sr studies of the pressure dependent superconducting
play

SR studies of the pressure dependent superconducting Formatvorlage - PowerPoint PPT Presentation

SR studies of the pressure dependent superconducting Formatvorlage des Untertitelmasters durch Klicken bearbeiten properties of Ca 3 Ir 4 Sn 13 Manuel Chinotti | | 17.01.16 1 Phase diagram of Ca 3 Ir 4 Sn 13 Anomaly around 33 K


  1. μSR studies of the pressure dependent superconducting Formatvorlage des Untertitelmasters durch Klicken bearbeiten properties of Ca 3 Ir 4 Sn 13 Manuel Chinotti | | 17.01.16 1

  2. Phase diagram of Ca 3 Ir 4 Sn 13 ● Anomaly around 33 K ● Critical temperature around 7 K Close to p c (around 18 kbar) find behavior of: CDW ● Superfluid density SC ● Superconducting gap CDW+SC ● Symmetry of the gap L.E. Klintberg et al ., PRL 109 , 237008 (2012) | | Manuel Chinotti 2

  3. μSR of Ca 3 Ir 4 Sn 13 under pressure Measurements in: ● TF-field: 500 G. ● Temperature range 0.25 K -10 K. ● Pressure range: 1.5 kbar-21.8 kbar Find average internal field, muon depolarization rate and penetration depth . | | Manuel Chinotti 3

  4. μSR: local probe technique | | Manuel Chinotti 4

  5. μSR of Ca 3 Ir 4 Sn 13 under pressure non SC SC Cu-Be p-cell MP35N p-cell | | Manuel Chinotti 5

  6. μSR of Ca 3 Ir 4 Sn 13 under pressure Cu-Be-cell MP35N-cell | | Manuel Chinotti 6

  7. μSR of Ca 3 Ir 4 Sn 13 under pressure | | Manuel Chinotti 7

  8. μSR of Ca 3 Ir 4 Sn 13 under pressure s-wave model in dirty limit ● Dirty superconductor: mean free path << BCS coherence length ● Nodeless superconductor at each pressure ● Behavior of Tc and of superfluid density different from BCS superconductors | | Manuel Chinotti 8

  9. μSR of Ca 3 Ir 4 Sn 13 under pressure L.E. Klintberg et al ., PRL 109 , 237008 (2012) ● Type II SC ● QCP: 15-16 kbar ● CDW gap suppressed | | Manuel Chinotti 9

  10. μSR of Ca 3 Ir 4 Sn 13 under pressure Strong-coupling SC | | Manuel Chinotti 10

  11. Summary ● Dirty, strong-coupling, type-II superconductor. ● Nodeless single gap BCS s-wave model. ● Superfluid density of Ca 3 Ir 4 Sn 13 increases dramatically under pressure. ● This is possibly due to suppression of CDW gap under pressure at about 15 kbar. | | Manuel Chinotti 11

  12. Literature ● P.K. Biswas et al., Phys. Rev. B 92 , 195122 (2015). ● P.K. Biswas et al., Phys. Rev. B 90 , 144505 (2014). ● S.J. Blundell, Contemporary Physics 40 , 203-225 (2004) | | Manuel Chinotti 12

Recommend


More recommend