1990
DOI: 10.1103/physrevlett.64.2963
|View full text |Cite
|
Sign up to set email alerts
|

Kwoket al. reply

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1

Citation Types

4
80
1
3

Year Published

1996
1996
2021
2021

Publication Types

Select...
7
1

Relationship

1
7

Authors

Journals

citations
Cited by 57 publications
(88 citation statements)
references
References 3 publications
4
80
1
3
Order By: Relevance
“…TPs strongly affect pinning and dynamics of vortices [23][24][25]. In particular, being plane defects they form channels of easy vortex motion along the plane of twins [24,25].…”
Section: T=t/(t C -∆T Irr ) (B)mentioning
confidence: 99%
“…TPs strongly affect pinning and dynamics of vortices [23][24][25]. In particular, being plane defects they form channels of easy vortex motion along the plane of twins [24,25].…”
Section: T=t/(t C -∆T Irr ) (B)mentioning
confidence: 99%
“…We observe this maximum for Hу1 T. The width of this peak, ϳ5°, is in the typical range of reported trapping angles for twins. [3][4][5]9,10 On the other hand, the fact that the peak is mounted over an inclined background implies that vortices are also trapped by the tracks. Thus vortices in this angular range contain segments both in the tracks and in the twins.…”
mentioning
confidence: 99%
“…13 Many experiments have confirmed the directional pinning due to columnar defects, twins, and Cu-O planes. [1][2][3][4][5][6][7][8][9][10][11] Evidence for a locked-in phase arises from the observation of the transverse Meissner effect, 10 but a quantitative determination of L (H,T) for columnar defects had not been done until now. The introduction of columnar defects inclined with respect to the crystallographic axis has been used 1,[6][7][8]10,11 to discriminate their pinning effects from those due to twin boundaries, and from anisotropy effects.…”
mentioning
confidence: 99%
See 1 more Smart Citation
“…С одной стороны, это неудивительно, поскольку в классическом рассмот-рении Бардина-Стефена для сверхпроводников второго рода зависящее от угла θ = ∠H, j магнитосопротивле-ние пропорционально sin 2 θ [14]. Скорость диссипации энергии на длину вихря зависит от произведения силы Лоренца на скорость движения вихря [14,15], а посколь-ку движение вихря возникает вследствие силы Лоренца, скорость вихря пропорциональна sin θ, что приводит к выражению R ∼ sin 2 θ.…”
Section: Introductionunclassified