journal article·2025-09-12

Structural Evolution of Tin Dioxide Nanoparticles under Acoustic Shocked Conditions for Aerospace Applications─Implications of Other Rutile-Type Dioxides Based on Superheating Approaches

Sivakumar Aswathappa, Lidong Dai, Sahaya Jude Dhas Sathiyadhas, Raju Suresh Kumar, Abdulrahman I. Almansour, Sabarinathan Arumugam, Muthu Devaraj, Mowlika Varadhappa Reddy

ACS Applied Nano Materials· Volume 8· Issue 36
Publisher page

Abstract

Nanoscale materials have wide applications in extreme conditions, including those related to aerospace- and defense-based technological aspects. However, for these kinds of applications, the sustainability of the crystal structure and related properties is highly required. In the present work, we investigate the rutile-type hexagonal-shaped SnO 2 NPs’ crystallographic, optical, and magnetic structural stabilities under acoustic shock wave-loaded conditions, and the observed structural stability results are compared with similar hexagonal-shaped rutile-type TiO 2 NPs under shocked conditions. From the observed X-ray diffraction results of the SnO 2 NPs, the rutile space group P 4 2 / mnm remains constant at 200 shock conditions without any structural deformations and distortions. The band gap energy is slightly increased due to the formation of surface defects, and the obtained values of band gap energy are found to be 3.55, 3.61, and 3.72 eV for the 0, 100, and 200 shocked conditions, respectively. According to the magnetic property results, the weak ferromagnetic state remains unaltered, and the thermal stability of the SnO 2 NPs is also unchanged, which demonstrates the absence of structural phase transitions under shocked conditions. However, the similar analogue-structured material of rutile-TiO 2 NPs transformed to the anatase phase after exposure to 90 shocks. Based on the observed overall structure–property stabilities and relationships of the SnO 2 and TiO 2 NPs, SnO 2 NPs have a high degree of structural stability under dynamic shocked conditions because of their higher thermal conductivity, and the observed results are discussed based on the shock wave-induced superheating approach. Due to their impressive stability profiles, SnO 2 NPs are highly deserving candidates for applications in extreme conditions, which include aerospace, defense, laser operation, and gas sensing.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Laser-Ablation Synthesis of Nanoparticles · Energetic Materials and Combustion · Rocket and propulsion systems research

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

Key Laboratory of High-Temperature and High-Pressure Study of the Earth’s Interior

Institute of Geochemistry, Chinese Academy of Sciences

Saveetha School of Engineering, Saveetha Institute of Medical and Technical Sciences

Saveetha University

Department of Chemistry, College of Science, King Saud University, P.O. Box 2455, Riyadh 11451, Saudi Arabia

Department of Physics

Sri Moogambigai Arts and Science College for Women

Environment Research Institute

Shandong University

Department of Physics, Er. Perumal Manimekalai College of Engineering, Koneripalli, Hosur, Tamil Nadu 635117, India

Funding

King Saud University · National Natural Science Foundation of China

References (69)

Show source-provided references
1. 10.1038/nmat176010.1038/nmat1760 ↗
2. 10.1016/j.scriptamat.2019.06.00510.1016/j.scriptamat.2019.06.005 ↗
3. 10.1021/jp067443v10.1021/jp067443v ↗
4. 10.1016/j.ssc.2007.11.00710.1016/j.ssc.2007.11.007 ↗
5. 10.1038/s41598-020-66340-y10.1038/s41598-020-66340-y ↗
6. 10.1038/nmat186310.1038/nmat1863 ↗
7. 10.1016/j.ceramint.2025.01.43310.1016/j.ceramint.2025.01.433 ↗
8. 10.1016/j.msea.2015.11.07410.1016/j.msea.2015.11.074 ↗
9. 10.1088/0034-4885/59/1/00210.1088/0034-4885/59/1/002 ↗
10. 10.1016/j.matlet.2018.02.06410.1016/j.matlet.2018.02.064 ↗
11. 10.1016/j.ceramint.2021.12.05510.1016/j.ceramint.2021.12.055 ↗
12. 10.1021/acs.cgd.0c0021410.1021/acs.cgd.0c00214 ↗
13. 10.1016/j.surfin.2022.10242210.1016/j.surfin.2022.102422 ↗
14. 10.1016/j.ceramint.2024.08.46710.1016/j.ceramint.2024.08.467 ↗
15. 10.1007/s10948-020-05435-z10.1007/s10948-020-05435-z ↗
16. 10.1021/acs.inorgchem.3c0346110.1021/acs.inorgchem.3c03461 ↗
17. 10.1007/s10854-020-04555-510.1007/s10854-020-04555-5 ↗
18. 10.1039/D2DT01101H10.1039/D2DT01101H ↗
19. 10.1016/j.jtice.2025.10610510.1016/j.jtice.2025.106105 ↗
20. 10.1016/j.molstruc.2024.13921510.1016/j.molstruc.2024.139215 ↗
21. 10.1021/acs.inorgchem.4c0272310.1021/acs.inorgchem.4c02723 ↗
22. 10.1007/s40097-019-00313-010.1007/s40097-019-00313-0 ↗
23. 10.1088/2053-1591/aafae610.1088/2053-1591/aafae6 ↗
24. 10.1021/acs.jpcc.0c0214610.1021/acs.jpcc.0c02146 ↗
25. 10.1016/j.ceramint.2021.09.28110.1016/j.ceramint.2021.09.281 ↗
26. 10.1007/s00339-022-05426-y10.1007/s00339-022-05426-y ↗
27. 10.1016/j.heliyon.2022.e0965310.1016/j.heliyon.2022.e09653 ↗
28. 10.1063/1.187135510.1063/1.1871355 ↗
29. 10.1021/acs.jpcc.7b0447710.1021/acs.jpcc.7b04477 ↗
30. 10.1016/j.ceramint.2016.02.09210.1016/j.ceramint.2016.02.092 ↗
31. 10.1007/s11051-012-0750-710.1007/s11051-012-0750-7 ↗
32. 10.1016/j.jpcs.2005.05.07910.1016/j.jpcs.2005.05.079 ↗
33. 10.1021/acs.jpcc.1c0677010.1021/acs.jpcc.1c06770 ↗
34. 10.1103/PhysRevB.72.21210210.1103/PhysRevB.72.212102 ↗
35. 10.1103/PhysRevB.73.01410510.1103/PhysRevB.73.014105 ↗
36. 10.1016/j.cplett.2009.08.06010.1016/j.cplett.2009.08.060 ↗
37. 10.1002/pssb.20145103610.1002/pssb.201451036 ↗
38. 10.1103/PhysRevB.55.1114410.1103/PhysRevB.55.11144 ↗
39. 10.1038/s41598-018-22965-810.1038/s41598-018-22965-8 ↗
40. 10.1021/acsomega.1c0706310.1021/acsomega.1c07063 ↗
41. 10.1016/j.matpr.2022.06.07510.1016/j.matpr.2022.06.075 ↗
42. 10.1007/s41314-019-0033-510.1007/s41314-019-0033-5 ↗
43. 10.1016/j.actamat.2025.12074210.1016/j.actamat.2025.120742 ↗
44. 10.1016/j.diamond.2024.11168010.1016/j.diamond.2024.111680 ↗
45. 10.1021/acs.cgd.3c0118010.1021/acs.cgd.3c01180 ↗
46. 10.1039/D4CP03750B10.1039/D4CP03750B ↗
47. 10.1039/D1CE01118A10.1039/D1CE01118A ↗
48. 10.1016/j.saa.2025.12623410.1016/j.saa.2025.126234 ↗
49. 10.1063/1.138557310.1063/1.1385573 ↗
50. 10.1016/j.ssc.2011.03.02910.1016/j.ssc.2011.03.029 ↗
51. 10.1103/PhysRevB.70.13410210.1103/PhysRevB.70.134102 ↗
52. 10.1021/acs.jpcc.7b0407910.1021/acs.jpcc.7b04079 ↗
53. 10.1103/PhysRevB.67.17411010.1103/PhysRevB.67.174110 ↗
54. 10.1016/j.physb.2020.41216910.1016/j.physb.2020.412169 ↗
55. 10.1016/j.physrep.2018.04.00210.1016/j.physrep.2018.04.002 ↗
56. 10.1016/j.materresbull.2023.11263610.1016/j.materresbull.2023.112636 ↗
57. 10.1016/j.solidstatesciences.2020.10634010.1016/j.solidstatesciences.2020.106340 ↗
58. 10.1039/c2ra20586f10.1039/c2ra20586f ↗
59. 10.1107/S002188989601145410.1107/S0021889896011454 ↗
60. 10.1063/1.165575210.1063/1.1655752 ↗
61. 10.1016/j.molstruc.2024.13849010.1016/j.molstruc.2024.138490 ↗
62. 10.1038/ncomms1066110.1038/ncomms10661 ↗
63. 10.1016/0022-3697(81)90074-310.1016/0022-3697(81)90074-3 ↗
64. 10.1016/j.diamond.2025.11203410.1016/j.diamond.2025.112034 ↗
65. 10.1016/j.jeurceramsoc.2006.04.06810.1016/j.jeurceramsoc.2006.04.068 ↗
66. 10.1016/j.ssc.2011.12.01710.1016/j.ssc.2011.12.017 ↗
67. 10.1016/j.physb.2014.12.02010.1016/j.physb.2014.12.020 ↗
68. 10.1016/j.jallcom.2013.10.23810.1016/j.jallcom.2013.10.238 ↗
69. 10.1016/0022-3697(91)90003-I10.1016/0022-3697(91)90003-I ↗