Project acronym A-BINGOS
Project Accreting binary populations in Nearby Galaxies: Observations and Simulations
Researcher (PI) Andreas Zezas
Host Institution (HI) IDRYMA TECHNOLOGIAS KAI EREVNAS
Call Details Consolidator Grant (CoG), PE9, ERC-2013-CoG
Summary "High-energy observations of our Galaxy offer a good, albeit not complete, picture of the X-ray source populations, in particular the accreting binary sources. Recent ability to study accreting binaries in nearby galaxies has shown that we would be short-sighted if we restricted ourselves to our Galaxy or to a few nearby ones. I propose an ambitious project that involves a comprehensive study of all the galaxies within 10 Mpc for which we can study in detail their X-ray sources and stellar populations. The study will combine data from a unique suite of observatories (Chandra, XMM-Newton, HST, Spitzer) with state-of-the-art theoretical modelling of binary systems. I propose a novel approach that links the accreting binary populations to their parent stellar populations and surpasses any current studies of X-ray binary populations, both in scale and in scope, by: (a) combining methods and results from several different areas of astrophysics (compact objects, binary systems, stellar populations, galaxy evolution); (b) using data from almost the whole electromagnetic spectrum (infrared to X-ray bands); (c) identifying and studying the different sub-populations of accreting binaries; and (d) performing direct comparison between observations and theoretical predictions, over a broad parameter space. The project: (a) will answer the long-standing question of the formation efficiency of accreting binaries in different environments; and (b) will constrain their evolutionary paths. As by-products the project will provide eagerly awaited input to the fields of gravitational-wave sources, γ-ray bursts, and X-ray emitting galaxies at cosmological distances and it will produce a heritage multi-wavelength dataset and library of models for future studies of galaxies and accreting binaries."
Summary
"High-energy observations of our Galaxy offer a good, albeit not complete, picture of the X-ray source populations, in particular the accreting binary sources. Recent ability to study accreting binaries in nearby galaxies has shown that we would be short-sighted if we restricted ourselves to our Galaxy or to a few nearby ones. I propose an ambitious project that involves a comprehensive study of all the galaxies within 10 Mpc for which we can study in detail their X-ray sources and stellar populations. The study will combine data from a unique suite of observatories (Chandra, XMM-Newton, HST, Spitzer) with state-of-the-art theoretical modelling of binary systems. I propose a novel approach that links the accreting binary populations to their parent stellar populations and surpasses any current studies of X-ray binary populations, both in scale and in scope, by: (a) combining methods and results from several different areas of astrophysics (compact objects, binary systems, stellar populations, galaxy evolution); (b) using data from almost the whole electromagnetic spectrum (infrared to X-ray bands); (c) identifying and studying the different sub-populations of accreting binaries; and (d) performing direct comparison between observations and theoretical predictions, over a broad parameter space. The project: (a) will answer the long-standing question of the formation efficiency of accreting binaries in different environments; and (b) will constrain their evolutionary paths. As by-products the project will provide eagerly awaited input to the fields of gravitational-wave sources, γ-ray bursts, and X-ray emitting galaxies at cosmological distances and it will produce a heritage multi-wavelength dataset and library of models for future studies of galaxies and accreting binaries."
Max ERC Funding
1 242 000 €
Duration
Start date: 2014-04-01, End date: 2019-03-31
Project acronym ASSESS
Project Episodic Mass Loss in the Most Massive Stars: Key to Understanding the Explosive Early Universe
Researcher (PI) Alceste BONANOS
Host Institution (HI) NATIONAL OBSERVATORY OF ATHENS
Call Details Consolidator Grant (CoG), PE9, ERC-2017-COG
Summary Massive stars dominate their surroundings during their short lifetimes, while their explosive deaths impact the chemical evolution and spatial cohesion of their hosts. After birth, their evolution is largely dictated by their ability to remove layers of hydrogen from their envelopes. Multiple lines of evidence are pointing to violent, episodic mass-loss events being responsible for removing a large part of the massive stellar envelope, especially in low-metallicity galaxies. Episodic mass loss, however, is not understood theoretically, neither accounted for in state-of-the-art models of stellar evolution, which has far-reaching consequences for many areas of astronomy. We aim to determine whether episodic mass loss is a dominant process in the evolution of the most massive stars by conducting the first extensive, multi-wavelength survey of evolved massive stars in the nearby Universe. The project hinges on the fact that mass-losing stars form dust and are bright in the mid-infrared. We plan to (i) derive physical parameters of a large sample of dusty, evolved targets and estimate the amount of ejected mass, (ii) constrain evolutionary models, (iii) quantify the duration and frequency of episodic mass loss as a function of metallicity. The approach involves applying machine-learning algorithms to existing multi-band and time-series photometry of luminous sources in ~25 nearby galaxies. Dusty, luminous evolved massive stars will thus be automatically classified and follow-up spectroscopy will be obtained for selected targets. Atmospheric and SED modeling will yield parameters and estimates of time-dependent mass loss for ~1000 luminous stars. The emerging trend for the ubiquity of episodic mass loss, if confirmed, will be key to understanding the explosive early Universe and will have profound consequences for low-metallicity stars, reionization, and the chemical evolution of galaxies.
Summary
Massive stars dominate their surroundings during their short lifetimes, while their explosive deaths impact the chemical evolution and spatial cohesion of their hosts. After birth, their evolution is largely dictated by their ability to remove layers of hydrogen from their envelopes. Multiple lines of evidence are pointing to violent, episodic mass-loss events being responsible for removing a large part of the massive stellar envelope, especially in low-metallicity galaxies. Episodic mass loss, however, is not understood theoretically, neither accounted for in state-of-the-art models of stellar evolution, which has far-reaching consequences for many areas of astronomy. We aim to determine whether episodic mass loss is a dominant process in the evolution of the most massive stars by conducting the first extensive, multi-wavelength survey of evolved massive stars in the nearby Universe. The project hinges on the fact that mass-losing stars form dust and are bright in the mid-infrared. We plan to (i) derive physical parameters of a large sample of dusty, evolved targets and estimate the amount of ejected mass, (ii) constrain evolutionary models, (iii) quantify the duration and frequency of episodic mass loss as a function of metallicity. The approach involves applying machine-learning algorithms to existing multi-band and time-series photometry of luminous sources in ~25 nearby galaxies. Dusty, luminous evolved massive stars will thus be automatically classified and follow-up spectroscopy will be obtained for selected targets. Atmospheric and SED modeling will yield parameters and estimates of time-dependent mass loss for ~1000 luminous stars. The emerging trend for the ubiquity of episodic mass loss, if confirmed, will be key to understanding the explosive early Universe and will have profound consequences for low-metallicity stars, reionization, and the chemical evolution of galaxies.
Max ERC Funding
1 128 750 €
Duration
Start date: 2018-09-01, End date: 2023-08-31
Project acronym dEMORY
Project Dissecting the Role of Dendrites in Memory
Researcher (PI) Panayiota Poirazi
Host Institution (HI) FOUNDATION FOR RESEARCH AND TECHNOLOGY HELLAS
Call Details Starting Grant (StG), LS5, ERC-2012-StG_20111109
Summary Understanding the rules and mechanisms underlying memory formation, storage and retrieval is a grand challenge in neuroscience. In light of cumulating evidence regarding non-linear dendritic events (dendritic-spikes, branch strength potentiation, temporal sequence detection etc) together with activity-dependent rewiring of the connection matrix, the classical notion of information storage via Hebbian-like changes in synaptic connections is inadequate. While more recent plasticity theories consider non-linear dendritic properties, a unifying theory of how dendrites are utilized to achieve memory coding, storing and/or retrieval is cruelly missing. Using computational models, we will simulate memory processes in three key brain regions: the hippocampus, the amygdala and the prefrontal cortex. Models will incorporate biologically constrained dendrites and state-of-the-art plasticity rules and will span different levels of abstraction, ranging from detailed biophysical single neurons and circuits to integrate-and-fire networks and abstract theoretical models. Our main goal is to dissect the role of dendrites in information processing and storage across the three different regions by systematically altering their anatomical, biophysical and plasticity properties. Findings will further our understanding of the fundamental computations supported by these structures and how these computations, reinforced by plasticity mechanisms, sub-serve memory formation and associated dysfunctions, thus opening new avenues for hypothesis driven experimentation and development of novel treatments for memory-related diseases. Identification of dendrites as the key processing units across brain regions and complexity levels will lay the foundations for a new era in computational and experimental neuroscience and serve as the basis for groundbreaking advances in the robotics and artificial intelligence fields while also having a large impact on the machine learning community.
Summary
Understanding the rules and mechanisms underlying memory formation, storage and retrieval is a grand challenge in neuroscience. In light of cumulating evidence regarding non-linear dendritic events (dendritic-spikes, branch strength potentiation, temporal sequence detection etc) together with activity-dependent rewiring of the connection matrix, the classical notion of information storage via Hebbian-like changes in synaptic connections is inadequate. While more recent plasticity theories consider non-linear dendritic properties, a unifying theory of how dendrites are utilized to achieve memory coding, storing and/or retrieval is cruelly missing. Using computational models, we will simulate memory processes in three key brain regions: the hippocampus, the amygdala and the prefrontal cortex. Models will incorporate biologically constrained dendrites and state-of-the-art plasticity rules and will span different levels of abstraction, ranging from detailed biophysical single neurons and circuits to integrate-and-fire networks and abstract theoretical models. Our main goal is to dissect the role of dendrites in information processing and storage across the three different regions by systematically altering their anatomical, biophysical and plasticity properties. Findings will further our understanding of the fundamental computations supported by these structures and how these computations, reinforced by plasticity mechanisms, sub-serve memory formation and associated dysfunctions, thus opening new avenues for hypothesis driven experimentation and development of novel treatments for memory-related diseases. Identification of dendrites as the key processing units across brain regions and complexity levels will lay the foundations for a new era in computational and experimental neuroscience and serve as the basis for groundbreaking advances in the robotics and artificial intelligence fields while also having a large impact on the machine learning community.
Max ERC Funding
1 398 000 €
Duration
Start date: 2012-10-01, End date: 2017-09-30
Project acronym FastBio
Project A genomics and systems biology approach to explore the molecular signature and functional consequences of long-term, structured fasting in humans
Researcher (PI) Antigoni DIMA
Host Institution (HI) BIOMEDICAL SCIENCES RESEARCH CENTER ALEXANDER FLEMING
Call Details Starting Grant (StG), LS2, ERC-2016-STG
Summary Dietary intake has an enormous impact on aspects of human health, yet scientific consensus about how what we eat affects our biology remains elusive. To address the complex biological impact of diet, I propose to apply an unconventional, ‘humans-as-model-organisms’ approach to compare the molecular and functional effects of a highly structured dietary regime, specified by the Eastern Orthodox Christian Church (EOCC), to the unstructured diet followed by the general population. Individuals who follow the EOCC regime abstain from meat, dairy products and eggs for 180-200 days annually, in a temporally-structured manner initiated in childhood. I aim to explore the biological signatures of structured vs. unstructured diet by addressing three objectives. First I will investigate the effects of the two regimes, and of genetic variation, on higher-level phenotypes including anthropometric, physiological and biomarker traits. Second, I will carry out a comprehensive set of omics assays (metabolomics, transcriptomics, epigenomics and investigation of the gut microbiome), will associate omics phenotypes with genetic variation, and will integrate data across biological levels to uncover complex molecular signatures. Third, I will interrogate the functional consequences of dietary regimes at the cellular level through primary cell culture. Acute and long-term effects of dietary intake will be explored for all objectives through a two timepoint sampling strategy. This proposal therefore comprises a unique opportunity to study a specific perturbation (EOCC structured diet) introduced to a steady-state system (unstructured diet followed by the general population) in a ground-breaking human systems biology type of study. This approach brings together expertise from genomics, computational biology, statistics, medicine and epidemiology. It will lead to novel insights regarding the potent signalling nature of nutrients and is likely to yield results of high translational value.
Summary
Dietary intake has an enormous impact on aspects of human health, yet scientific consensus about how what we eat affects our biology remains elusive. To address the complex biological impact of diet, I propose to apply an unconventional, ‘humans-as-model-organisms’ approach to compare the molecular and functional effects of a highly structured dietary regime, specified by the Eastern Orthodox Christian Church (EOCC), to the unstructured diet followed by the general population. Individuals who follow the EOCC regime abstain from meat, dairy products and eggs for 180-200 days annually, in a temporally-structured manner initiated in childhood. I aim to explore the biological signatures of structured vs. unstructured diet by addressing three objectives. First I will investigate the effects of the two regimes, and of genetic variation, on higher-level phenotypes including anthropometric, physiological and biomarker traits. Second, I will carry out a comprehensive set of omics assays (metabolomics, transcriptomics, epigenomics and investigation of the gut microbiome), will associate omics phenotypes with genetic variation, and will integrate data across biological levels to uncover complex molecular signatures. Third, I will interrogate the functional consequences of dietary regimes at the cellular level through primary cell culture. Acute and long-term effects of dietary intake will be explored for all objectives through a two timepoint sampling strategy. This proposal therefore comprises a unique opportunity to study a specific perturbation (EOCC structured diet) introduced to a steady-state system (unstructured diet followed by the general population) in a ground-breaking human systems biology type of study. This approach brings together expertise from genomics, computational biology, statistics, medicine and epidemiology. It will lead to novel insights regarding the potent signalling nature of nutrients and is likely to yield results of high translational value.
Max ERC Funding
1 500 000 €
Duration
Start date: 2017-06-01, End date: 2022-05-31
Project acronym NetVolution
Project Evolving Internet Routing:
A Paradigm Shift to Foster Innovation
Researcher (PI) Christos-Xenofon Dimitropoulos
Host Institution (HI) IDRYMA TECHNOLOGIAS KAI EREVNAS
Call Details Starting Grant (StG), PE7, ERC-2013-StG
Summary Although the Internet is a great technological achievement, more than 40 years after its creation some of its original security and reliability problems remain unsolved. The root cause of these problems is the rigidity of the Internet architecture or in other words the Internet ossification problem, i.e., the basic architectural components of the Internet are set to stone and cannot be changed. The most ossified component of the Internet architecture is the inter-domain routing system.
In this project, our goal is to address this challenge and to introduce a new Internet routing architecture that 1) enables innovation at the inter-domain level, 2) is backward-compatible with the present Internet architecture, and 3) provides concrete economic incentives for adopting it. We propose a new Internet routing paradigm based on a novel techno-economic framework, which exploits emerging technologies and meets these three goals. Our novel idea is that the combination of routing control logic outsourcing with Software Defined Networking (SDN) principles enables to innovate at the inter-domain level and therefore has the potential for a major break-through in the architecture of the Internet routing system. SDN is a rapidly emerging new computer networking architecture that makes the routing control plane of a network programmable. Based on our framework, we propose to design, build, and verify a better inter-domain routing system, which solves fundamental security, reliability, and manageability problems of the Internet architecture. Our work will be organized in four core topics 1) build a mutli-domain centralized routing control platform, 2) improve the reliability and security of the current inter-domain routing system, 3) design techniques for resolving tussles between competing network domains, 4) introduce advanced network monitoring and security techniques that intelligently correlate data from multiple domain to diagnose routing outages and attacks.
Summary
Although the Internet is a great technological achievement, more than 40 years after its creation some of its original security and reliability problems remain unsolved. The root cause of these problems is the rigidity of the Internet architecture or in other words the Internet ossification problem, i.e., the basic architectural components of the Internet are set to stone and cannot be changed. The most ossified component of the Internet architecture is the inter-domain routing system.
In this project, our goal is to address this challenge and to introduce a new Internet routing architecture that 1) enables innovation at the inter-domain level, 2) is backward-compatible with the present Internet architecture, and 3) provides concrete economic incentives for adopting it. We propose a new Internet routing paradigm based on a novel techno-economic framework, which exploits emerging technologies and meets these three goals. Our novel idea is that the combination of routing control logic outsourcing with Software Defined Networking (SDN) principles enables to innovate at the inter-domain level and therefore has the potential for a major break-through in the architecture of the Internet routing system. SDN is a rapidly emerging new computer networking architecture that makes the routing control plane of a network programmable. Based on our framework, we propose to design, build, and verify a better inter-domain routing system, which solves fundamental security, reliability, and manageability problems of the Internet architecture. Our work will be organized in four core topics 1) build a mutli-domain centralized routing control platform, 2) improve the reliability and security of the current inter-domain routing system, 3) design techniques for resolving tussles between competing network domains, 4) introduce advanced network monitoring and security techniques that intelligently correlate data from multiple domain to diagnose routing outages and attacks.
Max ERC Funding
1 410 600 €
Duration
Start date: 2014-01-01, End date: 2018-12-31
Project acronym NEUROPHAGY
Project The Role of Autophagy in Synaptic Plasticity
Researcher (PI) Vassiliki NIKOLETOPOULOU
Host Institution (HI) IDRYMA TECHNOLOGIAS KAI EREVNAS
Call Details Starting Grant (StG), LS5, ERC-2016-STG
Summary Neuronal metabolism is emerging as an essential regulator of brain function and its deregulation is a common denominator in neurological disorders entailing intellectual disability and synapse dys-morphogenesis. The autophagy-lysosome system is the major catabolic pathway dedicated to the recycling not only of protein aggregates but also lipids, nucleic acids, polysaccharides and defective or superfluous organelles, among others.
Appreciation of the role of autophagic pathways in the healthy and diseased brain continues to expand, as accumulating evidence indicates that proper regulation of autophagy is indispensable for neuronal integrity. At the cellular level, several lines of evidence implicate autophagy in the regulation of synaptic plasticity. However, the synapse-specific substrates of autophagy remain elusive. Similarly, the synaptic defects arising from autophagy impairment have never been thus far systematically addressed, yet they translate into severe behavioural deficiencies, such as compromised memory and cognition, pertinent to disorders of intellectual disability.
The present proposal aims to determine how autophagy regulates synaptic plasticity and how its deregulation contributes to synaptic defects. In particular, the objectives aim to: 1) Monitor and characterize the presence of the autophagic machinery in pre- and post-synaptic sites. 2) Identify autophagic substrates residing in synapses and whose turnover via autophagy determines synaptic plasticity. 3) Characterize the synaptic defects and ensuing behavioural deficits arising from impaired autophagy in the hippocampus. 4) Use C. elegans as a model system to address the evolutionary conservation of the synaptic role of autophagy and perform forward genetic screens to reveal novel regulators of autophagy in synapses.
Summary
Neuronal metabolism is emerging as an essential regulator of brain function and its deregulation is a common denominator in neurological disorders entailing intellectual disability and synapse dys-morphogenesis. The autophagy-lysosome system is the major catabolic pathway dedicated to the recycling not only of protein aggregates but also lipids, nucleic acids, polysaccharides and defective or superfluous organelles, among others.
Appreciation of the role of autophagic pathways in the healthy and diseased brain continues to expand, as accumulating evidence indicates that proper regulation of autophagy is indispensable for neuronal integrity. At the cellular level, several lines of evidence implicate autophagy in the regulation of synaptic plasticity. However, the synapse-specific substrates of autophagy remain elusive. Similarly, the synaptic defects arising from autophagy impairment have never been thus far systematically addressed, yet they translate into severe behavioural deficiencies, such as compromised memory and cognition, pertinent to disorders of intellectual disability.
The present proposal aims to determine how autophagy regulates synaptic plasticity and how its deregulation contributes to synaptic defects. In particular, the objectives aim to: 1) Monitor and characterize the presence of the autophagic machinery in pre- and post-synaptic sites. 2) Identify autophagic substrates residing in synapses and whose turnover via autophagy determines synaptic plasticity. 3) Characterize the synaptic defects and ensuing behavioural deficits arising from impaired autophagy in the hippocampus. 4) Use C. elegans as a model system to address the evolutionary conservation of the synaptic role of autophagy and perform forward genetic screens to reveal novel regulators of autophagy in synapses.
Max ERC Funding
1 493 750 €
Duration
Start date: 2017-03-01, End date: 2022-02-28
Project acronym PASIPHAE
Project Overcoming the Dominant Foreground of Inflationary B-modes: Tomography of Galactic Magnetic Dust via Measurements of Starlight Polarization
Researcher (PI) Konstantinos TASSIS
Host Institution (HI) IDRYMA TECHNOLOGIAS KAI EREVNAS
Call Details Consolidator Grant (CoG), PE9, ERC-2017-COG
Summary An inflation-probing B-mode signal in the polarization of the cosmic microwave background (CMB) would be a discovery of utmost importance in physics. While such a signal is aggressively pursued by experiments around the world, recent Planck results have showed that this breakthrough is still out of reach, because of contamination from Galactic dust. To get to the primordial B-modes, we need to subtract polarized emission of magnetized interstellar dust with high accuracy. A critical piece of this puzzle is the 3D structure of the magnetic field threading dust clouds, which cannot be accessed through microwave observations alone, since they record integrated emission along the line of sight. Instead, observations of a large number of stars at known distances in optical polarization, tracing the same CMB-obscuring dust, can map the magnetic field between them. The Gaia mission is measuring distances to a billion stars, providing an opportunity to produce, the first-ever tomographic map of the Galactic magnetic field, using optical polarization of starlight. Such a map would not only boost CMB polarization foreground removal, but it would also have a profound impact in a wide range of astrophysical research, including interstellar medium physics, high-energy astrophysics, and galactic evolution. Taking advantage of our privately-funded, novel-technology, high-accuracy WALOP optopolarimeters currently under construction, we propose an ambitious optopolarimetric program of unprecedented scale that can meet this challenge: a survey of both northern and southern Galactic polar regions targeted by CMB experiments, covering >10,000 square degrees, which will measure linear optical polarization at 0.2% accuracy of over 360 stars per square degree (over 3.5M stars, a 1000-fold increase over the state of the art), combining wide-field-optimized instruments and an extraordinary commitment of observing time by Skinakas Observatory and the South African Astronomical Observatory.
Summary
An inflation-probing B-mode signal in the polarization of the cosmic microwave background (CMB) would be a discovery of utmost importance in physics. While such a signal is aggressively pursued by experiments around the world, recent Planck results have showed that this breakthrough is still out of reach, because of contamination from Galactic dust. To get to the primordial B-modes, we need to subtract polarized emission of magnetized interstellar dust with high accuracy. A critical piece of this puzzle is the 3D structure of the magnetic field threading dust clouds, which cannot be accessed through microwave observations alone, since they record integrated emission along the line of sight. Instead, observations of a large number of stars at known distances in optical polarization, tracing the same CMB-obscuring dust, can map the magnetic field between them. The Gaia mission is measuring distances to a billion stars, providing an opportunity to produce, the first-ever tomographic map of the Galactic magnetic field, using optical polarization of starlight. Such a map would not only boost CMB polarization foreground removal, but it would also have a profound impact in a wide range of astrophysical research, including interstellar medium physics, high-energy astrophysics, and galactic evolution. Taking advantage of our privately-funded, novel-technology, high-accuracy WALOP optopolarimeters currently under construction, we propose an ambitious optopolarimetric program of unprecedented scale that can meet this challenge: a survey of both northern and southern Galactic polar regions targeted by CMB experiments, covering >10,000 square degrees, which will measure linear optical polarization at 0.2% accuracy of over 360 stars per square degree (over 3.5M stars, a 1000-fold increase over the state of the art), combining wide-field-optimized instruments and an extraordinary commitment of observing time by Skinakas Observatory and the South African Astronomical Observatory.
Max ERC Funding
1 887 500 €
Duration
Start date: 2018-06-01, End date: 2023-05-31
Project acronym SMARTGATE
Project "Smart Gates for the ""Green"" Transistor"
Researcher (PI) Athanasios Dimoulas
Host Institution (HI) "NATIONAL CENTER FOR SCIENTIFIC RESEARCH ""DEMOKRITOS"""
Call Details Advanced Grant (AdG), PE7, ERC-2011-ADG_20110209
Summary Ultra-low voltage/power operation is expected to be an important requirement for future nanoelectronics allowing more dense and fast circuits on one hand and enabling the operation of energy efficient intelligent autonomous systems on the other. In present day devices quite a lot of power is consumed during switching since it requires a minimum bias of 60 mV on the gate to overcome a potential barrier and increase the transistor current by a decade, a process which is fundamentally limited by thermal Boltzmann statistics. We propose the development of novel negative capacitance “smart” gates with a positive feedback and internal amplification to overcome the “Boltzmann tyranny” and obtain steeper slope “green” transistors capable of operating at very low voltage. Metallic systems with a low density of states could provide the required dominant negative contributions to the capacitance due to strong carrier correlation effects. Such metallic systems made of 2D Dirac fermions with linear dispersion bands are supported in graphene and on the surface of the newly discovered topological insulators having the very interesting property that they offer a nearly zero density of states at the band crossing near the charge neutral point. We propose here the graphene and Bi2Se3-based topological insulators as the key components of the targeted “smart” gates. We aim at developing complex gate structures facing the challenges of growth of high purity and high crystalline quality graphene and Bi2Se3 thin films in combination with conventional dielectrics and metals on Si semiconductor in an effort to obtain the required properties and ensure their robust functionality at room temperature. Possible negative capacitance effects will be investigated in terms of generic capacitor electrical characterization, while transistor devices with optimum smart gates will be fabricated to prove the principle of steep slope switching.
Summary
Ultra-low voltage/power operation is expected to be an important requirement for future nanoelectronics allowing more dense and fast circuits on one hand and enabling the operation of energy efficient intelligent autonomous systems on the other. In present day devices quite a lot of power is consumed during switching since it requires a minimum bias of 60 mV on the gate to overcome a potential barrier and increase the transistor current by a decade, a process which is fundamentally limited by thermal Boltzmann statistics. We propose the development of novel negative capacitance “smart” gates with a positive feedback and internal amplification to overcome the “Boltzmann tyranny” and obtain steeper slope “green” transistors capable of operating at very low voltage. Metallic systems with a low density of states could provide the required dominant negative contributions to the capacitance due to strong carrier correlation effects. Such metallic systems made of 2D Dirac fermions with linear dispersion bands are supported in graphene and on the surface of the newly discovered topological insulators having the very interesting property that they offer a nearly zero density of states at the band crossing near the charge neutral point. We propose here the graphene and Bi2Se3-based topological insulators as the key components of the targeted “smart” gates. We aim at developing complex gate structures facing the challenges of growth of high purity and high crystalline quality graphene and Bi2Se3 thin films in combination with conventional dielectrics and metals on Si semiconductor in an effort to obtain the required properties and ensure their robust functionality at room temperature. Possible negative capacitance effects will be investigated in terms of generic capacitor electrical characterization, while transistor devices with optimum smart gates will be fabricated to prove the principle of steep slope switching.
Max ERC Funding
1 221 611 €
Duration
Start date: 2012-01-01, End date: 2016-07-31