Vortex matter freezing inBi2Sr2CaCu2O8samples with a very dense distribution of columnar defects
Source abstract
Abstract
We show that the dynamical freezing of vortex structures nucleated at diluted densities in ${\mathrm{Bi}}2{\mathrm{Sr}}2{\mathrm{CaCu}}2{\mathrm{O}}8$ samples with a dense distribution of columnar defects, $B\ensuremath{\sim}{10}^{\ensuremath{-}2}{B}_{\mathrm{\ensuremath{\Phi}}}$ with ${B}_{\mathrm{\ensuremath{\Phi}}}=5\phantom{\rule{0.16em}{0ex}}\mathrm{kG}$, results in configurations with liquidlike correlations. We propose a freezing model considering a relaxation dynamics dominated by double-kink excitations driven by the local stresses obtained directly from experimental images. With this model we estimate the relaxation barrier and the freezing temperature. We argue that the low-field frozen vortex structures nucleated in a dense distribution of columnar defects thus correspond to an out-of-equilibrium nonentangled liquid with strongly reduced mobility rather than to a snapshot of a metastable state with divergent activation barriers as, for instance, expected for the Bose-glass phase at equilibrium.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Physics of Superconductivity and Magnetism · Magnetic properties of thin films · Theoretical and Computational Physics
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (43)
Show source-provided references
1. 10.1103/RevModPhys.66.112510.1103/RevModPhys.66.1125 ↗
2. 10.1073/pnas.040801610210.1073/pnas.0408016102 ↗
3. 10.1103/PhysRevLett.103.25700110.1103/PhysRevLett.103.257001 ↗
4. 10.1002/(SICI)1521-3951(199909)215:1%3C563::AID-PSSB563%3E3.0.CO;2-C10.1002/(SICI)1521-3951(199909)215:1%3C563::AID-PSSB563%3E3.0.CO;2-C ↗
5. 10.1016/S0038-1098(03)00645-810.1016/S0038-1098(03)00645-8 ↗
6. 10.1103/PhysRevB.84.09451710.1103/PhysRevB.84.094517 ↗
7. 10.1016/j.physb.2012.01.02110.1016/j.physb.2012.01.021 ↗
8. 10.1103/PhysRevB.87.09450610.1103/PhysRevB.87.094506 ↗
9. 10.1103/PhysRevB.85.01452410.1103/PhysRevB.85.014524 ↗
10. 10.1088/1742-6596/449/1/01202310.1088/1742-6596/449/1/012023 ↗
11. 10.1103/PhysRevLett.65.116410.1103/PhysRevLett.65.1164 ↗
12. 10.1103/PhysRevB.44.716710.1103/PhysRevB.44.7167 ↗
13. C. J. van der Beek · 2010
14. 10.1103/PhysRevB.48.1306010.1103/PhysRevB.48.13060 ↗
15. 10.1103/PhysRevLett.74.121410.1103/PhysRevLett.74.1214 ↗
16. 10.1103/PhysRevB.51.1549210.1103/PhysRevB.51.15492 ↗
17. 10.1103/PhysRevB.51.395710.1103/PhysRevB.51.3957 ↗
18. 10.1103/PhysRevB.61.980010.1103/PhysRevB.61.9800 ↗
19. 10.1103/PhysRevB.48.134110.1103/PhysRevB.48.1341 ↗
20. 10.1126/science.265.5178.155210.1126/science.265.5178.1552 ↗
21. 10.1103/PhysRevLett.90.14700110.1103/PhysRevLett.90.147001 ↗
22. 10.1103/PhysRevLett.90.08700410.1103/PhysRevLett.90.087004 ↗
23. 10.1023/B:JOLT.0000016975.59303.6610.1023/B:JOLT.0000016975.59303.66 ↗
24. 10.1016/j.physc.2004.03.18910.1016/j.physc.2004.03.189 ↗
25. 10.1016/j.physc.2004.03.06210.1016/j.physc.2004.03.062 ↗
26. M. Menghini · 2005
27. 10.1103/PhysRevB.55.1461010.1103/PhysRevB.55.14610 ↗
28. 10.1016/0022-0248(94)90138-410.1016/0022-0248(94)90138-4 ↗
29. 10.1016/0921-4534(92)90521-D10.1016/0921-4534(92)90521-D ↗
30. 10.1088/0953-2048/4/1S/09610.1088/0953-2048/4/1S/096 ↗
31. 10.1088/0953-2048/21/02/02300110.1088/0953-2048/21/02/023001 ↗
32. 10.1103/PhysRevLett.72.295110.1103/PhysRevLett.72.2951 ↗
33. 10.1038/375373a010.1038/375373a0 ↗
34. 10.1103/PhysRevLett.97.23700510.1103/PhysRevLett.97.237005 ↗
35. 10.1016/0921-4534(93)90484-810.1016/0921-4534(93)90484-8 ↗
36. 10.1103/PhysRevB.54.R378410.1103/PhysRevB.54.R3784 ↗
37. 10.1103/PhysRevB.90.14450710.1103/PhysRevB.90.144507 ↗
38. 10.1103/PhysRevB.61.425910.1103/PhysRevB.61.4259 ↗
39. 10.1103/PhysRevLett.86.513610.1103/PhysRevLett.86.5136 ↗
40. 10.1007/s10909-014-1218-110.1007/s10909-014-1218-1 ↗
41. 10.1103/PhysRevB.53.1461110.1103/PhysRevB.53.14611 ↗
42. 10.1103/PhysRevB.59.1362010.1103/PhysRevB.59.13620 ↗
43. 10.1103/PhysRevB.55.657710.1103/PhysRevB.55.6577 ↗