Project acronym AARTFAAC
Project Amsterdam-ASTRON Radio Transient Facility And Analysis Centre: Probing the Extremes of Astrophysics
Researcher (PI) Ralph Antoine Marie Joseph Wijers
Host Institution (HI) UNIVERSITEIT VAN AMSTERDAM
Call Details Advanced Grant (AdG), PE9, ERC-2009-AdG
Summary Some of the most extreme tests of physical law come from its manifestations in the behaviour of black holes and neutron stars, and as such these objects should be used as fundamental physics labs. Due to advances in both theoretical work and observational techniques, I have a major opportunity now to significantly push this agenda forward and get better answers to questions like: How are black holes born? How can energy be extracted from black holes? What is the origin of magnetic fields and cosmic rays in jets and shocks? Is their primary energy stream hadronic or magnetic? I propose to do this by exploiting the advent of wide-field radio astronomy: extreme objects are very rare and usually transient, so not only must one survey large areas of sky, but also must one do this often. I propose to form and shape a group that will use the LOFAR wide-field radio telescope to hunt for these extreme transients and systematically collect enough well-documented examples of the behaviour of each type of transient. Furthermore, I propose to expand LOFAR with a true 24/7 all-sky monitor to catch and study even the rarest of events. Next, I will use my experience in gamma-ray burst followup to conduct a vigorous multi-wavelength programme of study of these objects, to constrain their physics from as many angles as possible. This will eventually include results from multi-messenger astrophysics, in which we use neutrinos, gravity waves, and other non-electromagnetic messengers as extra diagnostics of the physics of these sources. Finally, I will build on my experience in modelling accretion phenomena and relativistic explosions to develop a theoretical framework for these phenomena and constrain the resulting models with the rich data sets we obtain.
Summary
Some of the most extreme tests of physical law come from its manifestations in the behaviour of black holes and neutron stars, and as such these objects should be used as fundamental physics labs. Due to advances in both theoretical work and observational techniques, I have a major opportunity now to significantly push this agenda forward and get better answers to questions like: How are black holes born? How can energy be extracted from black holes? What is the origin of magnetic fields and cosmic rays in jets and shocks? Is their primary energy stream hadronic or magnetic? I propose to do this by exploiting the advent of wide-field radio astronomy: extreme objects are very rare and usually transient, so not only must one survey large areas of sky, but also must one do this often. I propose to form and shape a group that will use the LOFAR wide-field radio telescope to hunt for these extreme transients and systematically collect enough well-documented examples of the behaviour of each type of transient. Furthermore, I propose to expand LOFAR with a true 24/7 all-sky monitor to catch and study even the rarest of events. Next, I will use my experience in gamma-ray burst followup to conduct a vigorous multi-wavelength programme of study of these objects, to constrain their physics from as many angles as possible. This will eventually include results from multi-messenger astrophysics, in which we use neutrinos, gravity waves, and other non-electromagnetic messengers as extra diagnostics of the physics of these sources. Finally, I will build on my experience in modelling accretion phenomena and relativistic explosions to develop a theoretical framework for these phenomena and constrain the resulting models with the rich data sets we obtain.
Max ERC Funding
3 499 128 €
Duration
Start date: 2010-10-01, End date: 2016-09-30
Project acronym ACUITY
Project Algorithms for coping with uncertainty and intractability
Researcher (PI) Nikhil Bansal
Host Institution (HI) TECHNISCHE UNIVERSITEIT EINDHOVEN
Call Details Consolidator Grant (CoG), PE6, ERC-2013-CoG
Summary The two biggest challenges in solving practical optimization problems are computational intractability, and the presence
of uncertainty: most problems are either NP-hard, or have incomplete input data which
makes an exact computation impossible.
Recently, there has been a huge progress in our understanding of intractability, based on spectacular algorithmic and lower bound techniques. For several problems, especially those with only local constraints, we can design optimum
approximation algorithms that are provably the best possible.
However, typical optimization problems usually involve complex global constraints and are much less understood. The situation is even worse for coping with uncertainty. Most of the algorithms are based on ad-hoc techniques and there is no deeper understanding of what makes various problems easy or hard.
This proposal describes several new directions, together with concrete intermediate goals, that will break important new ground in the theory of approximation and online algorithms. The particular directions we consider are (i) extend the primal dual method to systematically design online algorithms, (ii) build a structural theory of online problems based on work functions, (iii) develop new tools to use the power of strong convex relaxations and (iv) design new algorithmic approaches based on non-constructive proof techniques.
The proposed research is at the
cutting edge of algorithm design, and builds upon the recent success of the PI in resolving several longstanding questions in these areas. Any progress is likely to be a significant contribution to theoretical
computer science and combinatorial optimization.
Summary
The two biggest challenges in solving practical optimization problems are computational intractability, and the presence
of uncertainty: most problems are either NP-hard, or have incomplete input data which
makes an exact computation impossible.
Recently, there has been a huge progress in our understanding of intractability, based on spectacular algorithmic and lower bound techniques. For several problems, especially those with only local constraints, we can design optimum
approximation algorithms that are provably the best possible.
However, typical optimization problems usually involve complex global constraints and are much less understood. The situation is even worse for coping with uncertainty. Most of the algorithms are based on ad-hoc techniques and there is no deeper understanding of what makes various problems easy or hard.
This proposal describes several new directions, together with concrete intermediate goals, that will break important new ground in the theory of approximation and online algorithms. The particular directions we consider are (i) extend the primal dual method to systematically design online algorithms, (ii) build a structural theory of online problems based on work functions, (iii) develop new tools to use the power of strong convex relaxations and (iv) design new algorithmic approaches based on non-constructive proof techniques.
The proposed research is at the
cutting edge of algorithm design, and builds upon the recent success of the PI in resolving several longstanding questions in these areas. Any progress is likely to be a significant contribution to theoretical
computer science and combinatorial optimization.
Max ERC Funding
1 519 285 €
Duration
Start date: 2014-05-01, End date: 2019-04-30
Project acronym ADULT
Project Analysis of the Dark Universe through Lensing Tomography
Researcher (PI) Hendrik Hoekstra
Host Institution (HI) UNIVERSITEIT LEIDEN
Call Details Starting Grant (StG), PE9, ERC-2011-StG_20101014
Summary The discoveries that the expansion of the universe is accelerating due to an unknown “dark energy”
and that most of the matter is invisible, highlight our lack of understanding of the major constituents
of the universe. These surprising findings set the stage for research in cosmology at the start of the
21st century. The objective of this proposal is to advance observational constraints to a level where we can distinguish between physical mechanisms that aim to explain the properties of dark energy and the observed distribution of dark matter throughout the universe. We use a relatively new technique called weak gravitational lensing: the accurate measurement of correlations in the orientations of distant galaxies enables us to map the dark matter distribution directly and to extract the cosmological information that is encoded by the large-scale structure.
To study the dark universe we will analyse data from a new state-of-the-art imaging survey: the Kilo-
Degree Survey (KiDS) will cover 1500 square degrees in 9 filters. The combination of its large survey
area and the availability of exquisite photometric redshifts for the sources makes KiDS the first
project that can place interesting constraints on the dark energy equation-of-state using lensing data
alone. Combined with complementary results from Planck, our measurements will provide one of the
best views of the dark side of the universe before much larger space-based projects commence.
To reach the desired accuracy we need to carefully measure the shapes of distant background galaxies. We also need to account for any intrinsic alignments that arise due to tidal interactions, rather than through lensing. Reducing these observational and physical biases to negligible levels is a necessarystep to ensure the success of KiDS and an important part of our preparation for more challenging projects such as the European-led space mission Euclid.
Summary
The discoveries that the expansion of the universe is accelerating due to an unknown “dark energy”
and that most of the matter is invisible, highlight our lack of understanding of the major constituents
of the universe. These surprising findings set the stage for research in cosmology at the start of the
21st century. The objective of this proposal is to advance observational constraints to a level where we can distinguish between physical mechanisms that aim to explain the properties of dark energy and the observed distribution of dark matter throughout the universe. We use a relatively new technique called weak gravitational lensing: the accurate measurement of correlations in the orientations of distant galaxies enables us to map the dark matter distribution directly and to extract the cosmological information that is encoded by the large-scale structure.
To study the dark universe we will analyse data from a new state-of-the-art imaging survey: the Kilo-
Degree Survey (KiDS) will cover 1500 square degrees in 9 filters. The combination of its large survey
area and the availability of exquisite photometric redshifts for the sources makes KiDS the first
project that can place interesting constraints on the dark energy equation-of-state using lensing data
alone. Combined with complementary results from Planck, our measurements will provide one of the
best views of the dark side of the universe before much larger space-based projects commence.
To reach the desired accuracy we need to carefully measure the shapes of distant background galaxies. We also need to account for any intrinsic alignments that arise due to tidal interactions, rather than through lensing. Reducing these observational and physical biases to negligible levels is a necessarystep to ensure the success of KiDS and an important part of our preparation for more challenging projects such as the European-led space mission Euclid.
Max ERC Funding
1 316 880 €
Duration
Start date: 2012-01-01, End date: 2016-12-31
Project acronym ALERT
Project ALERT - The Apertif-LOFAR Exploration of the Radio Transient Sky
Researcher (PI) Albert Van Leeuwen
Host Institution (HI) STICHTING ASTRON, NETHERLANDS INSTITUTE FOR RADIO ASTRONOMY
Call Details Consolidator Grant (CoG), PE9, ERC-2013-CoG
Summary "In our largely unchanging radio Universe, a highly dynamic component was recently discovered: flashes of bright radio emission that last only milliseconds but appear all over the sky. Some of these radio bursts can be traced to intermittently pulsating neutron stars. Other bursts however, apparently originate far outside our Galaxy. Due to great observational challenges, the evolution of the neutron stars is not understood, while more importantly, the nature of the extragalactic bursts remains an outright mystery.
My overall aim is to understand the physics that drives both kinds of brief and luminous bursts.
My primary goal is to identify the highly compact astrophysical explosions powering the extragalactic bursts. My previous surveys are the state of the art in fast-transient detection; I will now increase by a factor of 10 this exploration volume. In real-time I will provide arcsec positions, 10,000-fold more accurate than currently possible, to localize such extragalactic bursts for the first time and understand their origin.
My secondary goal is to unravel the unexplained evolution of intermittently pulsating neutron stars (building on e.g., my recent papers in Science, 2013), by doubling their number and modeling their population.
To achieve these goals, I will carry out a highly innovative survey: the Apertif-LOFAR Exploration of the Radio Transient Sky. ALERT is over an order of magnitude more sensitive than all current state-of-the art fast-transient surveys.
Through its novel, extremely wide field-of-view, Westerbork/Apertif will detect many tens of extragalactic bursts. Through real-time triggers to LOFAR I will next provide the precise localisation that is essential for radio, optical and high-energy follow-up to, for the first time, shed light on the physics and objects driving these bursts – evaporating primordial black holes; explosions in host galaxies; or, the unknown?"
Summary
"In our largely unchanging radio Universe, a highly dynamic component was recently discovered: flashes of bright radio emission that last only milliseconds but appear all over the sky. Some of these radio bursts can be traced to intermittently pulsating neutron stars. Other bursts however, apparently originate far outside our Galaxy. Due to great observational challenges, the evolution of the neutron stars is not understood, while more importantly, the nature of the extragalactic bursts remains an outright mystery.
My overall aim is to understand the physics that drives both kinds of brief and luminous bursts.
My primary goal is to identify the highly compact astrophysical explosions powering the extragalactic bursts. My previous surveys are the state of the art in fast-transient detection; I will now increase by a factor of 10 this exploration volume. In real-time I will provide arcsec positions, 10,000-fold more accurate than currently possible, to localize such extragalactic bursts for the first time and understand their origin.
My secondary goal is to unravel the unexplained evolution of intermittently pulsating neutron stars (building on e.g., my recent papers in Science, 2013), by doubling their number and modeling their population.
To achieve these goals, I will carry out a highly innovative survey: the Apertif-LOFAR Exploration of the Radio Transient Sky. ALERT is over an order of magnitude more sensitive than all current state-of-the art fast-transient surveys.
Through its novel, extremely wide field-of-view, Westerbork/Apertif will detect many tens of extragalactic bursts. Through real-time triggers to LOFAR I will next provide the precise localisation that is essential for radio, optical and high-energy follow-up to, for the first time, shed light on the physics and objects driving these bursts – evaporating primordial black holes; explosions in host galaxies; or, the unknown?"
Max ERC Funding
1 999 823 €
Duration
Start date: 2014-12-01, End date: 2019-11-30
Project acronym ALGSTRONGCRYPTO
Project Algebraic Methods for Stronger Crypto
Researcher (PI) Ronald John Fitzgerald CRAMER
Host Institution (HI) STICHTING NEDERLANDSE WETENSCHAPPELIJK ONDERZOEK INSTITUTEN
Call Details Advanced Grant (AdG), PE6, ERC-2016-ADG
Summary Our field is cryptology. Our overarching objective is to advance significantly the frontiers in
design and analysis of high-security cryptography for the future generation.
Particularly, we wish to enhance the efficiency, functionality, and, last-but-not-least, fundamental understanding of cryptographic security against very powerful adversaries.
Our approach here is to develop completely novel methods by
deepening, strengthening and broadening the
algebraic foundations of the field.
Concretely, our lens builds on
the arithmetic codex. This is a general, abstract cryptographic primitive whose basic theory we recently developed and whose asymptotic part, which relies on algebraic geometry, enjoys crucial applications in surprising foundational results on constant communication-rate two-party cryptography. A codex is a linear (error correcting) code that, when endowing its ambient vector space just with coordinate-wise multiplication, can be viewed as simulating, up to some degree, richer arithmetical structures such as finite fields (or products thereof), or generally, finite-dimensional algebras over finite fields. Besides this degree, coordinate-localities for which simulation holds and for which it does not at all are also captured.
Our method is based on novel perspectives on codices which significantly
widen their scope and strengthen their utility. Particularly, we bring
symmetries, computational- and complexity theoretic aspects, and connections with algebraic number theory, -geometry, and -combinatorics into play in novel ways. Our applications range from public-key cryptography to secure multi-party computation.
Our proposal is subdivided into 3 interconnected modules:
(1) Algebraic- and Number Theoretical Cryptanalysis
(2) Construction of Algebraic Crypto Primitives
(3) Advanced Theory of Arithmetic Codices
Summary
Our field is cryptology. Our overarching objective is to advance significantly the frontiers in
design and analysis of high-security cryptography for the future generation.
Particularly, we wish to enhance the efficiency, functionality, and, last-but-not-least, fundamental understanding of cryptographic security against very powerful adversaries.
Our approach here is to develop completely novel methods by
deepening, strengthening and broadening the
algebraic foundations of the field.
Concretely, our lens builds on
the arithmetic codex. This is a general, abstract cryptographic primitive whose basic theory we recently developed and whose asymptotic part, which relies on algebraic geometry, enjoys crucial applications in surprising foundational results on constant communication-rate two-party cryptography. A codex is a linear (error correcting) code that, when endowing its ambient vector space just with coordinate-wise multiplication, can be viewed as simulating, up to some degree, richer arithmetical structures such as finite fields (or products thereof), or generally, finite-dimensional algebras over finite fields. Besides this degree, coordinate-localities for which simulation holds and for which it does not at all are also captured.
Our method is based on novel perspectives on codices which significantly
widen their scope and strengthen their utility. Particularly, we bring
symmetries, computational- and complexity theoretic aspects, and connections with algebraic number theory, -geometry, and -combinatorics into play in novel ways. Our applications range from public-key cryptography to secure multi-party computation.
Our proposal is subdivided into 3 interconnected modules:
(1) Algebraic- and Number Theoretical Cryptanalysis
(2) Construction of Algebraic Crypto Primitives
(3) Advanced Theory of Arithmetic Codices
Max ERC Funding
2 447 439 €
Duration
Start date: 2017-10-01, End date: 2022-09-30
Project acronym ARTECHNE
Project Technique in the Arts. Concepts, Practices, Expertise (1500-1950)
Researcher (PI) Sven Georges Mathieu Dupré
Host Institution (HI) UNIVERSITEIT UTRECHT
Call Details Consolidator Grant (CoG), SH5, ERC-2014-CoG
Summary The transmission of ‘technique’ in art has been a conspicuous ‘black box’ resisting analysis. The tools of the humanities used to study the transmission of ideas and concepts are insufficient when it comes to understanding the transmission of something as non-propositional and non-verbal as ‘technique’. The insights of the neurosciences in, for example, the acquisition and transmission of drawing skills are not yet sufficiently advanced to be historically restrictive. However, only in the most recent years, the history of science and technology has turned to how-to instructions as given in recipes. This project proposes to undertake the experimental reconstruction of historical recipes to finally open the black box of the transmission of technique in the visual and decorative arts. Considering ‘technique’ as a textual, material and social practice, this project will write a long-term history of the theory and practice of the study of ‘technique’ in the visual and decorative arts between 1500 and 1950. The three central research questions here are: (1) what is technique in the visual and decorative arts, (2) how is technique transmitted and studied, and (3) who is considered expert in technique, and why? This project will make a breakthrough in our understanding of the transmission of technique in the arts by integrating methodologies typical for the humanities and historical disciplines with laboratory work. Also, by providing a history of technique in the arts, this project lays the historical foundations of the epistemologies of conservation, restoration and technical art history precisely at a moment of greatest urgency. The connection between the history of science and technology and the expertise in conservation, restoration and technical art history (in the Ateliergebouw in Amsterdam) this project envisions builds the intellectual infrastructure of a new field of interdisciplinary research, unique in Europe.
Summary
The transmission of ‘technique’ in art has been a conspicuous ‘black box’ resisting analysis. The tools of the humanities used to study the transmission of ideas and concepts are insufficient when it comes to understanding the transmission of something as non-propositional and non-verbal as ‘technique’. The insights of the neurosciences in, for example, the acquisition and transmission of drawing skills are not yet sufficiently advanced to be historically restrictive. However, only in the most recent years, the history of science and technology has turned to how-to instructions as given in recipes. This project proposes to undertake the experimental reconstruction of historical recipes to finally open the black box of the transmission of technique in the visual and decorative arts. Considering ‘technique’ as a textual, material and social practice, this project will write a long-term history of the theory and practice of the study of ‘technique’ in the visual and decorative arts between 1500 and 1950. The three central research questions here are: (1) what is technique in the visual and decorative arts, (2) how is technique transmitted and studied, and (3) who is considered expert in technique, and why? This project will make a breakthrough in our understanding of the transmission of technique in the arts by integrating methodologies typical for the humanities and historical disciplines with laboratory work. Also, by providing a history of technique in the arts, this project lays the historical foundations of the epistemologies of conservation, restoration and technical art history precisely at a moment of greatest urgency. The connection between the history of science and technology and the expertise in conservation, restoration and technical art history (in the Ateliergebouw in Amsterdam) this project envisions builds the intellectual infrastructure of a new field of interdisciplinary research, unique in Europe.
Max ERC Funding
1 907 944 €
Duration
Start date: 2015-09-01, End date: 2020-08-31
Project acronym AsthmaVir
Project The roles of innate lymphoid cells and rhinovirus in asthma exacerbations
Researcher (PI) Hergen Spits
Host Institution (HI) ACADEMISCH MEDISCH CENTRUM BIJ DE UNIVERSITEIT VAN AMSTERDAM
Call Details Advanced Grant (AdG), LS6, ERC-2013-ADG
Summary Asthma exacerbations represent a high unmet medical need in particular in young children. Human Rhinoviruses (HRV) are the main triggers of these exacerbations. Till now Th2 cells were considered the main initiating effector cell type in asthma in general and asthma exacerbations in particular. However, exaggerated Th2 cell activities alone do not explain all aspects of asthma and exacerbations. Building on our recent discovery of type 2 human innate lymphoid cells (ILC2) capable of promptly producing high amounts of IL-5, IL-9 and IL-13 upon activation and on mouse data pointing to an essential role of these cells in asthma and asthma exacerbations, ILC2 may be the main initiating cells in asthma exacerbations in humans. Thus we hypothesize that HRV directly or indirectly stimulate ILC2s to produce cytokines driving the effector functions leading to the end organ effects that characterize this debilitating disease. Targeting ILC2 and HRV in parallel will provide a highly attractive therapeutic option for the treatment of asthma exacerbations. In depth study of the mechanisms of ILC2 differentiation and function will lead to the design effective drugs targeting these cells; thus the first two objectives of this project are: 1) To unravel the lineage relationship of ILC populations and to decipher the signal transduction pathways that regulate the function of ILCs, 2) to test the functions of lung-residing human ILCs and the effects of compounds that affect these functions in mice which harbour a human immune system and human lung epithelium under homeostatic conditions and after infections with respiratory viruses. The third objective of this project is developing reagents that target HRV; to this end we will develop broadly reacting highly neutralizing human monoclonal antibodies that can be used for prophylaxis and therapy of patients at high risk for developing severe asthma exacerbations.
Summary
Asthma exacerbations represent a high unmet medical need in particular in young children. Human Rhinoviruses (HRV) are the main triggers of these exacerbations. Till now Th2 cells were considered the main initiating effector cell type in asthma in general and asthma exacerbations in particular. However, exaggerated Th2 cell activities alone do not explain all aspects of asthma and exacerbations. Building on our recent discovery of type 2 human innate lymphoid cells (ILC2) capable of promptly producing high amounts of IL-5, IL-9 and IL-13 upon activation and on mouse data pointing to an essential role of these cells in asthma and asthma exacerbations, ILC2 may be the main initiating cells in asthma exacerbations in humans. Thus we hypothesize that HRV directly or indirectly stimulate ILC2s to produce cytokines driving the effector functions leading to the end organ effects that characterize this debilitating disease. Targeting ILC2 and HRV in parallel will provide a highly attractive therapeutic option for the treatment of asthma exacerbations. In depth study of the mechanisms of ILC2 differentiation and function will lead to the design effective drugs targeting these cells; thus the first two objectives of this project are: 1) To unravel the lineage relationship of ILC populations and to decipher the signal transduction pathways that regulate the function of ILCs, 2) to test the functions of lung-residing human ILCs and the effects of compounds that affect these functions in mice which harbour a human immune system and human lung epithelium under homeostatic conditions and after infections with respiratory viruses. The third objective of this project is developing reagents that target HRV; to this end we will develop broadly reacting highly neutralizing human monoclonal antibodies that can be used for prophylaxis and therapy of patients at high risk for developing severe asthma exacerbations.
Max ERC Funding
2 499 593 €
Duration
Start date: 2014-03-01, End date: 2019-02-28
Project acronym Auger-Horizon
Project A large-scale radio detector for the Pierre Auger cosmic-ray Observatory – precision measurements of ultra-high-energy cosmic rays
Researcher (PI) Jörg HÖRANDEL
Host Institution (HI) STICHTING KATHOLIEKE UNIVERSITEIT
Call Details Advanced Grant (AdG), PE9, ERC-2017-ADG
Summary Cosmic Rays (ionized atomic nuclei) are the only matter from beyond our solar system or even from extragalactic space, that we can directly investigate. Up to energies of 10^17 eV they most likely originate in our Galaxy. The highest-energy cosmic rays (>10^18 eV) cannot be magnetically bound any more to the Galaxy and are most likely of extragalactic origin.
The pure existence of these particles raises the question about their origin – how and where are they accelerated? How do they propagate through the universe and interact? How can we directly probe extragalactic matter and how can we locate its origin?
A key to understand the origin of cosmic rays is to measure the particle species (atomic mass). A precise mass measurement will allow discriminating astrophysical models and will clarify the reason for the observed suppression of the cosmic-ray flux at the highest energies, namely the maximum energy of the accelerators or the energy losses during propagation.
I address these questions by employing a new technique to precisely measure the cosmic-ray mass composition, which my group pioneered, the radio detection of air showers (induced by high-energy cosmic rays in the atmosphere) on very large scales, detecting horizontal air showers with zenith angles from 60° to 90°.
The new set-up will be the world-largest radio array, operated together with the well-established Auger surface and fluorescence detectors, forming a unique set-up to measure the properties of cosmic rays with unprecedented precision for energies above 10^17.5 eV. The radio technique is a cost-effective and robust method to measure the cosmic-ray energy and mass, complementary to established techniques. The energy scale of the radio measurements is established from first principles. The proposed detectors will also enhance the detection capabilities for high-energy neutrinos and the search for new physics through precision measurements of the electromagnetic and muonic shower components.
Summary
Cosmic Rays (ionized atomic nuclei) are the only matter from beyond our solar system or even from extragalactic space, that we can directly investigate. Up to energies of 10^17 eV they most likely originate in our Galaxy. The highest-energy cosmic rays (>10^18 eV) cannot be magnetically bound any more to the Galaxy and are most likely of extragalactic origin.
The pure existence of these particles raises the question about their origin – how and where are they accelerated? How do they propagate through the universe and interact? How can we directly probe extragalactic matter and how can we locate its origin?
A key to understand the origin of cosmic rays is to measure the particle species (atomic mass). A precise mass measurement will allow discriminating astrophysical models and will clarify the reason for the observed suppression of the cosmic-ray flux at the highest energies, namely the maximum energy of the accelerators or the energy losses during propagation.
I address these questions by employing a new technique to precisely measure the cosmic-ray mass composition, which my group pioneered, the radio detection of air showers (induced by high-energy cosmic rays in the atmosphere) on very large scales, detecting horizontal air showers with zenith angles from 60° to 90°.
The new set-up will be the world-largest radio array, operated together with the well-established Auger surface and fluorescence detectors, forming a unique set-up to measure the properties of cosmic rays with unprecedented precision for energies above 10^17.5 eV. The radio technique is a cost-effective and robust method to measure the cosmic-ray energy and mass, complementary to established techniques. The energy scale of the radio measurements is established from first principles. The proposed detectors will also enhance the detection capabilities for high-energy neutrinos and the search for new physics through precision measurements of the electromagnetic and muonic shower components.
Max ERC Funding
3 499 249 €
Duration
Start date: 2018-10-01, End date: 2023-09-30
Project acronym BinCosmos
Project The Impact of Massive Binaries Through Cosmic Time
Researcher (PI) Selma DE MINK
Host Institution (HI) UNIVERSITEIT VAN AMSTERDAM
Call Details Starting Grant (StG), PE9, ERC-2016-STG
Summary Massive stars play many key roles in Astrophysics. As COSMIC ENGINES they transformed the pristine Universe left after the Big Bang into our modern Universe. We use massive stars, their explosions and products as COSMIC PROBES to study the conditions in the distant Universe and the extreme physics inaccessible at earth. Models of massive stars are thus widely applied. A central common assumption is that massive stars are non-rotating single objects, in stark contrast with new data. Recent studies show that majority (70% according to our data) will experience severe interaction with a companion (Sana, de Mink et al. Science 2012).
I propose to conduct the most ambitious and extensive exploration to date of the effects of binarity and rotation on the lives and fates of massive stars to (I) transform our understanding of the complex physical processes and how they operate in the vast parameter space and (II) explore the cosmological implications after calibrating and verifying the models. To achieve this ambitious objective I will use an innovative computational approach that combines the strength of two highly complementary codes and seek direct confrontation with observations to overcome the computational challenges that inhibited previous work.
This timely project will provide the urgent theory framework needed for interpretation and guiding of observing programs with the new facilities (JWST, LSST, aLIGO/VIRGO). Public release of the model grids and code will ensure wide impact of this project. I am in the unique position to successfully lead this project because of my (i) extensive experience modeling the complex physical processes, (ii) leading role in introducing large statistical simulations in the massive star community and (iii) direct involvement in surveys that will be used in this project.
Summary
Massive stars play many key roles in Astrophysics. As COSMIC ENGINES they transformed the pristine Universe left after the Big Bang into our modern Universe. We use massive stars, their explosions and products as COSMIC PROBES to study the conditions in the distant Universe and the extreme physics inaccessible at earth. Models of massive stars are thus widely applied. A central common assumption is that massive stars are non-rotating single objects, in stark contrast with new data. Recent studies show that majority (70% according to our data) will experience severe interaction with a companion (Sana, de Mink et al. Science 2012).
I propose to conduct the most ambitious and extensive exploration to date of the effects of binarity and rotation on the lives and fates of massive stars to (I) transform our understanding of the complex physical processes and how they operate in the vast parameter space and (II) explore the cosmological implications after calibrating and verifying the models. To achieve this ambitious objective I will use an innovative computational approach that combines the strength of two highly complementary codes and seek direct confrontation with observations to overcome the computational challenges that inhibited previous work.
This timely project will provide the urgent theory framework needed for interpretation and guiding of observing programs with the new facilities (JWST, LSST, aLIGO/VIRGO). Public release of the model grids and code will ensure wide impact of this project. I am in the unique position to successfully lead this project because of my (i) extensive experience modeling the complex physical processes, (ii) leading role in introducing large statistical simulations in the massive star community and (iii) direct involvement in surveys that will be used in this project.
Max ERC Funding
1 926 634 €
Duration
Start date: 2017-09-01, End date: 2022-08-31
Project acronym BUILDUP
Project Galaxy Buildup in the Young Universe: from the First Billion Years through the Peak Activity Epoch
Researcher (PI) Karina Caputi
Host Institution (HI) RIJKSUNIVERSITEIT GRONINGEN
Call Details Consolidator Grant (CoG), PE9, ERC-2015-CoG
Summary Deep galaxy surveys are the most valuable asset to understand the history of our Universe. They are key to test galaxy formation models which, based on the Cold Dark Matter framework, are successful at reproducing general aspects of galaxy evolution with cosmic time. However, important discrepancies still exist between models and observations, most notably at high redshifts. This Project will reconstruct the history of galaxy buildup from the first billion years of cosmic time through the peak activity epoch of the Universe, which occurred 10 billion years ago, providing a fundamental constraint for galaxy formation models.
I am leading the largest ultra-deep galaxy survey that will ever be conducted with the Spitzer Space Telescope. In this Project, I will exploit my new Spitzer program to do a groundbreaking study of galaxy buildup in the young Universe, paving the way for further galaxy evolution studies with the forthcoming James Webb Space Telescope (JWST). My main objectives are: 1) quantifying galaxy stellar mass assembly beyond the peak activity epoch, through the study of the galaxy stellar mass function up to z~7; 2) measuring, for the first time, galaxy clustering with stellar mass information up to such high redshifts; 3) linking galaxy growth to dust-obscured star formation using Spitzer and new APEX/AMKID sub-millimetre data; 4) unveiling the first steps of galaxy buildup at z>7 with JWST; 5) optimizing the official JWST Mid Infrared Instrument (MIRI) data reduction pipeline for the analysis of deep galaxy surveys. The delivery of an optimized MIRI pipeline is an important added value to the scientific outcome of this Project, which will benefit the general Astronomical community.
This is the right time for this Project to make a maximum impact. We are now in a turning point for IR Astronomy, and this opportunity should not be missed. This Project will have a long-lasting legacy, bridging current and next generations of IR galaxy surveys.
Summary
Deep galaxy surveys are the most valuable asset to understand the history of our Universe. They are key to test galaxy formation models which, based on the Cold Dark Matter framework, are successful at reproducing general aspects of galaxy evolution with cosmic time. However, important discrepancies still exist between models and observations, most notably at high redshifts. This Project will reconstruct the history of galaxy buildup from the first billion years of cosmic time through the peak activity epoch of the Universe, which occurred 10 billion years ago, providing a fundamental constraint for galaxy formation models.
I am leading the largest ultra-deep galaxy survey that will ever be conducted with the Spitzer Space Telescope. In this Project, I will exploit my new Spitzer program to do a groundbreaking study of galaxy buildup in the young Universe, paving the way for further galaxy evolution studies with the forthcoming James Webb Space Telescope (JWST). My main objectives are: 1) quantifying galaxy stellar mass assembly beyond the peak activity epoch, through the study of the galaxy stellar mass function up to z~7; 2) measuring, for the first time, galaxy clustering with stellar mass information up to such high redshifts; 3) linking galaxy growth to dust-obscured star formation using Spitzer and new APEX/AMKID sub-millimetre data; 4) unveiling the first steps of galaxy buildup at z>7 with JWST; 5) optimizing the official JWST Mid Infrared Instrument (MIRI) data reduction pipeline for the analysis of deep galaxy surveys. The delivery of an optimized MIRI pipeline is an important added value to the scientific outcome of this Project, which will benefit the general Astronomical community.
This is the right time for this Project to make a maximum impact. We are now in a turning point for IR Astronomy, and this opportunity should not be missed. This Project will have a long-lasting legacy, bridging current and next generations of IR galaxy surveys.
Max ERC Funding
1 902 235 €
Duration
Start date: 2016-09-01, End date: 2021-08-31
