journal article·2022-12-22

Magnetic field tuning of parallel spin stripe order and fluctuations near the pseudogap quantum critical point in La1.36Nd0.4Sr0.24CuO4

Qianli Ma, Evan M. Smith, Zachary W. Cronkwright, Mirela Dragomir, Gabrielle Mitchell, Barry W. Winn, Travis J. Williams, Bruce D. Gaulin

Physical Review B· Volume 106· Issue 21
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Abstract

A quantum critical point in the single-layer, hole-doped cuprate system ${\mathrm{La}}_{1.6\ensuremath{-}x}{\mathrm{Nd}}0.4{\mathrm{Sr}}x{\mathrm{CuO}}4$ (Nd-LSCO) near $x=0.23$ has been proposed as an organizing principle for understanding high-temperature superconductivity. Our earlier neutron diffraction work on Nd-LSCO at optimal and high doping revealed static parallel spin stripes to exist out to the quantum critical point and slightly beyond, at $x=0.24$ and 0.26. We examine more closely the parallel spin stripe order parameter in Nd-LSCO in both zero magnetic field and fields up to 8 T for $H\ensuremath{\parallel}c$ in these single crystals. In contrast to earlier studies at lower doping, we observe that $H\ensuremath{\parallel}c$ in excess of $\ensuremath{\sim}2.5$ T eliminates the incommensurate quasi-Bragg peaks associated with parallel spin stripes. But this elastic scattering is not destroyed by the field; rather it is transferred to commensurate $\mathbf{Q}=\mathbf{0}$ Bragg positions, implying that the spins participating in the spin stripes have been polarized. Inelastic neutron scattering measurements at high fields show an increase in the low-energy, parallel spin stripe fluctuations and evidence for a spin gap ${\mathrm{\ensuremath{\Delta}}}_{\text{spin}}=3\ifmmode\pm\else\textpm\fi{}0.5$ meV for Nd-LSCO with $x=0.24$. This is shown to be consistent with spin-gap measurements as a function of superconducting ${T}C$ over five different families of cuprate superconductors, which follow the approximate linear relation ${\mathrm{\ensuremath{\Delta}}}_{\text{spin}}=3.5{k}B{T}C$.
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Research context

OpenAlex topics: Physics of Superconductivity and Magnetism · Advanced Condensed Matter Physics · Magnetic and transport properties of perovskites and related materials

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

Affiliations

Department of Physics and Astronomy, McMaster University, Hamilton, Ontario, Canada L8S 4M1

Brockhouse Institute for Materials Research, Hamilton, Ontario, Canada L8S 4M1

Electronic Ceramics Department, Jožef Stefan Institute, 1000 Ljubljana, Slovenia

Neutron Scattering Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37830, USA

Canadian Institute for Advanced Research, MaRS Centre, West Tower 661 University Ave., Suite 505, Toronto, Ontarion, Canada M5G 1M1

Funding

Natural Sciences and Engineering Research Council of Canada · Oak Ridge National Laboratory

References (51)

Show source-provided references
1. 10.1007/BF0130370110.1007/BF01303701 ↗
2. 10.1103/PhysRevLett.58.90810.1103/PhysRevLett.58.908 ↗
3. 10.1126/science.235.4793.119610.1126/science.235.4793.1196 ↗
4. 10.1103/PhysRevLett.58.279410.1103/PhysRevLett.58.2794 ↗
5. 10.1103/PhysRevB.36.399010.1103/PhysRevB.36.3990 ↗
6. 10.1103/PhysRevB.38.514210.1103/PhysRevB.38.5142 ↗
7. 10.1103/PhysRevLett.60.94410.1103/PhysRevLett.60.944 ↗
8. 10.1103/PhysRevB.37.375910.1103/PhysRevB.37.3759 ↗
9. J. P. Franck · 1994
10. 10.1103/PhysRevB.56.612010.1103/PhysRevB.56.6120 ↗
11. 10.1016/S0370-1573(00)00008-910.1016/S0370-1573(00)00008-9 ↗
12. 10.1103/RevModPhys.78.1710.1103/RevModPhys.78.17 ↗
13. 10.1143/JPSJ.81.01100810.1143/JPSJ.81.011008 ↗
14. 10.1103/RevModPhys.84.138310.1103/RevModPhys.84.1383 ↗
15. 10.1146/annurev-conmatphys-070909-10411710.1146/annurev-conmatphys-070909-104117 ↗
16. 10.1146/annurev-conmatphys-031218-01321010.1146/annurev-conmatphys-031218-013210 ↗
17. J. M. Tranquada · 2013
18. 10.1080/00018732.2021.193569810.1080/00018732.2021.1935698 ↗
19. 10.1103/RevModPhys.70.89710.1103/RevModPhys.70.897 ↗
20. 10.1103/PhysRevB.46.1403410.1103/PhysRevB.46.14034 ↗
21. 10.1038/375561a010.1038/375561a0 ↗
22. 10.1038/s41586-019-0932-x10.1038/s41586-019-0932-x ↗
23. 10.1103/PhysRevMaterials.4.11480110.1103/PhysRevMaterials.4.114801 ↗
24. 10.1103/PhysRevB.40.739110.1103/PhysRevB.40.7391 ↗
25. 10.1103/PhysRevLett.67.179110.1103/PhysRevLett.67.1791 ↗
26. 10.1103/PhysRevB.57.142210.1103/PhysRevB.57.1422 ↗
27. 10.1103/PhysRevB.96.08514210.1103/PhysRevB.96.085142 ↗
28. 10.1073/pnas.211942911910.1073/pnas.2119429119 ↗
29. 10.1103/PhysRevB.60.R76910.1103/PhysRevB.60.R769 ↗
30. 10.1103/PhysRevB.78.09250710.1103/PhysRevB.78.092507 ↗
31. 10.1103/PhysRevB.77.22441010.1103/PhysRevB.77.224410 ↗
32. 10.1103/PhysRevResearch.3.02315110.1103/PhysRevResearch.3.023151 ↗
33. 10.1103/PhysRevB.57.616510.1103/PhysRevB.57.6165 ↗
34. 10.1016/j.physc.2009.11.07310.1016/j.physc.2009.11.073 ↗
35. 10.1038/nphys110910.1038/nphys1109 ↗
36. 10.1038/nature1698310.1038/nature16983 ↗
37. 10.1103/PhysRevB.92.13452410.1103/PhysRevB.92.134524 ↗
38. 10.1103/RevModPhys.75.47310.1103/RevModPhys.75.473 ↗
39. 10.1103/PhysRevResearch.4.01317510.1103/PhysRevResearch.4.013175 ↗
40. 10.1103/PhysRevLett.92.21700410.1103/PhysRevLett.92.217004 ↗
41. 10.1103/PhysRevLett.98.24700310.1103/PhysRevLett.98.247003 ↗
42. 10.1038/415299a10.1038/415299a ↗
43. 10.1103/RevModPhys.76.90910.1103/RevModPhys.76.909 ↗
44. 10.1103/PhysRevB.78.10452510.1103/PhysRevB.78.104525 ↗
45. 10.1103/PhysRevB.78.21250610.1103/PhysRevB.78.212506 ↗
46. 10.1103/PhysRevB.67.18441910.1103/PhysRevB.67.184419 ↗
47. I. A. Zaliznyak · 2017
48. 10.1103/PhysRevLett.78.33810.1103/PhysRevLett.78.338 ↗
49. 10.1103/PhysRevB.98.22450810.1103/PhysRevB.98.224508 ↗
50. 10.1038/s41567-022-01514-110.1038/s41567-022-01514-1 ↗
51. 10.1103/PhysRevB.62.R1467710.1103/PhysRevB.62.R14677 ↗