Optically induced coherent transport far aboveTcin underdopedYBa2Cu3O6+δ
Open accessAbstract
We report on a photoinduced transient state of ${\mathrm{YBa}}_{2}{\mathrm{Cu}}_{2}$O${}_{6+\ensuremath{\delta}}$ in which transport perpendicular to the Cu-O planes becomes highly coherent. This effect is achieved by excitation with mid-infrared optical pulses, tuned to the resonant frequency of apical oxygen vibrations, which modulate both lattice and electronic properties. Below the superconducting transition temperature ${T}_{c}$, the equilibrium signatures of superconducting interlayer coupling are enhanced. Most strikingly, the optical excitation induces a new reflectivity edge at higher frequency than the equilibrium Josephson plasma resonance, with a concomitant enhancement of the low-frequency imaginary conductivity ${\ensuremath{\sigma}}_{2}(\ensuremath{\omega})$. Above ${T}_{c}$, the incoherent equilibrium conductivity becomes highly coherent, with the appearance of a reflectivity edge and a positive ${\ensuremath{\sigma}}_{2}(\ensuremath{\omega})$ that increases with decreasing frequency. These features are observed up to room temperature in ${\mathrm{YBa}}_{2}{\mathrm{Cu}}_{2}$O${}_{6.45}$ and ${\mathrm{YBa}}_{2}{\mathrm{Cu}}_{2}$O${}_{6.5.}$ The data above ${T}_{c}$ can be fitted by hypothesizing that the light establishes a transient superconducting state over only a fraction of the solid, with a lifetime of a few picoseconds. Non-superconducting transport could also explain these observations, although one would have to assume transient carrier mobilities near 10${}^{4}$ cm${}^{2}$/V sec at 100 K, with a density of charge carriers similar to the below-${T}_{c}$ superfluid density. Our results are indicative of highly unconventional nonequilibrium physics and open new prospects for optical control of complex solids.
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
In YBa2Cu3Oy, the signal is enhanced when the pump is tuned to specific phonon resonances, but if the photoconductivity saturates more easily at these resonances, the signal enhancement could be caused by changes in d_eff instead of ∆σ_s.
“Furthermore, this signal is enhanced when the pump is tuned to specific phonon resonances, but if the photoconductivity saturates more easily at these resonances, the signal enhancement could be caused by changes in d eff instead of ∆ σ s [10, 18].”
From Optical Saturation Produces Spurious Evidence for Photoinduced Superconductivity in K 3 C 60 (2023) · cites this paper as [10]
The discussion of Fig. 6 says the photoinduced response is observed in resonance with the IR-active apical oxygen mode at 15 μm, supporting the resonance-dependent enhancement. Our copy does not establish that photoconductivity saturates more easily at that resonance or that a change in d_eff, rather than Δσ_s, could explain the enhancement. (LLM, conf=0.86)
Experimental — accuracy not yet measuredIn YBa2Cu3Oy, a signal associated with photoinduced superconductivity appears to show a linear dependence on the peak electric field, but the dependence is also consistent with what we have described for a saturable medium.
“In YBa2Cu3O y , for example, a signal associated with photoinduced superconductivity appears to show a linear dependence on the peak electric field, but the dependence is also consistent with what we have described for a saturable medium [10, 18, 22].”
From Optical Saturation Produces Spurious Evidence for Photoinduced Superconductivity in K 3 C 60 (2023) · cites this paper as [10]
Assuming a Debye model, the specific heat is proportional to T^3, so the local temperature will increase by approximately ∆T ∝ E^{1/4}.
“Assuming a Debye model, for example, the specific heat is proportional to T 3 , so the local temperature will increase by approximately ∆ T ∝ E 1 / 4 [8, 10].”
From Optical Saturation Produces Spurious Evidence for Photoinduced Superconductivity in K 3 C 60 (2023) · cites this paper as [10]
The paper’s discussion of temperature-dependent optical properties (section labeled Abstract; page unavailable) concerns plasma frequency and the fraction of material transformed by light, not heat capacity or local heating. Searches for “Debye,” “specific heat,” and an energy-to-temperature scaling found no passage in our copy stating C ∝ T³ or ΔT ∝ E^(1/4). (LLM, conf=0.73)
Experimental — accuracy not yet measured
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
The citation lists haven’t been fetched yet
References 55 · Cited by 292
Research works printed but not linked: 53
- [1]1. Z. A. Xu, N. P. Ong, Y. Wang, T. Kakeshita, and S. Uchida, Nature (London) 406, 486 (2000).
- [2]2. T. Timusk and B. Statt, Rep. Prog. Phys. 62, 61 (1999).
- [3]3. D. N. Basov and T. Timusk, Rev. Mod. Phys. 77, 721 (2005).
- [4]4. A. Dubroka, M. Rössle, K. W. Kim, V. K. Malik, D. Munzar, D. N. Basov, A. A. Schafgans, S. J. Moon, C. T. Lin, D. Haug, V. Hinkov, B. Keimer, Th. Wolf, J. G. Storey, J. L. Tallon, and C. Bernhard, Phys. Rev. Lett. 106, 047006 (2011).
- [5]5. V. J. Emery and S. A. Kivelson, Nature (London) 374, 434 (1995).
- [6]6. J. Corson, R. Mallozzi, J. Orenstein, J. N. Eckstein, and I. Bozovic, Nature (London) 398, 221 (1999).
- [7]7. J. M. Tranquada, B. J. Sternlieb, J. D. Axe, Y. Nakamura, and S. Uchida, Nature (London) 375, 561 (1995).
- [8]8. G. Ghiringhelli, M. Le Tacon, M. Minola, S. Blanco-Canosa, C. Mazzoli, N. B. Brookes, G. M. De Luca, A. Frano, D. G. Hawthorn, F. He, T. Loew, M. Moretti Sala, D. C. Peets, M. Salluzzo, E. Schierle, R. Sutarto, G. A. Sawatzky, E. Weschke, B. Keimer, and L. Braicovich, Science 337, 821 (2012).
- [9]9. B. Lake, H. M. Rønnow, N. B. Christensen, G. Aeppli, K. Lefmann, D. F. McMorrow, P. Vorderwisch, P. Smeibidl, N. Mangkorntong, T. Sasagawa, M. Nohara, H. Takagi, and T. E. Mason, Nature (London) 415, 299 (2002).
- [10]10. E. Hoffman, E. W. Hudson, K. M. Lang, V. Madhavan, H. Eisaki, S. Uchida, and J. C. Davis, Science 295, 466 (2002).
- [11]11. J. Demsar, B. Podobnik, V. V. Kabanov, Th. Wolf, and D. Mihailovic, Phys. Rev. Lett. 82, 4918 (1999).
- [12]12. R. A. Kaindl, M. Woerner, T. Elsaesser1, D. C. Smith, J. F. Ryan, G. A. Farnan, M. P. McCurry, and D. G. Walmsley, Science 287, 470 (2000).
- [14]14. M. Rini, R. Tobey, N. Dean, J. Itatani, Y. Tomioka, Y. Tokura, R. W. Schoenlein, and A. Cavalleri, Nature (London) 449, 72 (2007).
- [15]15. A. D. Caviglia, R. Scherwitzl, P. Popovich, W. Hu, H. Bromberger, R. Singla, M. Mitrano, M. C. Hoffmann, S. Kaiser, P. Zubko, S. Gariglio, J.-M. Triscone, M. Först, and A. Cavalleri, Phys. Rev. Lett. 108, 136801 (2012).
- [16]16. M. Först, R. I. Tobey, H. Bromberger, S. B. Wilkins, V. Khanna, A. D. Caviglia, Y.-D. Chuang, W. S. Lee, W. F. Schlotter, J. J. Turner, M. P. Minitti, O. Krupin, Z. J. Xu, J. S. Wen, G. D. Gu, S. S. Dhesi, A. Cavalleri, and J. P. Hill, Phys. Rev. Lett. 112, 157002 (2014).
- [17]17. D. Fausti, R. I. Tobey, N. Dean, S. Kaiser, A. Dienst, M. C. Hoffmann, S. Pyon, T. Takayama, H. Takagi, and A. Cavalleri, Science 331, 189 (2011).
- [18]18. T. Wu, H. Mayaffre, S. Krämer, M. Horvatić, C. Berthier, W. N. Hardy, R. Liang, D. A. Bonn, and M.-H. Julien, Nature (London) 477, 191 (2011).
- [19]19. J. Chang, E. Blackburn, A. T. Holmes, N. B. Christensen, J. Larsen, J. Mesot, R. Liang, D. A. Bonn, W. N. Hardy, A. Watenphul, M. v. Zimmermann, E. M. Forgan, and S. M. Hayden, Nat. Phys. 8, 871 (2012).
- [20]20. S. Blanco-Canosa, A. Frano, T. Loew, Y. Lu, J. Porras, G. Ghiringhelli, M. Minola, C. Mazzoli, L. Braicovich, E. Schierle, E. Weschke, M. Le Tacon, and B. Keimer, Phys. Rev. Lett. 110, 187001 (2013).
- [21]21. E. Uykur, K. Tanaka, T. Masui, S. Miyasaka, and S. Tajima, Phys. Rev. Lett. 112, 127003 (2014).
- [23]23. S. I. Schlachter, U. Tutsch, W. H. Fietz, K.-P. Weiss, H. Leibrock, K. Grube, Th. Wolf, B. Obst, P. Schweiss, and H. Wühl, Int. J. Mod. Phys. B 14, 3673 (2000).
- [24]24. See Supplemental Material at http://link.aps.org/supplemental/ 10.1103/PhysRevB.89.184516 for details on the sample char- acterization, the derivation of the complex conductivity, the pump fluence dependence and the estimation of the peak lattice distortion.
- [25]25. G. Calestani and C. Rizzoli, Nature (London) 328, 606 (1987).
- [26]26. G. Burns, F. H. Dacol, P. P. Freitas, W. König, and T. S. Plaskett, Phys. Rev. B 37, 5171 (1988).
- [27]27. A. Pashkin, M. Porer, M. Beyer, K. W. Kim, A. Dubroka, C. Bernhard, X. Yao, Y. Dagan, R. Hackl, A. Erb, J. Demsar, R. Huber, and A. Leitenstorfer, Phys. Rev. Lett. 105, 067001 (2010).
- [29]29. D. J. Hilton, R. P. Prasankumar, S. Fourmaux, A. Cavalleri, D. Brassard, M. A. El Khakani, J. C. Kieffer, A. J. Taylor, and R. D. Averitt, Phys. Rev. Lett. 99, 226401 (2007).
- [30]30. M. M. Qazilbash, M. Brehm, Byung-Gyu Chae, P.-C. Ho, G. O. Andreev, Bong-Jun Kim, Sun Jin Yun, A. V. Balatsky, M. B. Maple, F. Keilmann, Hyun-Tak Kim, and D. N. Basov, Science 318, 1750 (2007).
- [31]31. C. C. Homes, T. Timusk, D. A. Bonn, R. Liang, and W. N. Hardy, Physica C 254, 265 (1995).
- [33]33. M. Dressel and G. Grüner, Electrodynamics of Solids (Cam- bridge University Press, 2002).
- [34]34. G. Gruener, Density Waves in Solids (Addison-Wesley Publish- ing Company, 1994).
- [35]35. G. M. Eliashberg, JETP Lett. 11, 114 (1970);
- [36]36. B. I. Ivlev and G. M. Eliashberg, ibid. 13, 464 (1971).
- [37]37. C. S. Owen and D. J. Scalapino, Phys. Rev. Lett. 28, 1559 (1972).
- [38]38. P. W. Anderson and A. H. Dayem, Phys. Rev. Lett. 13, 195 (1964).
- [39]39. A. F. G. Wyatt, V. M. Dmitriev, W. S. Moore, and F. W. Sheard, Phys. Rev. Lett. 16, 1166 (1966).
- [40]40. A. H. Dayem and J. J. Wiegand, Phys. Rev. 155, 419 (1967).
- [41]41. R. Escudero and H. J. T. Smith, Phys. Rev. B 31, 2725 (1985).
- [42]42. S. I. Vedeneev, D. K. Maude, and J. M. Byrne, Phys. Rev. B 78, 052509 (2008).
- [43]43. G. Yu, C. H. Lee, A. J. Heeger, N. Herron, and E. M. McCarron, Phys. Rev. Lett. 67, 2581 (1991).
- [44]44. G. Nieva, E. Osquiguil, J. Guimpel, M. Maenhoudt, B. Wuyts, Y. Bruynseraede, M. B. Maple, and Ivan K. Schuller, Appl. Phys. Lett. 60, 2159 (1992).
- [45]45. D. Haug, V. Hinkov, Y. Sidis, P. Bourges, N. B. Christensen, A. Ivanov, T. Keller, C .T. Lin, and B. Keimer, New J. Phys. 12, 105006 (2010).
- [46]46. V. Hinkov, P. Bourges, S. Pailhès, Y. Sidis, A. Ivanov, C. D. Frost, T. G. Perring, C. T. Lin, D. P. Chen, and B. Keimer, Nat. Phys. 3, 780 (2007).
- [47]47. M. Först, C. Manzoni, S. Kaiser, Y. Tomioka, Y. Tokura, R. Merlin, and A. Cavalleri, Nat. Phys. 7, 854 (2011).
- [48]48. M. Först, R. Mankowsky, H. Bromberger, D. M. Fritz, H. Lemke, D. Zhu, M. Chollet, Y. Tomioka, Y. Tokura, R. Merlin, J. P. Hill, S. L. Johnson, and A. Cavalleri, Solid State Commun. 169, 24 (2013).
- [49]49. E. Pavarini, I. Dasgupta, T. Saha-Dasgupta, O. Jepsen, and O. K. Andersen, Phys. Rev. Lett. 87, 047003 (2001).
- [50]50. C. Weber, K. Haule, and G. Kotliar, Phys. Rev. B 82, 125107 (2010).
- [51]51. J. A. Slezak, J. Lee, M. Wang, K. McElroy, K. Fujita, B. M. Andersen, P. J. Hirschfeld, H. Eisaki, S. Uchida, and J. C. Davis, Proc. Natl. Acad. Sci. USA 105, 3203 (2008).
- [52]52. M. Mori, G. Khaliullin, T. Tohyama, and S. Maekawa, Phys. Rev. Lett. 101, 247003 (2008).
- [53]53. H. Sakakibara, H. Usui, K. Kuroki, R. Arita, and H. Aoki, Phys. Rev. Lett. 105, 057003 (2010).
- [55]55. P. L. Kapitza, Zh. Eksp. Teor. Fiz. 21, 588 (1951).
- [56]56. L. D. Landau and E. M. Lifschitz, Mechanics (Pergamon, Oxford, 1976).
- [57]57. A. W. Overhauser, Phys. Rev. 92, 411 (1953).
- [58]58. He Rui-Hua, M. Hashimoto, and H. Karapetyan, Science 331, 1579 (2011).
- Authors
- Kaiser, S., Hunt, C. R., Nicoletti, D., Hu, W., Gierz, I., Liu, H. Y., Le Tacon, M., Loew, T., Haug, D., Keimer, B., & Cavalleri, A.
- Affiliations
- Max Planck Society (DE)
- Max Planck Institute for Solid State Research (DE)
- Venue
- Physical Review B
- Publisher
- American Physical Society (APS)
- Published
- 2014-05-30
- Volume
- 89
- Issue
- 18
- ISSN
- 1098-0121 (ISSN-L)
- 1550-235X
- OpenAlex
- W1633442599
- Cited by
- 292
- References
- 55
- Citations by year
- 2026: 18 · 2025: 19 · 2024: 17 · 2023: 17 · 2022: 25 · 2021: 26 · 2020: 35 · 2019: 21 · 2018: 24 · 2017: 25 · 2016: 30 · 2015: 25 · 2014: 10
- FWCI
- 19.34
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Physical Review B (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- Max Planck Digital Library (submittedVersion, other-oa)
- Desy publication database (The Deutsches Elektronen-Synchrotron) (submittedVersion, other-oa)
- MPG.PuRe (Max Planck Society) (submittedVersion, other-oa)
- arXiv (Cornell University)
- Funders
- European Commission (2007–2013, FP7 2007-2013, 319286, FP7/2007)
- FP7 Ideas: European Research Council (319286)
- Topics
- Physical Sciences › Physics and Astronomy › Condensed Matter Physics › Physics of Superconductivity and Magnetism
- Physical Sciences › Materials Science › Electronic, Optical and Magnetic Materials › Magnetic and transport properties of perovskites and related materials
- Physical Sciences › Physics and Astronomy › Condensed Matter Physics › Advanced Condensed Matter Physics
- Keywords
- underdoped cuprates, photoinduced superconductivity, coherent transport, mid-infrared excitation, interlayer coupling, Josephson plasma resonance, imaginary conductivity, nonequilibrium superconductivity, high-temperature superconductors
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review