Project acronym ANTINEUTRINONOVA
Project Probing Fundamental Physics with Antineutrinos at the NOvA Experiment
Researcher (PI) Jeffrey Hartnell
Host Institution (HI) THE UNIVERSITY OF SUSSEX
Country United Kingdom
Call Details Starting Grant (StG), PE2, ERC-2012-StG_20111012
Summary "This proposal addresses major questions in particle physics that are at the forefront of experimental and theoretical physics research today. The results offered would have far-reaching implications in other fields such as cosmology and could help answer some of the big questions such as why the universe contains so much more matter than antimatter. The research objectives of this proposal are to (i) make world-leading tests of CPT symmetry and (ii) discover the neutrino mass hierarchy and search for indications of leptonic CP violation.
The NOvA long-baseline neutrino oscillation experiment will use a novel ""totally active scintillator design"" for the detector technology and will be exposed to the world's highest power neutrino beam. Building on the first direct observation of muon antineutrino disappearance (that was made by a group founded and led by the PI at the MINOS experiment), tests of CPT symmetry will be performed by looking for differences in the mass squared splittings and mixing angles between neutrinos and antineutrinos. The potential to discover the mass hierarchy is unique to NOvA on the timescale of this proposal due to the long 810 km baseline and the well measured beam of neutrinos and antineutrinos.
This proposal addresses several key challenges in a long-baseline neutrino oscillation experiment with the following tasks: (i) development of a new approach to event energy reconstruction that is expected to have widespread applicability for future neutrino experiments; (ii) undertaking a comprehensive calibration project, exploiting a novel technique developed by the PI, that will be essential to achieving the physics goals; (iii) development of a sophisticated statistical analyses.
The results promised in this proposal surpass the sensitivity to antineutrino oscillation parameters of current 1st generation experiments by at least an order of magnitude, offering wide scope for profound discoveries with implications across disciplines."
Summary
"This proposal addresses major questions in particle physics that are at the forefront of experimental and theoretical physics research today. The results offered would have far-reaching implications in other fields such as cosmology and could help answer some of the big questions such as why the universe contains so much more matter than antimatter. The research objectives of this proposal are to (i) make world-leading tests of CPT symmetry and (ii) discover the neutrino mass hierarchy and search for indications of leptonic CP violation.
The NOvA long-baseline neutrino oscillation experiment will use a novel ""totally active scintillator design"" for the detector technology and will be exposed to the world's highest power neutrino beam. Building on the first direct observation of muon antineutrino disappearance (that was made by a group founded and led by the PI at the MINOS experiment), tests of CPT symmetry will be performed by looking for differences in the mass squared splittings and mixing angles between neutrinos and antineutrinos. The potential to discover the mass hierarchy is unique to NOvA on the timescale of this proposal due to the long 810 km baseline and the well measured beam of neutrinos and antineutrinos.
This proposal addresses several key challenges in a long-baseline neutrino oscillation experiment with the following tasks: (i) development of a new approach to event energy reconstruction that is expected to have widespread applicability for future neutrino experiments; (ii) undertaking a comprehensive calibration project, exploiting a novel technique developed by the PI, that will be essential to achieving the physics goals; (iii) development of a sophisticated statistical analyses.
The results promised in this proposal surpass the sensitivity to antineutrino oscillation parameters of current 1st generation experiments by at least an order of magnitude, offering wide scope for profound discoveries with implications across disciplines."
Max ERC Funding
1 415 848 €
Duration
Start date: 2012-10-01, End date: 2018-09-30
Project acronym ESSOG
Project Extracting science from surveys of our Galaxy
Researcher (PI) James Jeffrey Binney
Host Institution (HI) THE CHANCELLOR, MASTERS AND SCHOLARS OF THE UNIVERSITY OF OXFORD
Country United Kingdom
Call Details Advanced Grant (AdG), PE9, ERC-2012-ADG_20120216
Summary "The goal is to put in place the infrastructure required to extract the promised science for large surveys of our Galaxy that are underway and will culminate in ESA's Cornerstone Mission Gaia. Dynamical models are fundamental to this process because surveys are heavily biased by the Sun's location in the Galaxy. Novel dynamical models will be built and novel methods of fitting them to the data developed. With their help we will be able to constrain the distribution of dark matter in the Galaxy. By modelling the chemical and dynamical evolution of the Galaxy we expect to be able to infer much information about how the Galaxy was assembled, and thus test the prevailing cosmological paradigm. During the grant period we will be applying our tools to ground-based surveys, but the first version of the Gaia Catalogue will become available at the end of the grant period, and our goal is to have everything ready and tested for its prompt exploitation."
Summary
"The goal is to put in place the infrastructure required to extract the promised science for large surveys of our Galaxy that are underway and will culminate in ESA's Cornerstone Mission Gaia. Dynamical models are fundamental to this process because surveys are heavily biased by the Sun's location in the Galaxy. Novel dynamical models will be built and novel methods of fitting them to the data developed. With their help we will be able to constrain the distribution of dark matter in the Galaxy. By modelling the chemical and dynamical evolution of the Galaxy we expect to be able to infer much information about how the Galaxy was assembled, and thus test the prevailing cosmological paradigm. During the grant period we will be applying our tools to ground-based surveys, but the first version of the Gaia Catalogue will become available at the end of the grant period, and our goal is to have everything ready and tested for its prompt exploitation."
Max ERC Funding
1 954 460 €
Duration
Start date: 2013-04-01, End date: 2018-03-31
Project acronym HBAR12
Project Spectroscopy of Trapped Antihydrogen
Researcher (PI) Jeffrey Scott Hangst
Host Institution (HI) AARHUS UNIVERSITET
Country Denmark
Call Details Advanced Grant (AdG), PE2, ERC-2012-ADG_20120216
Summary Antihydrogen is the only stable, neutral antimatter system available for laboratory study. Recently, the ALPHA Collaboration at CERN has succeeded in synthesizing and trapping antihydrogen atoms, storing them for up to 1000 s, and performing the first resonant spectroscopy, using microwaves, on trapped antihydrogen. This last, historic result paves the way for precision microwave and laser spectroscopic measurements using small numbers of trapped antihydrogen atoms. Because of the breakthroughs made in our collaboration, it is now possible, for the first time, to design antimatter spectroscopic experiments that have achievable milestones of precision. These measurements require a next-generation apparatus, known as ALPHA-2, which is the subject of this proposal. The items sought are hardware components and radiation sources to help us to test CPT (charge conjugation, parity, time reversal) symmetry invariance by comparing the spectrum of antihydrogen to that of hydrogen. More generally, we will address the very fundamental question: do matter and antimatter obey the same laws of physics? The Standard Model says that they must, but mystery continues to cloud our understanding of antimatter - as evidenced by the unexplained baryon asymmetry in the universe. ALPHA's experiments offer a unique, high precision, model-independent view into the internal workings of antimatter.
Summary
Antihydrogen is the only stable, neutral antimatter system available for laboratory study. Recently, the ALPHA Collaboration at CERN has succeeded in synthesizing and trapping antihydrogen atoms, storing them for up to 1000 s, and performing the first resonant spectroscopy, using microwaves, on trapped antihydrogen. This last, historic result paves the way for precision microwave and laser spectroscopic measurements using small numbers of trapped antihydrogen atoms. Because of the breakthroughs made in our collaboration, it is now possible, for the first time, to design antimatter spectroscopic experiments that have achievable milestones of precision. These measurements require a next-generation apparatus, known as ALPHA-2, which is the subject of this proposal. The items sought are hardware components and radiation sources to help us to test CPT (charge conjugation, parity, time reversal) symmetry invariance by comparing the spectrum of antihydrogen to that of hydrogen. More generally, we will address the very fundamental question: do matter and antimatter obey the same laws of physics? The Standard Model says that they must, but mystery continues to cloud our understanding of antimatter - as evidenced by the unexplained baryon asymmetry in the universe. ALPHA's experiments offer a unique, high precision, model-independent view into the internal workings of antimatter.
Max ERC Funding
2 136 888 €
Duration
Start date: 2013-05-01, End date: 2018-12-31
Project acronym WATERUNDERTHEICE
Project Where is the water under the Greenland ice sheet?
Researcher (PI) Dorthe Dahl-Jensen
Host Institution (HI) KOBENHAVNS UNIVERSITET
Country Denmark
Call Details Advanced Grant (AdG), PE10, ERC-2009-AdG
Summary Recent analysis of radar-depth sounder data has shown that many areas of the Greenland ice sheet have melt water under the base. The extent of the wet base and distribution of melt water are poorly known. Also lakes under the ice have not been discovered in contrast with those in Antarctica. The effect of the water beneath the ice, however, is well documented: it lubricates the bed and removes the friction between the basal ice and underlying bedrock. The ice with a wet bed flows faster, reacts rapidly to changes in climate and the basal-melt water contributes to the fresh-water supply to the ocean from the Greenland ice sheet. The primary objectives of the project are to map melt water extent of the Greenland ice sheet and its impact by tracing internal layers and analyzing bedrock returns from airborne radio-echo sounding data, and use mapping results in conjunction with ice-sheet and hydrostatic models for the movement of the basal water to predict the ice-sheet s response to climate change. The information derived from deep ice-cores that reach the bed will be used to constrain models. We will also study the basal material (dust, DNA and microbiological material) and bedrock properties from the deep-ice core sites. This will add a further dimension to the study and provide opportunities to look for life under the ice and constrain the age of the Greenland ice sheet. The proposed research is a high risk project because of the difficulty in accessing basal conditions under 3-km of ice with a potential for high payoff science. The team will consist of scientists and engineers with expertise in the palaeoclimate, radar sounding and signal processing, and ice-sheet models.
Summary
Recent analysis of radar-depth sounder data has shown that many areas of the Greenland ice sheet have melt water under the base. The extent of the wet base and distribution of melt water are poorly known. Also lakes under the ice have not been discovered in contrast with those in Antarctica. The effect of the water beneath the ice, however, is well documented: it lubricates the bed and removes the friction between the basal ice and underlying bedrock. The ice with a wet bed flows faster, reacts rapidly to changes in climate and the basal-melt water contributes to the fresh-water supply to the ocean from the Greenland ice sheet. The primary objectives of the project are to map melt water extent of the Greenland ice sheet and its impact by tracing internal layers and analyzing bedrock returns from airborne radio-echo sounding data, and use mapping results in conjunction with ice-sheet and hydrostatic models for the movement of the basal water to predict the ice-sheet s response to climate change. The information derived from deep ice-cores that reach the bed will be used to constrain models. We will also study the basal material (dust, DNA and microbiological material) and bedrock properties from the deep-ice core sites. This will add a further dimension to the study and provide opportunities to look for life under the ice and constrain the age of the Greenland ice sheet. The proposed research is a high risk project because of the difficulty in accessing basal conditions under 3-km of ice with a potential for high payoff science. The team will consist of scientists and engineers with expertise in the palaeoclimate, radar sounding and signal processing, and ice-sheet models.
Max ERC Funding
2 499 999 €
Duration
Start date: 2010-01-01, End date: 2015-12-31
