Project acronym APOLLO
Project Advanced Signal Processing Technologies for Wireless Powered Communications
Researcher (PI) Ioannis Krikidis
Host Institution (HI) UNIVERSITY OF CYPRUS
Country Cyprus
Call Details Consolidator Grant (CoG), PE7, ERC-2018-COG
Summary Wireless power transfer (WPT), pioneered by Tesla, is an idea at least as old as radio communications. However, on the one hand, due to health concerns and the large antenna dimensions required for transmission of high energy levels, until recently WPT has been limited mostly to very short distance applications. On the other hand, recent advances in silicon technology have significantly reduced the energy needs of electronic systems, making WPT over radio waves a potential source of energy for low power devices. Although WPT through radio waves has already found various short-range applications (such as the radio-frequency identification technology, healthcare monitoring etc.), its integration as a building block in the operation of wireless communications systems is still unexploited. On the other hand, conventional radio wave based information and energy transmissions have largely been designed separately. However, many applications can benefit from simultaneous wireless information and power transfer (SWIPT).
The overall objective of the APOLLO project is to study the integration of WPT/SWIPT technology into future wireless communication systems. Compared to past and current research efforts in this area, our technical approach is deeply interdisciplinary and more comprehensive, combining the expertise of wireless communications, control theory, information theory, optimization, and electronics/microwave engineering.
The key outcomes of the project include: 1) a rigorous and complete mathematical theory for WPT/SWIPT via information/communication/control theoretic studies; 2) new physical and cross-layer mechanisms that will enable the integration of WPT/SWIPT into future communication systems; 3) new network architectures that will fully exploit potential benefits of WPT/SWIPT; and 4) development of a proof-of-concept by implementing highly-efficient and multi-band metamaterial energy harvesting sensors for SWIPT.
Summary
Wireless power transfer (WPT), pioneered by Tesla, is an idea at least as old as radio communications. However, on the one hand, due to health concerns and the large antenna dimensions required for transmission of high energy levels, until recently WPT has been limited mostly to very short distance applications. On the other hand, recent advances in silicon technology have significantly reduced the energy needs of electronic systems, making WPT over radio waves a potential source of energy for low power devices. Although WPT through radio waves has already found various short-range applications (such as the radio-frequency identification technology, healthcare monitoring etc.), its integration as a building block in the operation of wireless communications systems is still unexploited. On the other hand, conventional radio wave based information and energy transmissions have largely been designed separately. However, many applications can benefit from simultaneous wireless information and power transfer (SWIPT).
The overall objective of the APOLLO project is to study the integration of WPT/SWIPT technology into future wireless communication systems. Compared to past and current research efforts in this area, our technical approach is deeply interdisciplinary and more comprehensive, combining the expertise of wireless communications, control theory, information theory, optimization, and electronics/microwave engineering.
The key outcomes of the project include: 1) a rigorous and complete mathematical theory for WPT/SWIPT via information/communication/control theoretic studies; 2) new physical and cross-layer mechanisms that will enable the integration of WPT/SWIPT into future communication systems; 3) new network architectures that will fully exploit potential benefits of WPT/SWIPT; and 4) development of a proof-of-concept by implementing highly-efficient and multi-band metamaterial energy harvesting sensors for SWIPT.
Max ERC Funding
1 930 625 €
Duration
Start date: 2019-07-01, End date: 2025-03-31
Project acronym ECHO
Project Extending Coherence for Hardware-Driven Optimizations in Multicore Architectures
Researcher (PI) Alberto ROS BARDISA
Host Institution (HI) UNIVERSIDAD DE MURCIA
Country Spain
Call Details Consolidator Grant (CoG), PE6, ERC-2018-COG
Summary Multicore processors are present nowadays in most digital devices, from smartphones to high-performance
servers. The increasing computational power of these processors is essential for enabling many important
emerging application domains such as big-data, media, medical, or scientific modeling. A fundamental
technique to improve performance is speculation, a technique that consists in executing work before it is
known if it is actually needed. In hardware, speculation significantly increases energy consumption by
performing unnecessary operations, while speculation in software (e.g., compilers) is not the default thus
preventing performance optimizations. Since performance in current multicores is limited by their power
budget, it is imperative to make multicores as energy-efficient as possible to increase performance even
further.
In a multicore architecture, the cache coherence protocol is an essential component since its unique but
challenging role is to offer a simple and unified view of the memory hierarchy. This project envisions that
extending the role of the coherence protocol to simplify other system components will be the key to
overcome the performance and energy limitations of current multicores. In particular, ECHO proposes to
add simple but effective extensions to the cache coherence protocol in order to (i) reduce and even
eliminate misspeculations at the processing cores and synchronization mechanisms and to (ii) enable
speculative optimizations at compile time. The goal of this innovative approach is to improve the
performance and energy efficiency of future multicore architectures. To accomplish the objectives
proposed in this project, I will build on my 14 years expertise in cache coherence, documented in over 40
publications of high impact.
Summary
Multicore processors are present nowadays in most digital devices, from smartphones to high-performance
servers. The increasing computational power of these processors is essential for enabling many important
emerging application domains such as big-data, media, medical, or scientific modeling. A fundamental
technique to improve performance is speculation, a technique that consists in executing work before it is
known if it is actually needed. In hardware, speculation significantly increases energy consumption by
performing unnecessary operations, while speculation in software (e.g., compilers) is not the default thus
preventing performance optimizations. Since performance in current multicores is limited by their power
budget, it is imperative to make multicores as energy-efficient as possible to increase performance even
further.
In a multicore architecture, the cache coherence protocol is an essential component since its unique but
challenging role is to offer a simple and unified view of the memory hierarchy. This project envisions that
extending the role of the coherence protocol to simplify other system components will be the key to
overcome the performance and energy limitations of current multicores. In particular, ECHO proposes to
add simple but effective extensions to the cache coherence protocol in order to (i) reduce and even
eliminate misspeculations at the processing cores and synchronization mechanisms and to (ii) enable
speculative optimizations at compile time. The goal of this innovative approach is to improve the
performance and energy efficiency of future multicore architectures. To accomplish the objectives
proposed in this project, I will build on my 14 years expertise in cache coherence, documented in over 40
publications of high impact.
Max ERC Funding
1 999 955 €
Duration
Start date: 2019-09-01, End date: 2024-08-31
Project acronym ENFORCE
Project ENgineering FrustratiOn in aRtificial Colloidal icEs:degeneracy, exotic lattices and 3D states
Researcher (PI) pietro TIERNO
Host Institution (HI) UNIVERSITAT DE BARCELONA
Country Spain
Call Details Consolidator Grant (CoG), PE3, ERC-2018-COG
Summary Geometric frustration, namely the impossibility of satisfying competing interactions on a lattice, has recently
become a topic of considerable interest as it engenders emergent, fundamentally new phenomena and holds
the exciting promise of delivering a new class of nanoscale devices based on the motion of magnetic charges.
With ENFORCE, I propose to realize two and three dimensional artificial colloidal ices and investigate the
fascinating manybody physics of geometric frustration in these mesoscopic structures. I will use these soft
matter systems to engineer novel frustrated states through independent control of the single particle
positions, lattice topology and collective magnetic coupling. The three project work packages (WPs) will
present increasing levels of complexity, challenge and ambition:
(i) In WP1, I will demonstrate a way to restore the residual entropy in the square ice, a fundamental longstanding
problem in the field. Furthermore, I will miniaturize the square and the honeycomb geometries and investigate the dynamics of thermally excited topological defects and the formation of grain boundaries.
(ii) In WP2, I will decimate both lattices and realize mixed coordination geometries, where the similarity
between the colloidal and spin ice systems breaks down. I will then develop a novel annealing protocol based
on the simultaneous system visualization and magnetic actuation control.
(iii) In WP3, I will realize a three dimensional artificial colloidal ice, in which interacting ferromagnetic
inclusions will be located in the voids of an inverse opal, and arranged to form the FCC or the pyrochlore
lattices. External fields will be used to align, bias and stir these magnetic inclusions while monitoring in situ
their orientation and dynamics via laser scanning confocal microscopy.
ENFORCE will exploit the accessible time and length scales of the colloidal ice to shed new light on the
exciting and interdisciplinary field of geometric frustration.
Summary
Geometric frustration, namely the impossibility of satisfying competing interactions on a lattice, has recently
become a topic of considerable interest as it engenders emergent, fundamentally new phenomena and holds
the exciting promise of delivering a new class of nanoscale devices based on the motion of magnetic charges.
With ENFORCE, I propose to realize two and three dimensional artificial colloidal ices and investigate the
fascinating manybody physics of geometric frustration in these mesoscopic structures. I will use these soft
matter systems to engineer novel frustrated states through independent control of the single particle
positions, lattice topology and collective magnetic coupling. The three project work packages (WPs) will
present increasing levels of complexity, challenge and ambition:
(i) In WP1, I will demonstrate a way to restore the residual entropy in the square ice, a fundamental longstanding
problem in the field. Furthermore, I will miniaturize the square and the honeycomb geometries and investigate the dynamics of thermally excited topological defects and the formation of grain boundaries.
(ii) In WP2, I will decimate both lattices and realize mixed coordination geometries, where the similarity
between the colloidal and spin ice systems breaks down. I will then develop a novel annealing protocol based
on the simultaneous system visualization and magnetic actuation control.
(iii) In WP3, I will realize a three dimensional artificial colloidal ice, in which interacting ferromagnetic
inclusions will be located in the voids of an inverse opal, and arranged to form the FCC or the pyrochlore
lattices. External fields will be used to align, bias and stir these magnetic inclusions while monitoring in situ
their orientation and dynamics via laser scanning confocal microscopy.
ENFORCE will exploit the accessible time and length scales of the colloidal ice to shed new light on the
exciting and interdisciplinary field of geometric frustration.
Max ERC Funding
1 850 298 €
Duration
Start date: 2020-01-01, End date: 2024-12-31
Project acronym FeMiT
Project Ferrites-by-design for Millimeter-wave and Terahertz Technologies
Researcher (PI) MartI GICH
Host Institution (HI) AGENCIA ESTATAL CONSEJO SUPERIOR DEINVESTIGACIONES CIENTIFICAS
Country Spain
Call Details Consolidator Grant (CoG), PE8, ERC-2018-COG
Summary Robust disruptive materials will be essential for the “wireless everywhere” to become a reality. This is because we need a paradigm shift in mobile communications to meet the challenges of such an ambitious evolution. In particular, some of these emerging technologies will trigger the replacement of the magnetic microwave ferrites in use today. This will namely occur with the forecasted shift to high frequency mm-wave and THz bands and in novel antennas that can simultaneously transmit and receive data on the same frequency. In both cases, operating with state-of-the-art ferrites would require large external magnetic fields incompatible with future needs of smaller, power-efficient devices.
To overcome these issues, we target ferrites featuring the so far unmet combinations of low magnetic loss and large values of magnetocrystalline anisotropy, magnetostriction or magnetoelectric coupling.
The objective of FeMiT is developing a novel family of orthorhombic ferrites based on ε-Fe2O3, a room-temperature multiferroic with large magnetocrystalline anisotropy. Those properties and unique structural features make it an excellent platform to develop the sought-after functional materials for future compact and energy-efficient wireless devices.
In the first part of FeMiT we will explore the limits and diversity of this new family by exploiting rational chemical substitutions, high pressures and strain engineering. Soft chemistry and physical deposition methods will be both considered at this stage.
The second part of FeMiT entails a characterization of functional properties and selection of the best candidates to be integrated in composite and epitaxial films suitable for application. The expected outcomes will provide proof-of-concept self-biased or voltage-controlled signal-processing devices with low losses in the mm-wave to THz bands, with high potential impact in the development of future wireless technologies.
Summary
Robust disruptive materials will be essential for the “wireless everywhere” to become a reality. This is because we need a paradigm shift in mobile communications to meet the challenges of such an ambitious evolution. In particular, some of these emerging technologies will trigger the replacement of the magnetic microwave ferrites in use today. This will namely occur with the forecasted shift to high frequency mm-wave and THz bands and in novel antennas that can simultaneously transmit and receive data on the same frequency. In both cases, operating with state-of-the-art ferrites would require large external magnetic fields incompatible with future needs of smaller, power-efficient devices.
To overcome these issues, we target ferrites featuring the so far unmet combinations of low magnetic loss and large values of magnetocrystalline anisotropy, magnetostriction or magnetoelectric coupling.
The objective of FeMiT is developing a novel family of orthorhombic ferrites based on ε-Fe2O3, a room-temperature multiferroic with large magnetocrystalline anisotropy. Those properties and unique structural features make it an excellent platform to develop the sought-after functional materials for future compact and energy-efficient wireless devices.
In the first part of FeMiT we will explore the limits and diversity of this new family by exploiting rational chemical substitutions, high pressures and strain engineering. Soft chemistry and physical deposition methods will be both considered at this stage.
The second part of FeMiT entails a characterization of functional properties and selection of the best candidates to be integrated in composite and epitaxial films suitable for application. The expected outcomes will provide proof-of-concept self-biased or voltage-controlled signal-processing devices with low losses in the mm-wave to THz bands, with high potential impact in the development of future wireless technologies.
Max ERC Funding
1 989 967 €
Duration
Start date: 2019-05-01, End date: 2024-04-30
Project acronym LArcHer
Project Breaking barriers between Science and Heritage approaches to Levantine Rock Art through Archaeology, Heritage Science and IT
Researcher (PI) Ines DOMINGO SANZ
Host Institution (HI) UNIVERSITAT DE BARCELONA
Country Spain
Call Details Consolidator Grant (CoG), SH6, ERC-2018-COG
Summary LArcHer project aims at pioneering a new and more comprehensive way of understanding one of Europe’s most extraordinary bodies of prehistoric art, awarded Unesco World Heritage status in 1998: Levantine rock art (LRA). The ground-breaking nature of the project relies on combining a multidisciplinary (Archaeology, Heritage Science and IT) and multiscale approach (from microanalysis to landscape perspectives) to gain a holistic view of this art. It also aims at closing existing gaps between science and heritage mainstreams, to better understand the values and threats affecting this tradition and bring about a change in the way we understand, care, use and manage this millenary legacy. LArcHer aims are: a) Use cross-disciplinary knowledge and methods to redefine LRA (i.e. new dating techniques to refine chronology, new analytical methods to understand the creative process); b) Use LRA as a proxy to raise new questions of global interest on the evolution of creative thinking and human cognition (i.e. the timing and driving forces behind the birth of anthropocentrism and visual narratives in the history of prehistoric art); c) Develop new research agendas to set off complementary goals between science and heritage and define best practices for open air rock art conservation and management.
Spread across Mediterranean Iberia, LRA is the only European body of figurative art dominated by humans engaged in dynamic narratives of hunting, violence, warfare, dances and so forth. These scenes are unique to explore past social dynamics, human behaviour and cultural practices. As such, it is the only body of European rock art with potential to answer some of the new questions raised by LArcHer.
Key to LArcHer are the systematic recording and analysis of the art through 3D Digital technologies, management and data storage systems, GIS, physicochemical analysis of pigments and bedrock and comparative analysis with other major bodies of art with equivalent developments.
Summary
LArcHer project aims at pioneering a new and more comprehensive way of understanding one of Europe’s most extraordinary bodies of prehistoric art, awarded Unesco World Heritage status in 1998: Levantine rock art (LRA). The ground-breaking nature of the project relies on combining a multidisciplinary (Archaeology, Heritage Science and IT) and multiscale approach (from microanalysis to landscape perspectives) to gain a holistic view of this art. It also aims at closing existing gaps between science and heritage mainstreams, to better understand the values and threats affecting this tradition and bring about a change in the way we understand, care, use and manage this millenary legacy. LArcHer aims are: a) Use cross-disciplinary knowledge and methods to redefine LRA (i.e. new dating techniques to refine chronology, new analytical methods to understand the creative process); b) Use LRA as a proxy to raise new questions of global interest on the evolution of creative thinking and human cognition (i.e. the timing and driving forces behind the birth of anthropocentrism and visual narratives in the history of prehistoric art); c) Develop new research agendas to set off complementary goals between science and heritage and define best practices for open air rock art conservation and management.
Spread across Mediterranean Iberia, LRA is the only European body of figurative art dominated by humans engaged in dynamic narratives of hunting, violence, warfare, dances and so forth. These scenes are unique to explore past social dynamics, human behaviour and cultural practices. As such, it is the only body of European rock art with potential to answer some of the new questions raised by LArcHer.
Key to LArcHer are the systematic recording and analysis of the art through 3D Digital technologies, management and data storage systems, GIS, physicochemical analysis of pigments and bedrock and comparative analysis with other major bodies of art with equivalent developments.
Max ERC Funding
1 991 178 €
Duration
Start date: 2019-10-01, End date: 2024-09-30
Project acronym MAGNESIA
Project The impact of highly magnetic neutron stars in the explosive and transient Universe
Researcher (PI) Nanda Rea
Host Institution (HI) AGENCIA ESTATAL CONSEJO SUPERIOR DEINVESTIGACIONES CIENTIFICAS
Country Spain
Call Details Consolidator Grant (CoG), PE9, ERC-2018-COG
Summary The gravitational wave window is now open. It is then imperative to build quantitative models of neutron stars that use all the available tracers to constrain fundamental physics at the highest densities and magnetic fields. The most magnetic neutron stars, the magnetars, have been recently suggested to be powering a large variety of explosive and transient events. The enormous rotational power at birth, and the magnetic energy they can release via large flares, put the magnetars in the (yet) hand-wavy interpretations of gamma-ray bursts, the early phases of double neutron star mergers, super-luminous supernovae, hypernovae, fast radio bursts, and ultra-luminous X-ray sources. However, despite knowing about 30 magnetars, we are lacking a census of how many we expect within the pulsar population, nor we have robust constraints on their flaring rates. The recent discovery of transient magnetars, of magnetar-like flares from sources with measured low dipolar magnetic fields and from typical radio pulsars, clearly showed that the magnetar census in our Galaxy is largely under-estimated. This hampers our understanding not only of the pulsar and magnetar populations, but also of them as possibly related to many of Universe’s explosive events. MAGNESIA will infer a sound Magnetar Census via an innovative approach that will build the first Pulsar Population Synthesis model able to cope with constraints/limits from multi-band observations, and taking into account 3D magnetic field evolution models and flaring rates for neutron stars. Combining expertise in multi-band observations, numerical modeling, nuclear physics, and computation, MAGNESIA will solve the physics, the observational systematic errors, and the computational challenges that inhibited previous works, to finally constrain the spin period and magnetic field distribution at birth of the neutron star population.
Summary
The gravitational wave window is now open. It is then imperative to build quantitative models of neutron stars that use all the available tracers to constrain fundamental physics at the highest densities and magnetic fields. The most magnetic neutron stars, the magnetars, have been recently suggested to be powering a large variety of explosive and transient events. The enormous rotational power at birth, and the magnetic energy they can release via large flares, put the magnetars in the (yet) hand-wavy interpretations of gamma-ray bursts, the early phases of double neutron star mergers, super-luminous supernovae, hypernovae, fast radio bursts, and ultra-luminous X-ray sources. However, despite knowing about 30 magnetars, we are lacking a census of how many we expect within the pulsar population, nor we have robust constraints on their flaring rates. The recent discovery of transient magnetars, of magnetar-like flares from sources with measured low dipolar magnetic fields and from typical radio pulsars, clearly showed that the magnetar census in our Galaxy is largely under-estimated. This hampers our understanding not only of the pulsar and magnetar populations, but also of them as possibly related to many of Universe’s explosive events. MAGNESIA will infer a sound Magnetar Census via an innovative approach that will build the first Pulsar Population Synthesis model able to cope with constraints/limits from multi-band observations, and taking into account 3D magnetic field evolution models and flaring rates for neutron stars. Combining expertise in multi-band observations, numerical modeling, nuclear physics, and computation, MAGNESIA will solve the physics, the observational systematic errors, and the computational challenges that inhibited previous works, to finally constrain the spin period and magnetic field distribution at birth of the neutron star population.
Max ERC Funding
2 263 148 €
Duration
Start date: 2019-06-01, End date: 2024-05-31
Project acronym MarsFirstWater
Project The physicochemical nature of water on early Mars
Researcher (PI) Alberto Gonzalez Fairen
Host Institution (HI) AGENCIA ESTATAL CONSEJO SUPERIOR DEINVESTIGACIONES CIENTIFICAS
Country Spain
Call Details Consolidator Grant (CoG), PE9, ERC-2018-COG
Summary Concepts of large bodies of glacial ice and liquid standing water, a robust hydrological cycle, and a rich Martian history of climate change are part of the current consensus model for early Mars. However, questions still poorly constrained include: a precise understanding of the inventory of water during the first billion years of Mars history and its early evolution on both global and local scales; whether liquid or solid H2O dominated, for what duration of time and where the water resided; what were the host-rock weathering rates and patterns and the physicochemical parameters defining such interactions; what specific landforms and mineralogies were generated during those periods; and what implications all these processes had on the possible inception of life on Mars. These fundamental questions represent large uncertainties and knowledge gaps. Therefore, a quantitative understanding of the basic characteristics of water on early Mars is very much needed and is the focus of this proposal.
This application outlines a plan for my research in the next five years, and explains how I propose to fully characterize the aqueous environments of early Mars through a quantitative and truly interdisciplinary investigation. Spacecraft mission-derived datasets will be consistently used to test hypotheses through paleogeomorphological reconstructions, geochemical modeling, mineralogical studies, and astrobiological investigations. The derived results will produce hard constraints on the physical evolution, chemical alteration and habitability of surface and near-surface aqueous environments on early Mars. The planned investigations will benefit from the combination of working with first-hand data from ongoing Mars missions and with the state-of-the-art laboratory tools at the host institution. The final expected result will be a complete understanding of the physicochemical nature of water on early Mars, also opening new paths for the astrobiological exploration of the planet.
Summary
Concepts of large bodies of glacial ice and liquid standing water, a robust hydrological cycle, and a rich Martian history of climate change are part of the current consensus model for early Mars. However, questions still poorly constrained include: a precise understanding of the inventory of water during the first billion years of Mars history and its early evolution on both global and local scales; whether liquid or solid H2O dominated, for what duration of time and where the water resided; what were the host-rock weathering rates and patterns and the physicochemical parameters defining such interactions; what specific landforms and mineralogies were generated during those periods; and what implications all these processes had on the possible inception of life on Mars. These fundamental questions represent large uncertainties and knowledge gaps. Therefore, a quantitative understanding of the basic characteristics of water on early Mars is very much needed and is the focus of this proposal.
This application outlines a plan for my research in the next five years, and explains how I propose to fully characterize the aqueous environments of early Mars through a quantitative and truly interdisciplinary investigation. Spacecraft mission-derived datasets will be consistently used to test hypotheses through paleogeomorphological reconstructions, geochemical modeling, mineralogical studies, and astrobiological investigations. The derived results will produce hard constraints on the physical evolution, chemical alteration and habitability of surface and near-surface aqueous environments on early Mars. The planned investigations will benefit from the combination of working with first-hand data from ongoing Mars missions and with the state-of-the-art laboratory tools at the host institution. The final expected result will be a complete understanding of the physicochemical nature of water on early Mars, also opening new paths for the astrobiological exploration of the planet.
Max ERC Funding
1 998 368 €
Duration
Start date: 2019-06-01, End date: 2024-05-31
Project acronym MOF-reactors
Project Metal-Organic Frameworks as Chemical Reactors for the Synthesis of Well-Defined Sub-Nanometer Metal Clusters
Researcher (PI) Emilio PARDO
Host Institution (HI) UNIVERSITAT DE VALENCIA
Country Spain
Call Details Consolidator Grant (CoG), PE5, ERC-2018-COG
Summary Humankind advancement is connected to the use and development of metal forms. Recent works have unveiled exceptional properties –such as luminescence, biocompatibility, antitumoral activity or a superlative catalytic activity– for small aggregations of metal atoms, so–called sub–nanometer metal clusters (SNMCs). Despite this importance, the gram-scale synthesis of structurally and electronically well–defined SNMCs is still far from being a reality.
The present proposal situates at the centre of such weakness and aims at making a breakthrough step-change on the use of metal-organic frameworks (MOFs) as chemical reactors for the in–situ synthesis of stable ligand-free SNMCs with such unique properties. This challenging synthetic strategy, which is assisted by striking published and inedited preliminary results, has solid foundations. Firstly, the design and large-scale preparation of cheap and novel families of highly robust and crystalline MOFs with tailor-made functional channels to be used as chemical reactors. Secondly, the application of solid-state post-synthetic methods to drive the multigram-scale preparation of unique ligand-free homo- and heterometallic SNMCs, which are, in the best-case scenario, very difficult to be obtained and stabilised outside the channels. Last but not least, single-crystal X-Ray diffraction will be used as the definitive tool for the characterisation, at the atomic level, of such ultrasmall species offering unprecedented snapshots about their real structures and formation mechanisms.
The ultimate goal will be upscaling this synthetic strategy aiming at the large-scale fabrication of SNMCs and their industrial application will be then evaluated. A successful achievement of all the aforementioned objectives of this ground-breaking project would open new routes for the use of MOFs as chemical reactors to manufacture, at competitive prices, MOF-driven, structurally and electronically well–defined, ligand–free SNMCs in a multigram-scale.
Summary
Humankind advancement is connected to the use and development of metal forms. Recent works have unveiled exceptional properties –such as luminescence, biocompatibility, antitumoral activity or a superlative catalytic activity– for small aggregations of metal atoms, so–called sub–nanometer metal clusters (SNMCs). Despite this importance, the gram-scale synthesis of structurally and electronically well–defined SNMCs is still far from being a reality.
The present proposal situates at the centre of such weakness and aims at making a breakthrough step-change on the use of metal-organic frameworks (MOFs) as chemical reactors for the in–situ synthesis of stable ligand-free SNMCs with such unique properties. This challenging synthetic strategy, which is assisted by striking published and inedited preliminary results, has solid foundations. Firstly, the design and large-scale preparation of cheap and novel families of highly robust and crystalline MOFs with tailor-made functional channels to be used as chemical reactors. Secondly, the application of solid-state post-synthetic methods to drive the multigram-scale preparation of unique ligand-free homo- and heterometallic SNMCs, which are, in the best-case scenario, very difficult to be obtained and stabilised outside the channels. Last but not least, single-crystal X-Ray diffraction will be used as the definitive tool for the characterisation, at the atomic level, of such ultrasmall species offering unprecedented snapshots about their real structures and formation mechanisms.
The ultimate goal will be upscaling this synthetic strategy aiming at the large-scale fabrication of SNMCs and their industrial application will be then evaluated. A successful achievement of all the aforementioned objectives of this ground-breaking project would open new routes for the use of MOFs as chemical reactors to manufacture, at competitive prices, MOF-driven, structurally and electronically well–defined, ligand–free SNMCs in a multigram-scale.
Max ERC Funding
1 886 000 €
Duration
Start date: 2019-03-01, End date: 2024-02-29
Project acronym ReadCalibration
Project Phonemic representations in speech perception and production: Recalibration by readingacquisition
Researcher (PI) Clara, Dominique, Sylvie Martin
Host Institution (HI) BCBL BASQUE CENTER ON COGNITION BRAIN AND LANGUAGE
Country Spain
Call Details Consolidator Grant (CoG), SH4, ERC-2018-COG
Summary The main goal of this project is to demonstrate that reading acquisition (RA) drastically reshapes our phonemic inventory, and to investigate the time-course and fine-grained properties of this recalibration. The main innovative and ground-breaking aspect of this project is the merging of two research fields, (1) reading acquisition and (2) phonemic recalibration, together with a deep and extensive exploration of the (3) perception-production link, which results in a new research line that pushes the boundaries of our understanding of the complex interactions between auditory and visual language perception and production.
We will demonstrate that phonemic representations (PRs) become more stable (less dispersed) during the process of learning to read, and that this recalibration varies according to the grapheme-phoneme conversion rules of the reading system. We will explore such recalibration by means of the first cross-linguistic longitudinal study examining the position and dispersion of PRs, both in perception and production of phonemes and words. Secondly, we will explore how recalibration develops when RA is impaired as is the case in dyslexic children –informing the research field on (4) dyslexia– and when pre-reading PRs are unstable as is the case in deaf children with cochlear implants –informing the research field on (5) deafness. Finally, the research will also be extended to PR recalibration during RA in a second language –informing the research on (6) bilingualism.
This proposal provides the first systematic investigation of phonemic recalibration during literacy acquisition, and will provide important insight for pragmatic research and theoretical accounts of language perception and production and phonemic recalibration. This project will also have major implications for the clinical field (theories and remediation of dyslexia and deafness) and for social policies and education (bilingualism, spoken and written language teaching).
Summary
The main goal of this project is to demonstrate that reading acquisition (RA) drastically reshapes our phonemic inventory, and to investigate the time-course and fine-grained properties of this recalibration. The main innovative and ground-breaking aspect of this project is the merging of two research fields, (1) reading acquisition and (2) phonemic recalibration, together with a deep and extensive exploration of the (3) perception-production link, which results in a new research line that pushes the boundaries of our understanding of the complex interactions between auditory and visual language perception and production.
We will demonstrate that phonemic representations (PRs) become more stable (less dispersed) during the process of learning to read, and that this recalibration varies according to the grapheme-phoneme conversion rules of the reading system. We will explore such recalibration by means of the first cross-linguistic longitudinal study examining the position and dispersion of PRs, both in perception and production of phonemes and words. Secondly, we will explore how recalibration develops when RA is impaired as is the case in dyslexic children –informing the research field on (4) dyslexia– and when pre-reading PRs are unstable as is the case in deaf children with cochlear implants –informing the research field on (5) deafness. Finally, the research will also be extended to PR recalibration during RA in a second language –informing the research on (6) bilingualism.
This proposal provides the first systematic investigation of phonemic recalibration during literacy acquisition, and will provide important insight for pragmatic research and theoretical accounts of language perception and production and phonemic recalibration. This project will also have major implications for the clinical field (theories and remediation of dyslexia and deafness) and for social policies and education (bilingualism, spoken and written language teaching).
Max ERC Funding
1 875 000 €
Duration
Start date: 2019-10-01, End date: 2024-09-30
Project acronym SUBSILIENCE
Project Subsistence and human resilience to sudden climatic events in Europe during MIS3
Researcher (PI) ANA B. MARIN-ARROYO
Host Institution (HI) UNIVERSIDAD DE CANTABRIA
Country Spain
Call Details Consolidator Grant (CoG), SH6, ERC-2018-COG
Summary Climate has long been proposed as a possible trigger-factor for the extinction of Neanderthals and the rapid colonization of Europe by Anatomically Modern Humans (AMH). Abrupt and acute oscillations of climate, as recorded from polar ice sheets, are particularly threatening as they can push ecosystems towards catastrophic outcomes. Under these conditions, the survival of a species critically depends on their adaptive skills. Understanding the exact role that these episodes could have had in the Middle to Upper Palaeolithic transition is then essential to unravel the real causes of Neanderthal demise and AMH success. To do this, SUBSILIENCE will identify the subsistence strategies adopted by both human species in response to those climatic changes at 20 key archaeological sites located across southern European peninsulas. By applying zooarchaeological and taphonomic analyses, the behavioural flexibility and resilience of each human species will be assessed. In addition, to enable effective testing, local terrestrial climatic and environmental conditions will be accurately reconstructed using stable isotopes from animals consumed, producing a unique, continuous and properly-dated general environmental framework, improving existing knowledge. Finally, to further explore the problem, an innovative procedure to estimate prey abundance, ecology and human behaviour, involving the estimation of the ecosystem carrying capacity, will be developed. This multidisciplinary and novel approach will provide, for the first time, accurate answers to questions concerning a) which particular subsistence patterns (if any) favoured AMH over Neanderthals while coping with the changing environment and b) the extent to which climatic oscillations affected Neanderthal extinction. In this, it will be of relevance to the study of Prehistory on a pan-European scale.
Summary
Climate has long been proposed as a possible trigger-factor for the extinction of Neanderthals and the rapid colonization of Europe by Anatomically Modern Humans (AMH). Abrupt and acute oscillations of climate, as recorded from polar ice sheets, are particularly threatening as they can push ecosystems towards catastrophic outcomes. Under these conditions, the survival of a species critically depends on their adaptive skills. Understanding the exact role that these episodes could have had in the Middle to Upper Palaeolithic transition is then essential to unravel the real causes of Neanderthal demise and AMH success. To do this, SUBSILIENCE will identify the subsistence strategies adopted by both human species in response to those climatic changes at 20 key archaeological sites located across southern European peninsulas. By applying zooarchaeological and taphonomic analyses, the behavioural flexibility and resilience of each human species will be assessed. In addition, to enable effective testing, local terrestrial climatic and environmental conditions will be accurately reconstructed using stable isotopes from animals consumed, producing a unique, continuous and properly-dated general environmental framework, improving existing knowledge. Finally, to further explore the problem, an innovative procedure to estimate prey abundance, ecology and human behaviour, involving the estimation of the ecosystem carrying capacity, will be developed. This multidisciplinary and novel approach will provide, for the first time, accurate answers to questions concerning a) which particular subsistence patterns (if any) favoured AMH over Neanderthals while coping with the changing environment and b) the extent to which climatic oscillations affected Neanderthal extinction. In this, it will be of relevance to the study of Prehistory on a pan-European scale.
Max ERC Funding
2 000 000 €
Duration
Start date: 2019-06-01, End date: 2024-05-31