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Programme

30 May – 31 May 2024

thursday

30
May

8:30

Registration

8:45

Welcome and opening (Gyanendra Singh)

9:00-9:45
Lecture

Annika Johansson. Fundamentals of Rashba physics.

Introduction to Rashba physics, its origin and its relevance in the context of spintronics applications. Tight-binding approximations to describe Rashba interactions in t2g-systems and introduction to semiclassical approximations to describe transport. Discussion of Rashba splitting, trivial/nontrivial anticrossings and ensuing spin band-textures.
9:45-9:55

PENDING QUESTIONS

9:55-10:40
Lecture

Annika Johansson. Spin-charge conversion in Rashba systems.

Basics of the Edelstein effect, and what distinguishes it from other effects, such as the spin Hall effect. Discussion of spin and orbital Edelstein effects, and how can they be evaluated using semiclassical approximations. Edelstein effect applied to t2g systems. Specific contributions to orbital/spin Edelstein effects coming from the features of the band structure, paying particular attention to contributions coming from topologically trivial/nontrivial anticrossings, and their relevance for the spin-charge conversion problem.
10:40-10:45

PENDING QUESTIONS

10:45-11:15

Coffee Break

11:15-12:00
Lecture

Andrea Caviglia. Experimental detection of the Rashba effect and spin-charge conversion.

Detection of Rashba coefficients using transport. How Rashba parameters can be extracted from low-temperature measurements by analyzing quantum corrections to the conductivity (weak antilocalization) and the bilinear/quadratic magnetoresistance methods. Transport methods to evaluate spin-charge conversion through Edelstein effects and possible detection of orbital and spin sources through X-ray absorption (XAS) experiments and GHz/THz methods.
12:00-12:30

PENDING QUESTIONS / DISCUSSION LECTURES ON RASHBA PHYSICS

12:30-14:00

Lunch Break

14:00-16:00
Lecturer

Gyanendra Singh and Janine Gückelhorn. Practical session of training on the extraction of Rashba parameters.

. The lecture will guide on training technical session to use magnetotransport measurements on a 2DEG system (LaAlO3/SrTiO3 devices). Use of weak (anti)localization theory and bilinear magnetoresistance/quadratic magnetoresistance (BMR/QMR) method to fit experiments and extract Rashba parameters. The lecture will combine conventional presentations and recorded videos of real experiments.
DAY 1, 30 May 2024, RASHBA PHYSICS

friday

31
May

9:00-9:45
Lecture

Mario Cuoco. General introduction to Berry phase and Berry curvature.

Short introduction to the concept of Berry connection, Berry phase and Berry curvature, and their link to topological quantum matter. How Berry curvature generates an anomalous velocity and explain the analogy of Berry curvature as a source of “magnetic field”. Discussion of the role of symmetry, dimensionality and the occurrence of Berry curvature. Why Berry curvature is related to the anomalous Hall effect. These concepts will be applied to electronic structures in ferromagnetic systems with spin-orbit coupling, focusing first on SrRuO3 as a materials case where the effects of Berry curvatures can be analyzed. The concept of Weyl node will be introduced. Generality of these concepts to other ferromagnetic systems, considering the role of dimensionality and symmetry.
9:45-9:55

PENDING QUESTIONS

9:55-10:40
Lecture

Mario Cuoco. Berry physics beyond (without) Weyl cones.

The discussion will focus on the case of low-dimensional systems, in particular on oxides with (t2g) orbital close to the Fermi level. Discussion of oxide interfaces, as a platform for the design of sources of Berry curvature without Weyl cones. Differences between the previous case (Berry curvatures generated by Weyl cones) and the present (without Weyl cones). Berry curvatures with spin and orbital sources. Why it is important to design spin and orbital sources? What is the generality of these concepts? Are other materials relevant beyond oxide interfaces (e.g. antiferromagnets or superconductors)?
10:40-10:45

PENDING QUESTIONS

10:45-11:15

Coffee Break

11:15-12:00
Lecture

Andrea Caviglia. Experimental detection of Berry curvatures.

How the Berry curvature can be detected experimentally in condensed matter systems? Orbital and spin sources of Berry curvature (described in the previous lecture) can be distinguished experimentally by performing different transport characterization methods. To bring this point, the lecturer will describe and explain how to measure anomalous planar Hall effect and nonlinear Hall transport to differentiate orbital and spin sources of Berry curvature.
12:00-12:30

PENDING QUESTIONS / DISCUSSION LECTURES ON RASHBA PHYSICS

12:30

CLOSING REMARKS AND END OF LECTURE

DAY 2, 31 May 2024, BERRY PHYSICS