journal article·2015-11

Can Trihalide Lead Perovskites Support Continuous Wave Lasing?

Michele Cadelano, Valerio Sarritzu, Nicola Sestu, Daniela Marongiu, Feipeng Chen, Roberto Piras, Riccardo Corpino, Carlo Maria Carbonaro, Francesco Quochi, Michele Saba, Andrea Mura, Giovanni Bongiovanni

Advanced Optical Materials· Volume 3· Issue 11
Publisher page

Abstract

Amplified spontaneous emission in methylammonium lead halide perovskites over transients as long as 100 ns at 200 K temperature is demonstrated. Optical spectroscopy measurements highlight runaway heating dynamics limiting the duration of optical amplification, but also suggest materials and device improvements to circumvent such limitations and allow true continuous wave operation. As a service to our authors and readers, this journal provides supporting information supplied by the authors. Such materials are peer reviewed and may be re-organized for online delivery, but are not copy-edited or typeset. Technical support issues arising from supporting information (other than missing files) should be addressed to the authors. Please note: The publisher is not responsible for the content or functionality of any supporting information supplied by the authors. Any queries (other than missing content) should be directed to the corresponding author for the article.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Perovskite Materials and Applications · Solid-state spectroscopy and crystallography · Optical properties and cooling technologies in crystalline materials

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

Affiliations

Dipartimento di Fisica Università degli Studi di Cagliari I‐09042 Monserrato Italy

Funding

Regione Autonoma della Sardegna

References (42)

Show source-provided references
1. 10.1038/1639310.1038/16393 ↗
2. 10.1038/nature0249810.1038/nature02498 ↗
3. 10.1038/nphoton.2010.16010.1038/nphoton.2010.160 ↗
4. 10.1021/cr050152i10.1021/cr050152i ↗
5. 10.1038/369467a010.1038/369467a0 ↗
6. 10.1021/jz402016210.1021/jz4020162 ↗
7. 10.1002/smll.20140276710.1002/smll.201402767 ↗
8. 10.1038/nmat406510.1038/nmat4065 ↗
9. 10.1126/science.124547310.1126/science.1245473 ↗
10. 10.1126/science.124398210.1126/science.1243982 ↗
11. 10.1126/science.aaa272510.1126/science.aaa2725 ↗
12. 10.1002/adma.20130517210.1002/adma.201305172 ↗
13. 10.1126/science.124316710.1126/science.1243167 ↗
14. 10.1126/science.aaa576010.1126/science.aaa5760 ↗
15. 10.1002/adfm.20140442110.1002/adfm.201404421 ↗
16. 10.1557/mrc.2015.610.1557/mrc.2015.6 ↗
17. 10.1038/nphoton.2014.17110.1038/nphoton.2014.171 ↗
18. 10.1021/nl503057g10.1021/nl503057g ↗
19. 10.1038/nmat391110.1038/nmat3911 ↗
20. 10.1038/ncomms604910.1038/ncomms6049 ↗
21. 10.1039/c3ee43822h10.1039/c3ee43822h ↗
22. 10.1021/ic401215x10.1021/ic401215x ↗
23. 10.1039/C4EE01076K10.1039/C4EE01076K ↗
24. 10.1038/nphoton.2014.8210.1038/nphoton.2014.82 ↗
25. 10.1021/jz500211710.1021/jz5002117 ↗
26. 10.1021/jz400348q10.1021/jz400348q ↗
27. 10.1021/jp502340710.1021/jp5023407 ↗
28. 10.1021/jz402706q10.1021/jz402706q ↗
29. 10.1021/jp512936z10.1021/jp512936z ↗
30. 10.1021/jz500528510.1021/jz5005285 ↗
31. 10.1021/nn504856g10.1021/nn504856g ↗
32. 10.1038/nmat427110.1038/nmat4271 ↗
33. 10.1038/ncomms458610.1038/ncomms4586 ↗
34. 10.1103/PhysRevB.46.986110.1103/PhysRevB.46.9861 ↗
35. 10.1103/PhysRevB.38.194710.1103/PhysRevB.38.1947 ↗
36. 10.1021/jz502528c10.1021/jz502528c ↗
37. 10.1039/C4EE01358A10.1039/C4EE01358A ↗
38. 10.1063/1.11703210.1063/1.117032 ↗
39. Smart A. G. · Phys. Today · 2013 · 66 · 12
40. 10.1063/1.357065610.1063/1.3570656 ↗
41. 10.1063/1.12125010.1063/1.121250 ↗
42. 10.1021/jz501210910.1021/jz5012109 ↗