Project acronym 1st-principles-discs
Project A First Principles Approach to Accretion Discs
Researcher (PI) Martin Elias Pessah
Host Institution (HI) KOBENHAVNS UNIVERSITET
Country Denmark
Call Details Starting Grant (StG), PE9, ERC-2012-StG_20111012
Summary Most celestial bodies, from planets, to stars, to black holes; gain mass during their lives by means of an accretion disc. Understanding the physical processes that determine the rate at which matter accretes and energy is radiated in these discs is vital for unraveling the formation, evolution, and fate of almost every type of object in the Universe. Despite the fact that magnetic fields have been known to be crucial in accretion discs since the early 90’s, the majority of astrophysical questions that depend on the details of how disc accretion proceeds are still being addressed using the “standard” accretion disc model (developed in the early 70’s), where magnetic fields do not play an explicit role. This has prevented us from fully exploring the astrophysical consequences and observational signatures of realistic accretion disc models, leading to a profound disconnect between observations (usually interpreted with the standard paradigm) and modern accretion disc theory and numerical simulations (where magnetic turbulence is crucial). The goal of this proposal is to use several complementary approaches in order to finally move beyond the standard paradigm. This program has two main objectives: 1) Develop the theoretical framework to incorporate magnetic fields, and the ensuing turbulence, into self-consistent accretion disc models, and investigate their observational implications. 2) Investigate transport and radiative processes in collision-less disc regions, where non-thermal radiation originates, by employing a kinetic particle description of the plasma. In order to achieve these goals, we will use, and build upon, state-of-the-art magnetohydrodynamic and particle-in-cell codes in conjunction with theoretical modeling. This framework will make it possible to address fundamental questions on stellar and planet formation, binary systems with a compact object, and supermassive black hole feedback in a way that has no counterpart within the standard paradigm.
Summary
Most celestial bodies, from planets, to stars, to black holes; gain mass during their lives by means of an accretion disc. Understanding the physical processes that determine the rate at which matter accretes and energy is radiated in these discs is vital for unraveling the formation, evolution, and fate of almost every type of object in the Universe. Despite the fact that magnetic fields have been known to be crucial in accretion discs since the early 90’s, the majority of astrophysical questions that depend on the details of how disc accretion proceeds are still being addressed using the “standard” accretion disc model (developed in the early 70’s), where magnetic fields do not play an explicit role. This has prevented us from fully exploring the astrophysical consequences and observational signatures of realistic accretion disc models, leading to a profound disconnect between observations (usually interpreted with the standard paradigm) and modern accretion disc theory and numerical simulations (where magnetic turbulence is crucial). The goal of this proposal is to use several complementary approaches in order to finally move beyond the standard paradigm. This program has two main objectives: 1) Develop the theoretical framework to incorporate magnetic fields, and the ensuing turbulence, into self-consistent accretion disc models, and investigate their observational implications. 2) Investigate transport and radiative processes in collision-less disc regions, where non-thermal radiation originates, by employing a kinetic particle description of the plasma. In order to achieve these goals, we will use, and build upon, state-of-the-art magnetohydrodynamic and particle-in-cell codes in conjunction with theoretical modeling. This framework will make it possible to address fundamental questions on stellar and planet formation, binary systems with a compact object, and supermassive black hole feedback in a way that has no counterpart within the standard paradigm.
Max ERC Funding
1 793 697 €
Duration
Start date: 2013-02-01, End date: 2018-01-31
Project acronym LOBENA
Project Long Beamtime Experiments for Nuclear Astrophysics
Researcher (PI) Hans Otto Uldall Fynbo
Host Institution (HI) AARHUS UNIVERSITET
Country Denmark
Call Details Starting Grant (StG), PE2, ERC-2012-StG_20111012
Summary The goal of LOBENA is to measure key properties needed for understanding nuclear processes in the Cosmos. Nuclear Astrophysics plays a key role in our quest to understand the origin and distribution of the chemical elements in our galaxy. Nuclear processes are crucial for understanding the energy production in the universe and are essential for describing the creation of chemical elements from the ashes of the Big Bang. Uncertainties in the nuclear physics can therefore influence our understanding of many astrophysical processes, both those involving stable stellar burning phases and explosive phenomena such as X-ray bursts, gamma-ray bursts and supernovae.
In LOBENA (LOng Beamtime Experiments for Nuclear Astrophysics) I will initiate a series of studies in Nuclear Astrophysics, which have in common the need for long beam times and the use of complete kinematics detection of several particles emitted in reactions. The core of the project will focus on the systems 8Be, 12C and 16O where today key open questions of great importance remain to answered. These questions can be addressed by reactions induced by low energy (<5MeV) beams of protons and 3He on light targets such as 6,7Li, 9Be, 10,11B and 19F using a newly developed complete kinematics detection procedure. The department of Physics and Astronomy in Aarhus provides a unique scene for doing these measurements since it provides accelerators where long beam time can be guarantied. LOBENA will also include complimentary experiments at international user facilities such as ISOLDE (CERN), KVI (Groningen), JYFL and (Jyväskylä).
With this ERC starting grant proposal I wish to start up my own group around Nuclear Astrophysics experiments in house and at international user facilities. With two Post Doc.s and a Ph.D. I will be much better able to fully exploit the scientific potential of the proposed research, which will also help to consolidate my own research career and give me more independence.
Summary
The goal of LOBENA is to measure key properties needed for understanding nuclear processes in the Cosmos. Nuclear Astrophysics plays a key role in our quest to understand the origin and distribution of the chemical elements in our galaxy. Nuclear processes are crucial for understanding the energy production in the universe and are essential for describing the creation of chemical elements from the ashes of the Big Bang. Uncertainties in the nuclear physics can therefore influence our understanding of many astrophysical processes, both those involving stable stellar burning phases and explosive phenomena such as X-ray bursts, gamma-ray bursts and supernovae.
In LOBENA (LOng Beamtime Experiments for Nuclear Astrophysics) I will initiate a series of studies in Nuclear Astrophysics, which have in common the need for long beam times and the use of complete kinematics detection of several particles emitted in reactions. The core of the project will focus on the systems 8Be, 12C and 16O where today key open questions of great importance remain to answered. These questions can be addressed by reactions induced by low energy (<5MeV) beams of protons and 3He on light targets such as 6,7Li, 9Be, 10,11B and 19F using a newly developed complete kinematics detection procedure. The department of Physics and Astronomy in Aarhus provides a unique scene for doing these measurements since it provides accelerators where long beam time can be guarantied. LOBENA will also include complimentary experiments at international user facilities such as ISOLDE (CERN), KVI (Groningen), JYFL and (Jyväskylä).
With this ERC starting grant proposal I wish to start up my own group around Nuclear Astrophysics experiments in house and at international user facilities. With two Post Doc.s and a Ph.D. I will be much better able to fully exploit the scientific potential of the proposed research, which will also help to consolidate my own research career and give me more independence.
Max ERC Funding
1 476 075 €
Duration
Start date: 2012-11-01, End date: 2018-10-31
Project acronym LOWLANDS
Project Parsing low-resource languages and domains
Researcher (PI) Anders Soegaard
Host Institution (HI) KOBENHAVNS UNIVERSITET
Country Denmark
Call Details Starting Grant (StG), SH4, ERC-2012-StG_20111124
Summary "There are noticeable asymmetries in availability of high-quality natural language processing (NLP). We can adequately summarize English newspapers and translate them into Korean, but we cannot translate Korean newspaper articles into English, and summarizing micro-blogs is much more difficult than summarizing newspaper articles. This is a fundamental problem for modern societies, their development and democracy, as well as perhaps the most important research problem in NLP right now.
Most NLP technologies rely on highly accurate syntactic parsing. Reliable parsing models can be induced from large collections of manually annotated data, but such collections are typically limited to sampled newswire in major languages. Highly accurate parsing is therefore not available for other languages and other domains.
The NLP community is well aware of this problem, but unsupervised techniques that do not rely on manually annotated data cannot be used for real-world applications, where highly accurate parsing is needed, and sample bias correction methods that automatically correct the bias in newswire when parsing, say, micro-blogs, do not yet lead to robust improvements across the board.
The objective of this project is to develop new learning methods for parsing natural language for which no unbiased labeled data exists. In order to do so, we need to fundamentally rethink the unsupervised parsing problem, including how we evaluate unsupervised parsers, but we also need to supplement unsupervised learning techniques with robust methods for automatically correcting sample selection biases in related data. Such methods will be applicable to both cross-domain and cross-language syntactic parsing and will pave the way toward robust and scalable NLP. The societal impact of robust and scalable NLP is unforeseeable and comparable to how efficient information retrieval techniques have revolutionized modern societies."
Summary
"There are noticeable asymmetries in availability of high-quality natural language processing (NLP). We can adequately summarize English newspapers and translate them into Korean, but we cannot translate Korean newspaper articles into English, and summarizing micro-blogs is much more difficult than summarizing newspaper articles. This is a fundamental problem for modern societies, their development and democracy, as well as perhaps the most important research problem in NLP right now.
Most NLP technologies rely on highly accurate syntactic parsing. Reliable parsing models can be induced from large collections of manually annotated data, but such collections are typically limited to sampled newswire in major languages. Highly accurate parsing is therefore not available for other languages and other domains.
The NLP community is well aware of this problem, but unsupervised techniques that do not rely on manually annotated data cannot be used for real-world applications, where highly accurate parsing is needed, and sample bias correction methods that automatically correct the bias in newswire when parsing, say, micro-blogs, do not yet lead to robust improvements across the board.
The objective of this project is to develop new learning methods for parsing natural language for which no unbiased labeled data exists. In order to do so, we need to fundamentally rethink the unsupervised parsing problem, including how we evaluate unsupervised parsers, but we also need to supplement unsupervised learning techniques with robust methods for automatically correcting sample selection biases in related data. Such methods will be applicable to both cross-domain and cross-language syntactic parsing and will pave the way toward robust and scalable NLP. The societal impact of robust and scalable NLP is unforeseeable and comparable to how efficient information retrieval techniques have revolutionized modern societies."
Max ERC Funding
1 126 183 €
Duration
Start date: 2013-01-01, End date: 2017-12-31
Project acronym QIOS
Project Quantum Interfaces and Open Systems
Researcher (PI) Anders Soerensen
Host Institution (HI) KOBENHAVNS UNIVERSITET
Country Denmark
Call Details Starting Grant (StG), PE2, ERC-2012-StG_20111012
Summary "Researchers have strived to obtain control of a variety of different quantum systems, each characterized by their own distinct advantages: quantum optical systems offer excellent isolation from the environment while solid state systems allow for integrated micro-fabricated devices. At the same time nuclear spins in molecules can remain decoupled from the environment even under rather harsh conditions, and this is the basis of NMR experiments. Given these distinct advantages it is very fruitful to investigate hybrid devices merging the advantages of each of the systems. To do this it is essential to develop quantum interfaces to connect the different systems. By their very nature such quantum interfaces exchange information with their environment and are therefore open quantum systems.
In this project I wish to establish a strong theoretical quantum optics group which can guide and inspire the experiments towards breaking new grounds for open quantum systems and making quantum interfaces between distinct physical systems. The objective is to develop concrete proposals for how to experimentally control and exploit the interaction of quantum systems with their surroundings and for how this can be used for quantum interfaces.
The work in this project is particularly relevant for applications in quantum information processing, where the current challenge is to take the field from proof-of-principle demonstrations to truly scalable devices. Such challenge demands new interdisciplinary theoretical ideas for hybrid devices. This proposal addresses several key challenges for quantum information processing: scalable multimode quantum repeaters based on hybrid approaches, entanglement enabled quantum metrology, photonic engineering based on surface plasmons, dissipative preparation of entangled states, and phonon engineering for quantum dots. In addition applications towards nuclear spin cooling to improve NMR experiments as well as ultra cold atoms will be explored."
Summary
"Researchers have strived to obtain control of a variety of different quantum systems, each characterized by their own distinct advantages: quantum optical systems offer excellent isolation from the environment while solid state systems allow for integrated micro-fabricated devices. At the same time nuclear spins in molecules can remain decoupled from the environment even under rather harsh conditions, and this is the basis of NMR experiments. Given these distinct advantages it is very fruitful to investigate hybrid devices merging the advantages of each of the systems. To do this it is essential to develop quantum interfaces to connect the different systems. By their very nature such quantum interfaces exchange information with their environment and are therefore open quantum systems.
In this project I wish to establish a strong theoretical quantum optics group which can guide and inspire the experiments towards breaking new grounds for open quantum systems and making quantum interfaces between distinct physical systems. The objective is to develop concrete proposals for how to experimentally control and exploit the interaction of quantum systems with their surroundings and for how this can be used for quantum interfaces.
The work in this project is particularly relevant for applications in quantum information processing, where the current challenge is to take the field from proof-of-principle demonstrations to truly scalable devices. Such challenge demands new interdisciplinary theoretical ideas for hybrid devices. This proposal addresses several key challenges for quantum information processing: scalable multimode quantum repeaters based on hybrid approaches, entanglement enabled quantum metrology, photonic engineering based on surface plasmons, dissipative preparation of entangled states, and phonon engineering for quantum dots. In addition applications towards nuclear spin cooling to improve NMR experiments as well as ultra cold atoms will be explored."
Max ERC Funding
1 431 542 €
Duration
Start date: 2012-10-01, End date: 2017-09-30
