

200

Cu0.4/Ce0.1/HAp

50

140

175


2.2.3

Toluene Oxidation

The toluene oxidation of Cu/HAp and Cu0.4/Ce0.1/HAp is shown in [Fig. 13]. Following promotion with Ce, the T light–off, T 50, and T 100 for Cu/HAp are observed at 160, 275, and 353 °C, respectively. T 50 and T 100 were recorded for Cu0.4/Ce0.1/HAp Tlight–off at 144, 265, and 325 °C, respectively ([Table 8]). Due to the synergistic interaction between Cu and Ce, which produces more labile oxygen and promotes oxidation, this low-temperature activity was observed.

Zoom
Fig. 13 The toluene oxidation activity of Cu0.5/HAp and Cu0.4/Ce0.1/HAp. Reaction condition: 300 ppm Toluene, 5% O2, He balance, GHSV-20,000 mL g−1 h−1.
Table 8

T Light–off, T 50, and T 100 comparison of Cu0.5/HAp and Cu0.4/Ce0.1/HAp on toluene oxidation.

Catalyst

T Light–off (°C)

T 50 (°C)

T 100 (°C)

Cu0.5/HAp

160

275

353

Cu0.4/Ce0.1/HAp

144

265

325


2.2.4

Stability Study

The stability test was performed under stationary conditions at 400 °C to evaluate the long-term stability and reproducibility of the optimized catalyst. The Cu0.4/Ce0.1/HAp showed 100% propene, CO, and toluene conversion at 400 °C, and activity was found to be stable up to 1080 min ([Fig. 14]).

Zoom
Fig. 14 Stability study of Cu0.4/Ce0.1/HAp for CO, propene, and toluene.

2.2.5

Effect of Synthesis Methods on the Ce-modified Cu/HAp Catalysts in Propene Oxidation Reaction

The propene oxidation activity comparison of Cu0.5/HAp, Cu0.4-Ce0.1/HAp, and Cu0.4/Ce0.1/HAp is shown in [Fig. 15] and [Table 9]. The Cu0.4/Ce0.1/HAp catalyst prepared by the successive deposition method (bimetallic) showed a light-off temperature (T light–off) at 158 °C. However, 50% (T 50) and 100% (T 100) propene conversion into CO2 was observed at 267 and 339 °C, respectively. Whereas, Cu0.4/Ce0.1/HAp catalyst prepared by coprecipitation showed light-off temperature, 50% and 100% propene conversion to CO2 at 171, 287, and 354 °C, respectively. The Cu0.5/HAp showed T light–off, T 50, and T 100 for propene oxidation at 204, 290, and 368 °C. These results indicate that the catalyst (Cu0.4/Ce0.1/HAp) prepared by successive deposition showed higher propene oxidation activity at a lower temperature compared to the catalyst prepared by the coprecipitation method (Cu0.4/Ce0.1/HAp) and Cu0.5/HAp.

Zoom
Fig. 15 Catalytic propene oxidation of Cu0.5/HAp, Cu0.4–Ce0.1/Hap, and Cu0.4/Ce0.1/HAp catalysts. Reaction feed: 300 ppm propene, 5% O2, He balance, GHSV = 50,000 mL g−1 h−1.
Table 9

T Light–off, T 50, and T 100 comparison of Cu0.5/HAp, Cu0.4-Ce0.1/Hap, and Cu0.4/Ce0.1/HAp with different synthesis methods on propene oxidation.

Catalyst

T Light–off

T 50 (°C)

T 100 (°C)

Cu0.5/HAp

204

290

368

Ce0.5/HAp

292

>400

>400

Cu0.4/Ce0.1–HAp DP method

216

327

400

Cu0.4/Ce0.1/HAp Bimetallic

158

267

339

Cu0.4-Ce0.1/HAp CP method

171

287

354

Ce0.1/Cu0.4/HAp Bimetallic

216

294

371

2.2.5.1

Powder X-ray Diffraction and Surface Area Study

The XRD patterns of Ce-promoted Cu/HAp catalysts synthesized by successive deposition and coprecipitation methods ([Fig. 16]) confirmed the hexagonal HAp phase (JCPDS no. 09-0432) with characteristic peaks at 2θ = 22.7–64.06°, along with CuO reflections corresponding to the monoclinic phase (JCPDS no. 48-1548). After Cu incorporation, a slight shift of the HAp peaks toward lower Bragg angles was observed, indicating lattice distortion due to metal deposition. The absence of distinct CeO2 peaks suggests either low ceria loading (Ce0.1) or overlap with HAp reflections. A more pronounced peak shift in the Cu0.4–Ce0.1/HAp (co-precipitation) catalyst implies Cu2+ substitution into the Ce4+ lattice, forming a Cu–Ce solid solution and causing lattice contraction. In contrast, the Cu0.4/Ce0.1/HAp (successive deposition) catalyst showed minimal peak shifting, suggesting the formation of dispersed CuO species over Ce/HAp, generating surface defects that enhance redox interaction. BET analysis revealed that the coprecipitated sample exhibited a higher surface area (117.7 m2 g−1) than the successive deposition catalyst (65.4 m2 g−1), likely due to Cu incorporation into the Ce lattice ([Table 10]). The coprecipitated catalyst exhibits a higher surface area because all components form together as fine, uniformly dispersed particles, which prevents pore blocking and maintains an open structure. However, successive deposition tends to coat or partially cover the support surface, leading to pore blockage and the formation of larger aggregates, which reduces the overall surface area. However, the latter’s lower surface area and stronger Cu–Ce interfacial synergy favor the formation of active oxygen species, resulting in superior low-temperature propene oxidation activity.

Zoom
Fig. 16 Powder X-ray diffraction pattern of HAp, Cu/HAp, Cu0.4-Ce0.1/HAp, and Cu0.4/Ce0.1/HAp.
Table 10

Textural properties comparison of the Ce-modified catalyst prepared by the successive deposition and coprecipitation method.

Catalyst

S BET (m2/g)

HAp

31.98

28.8

Cu/HAp

31.76

40.1

Cu0.4-Ce0.1/HAp

31.94

117.7

Cu0.4/Ce0.1/HAp

31.88

65.4


2.2.5.2

ATR-FTIR Spectra Comparison of Cu0.4-Ce0.1/HAp and Cu0.4/Ce0.1/HAp Catalysts

The attenuated total reflectance Fourier transform infrared spectra are shown in [Fig. 17]. The fundamental vibrational modes for PO4 3− in hydroxyapatite were observed around 962, 1030, and 1090 cm−1.[31] [48] The strong bands at 962 cm−1 ʋ1 were associated with stretching vibrations of the P-O mode. The larger peak at 1030 cm−1 and the smaller peak at 1090 cm−1 correspond to the PO4 3− group. However, these bands were also observed for Cu/HAp, Cu0.4/Ce0.1/HAp, and Cu0.4-Ce0.1/HAp, suggesting that the HAp structure is preserved after deposition of Cu and Ce.

Zoom
Fig. 17 ATR-FTIR spectra of HAp, Cu/HAp, Cu0.4-Ce0.1/HAp, and Cu0.4/Ce0.1/HAp.

The peak observed at 562 cm−1 corresponds to the O–P–O bond, which showed shifting to the higher wave number at 565 cm−1, whereas 1025 and 1088 cm−1, corresponding to the P–O bond showed shifting to the higher wave number at 1032 and 1090 cm−1 after doping of Cu on the HAp support (Cu/HAp). The shifting of these bands suggested the increase in P–O bond strength after the deposition of Cu on HAp. However, the catalyst prepared by successive deposition (Cu0.4/Ce0.1/HAp) showed the band at 1030 cm−1, which is lower than Cu/HAp and Cu0.4-Ce0.1/HAp (1032 cm−1). The shifting of the band indicates the weakening of the P–O bond due to the successive deposition of Cu and Ce over HAp. The shifting of bands also indicates the interaction of Ce with HAp support and forms the more labile oxygen, favorable for the oxidation of propene at a lower temperature.


2.2.5.3

H2-Temperature Program Reduction Study of Cu/HAp, Cu0.4/Ce0.1/Hap, and Cu0.4-Ce0.1/Hap

[Fig. 18] shows the reduction profiles of the Ce-modified Cu/HAp catalyst prepared by successive deposition and coprecipitation methods. The Cu/HAp sample shows the reduction peaks at the small shoulder at 210, 266, 490, and 645 °C. The peaks observed at 210 and 261 °C are attributed to the complete reduction of Cu2+ to Cu1+ and Cu1+ to Cu0. However, Cu0.4/Ce0.1/HAp showed reduction peaks at 194 and 239 °C. Whereas Cu0.4-Ce0.1/HAp showed reduction peaks at 266 °C, which corresponds to the reduction of small clusters of CuO x . The Ce-modified Cu/HAp catalyst prepared by the coprecipitation method showed the formation of smaller CuO x clusters. The absence of reduction peaks for HAp is in the temperature range of 30 to 800 °C.[49] These suggest that HAp itself does not undergo a significant reduction in this temperature range. The observed peaks between 150 and 300 °C are attributed to the stepwise reduction of CuO to Cu2O and metallic Cu.[50] [51] The high-temperature Cu reduction peak (250 and 261 °C) was observed due to the small clusters of CuO x (CuO and Cu2O). However, the reduction peak at 400 and 485 °C was due to the bulk CuO. The reduction peaks above 600 °C were due to the reduction of Ce. The Cu0.4/Ce0.1/HAp showed a reduction of CuO and Cu2O to Cu at lower temperatures compared to the Cu0.4-Ce0.1/HAp and Cu/HAp. The low-temperature reduction peak of Cu was due to the highly dispersed and facile CuO species on the catalyst surface.

Zoom
Fig. 18 H2-TPR spectra of Cu/HAp, Cu0.4-Ce0.1/HAp, and Cu0.4/Ce0.1/HAp.




3

Conclusions

The Ce-modified Cu/HAp catalysts synthesized by successive deposition (Cu0.4/Ce0.1/HAp) exhibited significantly higher low-temperature propene oxidation activity than those prepared by coprecipitation (Cu0.4Ce0.1/HAp). The optimized Ce concentration in the successive deposition catalyst promoted strong Cu–Ce interactions, enhanced Cu2+/Ce3+redox behavior, and generated more labile oxygen species. XRD, XPS, and Raman analyses confirmed the presence of smaller CuO particles, Ce3+ formation, and weaker Cu–O and P–O bonds, indicating higher oxygen mobility and surface reactivity. In contrast, the coprecipitated catalyst formed a Cu–O–Ce solid solution, reducing the surface-active Cu sites and limiting oxidation efficiency. The improved redox properties and structural synergy in Cu0.4Ce0.1/HAp make it highly effective for CO, propene, and toluene oxidation at lower temperatures, although further testing under real diesel exhaust and VOC conditions is recommended.


4

Experimental Section

4.1

Reagents

All chemicals (reagents and solvents) purchased were of analytical grade and procured from S.D. Fine, Sigma-Aldrich, and Loba Chemie and were used without further purifications. The listed chemicals and reagents are Cu (NO3)2·3H2O (99.5%, Sigma-Aldrich), Ca (NO3)2·4H2O (99.5%, S D Fine Chemicals), (NH4)2HPO4 (97%, S D Fine Chemicals), Ce (NO3)2·6H2O (99.9%, Loba Chemie), NH4OH (25% v/v, S D Fine Chemicals), and NaOH (98%, S D Fine Chemicals). Distilled water was obtained from a Milli-Q purification system.


4.2

Catalyst Preparation

The catalysts Cu x /HAp, Ce x /HAp, and Cu x /Ce(0.5–x)-HAp were synthesized using a controlled deposition–precipitation (DP) method to ensure uniform incorporation of Cu and Ce into the hydroxyapatite (HAp) matrix. Solution A was prepared by dissolving cerium nitrate hexahydrate and calcium nitrate tetrahydrate in 100 mL of deionized water, while Solution B contained diammonium hydrogen orthophosphate dissolved in 50 mL of deionized water. Both solutions were adjusted to pH 10 using 25% NH4OH and stirred at 500 rpm for 30 min. Solution B was then added dropwise into Solution A under constant stirring, forming a dense precipitate. The precipitate was washed with ethanol, dried at 100 °C for 12 h, and calcined at 400 °C for 4 h to obtain Ce x -HAp. For copper incorporation, 2.0 g of HAp or Ce x -HAp (0.5 mol) was dispersed in 100 mL of deionized water, and an aqueous solution of copper nitrate trihydrate was added dropwise while maintaining pH 10 with 25% NH4OH. The slurry was stirred at 500 rpm for 24 h, washed thoroughly, dried at 100 °C for 12 h, and calcined at 400 °C for 4 h. This synthesis method demonstrates its potential for crafting catalysts enriched with Copper (Cu) supported on either HAp or Ce x -HAp, offering promising prospects for diverse applications and thorough investigations in the field.

The bimetallic catalysts denoted as Cu x /Ce(0.5–x)/HAp0.5 were synthesized using a successive impregnation method, based on a previously reported hydroxyapatite (HAp) synthesis procedure.[1] [21] Initially, HAp was prepared following the established method. For bimetallic catalyst preparation (x = 0.1, 0.2, 0.3, 0.4), the required amount of cerium nitrate hexahydrate [Ce(NO3)3·6H2O] was dissolved in 10 mL of distilled water and added to a 0.5 mol aqueous slurry of HAp. The suspension was stirred at 600 rpm for 24 h while maintaining a pH of 10 using 25% NH4OH. The resulting mixture was filtered, dried at 100 °C for 12 h, and calcined at 400 °C for 4 h to obtain Ce0.5/HAp. In the second impregnation step, an aqueous solution of copper nitrate trihydrate [Cu(NO3)2·3H2O] was added to a 100 mL slurry of Ce0.5/HAp under the same conditions (pH 10, 600 rpm). After 24 h of stirring, the mixture was filtered, dried at 100 °C for 12 h, and calcined at 400 °C for 4 h, yielding the Cu x /Ce(0.5–x)/HAp0.5 catalysts with varying Cu loadings (x = 0.1–0.4). Monometallic catalysts (Cu/HAp and Ce/HAp) were also synthesized using the same method by depositing 0.5 mol of either Cu or Ce on HAp. Similarly, the Cu x /Ce(0.5–x)/HAp0.5 catalysts were prepared by reversing the impregnation sequence. Initially, Cu was impregnated on HAp to form Cu0.5/HAp, followed by Ce incorporation using the same conditions of pH, stirring, drying, and calcination. For comparison, Cu x Ce(0.5–x)/HAp catalysts were also synthesized via a coprecipitation (CP) method.[52] In this process, calculated moles of Cu and Ce precursors were dissolved separately in 10 mL of distilled water and added dropwise into an aqueous HAp slurry (0.5 mol). The pH was maintained at 10 using 25% NH4OH, with continuous stirring at 600 rpm for 24 h. The obtained precipitate was filtered, dried at 100 °C for 12 h, and calcined at 400 °C for 4 h, resulting in the Cu x Ce(0.5–x)/HAp catalysts (x = 0.1–0.5).


4.3

Catalytic Activity Testing

The catalytic oxidation of propene as a model diesel engine exhaust and VOC was performed under atmospheric pressure by using a fixed-bed tubular downflow reactor. About 0.5 g of prepared catalyst was diluted with 2.0 g silica gel having a size of 60-120 mesh. Before the propene oxidation, the catalyst was pretreated in 10% O2 with helium balance for 1 h at 400 °C. The reaction feed consists of 300 ppm (CO/propene/toluene), 5% O2, and helium balance passed over the catalyst at 50,000 mL g−1 h−1. The catalyst performance was evaluated at 30–400 °C @ 2 °C min−1. The concentration of the gaseous feed was analyzed online by using micro-GC (Agilent 490) equipped with a thermal conductivity detector (TCD) and Porapack Q, MS-5A, and CP Sil 5CB columns. The CO, propene, and toluene conversions were calculated from their initial and final concentrations using the following formula.

% X conversion = X Initial X Final X × 100 %

where, X is CO, propene, and toluene.


4.4

Catalyst Characterizations

The X-ray diffraction patterns of the catalyst were obtained in the range of 2θ 20° to 80° with a step size of 0.02° and scan rate of 4° min−1 (Shimadzu XRD 6100 Cu Kα, λ = 1.54 Å, 40 kV, 30 mA). The nitrogen adsorption was determined on Smart Sorb 92/93 equipment from Smart Instrument Co. The catalyst was preheated at 250 °C in an environment of N2 purging for 90 min, followed by N2 adsorption. The Fourier transform infrared spectroscopy (FTIR) systematically monitors the variations of structural characteristic groups. The IR spectra were obtained using a Perkin Elmer (spectrum two) instrument in the range of 400–4000 cm−1. The redox properties of catalyst reducibility can be examined by hydrogen temperature programmed reduction (H2-TPR). The Micromeritics AutoChem II instrument with thermal conductivity detector (TCD) was used for the H2-TPR study. In typical TPR, the catalyst was pretreated in 10% O2 with He balance from room temperature to 400 °C. The catalyst was further heated in the temperature range of 50–800 °C in 5% H2 with Ar balance @ 20 mL min−1. Furthermore, the Raman spectra were recorded using a Raman spectrometer (Labram HR 800, Horiba Jobin Yvon) with an Ar laser (514.5 nm) in the range of 3000–10 cm−1. The X-ray photoelectron spectroscopy (XPS) was performed on a Kratos Analytical instrument (Model AXIS Supra) having a Monochromatic (AlKα) 600 W X-ray source; 1486.6 eV. The background correction was done by C1s peak at 284.8 eV. The SEM analysis was performed using the JEOL JSM-7600 (FEG-SEM) instrument. The high-resolution transmission electron microscopy (HR-TEM) study was done by using the FEI Tecnai G2 F30 instrument at 300 kV.




Contributors’ Statement

R.M.: Data curation, Formal analysis, Investigation, Writing – original draft. K.P.: Data curation, Writing – original draft. R.P.: Data curation, Writing – original draft. P.M.: Conceptualization, Data curation, Funding acquisition, Project administration, Supervision, Validation, Writing – review & editing.

Conflict of Interest

The authors declare that they have no conflict of interest.

Acknowledgement

Science and Engineering Research Board, Department of Science and Technology, Delhi, India, is acknowledged for financial support provided as an “Empowerment and equity opportunities for excellence in Science” having the sanction order no. EEQ/2016/000264.

  • References

  • 1 More RK, Lavande NR, More PM. Mol Catal 2019; 474: 110414
  • 2 Gennequin C, Lamallem M, Cousin R, Siffert S, Aïssi F, Aboukaïs A. Catal Today 2007; 122 (03/04) 301-306
  • 3 Lavande NR, More RK, More PM. Appl Surf Sci 2019; 2020: 502
  • 4 More R, More P. Bimetallic co and Mn Supported on Hydroxyapatite Catalyst for Carbon Monoxide Oxidation at Lower Temperature. 2021.
  • 5 Morgott DA. Int J Environ Res Public Health 2018; 15 (01)
  • 6 Reşitoğlu İA, Altinişik K, Keskin A. Clean Techn Environ Policy 2015; 17 (01) 15-27
  • 7 Labaki M, Siffert S, Lamonier JF, Zhilinskaya EA, Aboukaïs A. Appl Catal B Environ 2003; 43 (03) 261-271
  • 8 Gluhoi AC, Bogdanchikova N, Nieuwenhuys BE. Catal Today 2006; 113 (03/04) 178-181
  • 9 Twigg MV. Platin Met Rev 2010; 54 (03) 180-183
  • 10 Castoldi L, Matarrese R, Lietti L, Forzatti P. Appl Catal B Environ 2006; 64 (01/02) 25-34
  • 11 Granger P. Cat Sci Technol 2017; 7 (22) 5195-5211
  • 12 Cabello Galisteo F, Mariscal R, López Granados M. et al. Appl Catal B Environ 2007; 72 (03/04) 272-281
  • 13 Stein HJ. Appl Catal B Environ 1996; 10 (01/03) 69-82
  • 14 Wang W, McCool G, Kapur N. et al. Science 2012; 337 (6096) 832-835
  • 15 Binder AJ, Toops TJ, Unocic RR, Parks JE, Dai S. Angew Chem, Int Ed 2015; 54 (45) 13263-13267
  • 16 Boukha Z, González-Velasco JR, Gutiérrez-Ortiz MA. Appl Catal B Environ 2022; 312: 121384
  • 17 Kim M, Park E, Jurng J. Powder Technol 2018; 325 (25) C 368-372
  • 18 Tanaka H, Mizuno N, Misono M. Appl Catal A Gen 2003; 244 (02) 371-382
  • 19 Boukha Z, González-Prior J, de Rivas B, González-Velasco JR, López-Fonseca R, Gutiérrez-Ortiz JI. Appl Catal B Environ 2016; 190: 125-136
  • 20 Gluhoi AC, Bogdanchikova N, Nieuwenhuys BE. J Catal 2005; 229 (01) 154-162
  • 21 More R, Lavande N, More P. Catal Lett 2020; 150
  • 22 Trovarelli A. Catal Rev 1996; 38 (04) 439-520
  • 23 More RK, Lavande NR, More PM. Catal Commun 2018; 116: 52-56
  • 24 Zhang R, Haddadin T, Rubiano DP, Nair H, Polster CS, Baertsch CD. ACS Catal 2011; 1 (05) 519-525
  • 25 Boukha Z, Ayastuy JL, Iglesias-González A, Pereda-Ayo B, Gutiérrez-Ortiz MA, González-Velasco JR. Appl Catal B Environ 2014; 160–161 (01) 629-640
  • 26 Zhu H, Chen Y, Wang Z, Liu W, Wang L. RSC Adv 2018; 8 (27) 14888-14897
  • 27 Ayastuy JL, Gurbani A, González-Marcos MP, Gutiérrez-Ortiz MA. Appl Catal A Gen 2010; 387 (1/2) 119-128
  • 28 Védrine JC, Fechete I. C R Chim 2016; 19 (10) 1203-1225
  • 29 Bensaid S, Piumetti M, Novara C. et al. Nanoscale Res Lett 2016; 11 (01) 1-14
  • 30 More RK, Lavande NR, More PM. Mol Catal 2019; 474: 110414
  • 31 More RKMNRLPM. Catal Lett 2020; 150 (02) 419-428
  • 32 Chlala D, Giraudon J-M, Nuns N. et al. Appl Catal B Environ 2016; 184: 87-95
  • 33 Adegoke KA, Maxakato NW. Mater Today Energy 2021; 21: 100816
  • 34 Ram LA. Molecules 2022; 27: 6659
  • 35 Biesinger MC, Lau LWM, Gerson AR, Smart RSC. Appl Surf Sci 2010; 257 (03) 887-898
  • 36 Davis KA, Yoo S, Shuler EW, Sherman BD, Lee S. Nano Converg 2021;
  • 37 Pawar K, Megha B, More P. Chem – Asian J 2025; 00698
  • 38 Waikar JM, More RK, Lavande NR, More PM. J Rare Earths 2021; 39 (04) 434-439
  • 39 Dissanayake D, Achola LA, Kerns P. et al. Appl Catal B Environ 2019; 249: 32-41
  • 40 Pagare R, More P. Catal Surv Asia 2025;
  • 41 More RK, Lavande NR, More PM. Bull Mater Sci 2020; 43 (01) 164
  • 42 Konsolakis M. Appl Catal B Environ 2016; 198: 49-66
  • 43 Lykaki M, Papista E, Carabineiro S, Tavares P, Konsolakis M. Cat Sci Technol 2018; 8
  • 44 Wang W-W, Yu W-Z, Du P. et al. ACS Catal 2017; 7
  • 45 Pan F, Zhang W, Ferronato C, Giroir-fendler A. Appl Catal A: Gen. 2022 643.
  • 46 Waikar J, More P. Appl Surf Sci. 2022 7.
  • 47 Sung T, Se K, Jeong J, Park JH. Met Mater Int 2020; 26 (12) 1872-1880
  • 48 More RK, Lavande NR, More PM. Mol Catal 2019; 474: 110414
  • 49 Guo J, Yu H, Dong F, Zhu B, Huang W. RSC Adv 2017; 45420-45431
  • 50 Tavares PB, Konsolakis M. Promotion 2018; 2312-2322
  • 51 Waikar JM, More RK, Lavande NR, More PM. J Rare Earths 2021; 39 (04) 434-439
  • 52 Widegren JA, Finke RG. J Mol Catal A – Chem 2003; 198: 317-341

Correspondence

Dr. Pavan More
Department of Chemistry, Institute of Chemical Technology
400019 Mumbai
India   

Publication History

Received: 05 November 2025

Accepted after revision: 16 January 2026

Accepted Manuscript online:
16 January 2026

Article published online:
05 February 2026

© 2026. The Author(s). This is an open access article published by Thieme under the terms of the Creative Commons Attribution License, permitting unrestricted use, distribution, and reproduction so long as the original work is properly cited. (https://creativecommons.org/licenses/by/4.0/).

Georg Thieme Verlag KG
Oswald-Hesse-Straße 50, 70469 Stuttgart, Germany

Bibliographical Record
Rahul More, Kajal Pawar, Rushikesh Pagare, Pavan More. Complete Oxidation of CO, Propene, and Toluene as Model Components of Diesel Engine Exhaust and VOC using Ceria-modified Cu/Hydroxyapatite: Effect of Preparation Methods and Ce Concentration. Sustainability & Circularity NOW 2026; 03: a27913831.
DOI: 10.1055/a-2791-3831
  • References

  • 1 More RK, Lavande NR, More PM. Mol Catal 2019; 474: 110414
  • 2 Gennequin C, Lamallem M, Cousin R, Siffert S, Aïssi F, Aboukaïs A. Catal Today 2007; 122 (03/04) 301-306
  • 3 Lavande NR, More RK, More PM. Appl Surf Sci 2019; 2020: 502
  • 4 More R, More P. Bimetallic co and Mn Supported on Hydroxyapatite Catalyst for Carbon Monoxide Oxidation at Lower Temperature. 2021.
  • 5 Morgott DA. Int J Environ Res Public Health 2018; 15 (01)
  • 6 Reşitoğlu İA, Altinişik K, Keskin A. Clean Techn Environ Policy 2015; 17 (01) 15-27
  • 7 Labaki M, Siffert S, Lamonier JF, Zhilinskaya EA, Aboukaïs A. Appl Catal B Environ 2003; 43 (03) 261-271
  • 8 Gluhoi AC, Bogdanchikova N, Nieuwenhuys BE. Catal Today 2006; 113 (03/04) 178-181
  • 9 Twigg MV. Platin Met Rev 2010; 54 (03) 180-183
  • 10 Castoldi L, Matarrese R, Lietti L, Forzatti P. Appl Catal B Environ 2006; 64 (01/02) 25-34
  • 11 Granger P. Cat Sci Technol 2017; 7 (22) 5195-5211
  • 12 Cabello Galisteo F, Mariscal R, López Granados M. et al. Appl Catal B Environ 2007; 72 (03/04) 272-281
  • 13 Stein HJ. Appl Catal B Environ 1996; 10 (01/03) 69-82
  • 14 Wang W, McCool G, Kapur N. et al. Science 2012; 337 (6096) 832-835
  • 15 Binder AJ, Toops TJ, Unocic RR, Parks JE, Dai S. Angew Chem, Int Ed 2015; 54 (45) 13263-13267
  • 16 Boukha Z, González-Velasco JR, Gutiérrez-Ortiz MA. Appl Catal B Environ 2022; 312: 121384
  • 17 Kim M, Park E, Jurng J. Powder Technol 2018; 325 (25) C 368-372
  • 18 Tanaka H, Mizuno N, Misono M. Appl Catal A Gen 2003; 244 (02) 371-382
  • 19 Boukha Z, González-Prior J, de Rivas B, González-Velasco JR, López-Fonseca R, Gutiérrez-Ortiz JI. Appl Catal B Environ 2016; 190: 125-136
  • 20 Gluhoi AC, Bogdanchikova N, Nieuwenhuys BE. J Catal 2005; 229 (01) 154-162
  • 21 More R, Lavande N, More P. Catal Lett 2020; 150
  • 22 Trovarelli A. Catal Rev 1996; 38 (04) 439-520
  • 23 More RK, Lavande NR, More PM. Catal Commun 2018; 116: 52-56
  • 24 Zhang R, Haddadin T, Rubiano DP, Nair H, Polster CS, Baertsch CD. ACS Catal 2011; 1 (05) 519-525
  • 25 Boukha Z, Ayastuy JL, Iglesias-González A, Pereda-Ayo B, Gutiérrez-Ortiz MA, González-Velasco JR. Appl Catal B Environ 2014; 160–161 (01) 629-640
  • 26 Zhu H, Chen Y, Wang Z, Liu W, Wang L. RSC Adv 2018; 8 (27) 14888-14897
  • 27 Ayastuy JL, Gurbani A, González-Marcos MP, Gutiérrez-Ortiz MA. Appl Catal A Gen 2010; 387 (1/2) 119-128
  • 28 Védrine JC, Fechete I. C R Chim 2016; 19 (10) 1203-1225
  • 29 Bensaid S, Piumetti M, Novara C. et al. Nanoscale Res Lett 2016; 11 (01) 1-14
  • 30 More RK, Lavande NR, More PM. Mol Catal 2019; 474: 110414
  • 31 More RKMNRLPM. Catal Lett 2020; 150 (02) 419-428
  • 32 Chlala D, Giraudon J-M, Nuns N. et al. Appl Catal B Environ 2016; 184: 87-95
  • 33 Adegoke KA, Maxakato NW. Mater Today Energy 2021; 21: 100816
  • 34 Ram LA. Molecules 2022; 27: 6659
  • 35 Biesinger MC, Lau LWM, Gerson AR, Smart RSC. Appl Surf Sci 2010; 257 (03) 887-898
  • 36 Davis KA, Yoo S, Shuler EW, Sherman BD, Lee S. Nano Converg 2021;
  • 37 Pawar K, Megha B, More P. Chem – Asian J 2025; 00698
  • 38 Waikar JM, More RK, Lavande NR, More PM. J Rare Earths 2021; 39 (04) 434-439
  • 39 Dissanayake D, Achola LA, Kerns P. et al. Appl Catal B Environ 2019; 249: 32-41
  • 40 Pagare R, More P. Catal Surv Asia 2025;
  • 41 More RK, Lavande NR, More PM. Bull Mater Sci 2020; 43 (01) 164
  • 42 Konsolakis M. Appl Catal B Environ 2016; 198: 49-66
  • 43 Lykaki M, Papista E, Carabineiro S, Tavares P, Konsolakis M. Cat Sci Technol 2018; 8
  • 44 Wang W-W, Yu W-Z, Du P. et al. ACS Catal 2017; 7
  • 45 Pan F, Zhang W, Ferronato C, Giroir-fendler A. Appl Catal A: Gen. 2022 643.
  • 46 Waikar J, More P. Appl Surf Sci. 2022 7.
  • 47 Sung T, Se K, Jeong J, Park JH. Met Mater Int 2020; 26 (12) 1872-1880
  • 48 More RK, Lavande NR, More PM. Mol Catal 2019; 474: 110414
  • 49 Guo J, Yu H, Dong F, Zhu B, Huang W. RSC Adv 2017; 45420-45431
  • 50 Tavares PB, Konsolakis M. Promotion 2018; 2312-2322
  • 51 Waikar JM, More RK, Lavande NR, More PM. J Rare Earths 2021; 39 (04) 434-439
  • 52 Widegren JA, Finke RG. J Mol Catal A – Chem 2003; 198: 317-341

Zoom
Fig. 1 Powder X-ray diffraction patterns of HAp, Cu/HAp, and Cu x /Ce0.5−x /HAp.
Zoom
Fig. 2 ATR-FTIR spectra of HAp and Ce-modified Cu/HAp.
Zoom
Fig. 3 Raman spectra of Cu/HAp, Ce/Hap, and Ce-modified Cu/HAp.
Zoom
Fig. 4 H2-TPR spectra of Cu/HAp and Ce-modified Cu/HAp.
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Fig. 5 XPS spectra of Cu/HAp and Cu0.4/Ce0.1/HAp (A) Cu 2p (B) Ce 3d (C) O 1.
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Fig. 6 FESEM and HRTEM images of (a, c, e) Cu/HAp and (b, d, f) Cu0.4/Ce0.1/HAp.
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Fig. 7 Propene oxidation activity of Cu/HAp and Ce-promoted Cu/HAp catalyst prepared by the successive deposition method. Reaction feed: −300 ppm propene, 5% O2, He balance, GHSV = 50,000 mL g−1 h−1.
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Fig. 8 Propene oxidation activity of Cu/HAp and Cu-promoted Ce/HAp catalysts prepared by the successive deposition method. Reaction feed: 300 ppm propene, 5% O2, He balance, GHSV = 50,000 mL g−1 h−1.
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Fig. 9 Propene oxidation activity of Cu/HAp and Ce-promoted Cu/HAp catalyst with and without H2O. Reaction feed: 300 ppm Propene, 0.5% H2O, 5%O2, He balance, GHSV = 50,000 mL g−1 h−1.
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Fig. 10 ATR-FTIR spectra of HAp, Cu/HAp, and Cu0.4/Ce0.1/HAp with and without H2O.
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Fig. 11 Propene oxidation activity of Cu/HAp and Ce-promoted Cu/HAp catalyst with and without SO2. Reaction feed: 300 ppm Propene, 0.5% SO2, 5% O2, He balance, GHSV = 50,000 mL g−1 h−1.
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Fig. 12 The CO oxidation activity of Cu0.5/HAp and Cu0.4/Ce0.1/HAp. Reaction condition: −300 ppm CO, 5% O2, He balance, GHSV-50,000 mL g−1 h−1.
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Fig. 13 The toluene oxidation activity of Cu0.5/HAp and Cu0.4/Ce0.1/HAp. Reaction condition: 300 ppm Toluene, 5% O2, He balance, GHSV-20,000 mL g−1 h−1.
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Fig. 14 Stability study of Cu0.4/Ce0.1/HAp for CO, propene, and toluene.
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Fig. 15 Catalytic propene oxidation of Cu0.5/HAp, Cu0.4–Ce0.1/Hap, and Cu0.4/Ce0.1/HAp catalysts. Reaction feed: 300 ppm propene, 5% O2, He balance, GHSV = 50,000 mL g−1 h−1.
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Fig. 16 Powder X-ray diffraction pattern of HAp, Cu/HAp, Cu0.4-Ce0.1/HAp, and Cu0.4/Ce0.1/HAp.
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Fig. 17 ATR-FTIR spectra of HAp, Cu/HAp, Cu0.4-Ce0.1/HAp, and Cu0.4/Ce0.1/HAp.
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Fig. 18 H2-TPR spectra of Cu/HAp, Cu0.4-Ce0.1/HAp, and Cu0.4/Ce0.1/HAp.