journal article·2016-02-04Open access

Direct band gap carbon superlattices with efficient optical transition

Young Jun Oh, Sunghyun Kim, In-Ho Lee, Jooyoung Lee, K. J. Chang

Physical Review B· Volume 93· Issue 8

Abstract

We report pure carbon-based superlattices that exhibit direct band gaps and excellent optical absorption and emission properties at the threshold energy. The structures are nearly identical to that of cubic diamond except that defective layers characterized by five- and seven-membered rings are intercalated in the diamond lattice. The direct band gaps lie in the range of 5.6--5.9 eV, corresponding to wavelengths of 210--221 nm. The dipole matrix elements of direct optical transition are comparable to that of GaN, suggesting that the superlattices are promising materials as an efficient deep ultraviolet light emitter. Molecular dynamics simulations show that the superlattices are thermally stable even at a high temperature of 2000 K. We provide a possible route to the synthesis of superlattices through wafer bonding of diamond (100) surfaces.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Diamond and Carbon-based Materials Research · Graphene research and applications · Semiconductor materials and devices

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

References (62)

Show source-provided references
1. 10.1103/RevModPhys.81.10910.1103/RevModPhys.81.109 ↗
2. 10.1016/S1369-7021(07)70349-810.1016/S1369-7021(07)70349-8 ↗
3. 10.1103/RevModPhys.79.67710.1103/RevModPhys.79.677 ↗
4. 10.1038/nnano.2007.30010.1038/nnano.2007.300 ↗
5. 10.1038/nphoton.2008.9410.1038/nphoton.2008.94 ↗
6. 10.1126/science.140.3568.81710.1126/science.140.3568.817 ↗
7. 10.1063/1.184123610.1063/1.1841236 ↗
8. 10.1103/PhysRevB.39.1259810.1103/PhysRevB.39.12598 ↗
9. 10.1103/PhysRevB.40.99310.1103/PhysRevB.40.993 ↗
10. 10.1126/science.252.5012.154210.1126/science.252.5012.1542 ↗
11. 10.1038/srep0052010.1038/srep00520 ↗
12. 10.1103/PhysRevLett.85.188710.1103/PhysRevLett.85.1887 ↗
13. 10.1021/jp025983w10.1021/jp025983w ↗
14. 10.1073/pnas.040587710110.1073/pnas.0405877101 ↗
15. 10.1103/PhysRevLett.102.17550610.1103/PhysRevLett.102.175506 ↗
16. 10.1103/PhysRevLett.106.07550110.1103/PhysRevLett.106.075501 ↗
17. 10.1016/S0379-6779(97)81165-410.1016/S0379-6779(97)81165-4 ↗
18. 10.1103/PhysRevLett.104.12550410.1103/PhysRevLett.104.125504 ↗
19. 10.1103/PhysRevLett.108.06550110.1103/PhysRevLett.108.065501 ↗
20. 10.1103/PhysRevB.84.16141110.1103/PhysRevB.84.161411 ↗
21. 10.1103/PhysRevLett.107.21550210.1103/PhysRevLett.107.215502 ↗
22. 10.1103/PhysRevLett.108.13550110.1103/PhysRevLett.108.135501 ↗
23. 10.1103/PhysRevB.85.03341010.1103/PhysRevB.85.033410 ↗
24. 10.1016/j.ssc.2012.05.02210.1016/j.ssc.2012.05.022 ↗
25. 10.1039/c2cp40531h10.1039/c2cp40531h ↗
26. 10.1039/c2cp24066a10.1039/c2cp24066a ↗
27. 10.1088/0953-8984/24/16/16550410.1088/0953-8984/24/16/165504 ↗
28. 10.1063/1.473253810.1063/1.4732538 ↗
29. 10.1039/c3cp51746b10.1039/c3cp51746b ↗
30. 10.1016/j.ssc.2013.11.03510.1016/j.ssc.2013.11.035 ↗
31. 10.1039/C4CP04569F10.1039/C4CP04569F ↗
32. 10.1134/S106378340607029810.1134/S1063783406070298 ↗
33. 10.1103/PhysRevLett.106.15570310.1103/PhysRevLett.106.155703 ↗
34. 10.1103/PhysRevB.86.07515110.1103/PhysRevB.86.075151 ↗
35. 10.1039/C2CP43221H10.1039/C2CP43221H ↗
36. 10.1209/0295-5075/108/4600610.1209/0295-5075/108/46006 ↗
37. 10.1143/JJAP.41.L143410.1143/JJAP.41.L1434 ↗
38. 10.1088/0268-1242/29/8/08400410.1088/0268-1242/29/8/084004 ↗
39. 10.1038/nphoton.2007.29310.1038/nphoton.2007.293 ↗
40. 10.1038/nature0476010.1038/nature04760 ↗
41. 10.1103/PhysRevB.90.11520910.1103/PhysRevB.90.115209 ↗
42. 10.1103/PhysRevLett.91.08020110.1103/PhysRevLett.91.080201 ↗
43. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
44. 10.1103/PhysRevB.59.175810.1103/PhysRevB.59.1758 ↗
45. 10.1016/0927-0256(96)00008-010.1016/0927-0256(96)00008-0 ↗
46. 10.1038/srep1808610.1038/srep18086 ↗
47. 10.1103/PhysRevB.34.539010.1103/PhysRevB.34.5390 ↗
48. 10.1016/0022-3697(59)90394-410.1016/0022-3697(59)90394-4 ↗
49. 10.1103/PhysRevB.46.448310.1103/PhysRevB.46.4483 ↗
50. 10.1103/PhysRev.84.123210.1103/PhysRev.84.1232 ↗
51. 10.1063/1.34953910.1063/1.349539 ↗
52. 10.1063/1.11250310.1063/1.112503 ↗
53. 10.1016/0039-6028(86)90665-510.1016/0039-6028(86)90665-5 ↗
54. 10.1016/0039-6028(90)90517-C10.1016/0039-6028(90)90517-C ↗
55. 10.1063/1.152769710.1063/1.1527697 ↗
56. 10.1103/PhysRevB.53.733410.1103/PhysRevB.53.7334 ↗
57. 10.1103/PhysRevB.88.03520510.1103/PhysRevB.88.035205 ↗
58. 10.1016/j.commatsci.2010.05.01010.1016/j.commatsci.2010.05.010 ↗
59. 10.1103/PhysRevB.48.1120410.1103/PhysRevB.48.11204 ↗
60. 10.1088/0953-8984/25/34/34550110.1088/0953-8984/25/34/345501 ↗
61. 10.1103/PhysRevB.90.19512110.1103/PhysRevB.90.195121 ↗
62. 10.1007/BF0133953010.1007/BF01339530 ↗