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Master Thesis Effect of vortex shaking on the ... - Physik-Institut

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12 This figure shows <strong>the</strong> difference between measurements with<br />

and without <str<strong>on</strong>g>shaking</str<strong>on</strong>g> for 9T main field. Obviously, <strong>the</strong> <str<strong>on</strong>g>shaking</str<strong>on</strong>g><br />

did not have an observable effect. . . . . . . . . . . . . . . . . 18<br />

13 The crystal structure <str<strong>on</strong>g>of</str<strong>on</strong>g> LuNi 2 B 2 C. Filled circles are Ni<br />

atoms, <strong>the</strong> largest open circles are Lu atoms. The Ni-B-C<br />

framework is indicated by <strong>the</strong> b<strong>on</strong>ds between <strong>the</strong> atoms. [26] . 20<br />

14 Temperature vs Resistance <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> LuNiBC crystal from 0 to<br />

7T, with <str<strong>on</strong>g>shaking</str<strong>on</strong>g>. . . . . . . . . . . . . . . . . . . . . . . . . . 21<br />

15 Temperature vs Resistance <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> LuNiBC crystal at 2T, with<br />

<str<strong>on</strong>g>shaking</str<strong>on</strong>g>. × represent pre-<str<strong>on</strong>g>shaking</str<strong>on</strong>g> results, + results after <str<strong>on</strong>g>shaking</str<strong>on</strong>g>.<br />

The dotted line follows <strong>the</strong> × as an aid. . . . . . . . . . 22<br />

16 To approach <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> current density J c towards Jc<br />

st is schematically<br />

shown as a functi<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> field B for a fixed Jc st . (i) At point<br />

A, J c > Jc<br />

st and J c decreases when <strong>the</strong> field is increased (path<br />

b) or decreased (path a). Similarly, at point C, J c < Jc<br />

st and<br />

J c increases when <strong>the</strong> field is increased (path d) or decreased<br />

(path c). (ii) The same is shown under <strong>the</strong> applicati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> an<br />

oscillatory field. [27] . . . . . . . . . . . . . . . . . . . . . . . 23<br />

17 Results for <strong>the</strong> two slow cooling measurements, <strong>the</strong> feature<br />

can be seen at ≈ 9.8K. . . . . . . . . . . . . . . . . . . . . . . 24<br />

18 Results <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> sec<strong>on</strong>d LuNiBC experiments. Adjusted data for<br />

all four runs. . . . . . . . . . . . . . . . . . . . . . . . . . . . . 25<br />

19 Zoom into <strong>the</strong> area around <strong>the</strong> feature. Within <strong>the</strong> experimental<br />

scatter, <strong>the</strong> two features (after fast and slow cooling)<br />

are nearly identical. . . . . . . . . . . . . . . . . . . . . . . . . 26<br />

20 In-plane resistance ρ(H, T) <str<strong>on</strong>g>of</str<strong>on</strong>g> a clean high-temperature superc<strong>on</strong>ductor.<br />

After [28]. . . . . . . . . . . . . . . . . . . . . . . . 29<br />

21 In-plane resistance ρ(H, T) <str<strong>on</strong>g>of</str<strong>on</strong>g> a high-temperature superc<strong>on</strong>ductor<br />

with pinning centers, without <str<strong>on</strong>g>shaking</str<strong>on</strong>g>. . . . . . . . . . 29<br />

22 Sketch <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> experimental setup, top view. . . . . . . . . . . . 30<br />

23 Comparis<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> fast and slow cooling in <strong>the</strong> sec<strong>on</strong>d LuNi 2 B 2 C<br />

experiment. The feature at 9.8K is both times clearly visible. . 31<br />

24 Comparis<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> runs without and with cycling. The upper figure<br />

shows that <strong>the</strong> velocity <str<strong>on</strong>g>of</str<strong>on</strong>g> cooling did not make a difference. 32<br />

34

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