journal article·2023-07-12Open access

Exploring the Origin of the Thermal Sensitivity of Near-Infrared-II Emitting Rare Earth Nanoparticles

Khouloud Hamraoui, Vivian Andrea Torres-Vera, Irene Zabala Gutierrez, Alejandro Casillas-Rubio, Mohammed Alqudwa Fattouh, Antonio Benayas, Riccardo Marin, Marta Maria Natile, Miguel Manso Silvan, Juan Rubio-Zuazo, Daniel Jaque, Sonia Melle, Oscar G. Calderón, Jorge Rubio-Retama

ACS Applied Materials & Interfaces· Volume 15· Issue 27

Abstract

Rare-earth doped nanoparticles (RENPs) are attracting increasing interest in materials science due to their optical, magnetic, and chemical properties. RENPs can emit and absorb radiation in the second biological window (NIR-II, 1000-1400 nm) making them ideal optical probes for photoluminescence (PL) in vivo imaging. Their narrow emission bands and long PL lifetimes enable autofluorescence-free multiplexed imaging. Furthermore, the strong temperature dependence of the PL properties of some of these RENPs makes remote thermal imaging possible. This is the case of neodymium and ytterbium co-doped NPs that have been used as thermal reporters for in vivo diagnosis of, for instance, inflammatory processes. However, the lack of knowledge about how the chemical composition and architecture of these NPs influence their thermal sensitivity impedes further optimization. To shed light on this, we have systematically studied their emission intensity, PL decay time curves, absolute PL quantum yield, and thermal sensitivity as a function of the core chemical composition and size, active-shell, and outer-inert-shell thicknesses. The results revealed the crucial contribution of each of these factors in optimizing the NP thermal sensitivity. An optimal active shell thickness of around 2 nm and an outer inert shell of 3.5 nm maximize the PL lifetime and the thermal response of the NPs due to the competition between the temperature-dependent back energy transfer, the surface quenching effects, and the confinement of active ions in a thin layer. These findings pave the way for a rational design of RENPs with optimal thermal sensitivity.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Luminescence Properties of Advanced Materials · Optical properties and cooling technologies in crystalline materials · Nanoplatforms for cancer theranostics

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

Affiliations

Department of Chemistry in Pharmaceutical Sciences, Complutense University of Madrid, E-28040 Madrid, Spain

Department of Optics, Complutense University of Madrid, E-28037 Madrid, Spain

Nanobiology Group, Instituto Ramón y Cajal de Investigación Sanitaria, IRYCIS, 28034 Madrid, Spain

Departamento de Física de Materiales, Universidad Autónoma de Madrid, 28049 Madrid, Spain

Dipartimento di Scienze Chimiche, Università di Padova, 35131 Padova, Padua, Italy

Istituto di Chimica della Materia Condensata e Tecnologie per l’Energia (ICMATE), Consiglio Nazionale delle Ricerche (CNR), 35131 Padova, Padua, Italy

Departamento de Física Aplicada, Universidad Autónoma de Madrid, 28049 Madrid, Spain

Spanish CRG BM25-SpLine Beamline at the ESRF, 38043 Grenoble, France

Instituto de Ciencias de los Materiales de Madrid-Consejo Superior de Investigaciones Científicas, Cantoblanco, 28049 Madrid, Spain

Institute for Advanced Research in Chemical Sciences (IAdChem), Universidad Autónoma de Madrid, Madrid 28049, Spain

Funding

Comunidad de Madrid · Universidad Complutense de Madrid · Ministerio de Ciencia e Innovaci?n · Agencia Espa?ola de Cooperaci?n Internacional para el Desarrollo · Horizon 2020 Framework Programme

References (49)

Show source-provided references
1. 10.1002/adom.20180141710.1002/adom.201801417 ↗
2. 10.1002/adma.20160543410.1002/adma.201605434 ↗
3. 10.1038/s41427-018-0065-y10.1038/s41427-018-0065-y ↗
4. 10.1021/am507591u10.1021/am507591u ↗
5. 10.1016/j.cis.2017.06.00310.1016/j.cis.2017.06.003 ↗
6. 10.1039/c2cs35288e10.1039/c2cs35288e ↗
7. 10.1021/acs.inorgchem.6b0002010.1021/acs.inorgchem.6b00020 ↗
8. 10.1021/nn202490m10.1021/nn202490m ↗
9. 10.1021/acsami.0c1551410.1021/acsami.0c15514 ↗
10. 10.1039/c8nr02382d10.1039/c8nr02382d ↗
11. 10.1021/acsnano.7b0918910.1021/acsnano.7b09189 ↗
12. 10.1002/smll.20130171610.1002/smll.201301716 ↗
13. 10.1002/smll.20160086610.1002/smll.201600866 ↗
14. 10.1002/adfm.20140365310.1002/adfm.201403653 ↗
15. 10.1039/c6nr08472a10.1039/c6nr08472a ↗
16. 10.1002/smll.20180496910.1002/smll.201804969 ↗
17. 10.1039/c5nr05631d10.1039/c5nr05631d ↗
18. 10.1002/smll.20200411810.1002/smll.202004118 ↗
19. 10.1021/acs.nanolett.9b0105710.1021/acs.nanolett.9b01057 ↗
20. 10.1039/c8nr02307g10.1039/c8nr02307g ↗
21. 10.1038/s41565-018-0221-010.1038/s41565-018-0221-0 ↗
22. 10.1021/acsnano.7b0055910.1021/acsnano.7b00559 ↗
23. 10.1016/j.nima.2005.05.01310.1016/j.nima.2005.05.013 ↗
24. 10.1063/1.339844110.1063/1.3398441 ↗
25. 10.1021/ja01466a02010.1021/ja01466a020 ↗
26. 10.1007/pl0001012210.1007/pl00010122 ↗
27. Jaque D. · Phys. Rev. B: Condens. Matter Mater. Phys. · 2003 · 68 · 03511810.1103/PhysRevB.68.035118 ↗
28. 10.1063/1.282690810.1063/1.2826908 ↗
29. 10.1103/PhysRevB.4.315310.1103/PhysRevB.4.3153 ↗
30. 10.1088/0953-8984/10/35/02210.1088/0953-8984/10/35/022 ↗
31. 10.1021/acs.jpclett.6b0143410.1021/acs.jpclett.6b01434 ↗
32. 10.1063/1.222047210.1063/1.2220472 ↗
33. 10.1021/acs.accounts.9b0045310.1021/acs.accounts.9b00453 ↗
34. 10.1021/jacs.8b0145810.1021/jacs.8b01458 ↗
35. 10.1021/acsnano.8b0154510.1021/acsnano.8b01545 ↗
36. 10.1021/acs.jpcc.5b0677010.1021/acs.jpcc.5b06770 ↗
37. 10.1016/j.jallcom.2020.15589310.1016/j.jallcom.2020.155893 ↗
38. 10.3390/ma1510366010.3390/ma15103660 ↗
39. 10.1007/s12039-009-0092-x10.1007/s12039-009-0092-x ↗
40. 10.1021/nl400176b10.1021/nl400176b ↗
41. 10.1021/cm402342510.1021/cm4023425 ↗
42. 10.1021/cr400425h10.1021/cr400425h ↗
43. 10.1021/jacs.9b0957110.1021/jacs.9b09571 ↗
44. 10.1021/acsphotonics.8b0011210.1021/acsphotonics.8b00112 ↗
45. 10.1039/d1na00285f10.1039/d1na00285f ↗
46. 10.1016/j.matpr.2020.01.24310.1016/j.matpr.2020.01.243 ↗
47. 10.1016/j.jlumin.2005.03.01110.1016/j.jlumin.2005.03.011 ↗
48. 10.7150/thno.511310.7150/thno.5113 ↗
49. 10.1063/1.188688710.1063/1.1886887 ↗