Over the last 20 years, femtosecond lasers have led to a host of novel scientific and industrial instrumentation enabling the direct measurement of optical frequencies and the realization of optical clocks, a Nobel Prize winning technology. Initially developed for fundamental science, the potential of femtosecond lasers for a wide range of cross-disciplinary applications has been demonstrated, including e.g. those in optical telecommunication, photonic analog-to-digital conversion, ultra-high precision signal sources for the upcoming quantum technologies and broadband optical spectroscopy in the environmental or bio-medical sciences and many more. Although, impressive cross-disciplinary demonstrations of the potential of femtosecond lasers are numerous, the technology has been hampered by its large size and high cost per system. The existing mode-locked semiconductor diode laser technology does not fulfil the needed performance specifications. The aim of the FEMTOCHIP project is to deliver a fully integrated chip-scale mode-locked laser with pulse energy, peak power and jitter specifications of a shoebox sized fiber laser system enabling a large fraction of the above-mentioned applications. Key challenges addressed are large cross-section, high gain, low background loss waveguide amplifiers, low loss passive waveguide technology and chirped waveguide gratings to accommodate high pulse peak power, to suppress Q-switching instabilities and to implement short pulse production by on-chip dispersion compensation and artificial saturable absorption. Therefore, the FEMTOCHIP consortium is composed of leaders in CMOS compatible ultra-low loss integrated SiN-photonics, rare-earth gain media development and deposition technology as well as ultrafast laser physics and technology for design, simulation and characterization to identify and address the key challenges in demonstrating a highly stable integrated femtosecond laser with table-top performance.

The prime objective of the project is to uplift the existing Centre of Excellence AstroCeNT by transforming it into a fully independent, interdisciplinary, new legal entity: Astrocent Plus Particle Astrophysics Science and Technology Centre. Astrocent Plus will engage in cutting-edge research and development in astroparticle physics and in related aspects of innovative technology, addressing global challenges, such as healthcare, climate change and sustainable sources of energy. As a fully autonomous entity with a modern professional management and administrative structure, it will be the first scientific institution in astroparticle physics supported by Teaming for Excellence and the first one in the field in Poland. Acting in close cooperation with world-leading consortium partners, Astrocent Plus will be embedded in a network of international collaborations involved in frontier research, probing the invisible Universe through neutrino, cosmic-ray, gravitational-wave and dark matter detection. AstroCeNT and the field have a proven record of medical and commercial applications and after the uplift will bring further high-impact benefits to society and economy. The buildup of internationally-rooted research capacity, gained through strategic partnerships, will position the Centre to achieve a significant, measurable, improvement in research and innovation culture and long-term financial sustainability, in part through commercialisation. The Centre will improve mobility and gender balance, train new cadres of highly-qualified researchers in science and hi-tech industry, promote innovation and cooperation between scientists and industry and help Poland and the EU attain a competitive position in the global value chains. With modern management practices, Astrocent Plus will become the main hub for the rapidly-developing field of particle astrophysics and a role model for Poland and the region for excellence in basic sciences and fruitful cooperation with industry.

One of the highlights of the European research infrastructure landscape is the world's most powerful X-ray-laser, the European XFEL. The ELBEX (Extracted Lepton Beam at the European XFEL) proposal builds on this strength and will set up new opportunities for European scientists and innovators, by providing an extracted high energy electron beam for experiments. With ELBEX we propose a pathfinder project to demonstrate the feasibility of such a facility at the European XFEL. This unique new possibility would strengthen the global competitiveness of the European Research Area and create opportunities for new user groups. The high energy, high charge density and excellent quality of the electron beam, if brought into interaction with a strong laser beam, opens up the study of a range of scientific topics, most prominently, of strong field Quantum Electrodynamics (QED). For the first time, the Schwinger limit for the electromagnetic field strength, at which non-perturbative QED effects become relevant, could be reached experimentally in this facility. Studying the particles created in the photon beam dump opens up the possibility to search for feebly interacting particles, complementing current or planned experiments like FASER II or SHiP. In addition, the electron beam itself is at the centre of a range of highly relevant and ambitious experiments in the area of accelerator science and detector science. Within the ELBEX project, the installation of a facility to extract an electron beam from the European XFEL using a fast kicker magnet and to transport it into a multi-purpose experimental area will be prepared. On the condition that a positive decision by the European XFEL council is reached to grant an extended 12-week XFEL shutdown, the installation of the ELBEX facility is an option.

OpenDreamKit will deliver a flexible toolkit enabling research groups to set up Virtual Research Environments, customised to meet the varied needs of research projects in pure mathematics and applications and supporting the full research life-cycle from exploration, through proof and publication, to archival and sharing of data and code. OpenDreamKit will be built out of a sustainable ecosystem of community-developed open software, databases, and services, including popular tools such as LinBox, MPIR, Sage(sagemath.org), GAP, PariGP, LMFDB, and Singular. We will extend the Jupyter Notebook environment to provide a flexible UI. By improving and unifying existing building blocks, OpenDreamKit will maximise both sustainability and impact, with beneficiaries extending to scientific computing, physics, chemistry, biology and more and including researchers, teachers, and industrial practitioners. We will define a novel component-based VRE architecture and the adapt existing mathematical software, databases, and UI components to work well within it on varied platforms. Interfaces to standard HPC and grid services will be built in. Our architecture will be informed by recent research into the sociology of mathematical collaboration, so as to properly support actual research practice. The ease of set up, adaptability and global impact will be demonstrated in a variety of demonstrator VREs. We will ourselves study the social challenges associated with large-scale open source code development and of publications based on executable documents, to ensure sustainability. OpenDreamKit will be conducted by a Europe-wide demand-steered collaboration, including leading mathematicians, computational researchers, and software developers long track record of delivering innovative open source software solutions for their respective communities. All produced code and tools will be open source.

This project aims at predicting the energy scale of cosmological inflation and the strength of the inflationary gravitational wave signal from string theory. Observations of the cosmic microwave background (CMB) temperature fluctuations have drastically changed cosmology into quantitative science. The results provide strong evidence for two phases of accelerated expansion in our Universe. The late-time phase of acceleration, termed ’dark energy’, is consistent with an extremely small positive cosmological constant, while the evidence for a very early phase of acceleration increasingly supports cosmological inflation. Very recently, the BICEP2 experiment reported the detection of B-mode polarization in the CMB. Pending future corroboration, this may correspond to a detection of primordial gravitational waves with a fractional power of about 10% of the CMB temperature fluctuations. In the context of inflation this implies an inflationary energy scale close to the scale of Grand Unification, and a large field excursion of the inflationary scalar field. Hence, the inflationary scalar potential needs symmetries to protect it from dangerous quantum corrections. These features strongly motivate the study of high-scale inflation in string theory as a candidate theory of quantum gravity. We will determine the range of predictions for large-field high-scale inflation in string theory driven by the mechanism of axion monodromy, which was co-discovered by the PI. For this purpose, we will establish a catalog of primary sources for large field ranges from axion monodromy in combination with assistance effects from multiple axion fields. We will analyze the generic effects of the interplay between large-field models of inflation in string theory with its necessary prerequisite, moduli stabilization. Finally, we will study the distribution of inflation mechanisms among the many vacua of string theory. In combination, this gives us a first chance to make string theory testable.