Project acronym PLASMATS
Project Plasma-assisted development and functionalization of electrospun mats for tissue engineering purposes
Researcher (PI) Nathalie Marie-Thérèse De Geyter
Host Institution (HI) UNIVERSITEIT GENT
Call Details Starting Grant (StG), PE8, ERC-2013-StG
Summary "In this project, I will explore the unique combination of two fascinating research themes: electrospinning and plasma technology. Electrospun nanofibrous matrices (so-called mats) are an exciting class of materials with a wide range of possible applications. Nevertheless, the development and functionalization of these electrospun materials remain very challenging tasks.
Atmospheric pressure plasma technology will be utilized by my research group to create advanced biodegradable electrospun mats with unprecedented functionality and performance. To realise such a major breakthrough, plasma technology will be implemented in different steps of the manufacturing process: pre-electrospinning and post-electrospinning.
My group will focus on four cornerstone research lines, which have been carefully chosen so that all critical issues one could encounter in creating advanced biodegradable electrospun mats are tackled. Research cornerstone A aims to develop biodegradable electrospun mats with appropriate bulk properties, while in research cornerstone B pre-electrospinning polymer solutions will be exposed to non-thermal atmospheric plasmas. This will be realized by probing unexplored concepts such as discharges created inside polymer solutions. In a third cornerstone C, an in-depth study of the interactions between an atmospheric pressure plasma and an electrospun mat will be carried out. Finally, the last cornerstone D will focus on plasma-assisted surface modification of biodegradable electrospun mats for tissue engineering purposes.
Realization of these four cornerstones would result in a major breakthrough in their specific field which makes this proposal inherently a relatively high risk/very high gain proposal. I therefore strongly believe that this research program will open a whole new window of opportunities for electrospun materials with a large impact on science and society."
Summary
"In this project, I will explore the unique combination of two fascinating research themes: electrospinning and plasma technology. Electrospun nanofibrous matrices (so-called mats) are an exciting class of materials with a wide range of possible applications. Nevertheless, the development and functionalization of these electrospun materials remain very challenging tasks.
Atmospheric pressure plasma technology will be utilized by my research group to create advanced biodegradable electrospun mats with unprecedented functionality and performance. To realise such a major breakthrough, plasma technology will be implemented in different steps of the manufacturing process: pre-electrospinning and post-electrospinning.
My group will focus on four cornerstone research lines, which have been carefully chosen so that all critical issues one could encounter in creating advanced biodegradable electrospun mats are tackled. Research cornerstone A aims to develop biodegradable electrospun mats with appropriate bulk properties, while in research cornerstone B pre-electrospinning polymer solutions will be exposed to non-thermal atmospheric plasmas. This will be realized by probing unexplored concepts such as discharges created inside polymer solutions. In a third cornerstone C, an in-depth study of the interactions between an atmospheric pressure plasma and an electrospun mat will be carried out. Finally, the last cornerstone D will focus on plasma-assisted surface modification of biodegradable electrospun mats for tissue engineering purposes.
Realization of these four cornerstones would result in a major breakthrough in their specific field which makes this proposal inherently a relatively high risk/very high gain proposal. I therefore strongly believe that this research program will open a whole new window of opportunities for electrospun materials with a large impact on science and society."
Max ERC Funding
1 391 100 €
Duration
Start date: 2014-02-01, End date: 2019-01-31
Project acronym PrintPack
Project Arranging the Particles: Step Changing Chemical Measurement Technology
Researcher (PI) Gert DESMET
Host Institution (HI) VRIJE UNIVERSITEIT BRUSSEL
Call Details Advanced Grant (AdG), PE8, ERC-2015-AdG
Summary The progress in liquid chromatography (LC), basically following Moore’s law over the last decade, will soon come to a halt. LC is the current state-of-the-art chemical separation method to measure the composition of complex mixtures. Driven by the ever growing complexity of the samples in e.g., environmental and biomedical research, LC is constantly pushed to higher efficiencies. Using highly optimized and monodisperse spherical particles, randomly packed in high pressure columns, the progress in LC has up till now been realized by reducing the particle size and concomitantly increasing the pressure. With pressure already up at 1500 bar, groundbreaking progress is still badly needed, e.g., to fully unravel the complex reaction networks in human cells.
For this purpose, it is proposed to leave the randomly packed bed paradigm and move to structures wherein the 1 to 5 micrometer particles currently used in LC are arranged in perfectly ordered and open-structured geometries. This is now possible, as the latest advances in nano-manufacturing and positioning allow proposing and developing an inventive high-throughput particle assembly and deposition strategy. The PI's ability to develop new parts of chromatography will be used to rationally optimize the many possible geometries accessible through this disruptive new technology, and identify those structures coping best with any remaining degree of disorder. Using the PI's experimental know-how on microfluidic chromatography systems, these structures will be used to pursue the disruptive gain margin (order of factor 100 in separation speed) that is expected based on general chromatography theory.
Testing this groundbreaking new generation of LC columns together with world-leading bio-analytical scientists will illustrate their potential in making new discoveries in biology and life sciences. The new nano-assembly strategies might also be pushed to other applications, such as photonic crystals.
Summary
The progress in liquid chromatography (LC), basically following Moore’s law over the last decade, will soon come to a halt. LC is the current state-of-the-art chemical separation method to measure the composition of complex mixtures. Driven by the ever growing complexity of the samples in e.g., environmental and biomedical research, LC is constantly pushed to higher efficiencies. Using highly optimized and monodisperse spherical particles, randomly packed in high pressure columns, the progress in LC has up till now been realized by reducing the particle size and concomitantly increasing the pressure. With pressure already up at 1500 bar, groundbreaking progress is still badly needed, e.g., to fully unravel the complex reaction networks in human cells.
For this purpose, it is proposed to leave the randomly packed bed paradigm and move to structures wherein the 1 to 5 micrometer particles currently used in LC are arranged in perfectly ordered and open-structured geometries. This is now possible, as the latest advances in nano-manufacturing and positioning allow proposing and developing an inventive high-throughput particle assembly and deposition strategy. The PI's ability to develop new parts of chromatography will be used to rationally optimize the many possible geometries accessible through this disruptive new technology, and identify those structures coping best with any remaining degree of disorder. Using the PI's experimental know-how on microfluidic chromatography systems, these structures will be used to pursue the disruptive gain margin (order of factor 100 in separation speed) that is expected based on general chromatography theory.
Testing this groundbreaking new generation of LC columns together with world-leading bio-analytical scientists will illustrate their potential in making new discoveries in biology and life sciences. The new nano-assembly strategies might also be pushed to other applications, such as photonic crystals.
Max ERC Funding
2 488 813 €
Duration
Start date: 2016-10-01, End date: 2021-09-30
Project acronym PROMINENT
Project Solar prominences: unraveling the ultimate condensation catastrophe
Researcher (PI) Rony KEPPENS
Host Institution (HI) KATHOLIEKE UNIVERSITEIT LEUVEN
Call Details Advanced Grant (AdG), PE9, ERC-2018-ADG
Summary The most spectacular solar eruptions recorded in history - such as the Grand Daddy Prominence eruption on the 4th of June 1946 - invariably involve the violent ejection of a prominence: a giant, cool and dense plasma cloud that formed spontaneously within the million-degree solar corona. The role of the dominant prominence mass in all magnetically mediated coronal mass ejections is poorly understood, and yet a typical prominence easily outweighs our Earth population in mass (and the Earth itself in size). While they pervade the solar corona in all shapes and sizes, surprisingly little is known on their formation and ultimate disappearance. At the advent of two revolutionary space missions to the inner reaches of our heliosphere (Parker Probe and Solar Orbiter), a dedicated effort on ab initio prominence simulations beyond current resolution limits is needed. This must provide conclusive answers to intriguing riddles: How, where and why does the solar corona spontaneously condense to form these gigantic structures? What is the magnetic field topology throughout the prominence body, and how can it support their weight against solar gravity? What causes the fine structure (so-called threads and barbs) throughout the prominence body, and what is the role of the mysterious solar tornadoes often found at their feet? Can we use their natural oscillation frequencies seismologically? Is it feasible to predict their eruption, and can one quantify their role in space weather contexts? Armed with state-of-the-art, grid-adaptive software to efficiently exploit current and next generation supercomputers, we will resolve these mysteries, confront historic and forthcoming observations, and train a new generation of solar physicists. Along the way, we unravel fundamental processes relevant in many astrophysical contexts: how do radiatively driven, thermal instabilities induce catastrophic, non-gravitationally mediated condensations?
Summary
The most spectacular solar eruptions recorded in history - such as the Grand Daddy Prominence eruption on the 4th of June 1946 - invariably involve the violent ejection of a prominence: a giant, cool and dense plasma cloud that formed spontaneously within the million-degree solar corona. The role of the dominant prominence mass in all magnetically mediated coronal mass ejections is poorly understood, and yet a typical prominence easily outweighs our Earth population in mass (and the Earth itself in size). While they pervade the solar corona in all shapes and sizes, surprisingly little is known on their formation and ultimate disappearance. At the advent of two revolutionary space missions to the inner reaches of our heliosphere (Parker Probe and Solar Orbiter), a dedicated effort on ab initio prominence simulations beyond current resolution limits is needed. This must provide conclusive answers to intriguing riddles: How, where and why does the solar corona spontaneously condense to form these gigantic structures? What is the magnetic field topology throughout the prominence body, and how can it support their weight against solar gravity? What causes the fine structure (so-called threads and barbs) throughout the prominence body, and what is the role of the mysterious solar tornadoes often found at their feet? Can we use their natural oscillation frequencies seismologically? Is it feasible to predict their eruption, and can one quantify their role in space weather contexts? Armed with state-of-the-art, grid-adaptive software to efficiently exploit current and next generation supercomputers, we will resolve these mysteries, confront historic and forthcoming observations, and train a new generation of solar physicists. Along the way, we unravel fundamental processes relevant in many astrophysical contexts: how do radiatively driven, thermal instabilities induce catastrophic, non-gravitationally mediated condensations?
Max ERC Funding
2 331 250 €
Duration
Start date: 2019-09-01, End date: 2024-08-31
Project acronym PROSPER
Project Design of polymer optical fibre gratings for endoscopic biosensing purposes
Researcher (PI) Christophe Caucheteur
Host Institution (HI) UNIVERSITE DE MONS
Call Details Starting Grant (StG), PE8, ERC-2011-StG_20101014
Summary "PROSPER is a multidisciplinary project covering the emerging fields of photonics, bio-chemistry and endoscopy, targeting to contribute to the development of a new class of biochemical optical sensors that would significantly improve the healthcare of the future.
PROSPER will address this objective through the demonstration of biosensors based on a functionalized polymer optical fibre (POF) in which specially-designed refractive-index gratings have been written. Immobilised biomolecular receptors on the grafted fibre surface will allow label-free recognition through the monitoring of wavelength shifts in the grating spectral response. Such biosensors are predicted to exhibit a surrounding refractive index detection limit of 10-6 in real time, which is classical for biodetection. Although generic and able to work in various areas such as environmental monitoring, food analysis, agriculture or security, the proposed biosensors will be targeted for medical diagnostics where they present the most ground-breaking nature. Indeed, unlike bulk structures, they require reduced reaction volumes for ex-vivo measurements and present the advantageous possibility of assaying several parameters simultaneously (e.g. several cancer-associated antigens in one sample). As a result, statistical analysis of these parameters can potentially increase the reliability and reduce the measurement uncertainty of a diagnostic over single-parameter assays. More importantly, the proposed biosensors have the unique potential to be used in-vivo in an endoscope (for this reason POFs are privileged over silica), which would considerably improve the diagnostic. The ultimate target of PROSPER is thus to demonstrate the feasibility of diagnostics outside of laboratory settings. A final prototype consisting of a packaged polymer biosensor will be validated."
Summary
"PROSPER is a multidisciplinary project covering the emerging fields of photonics, bio-chemistry and endoscopy, targeting to contribute to the development of a new class of biochemical optical sensors that would significantly improve the healthcare of the future.
PROSPER will address this objective through the demonstration of biosensors based on a functionalized polymer optical fibre (POF) in which specially-designed refractive-index gratings have been written. Immobilised biomolecular receptors on the grafted fibre surface will allow label-free recognition through the monitoring of wavelength shifts in the grating spectral response. Such biosensors are predicted to exhibit a surrounding refractive index detection limit of 10-6 in real time, which is classical for biodetection. Although generic and able to work in various areas such as environmental monitoring, food analysis, agriculture or security, the proposed biosensors will be targeted for medical diagnostics where they present the most ground-breaking nature. Indeed, unlike bulk structures, they require reduced reaction volumes for ex-vivo measurements and present the advantageous possibility of assaying several parameters simultaneously (e.g. several cancer-associated antigens in one sample). As a result, statistical analysis of these parameters can potentially increase the reliability and reduce the measurement uncertainty of a diagnostic over single-parameter assays. More importantly, the proposed biosensors have the unique potential to be used in-vivo in an endoscope (for this reason POFs are privileged over silica), which would considerably improve the diagnostic. The ultimate target of PROSPER is thus to demonstrate the feasibility of diagnostics outside of laboratory settings. A final prototype consisting of a packaged polymer biosensor will be validated."
Max ERC Funding
1 438 368 €
Duration
Start date: 2011-12-01, End date: 2016-11-30
Project acronym PROSPERITY
Project Probing Stellar Physics and Testing Stellar Evolution through Asteroseismology
Researcher (PI) Conny Aerts
Host Institution (HI) KATHOLIEKE UNIVERSITEIT LEUVEN
Call Details Advanced Grant (AdG), PE9, ERC-2008-AdG
Summary Our goal is to achieve a physical description of stellar interiors with an order of magnitude better precision in the physical quantities than we have now. We will concentrate on three outstanding critical issues in current stellar structure theory and solve them through a novel approach termed asteroseismology. 1. We will obtain a quantitative estimate of the amount of convective mixing and of the internal rotation profile for a broad range of stellar masses and evolutionary states, with specific emphasis on massive stars and on red giant stars. This will be done using new seismic data assembled by the space missions MOST, CoRoT and Kepler, which have a factor 1000 better precision than the ground-based data we had to rely on so far. 2. We will include, for the first time, the effect of a radiation-driven stellar wind on the theoretical description of stellar oscillations. This opens a new avenu: the seismic calibration of stellar evolution models of the most massive stars from the core-hydrogen burning up to the supernova stage. 3. We will build a new dedicated camera, MAIA, for the Mercator telescope at La Palma (Canary Islands), to investigate the badly understood common envelope phase of close binary stars. There are large unknowns in their evolution, mainly during the red giant phase when the two stellar components may share a common envelope. The recently discovered pulsating subdwarf O and B binaries must have lost their hydrogen envelope during a common envelope phase near the tip of the red giant branch. We will put tight seismic constraints on their outer hydrogen layer and mass and use these two diagnostics to perform a critical evaluation of close binary evolution theory along the giant branch. Our project encompasses engineering, observational astronomy, theoretical astrophysics, time series analysis and statistical clustering. It will revolutionise stellar evolution theory for a variety of stars and all topics in astrophysics that build on it.
Summary
Our goal is to achieve a physical description of stellar interiors with an order of magnitude better precision in the physical quantities than we have now. We will concentrate on three outstanding critical issues in current stellar structure theory and solve them through a novel approach termed asteroseismology. 1. We will obtain a quantitative estimate of the amount of convective mixing and of the internal rotation profile for a broad range of stellar masses and evolutionary states, with specific emphasis on massive stars and on red giant stars. This will be done using new seismic data assembled by the space missions MOST, CoRoT and Kepler, which have a factor 1000 better precision than the ground-based data we had to rely on so far. 2. We will include, for the first time, the effect of a radiation-driven stellar wind on the theoretical description of stellar oscillations. This opens a new avenu: the seismic calibration of stellar evolution models of the most massive stars from the core-hydrogen burning up to the supernova stage. 3. We will build a new dedicated camera, MAIA, for the Mercator telescope at La Palma (Canary Islands), to investigate the badly understood common envelope phase of close binary stars. There are large unknowns in their evolution, mainly during the red giant phase when the two stellar components may share a common envelope. The recently discovered pulsating subdwarf O and B binaries must have lost their hydrogen envelope during a common envelope phase near the tip of the red giant branch. We will put tight seismic constraints on their outer hydrogen layer and mass and use these two diagnostics to perform a critical evaluation of close binary evolution theory along the giant branch. Our project encompasses engineering, observational astronomy, theoretical astrophysics, time series analysis and statistical clustering. It will revolutionise stellar evolution theory for a variety of stars and all topics in astrophysics that build on it.
Max ERC Funding
2 491 200 €
Duration
Start date: 2009-01-01, End date: 2013-12-31
Project acronym QUTE
Project Quantum Tensor Networks and Entanglement
Researcher (PI) Frank Paul Bernard Verstraete
Host Institution (HI) UNIVERSITEIT GENT
Call Details Consolidator Grant (CoG), PE2, ERC-2014-CoG
Summary One of the major challenges in theoretical physics is the development of systematic methods for describing and simulating quantum many body systems with strong interactions. Given the huge experimental progress and technological potential in manipulating strongly correlated atoms and electrons, there is a pressing need for such a better theory.
The study of quantum entanglement holds the promise of being a game changer for this question. By mapping out the entanglement structure of the low-energy wavefunctions of quantum spin systems on the lattice, the prototypical example of strongly correlated systems, we have found that the associated wavefunctions can be very well modeled by a novel class of variational wavefunctions, called tensor network states. Tensor networks are changing the ways in which strongly correlated systems can be simulated, classified and understood: as opposed to the usual many body methods, these tensor networks are generic and describe non-perturbative effects in a very natural way.
The goal of this proposal is to advance the scope and use of tensor networks in several directions, both from the numerical and theoretical point of view. We plan to study the differential geometric character of the manifold of tensor network states and the associated nonlinear differential equations of motion on it, develop post tensor network methods in the form of effective theories on top of the tensor network vacuum, study tensor networks in the context of lattice gauge theories and topologically ordered systems, and investigate the novel insights that tensor networks are providing to the renormalization group and the holographic principle.
Colloquially, we believe that tensor networks and the theory of entanglement provide a basic new vocabulary for describing strongly correlated quantum systems, and the main goal of this proposal is to develop the syntax and semantics of that new language.
Summary
One of the major challenges in theoretical physics is the development of systematic methods for describing and simulating quantum many body systems with strong interactions. Given the huge experimental progress and technological potential in manipulating strongly correlated atoms and electrons, there is a pressing need for such a better theory.
The study of quantum entanglement holds the promise of being a game changer for this question. By mapping out the entanglement structure of the low-energy wavefunctions of quantum spin systems on the lattice, the prototypical example of strongly correlated systems, we have found that the associated wavefunctions can be very well modeled by a novel class of variational wavefunctions, called tensor network states. Tensor networks are changing the ways in which strongly correlated systems can be simulated, classified and understood: as opposed to the usual many body methods, these tensor networks are generic and describe non-perturbative effects in a very natural way.
The goal of this proposal is to advance the scope and use of tensor networks in several directions, both from the numerical and theoretical point of view. We plan to study the differential geometric character of the manifold of tensor network states and the associated nonlinear differential equations of motion on it, develop post tensor network methods in the form of effective theories on top of the tensor network vacuum, study tensor networks in the context of lattice gauge theories and topologically ordered systems, and investigate the novel insights that tensor networks are providing to the renormalization group and the holographic principle.
Colloquially, we believe that tensor networks and the theory of entanglement provide a basic new vocabulary for describing strongly correlated quantum systems, and the main goal of this proposal is to develop the syntax and semantics of that new language.
Max ERC Funding
1 927 500 €
Duration
Start date: 2015-09-01, End date: 2020-08-31
Project acronym RadNu
Project Radio detection of the PeV - EeV cosmic-neutrino flux
Researcher (PI) Krijn DE VRIES
Host Institution (HI) VRIJE UNIVERSITEIT BRUSSEL
Call Details Starting Grant (StG), PE9, ERC-2018-STG
Summary With the detection of the high-energy cosmic-neutrino flux by the IceCube neutrino observatory at the South-Pole, IceCube opened the field of neutrino astronomy. Nevertheless, due to the steeply falling energy spectrum, IceCube runs low in statistics at energies above a few PeV. To probe this flux at the highest energies (>PeV), therefore asks for an even larger detection volume than the cubic-kilometer currently instrumented by IceCube.
Due to its long attenuation length the radio signal is an ideal probe to cover such a large volume. When a high-energy cosmic neutrino interacts in a dense medium like ice, a relativistic particle cascade is induced. In 1962 Askaryan already predicted that due to the net charge build-up inside the cascade, coherent radio emission is expected. However, this signal is only detectable for initial neutrino energies in access of a few EeV. Therefore, currently there is a sensitivity gap to probe the high-energy cosmic neutrino flux in the PeV – EeV energy range.
This project aims to fill this sensitivity gap by the development of a novel radio detection technique to measure high-energy particle cascades in dense media, the radar detection technique. By directly probing the ionization plasma which is left behind after the neutrino induced particle cascade propagates through the medium, the radio detection energy threshold is lowered to a few PeV. The feasibility of the radar detection technique, was shown in a recent experiment. To determine the radar scattering efficiency more accurately, a new beam-test at the SLAC facility is planned as part of this proposal.
Once the scattering parameters have been determined accurately, a detailed modeling and sensitivity study will be performed to achieve the main goal of this research proposal: The construction of an in-nature experiment at the South-Pole with the sensitivity to observe 1-10 cosmic neutrino events per year in the PeV – EeV energy range.
Summary
With the detection of the high-energy cosmic-neutrino flux by the IceCube neutrino observatory at the South-Pole, IceCube opened the field of neutrino astronomy. Nevertheless, due to the steeply falling energy spectrum, IceCube runs low in statistics at energies above a few PeV. To probe this flux at the highest energies (>PeV), therefore asks for an even larger detection volume than the cubic-kilometer currently instrumented by IceCube.
Due to its long attenuation length the radio signal is an ideal probe to cover such a large volume. When a high-energy cosmic neutrino interacts in a dense medium like ice, a relativistic particle cascade is induced. In 1962 Askaryan already predicted that due to the net charge build-up inside the cascade, coherent radio emission is expected. However, this signal is only detectable for initial neutrino energies in access of a few EeV. Therefore, currently there is a sensitivity gap to probe the high-energy cosmic neutrino flux in the PeV – EeV energy range.
This project aims to fill this sensitivity gap by the development of a novel radio detection technique to measure high-energy particle cascades in dense media, the radar detection technique. By directly probing the ionization plasma which is left behind after the neutrino induced particle cascade propagates through the medium, the radio detection energy threshold is lowered to a few PeV. The feasibility of the radar detection technique, was shown in a recent experiment. To determine the radar scattering efficiency more accurately, a new beam-test at the SLAC facility is planned as part of this proposal.
Once the scattering parameters have been determined accurately, a detailed modeling and sensitivity study will be performed to achieve the main goal of this research proposal: The construction of an in-nature experiment at the South-Pole with the sensitivity to observe 1-10 cosmic neutrino events per year in the PeV – EeV energy range.
Max ERC Funding
1 410 000 €
Duration
Start date: 2019-02-01, End date: 2024-01-31
Project acronym SmartCast
Project Smart casting of concrete structures by active control of rheology
Researcher (PI) Geert De schutter
Host Institution (HI) UNIVERSITEIT GENT
Call Details Advanced Grant (AdG), PE8, ERC-2015-AdG
Summary Concrete production processes do not take full advantage of the rheological potential of fresh cementitious materials, and are still largely labour-driven and sensitive to the human factor. SmartCast proposes a new concrete casting concept to transform the concrete industry into a highly automated technological industry. Currently, the rheological properties of the concrete are defined by mix design and mixing procedure without any further active adjustment during casting. The goal of this proposal is the active control of concrete rheology during casting, and the active triggering of early stiffening of the concrete as soon as it is put in place. The ground-breaking idea to achieve this goal, is to develop concrete with actively controllable rheology by adding admixtures responsive to externally activated electromagnetic frequencies. Inter-disciplinary insights are important to achieve these goals, including inputs from concrete technology, polymer science, electrochemistry, rheology and computational fluid dynamics.
We will develop 4 new experimental test set-ups allowing to study active rheology control during different phases of the casting process: 1)concrete pumping (control of slip layer), 2)while flowing in the formwork (bulk control of rheology), 3)while flowing through formwork joints (control of formwork tightness), and 4)once the concrete is in its final position (trigger stiffening). Well-designed polymers with the desired response to the applied activation will be added to the concrete during mixing. The experiments will be analysed by advanced computational flow modelling based on fundamental rheological laws. Special attention will be paid to the compatibility of all responsive polymers selected for the different control phases. SmartCast will mean a paradigm shift for formwork-based concrete casting. The developed active rheology control will provide a fundamental basis for the development of future-proof 3D printing techniques in concrete industry
Summary
Concrete production processes do not take full advantage of the rheological potential of fresh cementitious materials, and are still largely labour-driven and sensitive to the human factor. SmartCast proposes a new concrete casting concept to transform the concrete industry into a highly automated technological industry. Currently, the rheological properties of the concrete are defined by mix design and mixing procedure without any further active adjustment during casting. The goal of this proposal is the active control of concrete rheology during casting, and the active triggering of early stiffening of the concrete as soon as it is put in place. The ground-breaking idea to achieve this goal, is to develop concrete with actively controllable rheology by adding admixtures responsive to externally activated electromagnetic frequencies. Inter-disciplinary insights are important to achieve these goals, including inputs from concrete technology, polymer science, electrochemistry, rheology and computational fluid dynamics.
We will develop 4 new experimental test set-ups allowing to study active rheology control during different phases of the casting process: 1)concrete pumping (control of slip layer), 2)while flowing in the formwork (bulk control of rheology), 3)while flowing through formwork joints (control of formwork tightness), and 4)once the concrete is in its final position (trigger stiffening). Well-designed polymers with the desired response to the applied activation will be added to the concrete during mixing. The experiments will be analysed by advanced computational flow modelling based on fundamental rheological laws. Special attention will be paid to the compatibility of all responsive polymers selected for the different control phases. SmartCast will mean a paradigm shift for formwork-based concrete casting. The developed active rheology control will provide a fundamental basis for the development of future-proof 3D printing techniques in concrete industry
Max ERC Funding
2 498 750 €
Duration
Start date: 2016-10-01, End date: 2021-09-30
Project acronym SOLCRIMET
Project Solvometallurgy for critical metals
Researcher (PI) Koen Binnemans
Host Institution (HI) KATHOLIEKE UNIVERSITEIT LEUVEN
Call Details Advanced Grant (AdG), PE8, ERC-2015-AdG
Summary The recent “rare-earth crisis” has brought about the widespread realisation that the long-term availability and cost stability of many materials – not just the rare earths – can no longer be guaranteed. Increasing the levels of critical metal recycling from pre-consumer, manufacturing waste and complex, multicomponent end-of-life consumer products is considered as arguably the most important and realistic mitigation strategy. However, extracting a critical metal from complex waste is a very different challenge to that faced when attempting to produce a pure metal from a primary ore deposit. SOLCRIMET therefore develops a ground-breaking, novel approach called “solvometallurgy”, a new branch within metallurgy, next to conventional hydro- and pyrometallurgy. SOLCRIMET’s aim is to successfully apply this approach to the extraction of specific critical metals, i.e. rare earths, tantalum, niobium, cobalt, indium, gallium, germanium and antimony. As these critical metals are essential components for clean-tech and high-tech applications, they are key enablers of the required transition to a low-carbon, circular economy. The approach involves the discovery of non-aqueous solvent pairs that are immiscible and allow the extraction of metal complexes at moderate temperatures, leading to high-purity recycled metals. The idea is certainly high risk, but the preliminary results already obtained are highly encouraging. The main outcomes of the project will be lab-scale demonstrators that show the enhanced efficiency, utility and applicability of the new solvometallurgical process, with respect to conventional hydro- and pyrometallurgy. SOLCRIMET’s impact on chemistry, chemical technology, metallurgy and materials engineering science will be game-changing. The possibility to recycle critical metals with energy-efficient, low-cost processes could have a significant impact on the global recycling rates of these metals.
Summary
The recent “rare-earth crisis” has brought about the widespread realisation that the long-term availability and cost stability of many materials – not just the rare earths – can no longer be guaranteed. Increasing the levels of critical metal recycling from pre-consumer, manufacturing waste and complex, multicomponent end-of-life consumer products is considered as arguably the most important and realistic mitigation strategy. However, extracting a critical metal from complex waste is a very different challenge to that faced when attempting to produce a pure metal from a primary ore deposit. SOLCRIMET therefore develops a ground-breaking, novel approach called “solvometallurgy”, a new branch within metallurgy, next to conventional hydro- and pyrometallurgy. SOLCRIMET’s aim is to successfully apply this approach to the extraction of specific critical metals, i.e. rare earths, tantalum, niobium, cobalt, indium, gallium, germanium and antimony. As these critical metals are essential components for clean-tech and high-tech applications, they are key enablers of the required transition to a low-carbon, circular economy. The approach involves the discovery of non-aqueous solvent pairs that are immiscible and allow the extraction of metal complexes at moderate temperatures, leading to high-purity recycled metals. The idea is certainly high risk, but the preliminary results already obtained are highly encouraging. The main outcomes of the project will be lab-scale demonstrators that show the enhanced efficiency, utility and applicability of the new solvometallurgical process, with respect to conventional hydro- and pyrometallurgy. SOLCRIMET’s impact on chemistry, chemical technology, metallurgy and materials engineering science will be game-changing. The possibility to recycle critical metals with energy-efficient, low-cost processes could have a significant impact on the global recycling rates of these metals.
Max ERC Funding
2 496 250 €
Duration
Start date: 2016-09-01, End date: 2021-08-31
Project acronym SpecMAT
Project Spectroscopy of exotic nuclei in a Magnetic Active Target
Researcher (PI) Riccardo Raabe
Host Institution (HI) KATHOLIEKE UNIVERSITEIT LEUVEN
Call Details Consolidator Grant (CoG), PE2, ERC-2013-CoG
Summary SpecMAT aims at providing crucial experimental information to answer key questions about the structure of atomic nuclei:
- What are the forces driving the shell structure in nuclei and how do they change in nuclei far from stability?
- What remains of the Z = 28 and N = 50 “magic numbers” in 78Ni?
- Do we understand shape coexistence in nuclei, and what are the mechanisms controlling its appearance?
The position of natural and “intruder” shells will be mapped in two critical regions, the neutron-rich nuclei around Z = 28 and the neutron-deficient nuclei around Z = 82. The centroids of the shell strength are derived from the complete spectroscopy of those systems in nucleon-transfer measurements. This method will be applied for the first time in the region of neutron-deficient Pb nuclei.
In SpecMAT (Spectroscopy of exotic nuclei in a Magnetic Active Target) a novel instrument will overcome the present challenges in performing such measurements with very weak beams of unstable nuclei. It combines high luminosity, high efficiency and a very large dynamic range and allows detection of both charged-particle and gamma-ray radiation. The instrument owns its remarkable performances to a number of advanced technologies concerning the use of electronics, gaseous detectors and gamma-ray detectors in a magnetic field.
The SpecMAT detector will be coupled to the HIE-ISOLDE facility for the production and post-acceleration of radioactive ion beams in construction at CERN in Geneva. HIE-ISOLDE will provide world-unique beams thanks to the use of the proton injector of the CERN complex.
If successful, SpecMAT at HIE-ISOLDE will produce specific results in nuclear structure which cannot be reached by other programmes elsewhere. Such results will have a significant impact on the present theories and models of the atomic nucleus.
Summary
SpecMAT aims at providing crucial experimental information to answer key questions about the structure of atomic nuclei:
- What are the forces driving the shell structure in nuclei and how do they change in nuclei far from stability?
- What remains of the Z = 28 and N = 50 “magic numbers” in 78Ni?
- Do we understand shape coexistence in nuclei, and what are the mechanisms controlling its appearance?
The position of natural and “intruder” shells will be mapped in two critical regions, the neutron-rich nuclei around Z = 28 and the neutron-deficient nuclei around Z = 82. The centroids of the shell strength are derived from the complete spectroscopy of those systems in nucleon-transfer measurements. This method will be applied for the first time in the region of neutron-deficient Pb nuclei.
In SpecMAT (Spectroscopy of exotic nuclei in a Magnetic Active Target) a novel instrument will overcome the present challenges in performing such measurements with very weak beams of unstable nuclei. It combines high luminosity, high efficiency and a very large dynamic range and allows detection of both charged-particle and gamma-ray radiation. The instrument owns its remarkable performances to a number of advanced technologies concerning the use of electronics, gaseous detectors and gamma-ray detectors in a magnetic field.
The SpecMAT detector will be coupled to the HIE-ISOLDE facility for the production and post-acceleration of radioactive ion beams in construction at CERN in Geneva. HIE-ISOLDE will provide world-unique beams thanks to the use of the proton injector of the CERN complex.
If successful, SpecMAT at HIE-ISOLDE will produce specific results in nuclear structure which cannot be reached by other programmes elsewhere. Such results will have a significant impact on the present theories and models of the atomic nucleus.
Max ERC Funding
1 944 900 €
Duration
Start date: 2014-06-01, End date: 2019-05-31