About 30 per cent of the world’s population are children. Children are not only the most important people for their parents, but also the future of our societies. Providing them with the best possible education is of inestimable importance. Which education is best, however, is a question that is continually being negotiated. For a long time, this question was answered primarily by national governments. For some years, however, ongoing processes of globalisation are significantly shaping education, leading to what scholars term the global turn in education. Non-governmental organisations (NGOs) have become core actors in this global turnaround. They are increasingly joining forces in education-related transnational networks (i.e., global non-governmental spaces) that express an obvious claim to influence schools and education systems worldwide. Hence, questions arise about the associated risks and benefits for schools, particularly with regard to education's role in promoting educational achievement and equal opportunity among students from different backgrounds. However, despite this increasing relevance scholars have neglected to investigate transnational networks of NGOs in the field of education. EmergEd aims to drastically improve scientific knowledge on NGOs in education by analysing the emergence of global non-governmental spaces in education and how they influence education systems and schools – a contribution from which a far-reaching scientific – and in the long run societal – impact is to be expected. It will do so by developing an inter-disciplinary methodology integrating (inferential) Social Network Analysis (SNA) and Discourse Network Analysis (DNA), alongside qualitative data analysis based on Grounded Theory, to contribute to further theory building. This methodology is highly innovative as it draws theories and methods from different disciplines together in novel ways and thus follows an approach at and beyond the frontiers of disciplines.

What is the nature of matter at supranuclear densities? What is the expansion rate of our Universe? These open questions of nuclear physics and cosmology can be answered with multi-messenger observation of merging binary neutron stars. The window to study these fascinating events has only recently been opened with the upgrades of gravitational-wave observatories and by combining gravitational-wave information with that of powerful telescopes in the electromagnetic spectrum - from infrared, to optical, to gamma-rays. In the near future, we expect numerous multi-messenger observations of compact binary systems. We are currently at a crossroads in which the development of accurate and robust theoretical models is crucial to keeping up with the development of experimental instrumentation. Without noticeable upgrades of our models, future analyses will be biased through modelling uncertainties. The proposed research project will focus on the development of theoretical models to interpret the binary neutron star coalescence and will pave the way for a thorough understanding of the merger process. Novel methods and algorithms that we will implement in our numerical-relativity code will allow us to study previously inaccessible regions of the binary neutron star parameter space with unprecedented accuracy. This accuracy in the determination of the gravitational-wave and electromagnetic emission from binary neutron star mergers is essential for connecting our theoretical computations with observational data. We will push for a publicly available framework for the simultaneous analysis of gravitational-wave and electromagnetic signals from binary neutron star mergers incorporating also nuclear-physics calculations, nuclear-physics experiments, and other astrophysical observations of isolated neutron stars. This framework will enable us to use upcoming detections to determine the neutron star radius and the Hubble constant.