See photos from Nordita


Current Events

From Molecular Basis to Predictability and Control of Evolution


1—26 July 2019

Coordinators: Marta Luksza, Armita Nourmouhammad, Fernanda Pinheiro

Growing amount of molecular biological data combined with current advances in modeling of complex systems provide unprecedented opportunities to understand biological evolution in a quantitative way. A quantitative description of an evolving system is the first step towards prediction and control, and it opens new exciting directions for highly interdisciplinary research. The central questions are: (i) to what degree we can predict the outcome of biological evolution, (ii) what features of the system are predictable and (iii) which features confer predictive value for a quantitative description of the system. This program brings together theoretical and experimental physicists, experimental biologists with an interest in quantitative modelling and mathematicians with interest in biological systems.

Integrability in Gauge and String Theories 2019


15—19 July 2019

Coordinators: Valentina Giangreco Marotta Puletti, Monica Guica, Henrik Johansson, Joseph Minahan, Olof Ohlsson Sax, Michelangelo Preti, Dmytro Volin, Konstantin Zarembo

The conference will cover cutting-edge non-perturbative methods in quantum field theory, as well as mathematical aspects of integrability and its more traditional applications in condensed-matter physics and statistical mechanics. Solvable models play a valuable a role in theoretical physics, as they illustrate general concepts in a simpler setting and provide insights into the qualitative features of more complex phenomena.

Show:  All events  Programs  Workshops, Conferences, Meetings  Schools
Info: Full Medium Brief
Period: All Current & Future

Future Events


Holographic QCD


22—26 July 2019

Coordinators: Elias Kiritsis, Jacob Sonnenschein, Ismail Zahed, Konstantin Zarembo

In the last few years there has been renewed interest in QCD and hadronic dynamics using holographic gauge/gravity duality, resurge of the large N methods, progress in string models, integrability, unitarity and bootstrap and more. Also, many new experimental results were reported by ALICE at LHC regarding collectivization in pp and pA collisions, by LHCb at CERN and the B- and C-factories regarding the existence of exotics and the spectroscopy of heavy-light systems, and more recently the reporting of 2 neutron star mergers by the LIGO collaboration and its constraint on the nuclear dense equation of state. The conference will bring together practitioners of these interdisciplinary fields to discuss these exciting new developments, and explore the relevance of the holographic framework for addressing these observations.

Topological Quantum Matter: From Low-Temperature Physics to Non-Equilibrium Dynamics


29 July — 23 August 2019

Coordinators: Jens H. Bardarson, Emil J. Bergholtz, Annica Black-Schaffer, Jan Budich, Roni Ilan

Recent advances in the band theory of crystalline materials have singled out topology as a key ingredient in the modern classification of matter, with major impact on measurable electronic properties. Topological band theory has also grown into an emerging paradigm in many areas of physics, and is now used to characterize metamaterials, including photonic, atomic, acoustic, and elastic systems, in both the quantum and classical regimes. As our understanding of topology in physics widens, the incorporation of out-of-equilibrium phenomena is gaining in importance.

Nordita Master Class in Physics 2019


10—15 August 2019

Coordinators: Dhrubaditya Mitra

The traditional Nordita summer school in physics for students from the Nordic and Baltic countries aims at introducing frontier areas of physics research by world top scientists at a level understandable for master's and undergraduate students, and also to stimulate further studies. The lectures will be accompanied by exercises in groups and discussion sessions.

Gravitational Waves from the Early Universe


26 August — 20 September 2019

Coordinators: Axel Brandenburg, Mark Hindmarsh, Tina Kahniashvili

Gravitational waves promise a new window into the highest-energy events in the evolution of the universe. The recent LIGO/Virgo detections of gravitational waves from the mergers of binary black holes and binary neutron stars and have ignited interest in the future direction of gravitational wave astronomy. A space-based laser interferometer, pioneered by NASA's LISA concept and the European Space Agency's eLISA program and ESA's recent spectacularly successful LISA Pathfinder mission, would enable direct detection of gravitational waves in the milliHertz range. A lower frequency range would allow detection of supermassive black hole mergers, tracing the galaxy merger history and serving as cosmic sirens to probe the universe's expansion history, as well as precursors for the LIGO sources. A space-based detector would also be sensitive to stochastic gravitational wave backgrounds produced by unknown physics operating in the very early universe, including an electroweak phase transition. This Nordita program will bring scientists together to engage in an effort to characterize and detect sources contributing to the gravitational wave background from the early universe, and the implications for new physics at the TeV scale and beyond.

Machine Learning for Quantum Matter


26—28 August 2019

Coordinators: Alexander Balatsky, Jens H. Bardarson, Mathias Geilhufe, Bart Olsthoorn

Machine learning has entered the field of quantum matter with applications covering quantum materials and the many-body problem. For example, interpretable and computationally-efficient machine learning models are able to capture the structure-property relationship in materials science. In case of the many-body problem, machine learning architectures provide versatile wavefunctions that lead to accurate results and prove to be more flexible than traditional methods. Conversely, methods in physics have also influenced the development of machine learning methods in the case of tensor networks. The workshop will feature talks by leading experts combined with the talks of younger participants to present a broad picture of the activities and best ideas on the use of ML methods in quantum matter.

Quantum Materials for Dark Matter Detection


9—13 September 2019

Coordinators: Alexander Balatsky, Jan Conrad, Alfredo Ferella, Mathias Geilhufe, Felix Kahlhoefer, Mathew Lawson

In the search for dark matter (DM), one particular focus is on light and ultra-light dark matter, i.e. sub-GeV mass dark matter from a hidden dark sector with a new force interacting with the standard model or ultra-light DM with mass range from 10−22 eV to keV. The arguably most popular example of the latter class is the axion, invoked to solve the apparent absence of CP violation in Quantum Chromo Dynamics. Detection of these particles poses new challenges to potential sensor materials: very small energy depositions, magnetic properties and anisotropic response to particle interactions for example become crucial requirements. The challenge of finding suitable materials fits well with recent developments in solid state physics: Motivated by the exponential growth of computational power and the resulting data, we witness the rapid adoption of functional materials prediction within the framework of materials informatics. Here, methods adapted from computer science based on data-mining and machine learning are applied to identify materials with requested target properties.

Challenges in Theoretical High-Energy Physics


23—27 September 2019

Coordinators: Agnese Bissi, Valentina Giangreco Puletti, Magdalena Larfors, Marta Orselli



Particle Growth in Turbulence


18 May — 12 June 2020

Coordinators: Axel Brandenburg, Bernhard Mehlig

The question of how particles and droplets can grow in a turbulent environment is of great current interest in many fields, in astrophysics, cloud microphysics, in biology, and in the engineering sciences. For example, coagulation and condensation in turbulent clouds turn microscopic cloud droplets into rain drops. In astrophysics, planetesimals are thought to form by aggregation of microscopic dust grains in the turbulent environment surrounding a forming star. In both cases, turbulence is believed to be a crucial factor for particle growth. Yet the microscopic mechanisms determining this growth are far from understood. In the past few years there has been substantial progress in understanding the mechanisms that determine how particles move in turbulence, albeit mostly for simplified model systems. The challenge is now to understand how these mechanisms lead to rapid particle growth.

nw-4.6 (870)
11 Jun 2019

This page was printed on 2019-07-19 from