TY - JOUR
T1 - Vortex pinning by natural linear defects in thin films of YBa2Cu3O7-δ
AU - Klaassen, F. C.
AU - Doornbos, G.
AU - Huijbregtse, J. M.
AU - Van der Geest, R. C.F.
AU - Dam, B.
AU - Griessen, R.
PY - 2001/11/1
Y1 - 2001/11/1
N2 - The behavior of the superconducting current density j s(B,T) and the dynamical relaxation rate Q(B,T) of YBa2Cu3O7-δ thin films exhibits a number of features typical for strong pinning of vortices by growth induced linear defects. At low magnetic fields js(B) and Q(B) are constant up to a characteristic field B*, that is directly proportional to the linear defect density ndisl. The pinning energy Uc(B=0)≈600 K can be explained by half-loop excitations determining the thermal activation of vortices at low magnetic fields. Extending the Bose glass theory [D. R. Nelson and V. M. Vinokur, Phys. Rev. B 48, 13 060 (1993)], we derive a different expression for the vortex pinning potential εr(R), which is valid for all defect sizes and describes its renormalization due to thermal fluctuations. With this expression we explain the temperature dependence of the true critical current density jc(O,T) and of the pinning energy Uc(0,T) at low magnetic fields. At high magnetic fields μ0H≫B* the current density experiences a power law behavior js(B)∼Bα with α≈-0.58 for films with low ndisl and α≈-0.8 to -1.1 for films with high ndisl. The pinning energy in this regime, Uc(high B)≈60-200 K is independent of magnetic field, but depends on the dislocation density. This implies that vortex pinning is still largely determined by the linear defects, even when the vortex density is much larger than the linear defect density. Our results show that natural linear defects in thin films form an analogous system to columnar tracks in irradiated samples. There are, however, three essential differences: (i) typical matching fields are at least one order of magnitude smaller, (ii) linear defects are smaller than columnar tracks, and (iii) the distribution of natural linear defects is nonrandom, whereas columnar tracks are randomly distributed. Nevertheless the Bose glass theory, that has successfully described many properties of pinning by columnar tracks, can be applied also to thin films. A better understanding of pinning in thin films is thus useful to put the properties of irradiated samples in a broader perspective.
AB - The behavior of the superconducting current density j s(B,T) and the dynamical relaxation rate Q(B,T) of YBa2Cu3O7-δ thin films exhibits a number of features typical for strong pinning of vortices by growth induced linear defects. At low magnetic fields js(B) and Q(B) are constant up to a characteristic field B*, that is directly proportional to the linear defect density ndisl. The pinning energy Uc(B=0)≈600 K can be explained by half-loop excitations determining the thermal activation of vortices at low magnetic fields. Extending the Bose glass theory [D. R. Nelson and V. M. Vinokur, Phys. Rev. B 48, 13 060 (1993)], we derive a different expression for the vortex pinning potential εr(R), which is valid for all defect sizes and describes its renormalization due to thermal fluctuations. With this expression we explain the temperature dependence of the true critical current density jc(O,T) and of the pinning energy Uc(0,T) at low magnetic fields. At high magnetic fields μ0H≫B* the current density experiences a power law behavior js(B)∼Bα with α≈-0.58 for films with low ndisl and α≈-0.8 to -1.1 for films with high ndisl. The pinning energy in this regime, Uc(high B)≈60-200 K is independent of magnetic field, but depends on the dislocation density. This implies that vortex pinning is still largely determined by the linear defects, even when the vortex density is much larger than the linear defect density. Our results show that natural linear defects in thin films form an analogous system to columnar tracks in irradiated samples. There are, however, three essential differences: (i) typical matching fields are at least one order of magnitude smaller, (ii) linear defects are smaller than columnar tracks, and (iii) the distribution of natural linear defects is nonrandom, whereas columnar tracks are randomly distributed. Nevertheless the Bose glass theory, that has successfully described many properties of pinning by columnar tracks, can be applied also to thin films. A better understanding of pinning in thin films is thus useful to put the properties of irradiated samples in a broader perspective.
UR - http://www.scopus.com/inward/record.url?scp=0000288196&partnerID=8YFLogxK
M3 - Article
AN - SCOPUS:0000288196
SN - 0163-1829
VL - 64
SP - 1845231
EP - 18452320
JO - Physical Review B - Condensed Matter and Materials Physics
JF - Physical Review B - Condensed Matter and Materials Physics
IS - 18
M1 - 184523
ER -