Project acronym AxScale
Project Axions and relatives across different mass scales
Researcher (PI) Babette DoeBRICH
Host Institution (HI) EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH
Country Switzerland
Call Details Starting Grant (StG), PE2, ERC-2018-STG
Summary Pseudoscalar QCD axions and axion-like Particles (ALPs) are an excellent candidate for Dark Matter or can act as a mediator particle for Dark Matter. Since the discovery of the Higgs boson, we know that fundamental scalars exist and it is timely to explore the Axion/ALP parameter space more intensively. A look at the allowed axion/ALP parameter space makes it clear that these might exist at low mass (below few eV), as (part of) Dark Matter. Alternatively they might exist at higher mass, above roughly the MeV scale, potentially as a Dark Matter mediator particle. AxScale explores parts of these different mass regions, with complementary techniques but with one research team.
Firstly, with RADES, it develops a novel concept for a filter-like cavity for the search of QCD axion Dark matter at a few tens of a micro-eV. Dark Matter Axions can be discovered by their resonant conversion in that cavity embedded in a strong magnetic field. The `classical axion window' has recently received much interest from cosmological model-building and I will implement a novel cavity concept that will allow to explore this Dark Matter parameter region.
Secondly, AxScale searches for axions and ALPs using the NA62 detector at CERN's SPS. Especially the mass region above a few MeV can be efficiently searched by the use of a proton fixed-target facility. During nominal data taking NA62 investigates a Kaon beam. NA62 can also run in a mode in which its primary proton beam is fully dumped. With the resulting high interaction rate, the existence of weakly coupled particles can be efficiently probed. Thus, searches for ALPs from Kaon decays as well as from production in dumped protons with NA62 are foreseen in AxScale. More generally, NA62 can look for a plethora of `Dark Sector' particles with recorded and future data. With the AxScale program I aim at maximizing the reach of NA62 for these new physics models.
Summary
Pseudoscalar QCD axions and axion-like Particles (ALPs) are an excellent candidate for Dark Matter or can act as a mediator particle for Dark Matter. Since the discovery of the Higgs boson, we know that fundamental scalars exist and it is timely to explore the Axion/ALP parameter space more intensively. A look at the allowed axion/ALP parameter space makes it clear that these might exist at low mass (below few eV), as (part of) Dark Matter. Alternatively they might exist at higher mass, above roughly the MeV scale, potentially as a Dark Matter mediator particle. AxScale explores parts of these different mass regions, with complementary techniques but with one research team.
Firstly, with RADES, it develops a novel concept for a filter-like cavity for the search of QCD axion Dark matter at a few tens of a micro-eV. Dark Matter Axions can be discovered by their resonant conversion in that cavity embedded in a strong magnetic field. The `classical axion window' has recently received much interest from cosmological model-building and I will implement a novel cavity concept that will allow to explore this Dark Matter parameter region.
Secondly, AxScale searches for axions and ALPs using the NA62 detector at CERN's SPS. Especially the mass region above a few MeV can be efficiently searched by the use of a proton fixed-target facility. During nominal data taking NA62 investigates a Kaon beam. NA62 can also run in a mode in which its primary proton beam is fully dumped. With the resulting high interaction rate, the existence of weakly coupled particles can be efficiently probed. Thus, searches for ALPs from Kaon decays as well as from production in dumped protons with NA62 are foreseen in AxScale. More generally, NA62 can look for a plethora of `Dark Sector' particles with recorded and future data. With the AxScale program I aim at maximizing the reach of NA62 for these new physics models.
Max ERC Funding
1 134 375 €
Duration
Start date: 2018-11-01, End date: 2023-10-31
Project acronym BARB
Project Biomedical Applications of Radioactive ion Beams
Researcher (PI) Marco DURANTE
Host Institution (HI) GSI HELMHOLTZZENTRUM FUER SCHWERIONENFORSCHUNG GMBH
Country Germany
Call Details Advanced Grant (AdG), PE2, ERC-2019-ADG
Summary Cancer remains one of the main causes of death worldwide. In 2018, >50% cancer patients in Europe underwent radiotherapy. While over 80% were treated using high-energy X-rays, the number of patients receiving accelerated protons or heavy ions (charged particle therapy: CPT) is rapidly growing, with nearly 200,000 patients treated up till now. Although CPT offers a better depth-dose distribution compared to common X-ray based techniques, range uncertainty and poor image guidance still limit its application.
Improving accuracy is key to broadening the applicability of CPT. In BARB, we will open a new paradigm in the clinical use of CPT by using high-intensity radioactive ion beams (RIB), produced at GSI/FAIR-phase-0 in Darmstadt, for simultaneous treatment and visualization. This will reduce range uncertainty and extend the applicability of CPT to treatment of small lesions (e.g. metastasis and heart ventricles) with unprecedented precision.
The Facility for Antiprotons and Ion Research (FAIR) is currently under construction at GSI. RIB are one of the main tools for basic nuclear physics studies in the new facility. As part of the ongoing FAIR-phase-0, an intensity upgrade will increase the light ion currents in the existing SIS18 synchrotron. Within this project BARB, we will study four b+ emitters (10,11C, and 14,15O) and build an innovative hybrid detector for online positron emission tomography (PET) and g-ray imaging. This novel detector will acquire both prompt g-rays during the beam-on phase of the pulsed synchrotron beam delivery, and the delayed emission from b+ annihilation during the pulse intervals. The technique will be further validated in vivo by applying it to treatment of small tumors in a mouse model.
BARB will exploit the potential of the Bragg peak in medicine. The project will tweak RIB production in nuclear physics and validate the therapeutic potential of RIB therapy in vivo by empowering simultaneous treatment and visualization.
Summary
Cancer remains one of the main causes of death worldwide. In 2018, >50% cancer patients in Europe underwent radiotherapy. While over 80% were treated using high-energy X-rays, the number of patients receiving accelerated protons or heavy ions (charged particle therapy: CPT) is rapidly growing, with nearly 200,000 patients treated up till now. Although CPT offers a better depth-dose distribution compared to common X-ray based techniques, range uncertainty and poor image guidance still limit its application.
Improving accuracy is key to broadening the applicability of CPT. In BARB, we will open a new paradigm in the clinical use of CPT by using high-intensity radioactive ion beams (RIB), produced at GSI/FAIR-phase-0 in Darmstadt, for simultaneous treatment and visualization. This will reduce range uncertainty and extend the applicability of CPT to treatment of small lesions (e.g. metastasis and heart ventricles) with unprecedented precision.
The Facility for Antiprotons and Ion Research (FAIR) is currently under construction at GSI. RIB are one of the main tools for basic nuclear physics studies in the new facility. As part of the ongoing FAIR-phase-0, an intensity upgrade will increase the light ion currents in the existing SIS18 synchrotron. Within this project BARB, we will study four b+ emitters (10,11C, and 14,15O) and build an innovative hybrid detector for online positron emission tomography (PET) and g-ray imaging. This novel detector will acquire both prompt g-rays during the beam-on phase of the pulsed synchrotron beam delivery, and the delayed emission from b+ annihilation during the pulse intervals. The technique will be further validated in vivo by applying it to treatment of small tumors in a mouse model.
BARB will exploit the potential of the Bragg peak in medicine. The project will tweak RIB production in nuclear physics and validate the therapeutic potential of RIB therapy in vivo by empowering simultaneous treatment and visualization.
Max ERC Funding
2 500 000 €
Duration
Start date: 2020-10-01, End date: 2025-09-30
Project acronym BEAM-EDM
Project Unique Method for a Neutron Electric Dipole Moment Search using a Pulsed Beam
Researcher (PI) Florian Michael PIEGSA
Host Institution (HI) UNIVERSITAET BERN
Country Switzerland
Call Details Starting Grant (StG), PE2, ERC-2016-STG
Summary My research encompasses the application of novel methods and strategies in the field of low energy particle physics. The goal of the presented program is to lead an independent and highly competitive experiment to search for a CP violating neutron electric dipole moment (nEDM), as well as for new exotic interactions using highly sensitive neutron and proton spin resonance techniques.
The measurement of the nEDM is considered to be one of the most important fundamental physics experiments at low energy. It represents a promising route for finding new physics beyond the standard model (SM) and describes an important search for new sources of CP violation in order to understand the observed large baryon asymmetry in our universe. The main project will follow a novel concept based on my original idea, which plans to employ a pulsed neutron beam at high intensity instead of the established use of storable ultracold neutrons. This complementary and potentially ground-breaking method provides the possibility to distinguish between the signal due to a nEDM and previously limiting systematic effects, and should lead to an improved result compared to the present best nEDM beam experiment. The findings of these investigations will be of paramount importance and will form the cornerstone for the success of the full-scale experiment intended for the European Spallation Source. A second scientific question will be addressed by performing spin precession experiments searching for exotic short-range interactions and associated light bosons. This is a vivid field of research motivated by various extensions to the SM. The goal of these measurements, using neutrons and protons, is to search for additional interactions such new bosons mediate between ordinary particles.
Both topics describe ambitious and unique efforts. They use related techniques, address important questions in fundamental physics, and have the potential of substantial scientific implications and high-impact results.
Summary
My research encompasses the application of novel methods and strategies in the field of low energy particle physics. The goal of the presented program is to lead an independent and highly competitive experiment to search for a CP violating neutron electric dipole moment (nEDM), as well as for new exotic interactions using highly sensitive neutron and proton spin resonance techniques.
The measurement of the nEDM is considered to be one of the most important fundamental physics experiments at low energy. It represents a promising route for finding new physics beyond the standard model (SM) and describes an important search for new sources of CP violation in order to understand the observed large baryon asymmetry in our universe. The main project will follow a novel concept based on my original idea, which plans to employ a pulsed neutron beam at high intensity instead of the established use of storable ultracold neutrons. This complementary and potentially ground-breaking method provides the possibility to distinguish between the signal due to a nEDM and previously limiting systematic effects, and should lead to an improved result compared to the present best nEDM beam experiment. The findings of these investigations will be of paramount importance and will form the cornerstone for the success of the full-scale experiment intended for the European Spallation Source. A second scientific question will be addressed by performing spin precession experiments searching for exotic short-range interactions and associated light bosons. This is a vivid field of research motivated by various extensions to the SM. The goal of these measurements, using neutrons and protons, is to search for additional interactions such new bosons mediate between ordinary particles.
Both topics describe ambitious and unique efforts. They use related techniques, address important questions in fundamental physics, and have the potential of substantial scientific implications and high-impact results.
Max ERC Funding
1 404 062 €
Duration
Start date: 2017-04-01, End date: 2022-03-31
Project acronym Beauty2Charm
Project Precision tests of the Standard Model using Beauty to Charm decays
Researcher (PI) Conor Thomas Fitzpatrick
Host Institution (HI) THE UNIVERSITY OF MANCHESTER
Country United Kingdom
Call Details Starting Grant (StG), PE2, ERC-2019-STG
Summary The present matter-antimatter asymmetry of the universe cannot be explained by the Standard Model (SM) of particle physics. I propose to look for the presence of new physics beyond the SM in Charge-Parity (CP) asymmetries using beauty mesons decaying to charmed mesons (Beauty2Charm). A unique feature of these decays is that the SM contribution can be precisely measured using relations between ten decay modes all of which can be measured with in a coherent manner at a single experiment: LHCb at the Large Hadron Collier (LHC). The proposal will make measurements of ten branching ratios and eight analyses sensitive to CP violation using data collected by LHCb in order to test these relations. CP asymmetries larger than a few percent would be an unambiguous signal of the presence of new physics. In order to make these measurements at the required level of precision, I will lead a major upgrade to the way that the LHCb experiment selects proton proton collisions and for which I have laid the conceptual foundations. Real-Time Analysis will enable a dramatic increase in the the efficiency and signal yield of the decay modes relevant to this proposal, and reduce systematic uncertainties. To test and commission this upgrade I will lead the first ever measurements of beauty hadron production using final states without leptons. The experience gained in the commissioning phase will result in increased efficiencies for the CP sensitive channels leading to the world's most precise measurements and world-leading sensitivity to new physics.
Summary
The present matter-antimatter asymmetry of the universe cannot be explained by the Standard Model (SM) of particle physics. I propose to look for the presence of new physics beyond the SM in Charge-Parity (CP) asymmetries using beauty mesons decaying to charmed mesons (Beauty2Charm). A unique feature of these decays is that the SM contribution can be precisely measured using relations between ten decay modes all of which can be measured with in a coherent manner at a single experiment: LHCb at the Large Hadron Collier (LHC). The proposal will make measurements of ten branching ratios and eight analyses sensitive to CP violation using data collected by LHCb in order to test these relations. CP asymmetries larger than a few percent would be an unambiguous signal of the presence of new physics. In order to make these measurements at the required level of precision, I will lead a major upgrade to the way that the LHCb experiment selects proton proton collisions and for which I have laid the conceptual foundations. Real-Time Analysis will enable a dramatic increase in the the efficiency and signal yield of the decay modes relevant to this proposal, and reduce systematic uncertainties. To test and commission this upgrade I will lead the first ever measurements of beauty hadron production using final states without leptons. The experience gained in the commissioning phase will result in increased efficiencies for the CP sensitive channels leading to the world's most precise measurements and world-leading sensitivity to new physics.
Max ERC Funding
1 450 020 €
Duration
Start date: 2020-09-01, End date: 2025-08-31
Project acronym BEC-NETWORKS
Project Networks of coupled photon Bose-Einstein condensates: when condensation becomes a computation
Researcher (PI) Jan KLAERS
Host Institution (HI) UNIVERSITEIT TWENTE
Country Netherlands
Call Details Consolidator Grant (CoG), PE2, ERC-2020-COG
Summary Despite large advances in both algorithms and computer technology, even typical instances of computationally hard problems are too difficult to be solved on today’s computers. Unconventional computational devices that break with the usual paradigms of digital electronic computers can help to overcome these limitations. In this project, a network of coupled photon Bose-Einstein condensates will be developed and used as experimental platform to perform ultrafast simulations of classical spin systems. Specifically, the network will be capable of solving the ground-state problem in spin glasses (disordered magnets). The latter constitutes a well-known combinatorial problem that can be mapped mathematically to many other computationally hard problems in machine learning, logistics, computer chip design and DNA sequencing. In a proof-of-principle experiment, I aim to demonstrate that the proposed spin glass simulator performs this computationally hard optimisation problem significantly faster than any other computer today. I have pioneered the Bose-Einstein condensation of photons in optical microcavities, which has enabled us to investigate this genuine quantum-mechanical effect with all-optical methods. In a recent work of my group, we experimentally demonstrate controllable phase relations between photon Bose-Einstein condensates in an optical microcavity. The investigated device realises an optical analogue of a Josephson junction. Similar to a transistor for electronics, a controllable photonic Josephson junction represents the key component for ultrafast optical spin glass simulation and, thus, is the crucial basis for the proposed project. The BEC-NETWORKS project will be the main research project of my research group at the University of Twente.
Summary
Despite large advances in both algorithms and computer technology, even typical instances of computationally hard problems are too difficult to be solved on today’s computers. Unconventional computational devices that break with the usual paradigms of digital electronic computers can help to overcome these limitations. In this project, a network of coupled photon Bose-Einstein condensates will be developed and used as experimental platform to perform ultrafast simulations of classical spin systems. Specifically, the network will be capable of solving the ground-state problem in spin glasses (disordered magnets). The latter constitutes a well-known combinatorial problem that can be mapped mathematically to many other computationally hard problems in machine learning, logistics, computer chip design and DNA sequencing. In a proof-of-principle experiment, I aim to demonstrate that the proposed spin glass simulator performs this computationally hard optimisation problem significantly faster than any other computer today. I have pioneered the Bose-Einstein condensation of photons in optical microcavities, which has enabled us to investigate this genuine quantum-mechanical effect with all-optical methods. In a recent work of my group, we experimentally demonstrate controllable phase relations between photon Bose-Einstein condensates in an optical microcavity. The investigated device realises an optical analogue of a Josephson junction. Similar to a transistor for electronics, a controllable photonic Josephson junction represents the key component for ultrafast optical spin glass simulation and, thus, is the crucial basis for the proposed project. The BEC-NETWORKS project will be the main research project of my research group at the University of Twente.
Max ERC Funding
2 000 000 €
Duration
Start date: 2021-02-01, End date: 2026-01-31
Project acronym BetaDropNMR
Project Ultra-sensitive NMR in liquids
Researcher (PI) Magdalena Kowalska-Wyrowska
Host Institution (HI) EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH
Country Switzerland
Call Details Starting Grant (StG), PE2, ERC-2014-STG
Summary "The nuclear magnetic resonance spectroscopy (NMR) is a versatile and powerful tool, especially in chemistry and in biology. However, its limited sensitivity and small amount of suitable probe nuclei pose severe constraints on the systems that may be explored.
This project aims at overcoming the above limitations by giving NMR an ultra-high sensitivity and by enlarging the NMR ""toolbox"" to dozens of nuclei across the periodic table. This will be achieved by applying the β-NMR method to the soft matter samples. The method relies on anisotropic emission of β particles in the decay of highly spin-polarized nuclei. This feature results in 10 orders of magnitude more sensitivity compared to conventional NMR and makes it applicable to elements which are otherwise difficult to investigate spectroscopically. β-NMR has been successfully applied in nuclear physics and material science in solid samples and high-vacuum environments, but never before to liquid samples placed in atmospheric pressure. With this novel approach I want to create a new universal and extremely sensitive tool to study various problems in biochemistry.
The first questions which I envisage addressing with this ground-breaking and versatile method concern the interaction of essential metal ions, which are spectroscopically silent in most techniques, Mg2+, Cu+, and Zn2+, with proteins and nucleic acids. The importance of these studies is well motivated by the fact that half of the proteins in our human body contain metal ions, but their interaction mechanism and factors influencing it are still not fully understood. In this respect NMR spectroscopy is of great help: it provides information on the structure, dynamics, and chemical properties of the metal complexes, by revealing the coordination number, oxidation state, bonding situation and electronic configuration of the interacting metal.
My long-term aim is to establish a firm basis for β-NMR in soft matter studies in biology, chemistry and physics."
Summary
"The nuclear magnetic resonance spectroscopy (NMR) is a versatile and powerful tool, especially in chemistry and in biology. However, its limited sensitivity and small amount of suitable probe nuclei pose severe constraints on the systems that may be explored.
This project aims at overcoming the above limitations by giving NMR an ultra-high sensitivity and by enlarging the NMR ""toolbox"" to dozens of nuclei across the periodic table. This will be achieved by applying the β-NMR method to the soft matter samples. The method relies on anisotropic emission of β particles in the decay of highly spin-polarized nuclei. This feature results in 10 orders of magnitude more sensitivity compared to conventional NMR and makes it applicable to elements which are otherwise difficult to investigate spectroscopically. β-NMR has been successfully applied in nuclear physics and material science in solid samples and high-vacuum environments, but never before to liquid samples placed in atmospheric pressure. With this novel approach I want to create a new universal and extremely sensitive tool to study various problems in biochemistry.
The first questions which I envisage addressing with this ground-breaking and versatile method concern the interaction of essential metal ions, which are spectroscopically silent in most techniques, Mg2+, Cu+, and Zn2+, with proteins and nucleic acids. The importance of these studies is well motivated by the fact that half of the proteins in our human body contain metal ions, but their interaction mechanism and factors influencing it are still not fully understood. In this respect NMR spectroscopy is of great help: it provides information on the structure, dynamics, and chemical properties of the metal complexes, by revealing the coordination number, oxidation state, bonding situation and electronic configuration of the interacting metal.
My long-term aim is to establish a firm basis for β-NMR in soft matter studies in biology, chemistry and physics."
Max ERC Funding
1 500 000 €
Duration
Start date: 2015-10-01, End date: 2022-03-31
Project acronym BINGO
Project Bi-Isotope 0n2b Next Generation Observatory
Researcher (PI) Claudia NONES
Host Institution (HI) COMMISSARIAT A L ENERGIE ATOMIQUE ET AUX ENERGIES ALTERNATIVES
Country France
Call Details Consolidator Grant (CoG), PE2, ERC-2019-COG
Summary BINGO will set the grounds for a large-scale bolometric experiment searching for neutrinoless double beta decay with a background index of about 10-5 counts/(keV kg y) and with very high energy resolution – of the order of 1.5‰ – in the region of interest. These features will enable a search for lepton number violation with unprecedented sensitivity. The BINGO approach can lead to the demonstration of the Majorana nature of neutrino even in the unfavourable case of direct ordering of neutrino masses.
BINGO is based on luminescent bolometers for the rejection of the dominant alpha surface background. It will focus on two extremely promising isotopes – 100Mo and 130Te – that have complementary merits and deserve to be both considered for future large-scale searches.
The project will bring three original ingredients to the well-established technology of hybrid heat-light bolometers: i) the light-detector sensitivity will be increased by an order of magnitude thanks to Neganov-Luke amplification; (ii) a revolutionary detector assembly will reduce the total surface radioactivity contribution by at least one order of magnitude; (iii) for the first time in an array of macrobolometers, an internal active shield, based on ultrapure ZnWO4 scintillators with bolometric light readout, will suppress the external gamma background. These challenging technologies will be extensively tested in a two-isotope demonstrator, dubbed MINI‑BINGO, which will be located in an underground laboratory in a dedicated cryogenic infrastructure built with ERC funds.
The BINGO approach can be implemented in the next-generation search CUPID, a proposed follow up of the CUORE experiment. BINGO can improve dramatically the sensitivity of CUPID, using two isotopes at the same time and providing the demonstration of its background goal. Subsequently, the intrinsic modularity of the bolometric technique would make sensible to proceed to further expansions, capable of penetrating the direct-ordering band.
Summary
BINGO will set the grounds for a large-scale bolometric experiment searching for neutrinoless double beta decay with a background index of about 10-5 counts/(keV kg y) and with very high energy resolution – of the order of 1.5‰ – in the region of interest. These features will enable a search for lepton number violation with unprecedented sensitivity. The BINGO approach can lead to the demonstration of the Majorana nature of neutrino even in the unfavourable case of direct ordering of neutrino masses.
BINGO is based on luminescent bolometers for the rejection of the dominant alpha surface background. It will focus on two extremely promising isotopes – 100Mo and 130Te – that have complementary merits and deserve to be both considered for future large-scale searches.
The project will bring three original ingredients to the well-established technology of hybrid heat-light bolometers: i) the light-detector sensitivity will be increased by an order of magnitude thanks to Neganov-Luke amplification; (ii) a revolutionary detector assembly will reduce the total surface radioactivity contribution by at least one order of magnitude; (iii) for the first time in an array of macrobolometers, an internal active shield, based on ultrapure ZnWO4 scintillators with bolometric light readout, will suppress the external gamma background. These challenging technologies will be extensively tested in a two-isotope demonstrator, dubbed MINI‑BINGO, which will be located in an underground laboratory in a dedicated cryogenic infrastructure built with ERC funds.
The BINGO approach can be implemented in the next-generation search CUPID, a proposed follow up of the CUORE experiment. BINGO can improve dramatically the sensitivity of CUPID, using two isotopes at the same time and providing the demonstration of its background goal. Subsequently, the intrinsic modularity of the bolometric technique would make sensible to proceed to further expansions, capable of penetrating the direct-ordering band.
Max ERC Funding
2 420 370 €
Duration
Start date: 2020-10-01, End date: 2025-09-30
Project acronym BinGraSp
Project Modeling the Gravitational Spectrum of Neutron Star Binaries
Researcher (PI) Sebastiano Bernuzzi
Host Institution (HI) FRIEDRICH-SCHILLER-UNIVERSITAT JENA
Country Germany
Call Details Starting Grant (StG), PE2, ERC-2016-STG
Summary The most energetic electromagnetic phenomena in the Universe are believed to be powered by the collision of two neutron stars, the smallest and densest stars on which surface gravity is about 2 billion times stronger than gravity on Earth. However, a definitive identification of neutron star mergers as central engines for short-gamma-ray bursts and kilonovae transients is possible only by direct gravitational-wave observations. The latter provide us with unique information on neutron stars' masses, radii, and spins, including the possibility to set the strongest observational constraints on the unknown equation-of-state of matter at supranuclear densities.
Neutron stars binary mergers are among the main targets for ground-based gravitational-wave interferometers like Advanced LIGO and Virgo, which start operations this year. The astrophysical data analysis of the signals emitted by these sources requires the availability of accurate waveform models, which are missing to date. Hence, the theoretical understanding of the gravitational spectrum is a necessary and urgent step for the development of a gravitational-based astrophysics in the next years.
This project aims at developing, for the first time, a precise theoretical model for the complete gravitational spectrum of neutron star binaries, including the merger and postmerger stages of the coalescence process. Building on the PI's unique expertise and track record, the proposed research exploits synergy between analytical and numerical methods in General Relativity. Results from state of the art nonlinear 3D numerical relativity simulations will be combined with the most advanced analytical framework for the relativistic two-body problem. The model developed here will be used in the first gravitational-wave observations and will dramatically impact multimessenger astrophysics.
Summary
The most energetic electromagnetic phenomena in the Universe are believed to be powered by the collision of two neutron stars, the smallest and densest stars on which surface gravity is about 2 billion times stronger than gravity on Earth. However, a definitive identification of neutron star mergers as central engines for short-gamma-ray bursts and kilonovae transients is possible only by direct gravitational-wave observations. The latter provide us with unique information on neutron stars' masses, radii, and spins, including the possibility to set the strongest observational constraints on the unknown equation-of-state of matter at supranuclear densities.
Neutron stars binary mergers are among the main targets for ground-based gravitational-wave interferometers like Advanced LIGO and Virgo, which start operations this year. The astrophysical data analysis of the signals emitted by these sources requires the availability of accurate waveform models, which are missing to date. Hence, the theoretical understanding of the gravitational spectrum is a necessary and urgent step for the development of a gravitational-based astrophysics in the next years.
This project aims at developing, for the first time, a precise theoretical model for the complete gravitational spectrum of neutron star binaries, including the merger and postmerger stages of the coalescence process. Building on the PI's unique expertise and track record, the proposed research exploits synergy between analytical and numerical methods in General Relativity. Results from state of the art nonlinear 3D numerical relativity simulations will be combined with the most advanced analytical framework for the relativistic two-body problem. The model developed here will be used in the first gravitational-wave observations and will dramatically impact multimessenger astrophysics.
Max ERC Funding
1 432 301 €
Duration
Start date: 2017-10-01, End date: 2022-09-30
Project acronym BlackHoleMaps
Project Mapping gravitational waves from collisions of black holes
Researcher (PI) Mark Douglas Hannam
Host Institution (HI) CARDIFF UNIVERSITY
Country United Kingdom
Call Details Consolidator Grant (CoG), PE2, ERC-2014-CoG
Summary Breakthroughs in numerical relativity in 2005 gave us unprecedented access to the strong-field regime of general relativity, making possible solutions of the full nonlinear Einstein equations for the merger of two black holes. Numerical relativity is also crucial to study fundamental physics with gravitational-wave (GW) observations: numerical solutions allow us to construct models that will be essential to extract physical information from observations in data from Advanced LIGO and Virgo, which will operate from late 2015. Complete signal models will allow us to follow up our first theoretical predictions of the nature of black-hole mergers with their first observational measurements.
The goal of this project is to advance numerical-relativity methods, deepen our understanding of black-hole mergers, and map the parameter space of binary configurations with the most comprehensive and systematic set of numerical calculations performed to date, in order to produce a complete GW signal model. Central to this problem is the purely general-relativistic effect of orbital precession. The inclusion of precession in waveform models is the most challenging and urgent theoretical problem in the build-up to GW astronomy. Simulations must cover a seven-dimensional parameter space of binary configurations, but their computational cost makes a naive covering unfeasible. This project capitalizes on a breakthrough preliminary model produced by my team in 2013, with the pragmatic goal of focussing on the physics that will be measurable with GW detectors over the next five years.
My team at Cardiff is uniquely placed to tackle this problem. Since 2005 I have been at the forefront of black-hole simulations and waveform modelling, and the Cardiff group is a world leader in analysis of GW detector data. This project will consolidate my team to make breakthroughs in strong-field gravity, astrophysics, fundamental physics and cosmology using GW observations.
Summary
Breakthroughs in numerical relativity in 2005 gave us unprecedented access to the strong-field regime of general relativity, making possible solutions of the full nonlinear Einstein equations for the merger of two black holes. Numerical relativity is also crucial to study fundamental physics with gravitational-wave (GW) observations: numerical solutions allow us to construct models that will be essential to extract physical information from observations in data from Advanced LIGO and Virgo, which will operate from late 2015. Complete signal models will allow us to follow up our first theoretical predictions of the nature of black-hole mergers with their first observational measurements.
The goal of this project is to advance numerical-relativity methods, deepen our understanding of black-hole mergers, and map the parameter space of binary configurations with the most comprehensive and systematic set of numerical calculations performed to date, in order to produce a complete GW signal model. Central to this problem is the purely general-relativistic effect of orbital precession. The inclusion of precession in waveform models is the most challenging and urgent theoretical problem in the build-up to GW astronomy. Simulations must cover a seven-dimensional parameter space of binary configurations, but their computational cost makes a naive covering unfeasible. This project capitalizes on a breakthrough preliminary model produced by my team in 2013, with the pragmatic goal of focussing on the physics that will be measurable with GW detectors over the next five years.
My team at Cardiff is uniquely placed to tackle this problem. Since 2005 I have been at the forefront of black-hole simulations and waveform modelling, and the Cardiff group is a world leader in analysis of GW detector data. This project will consolidate my team to make breakthroughs in strong-field gravity, astrophysics, fundamental physics and cosmology using GW observations.
Max ERC Funding
1 998 009 €
Duration
Start date: 2015-10-01, End date: 2022-03-31
Project acronym BoostDiscovery
Project Boosting the discovery using τs in the ATLAS detector at the Large Hadron Collider
Researcher (PI) Liron Barak
Host Institution (HI) TEL AVIV UNIVERSITY
Country Israel
Call Details Starting Grant (StG), PE2, ERC-2020-STG
Summary Almost ten years into the highly successful program both in ATLAS and CMS, our understanding of the Standard Model (SM) of particle physics has deepened. Nonetheless, what lies beyond the SM remains one of the most urgent questions of physics in the 21st century. To move forward, one must think outside of the box and leap into uncharted waters. Searches today are aiming at the high-energy frontier, while low-mass resonances are mostly overlooked by the Large Hadron Collider (LHC). Consequently, far-reaching hints of new physics may silentlyhide in the data. Motivated by numerous New Physics (NP) scenarios that often predict light states, such as extended Higgs sectors, axion physics, or dark sector models, among others, the PI will develop new techniques to search for low-mass resonances decaying into two collimated low-pT hadronic τ leptons. τs, being the heaviest, third-generation leptons, provide a unique experimental opportunity to search for low-lying states that would otherwise go undetected. In particular, novel methods to identify boosted hadronic τ+τ− pairs will be established. These techniques will then be used to pave a new path towards discovery of low-mass resonances produced through various production modes. As part of this proposal, the PI will also develop new trigger-level capabilities to further extend the reach of this program at Run-3. As a former leader of the ATLAS Beyond the Standard Model physics group, and current leader of low-mass resonance searches, the PI is ideally positioned to establish a strong research team and take this project to completion, laying the groundwork for the discovery of new physics beyond the SM.
Summary
Almost ten years into the highly successful program both in ATLAS and CMS, our understanding of the Standard Model (SM) of particle physics has deepened. Nonetheless, what lies beyond the SM remains one of the most urgent questions of physics in the 21st century. To move forward, one must think outside of the box and leap into uncharted waters. Searches today are aiming at the high-energy frontier, while low-mass resonances are mostly overlooked by the Large Hadron Collider (LHC). Consequently, far-reaching hints of new physics may silentlyhide in the data. Motivated by numerous New Physics (NP) scenarios that often predict light states, such as extended Higgs sectors, axion physics, or dark sector models, among others, the PI will develop new techniques to search for low-mass resonances decaying into two collimated low-pT hadronic τ leptons. τs, being the heaviest, third-generation leptons, provide a unique experimental opportunity to search for low-lying states that would otherwise go undetected. In particular, novel methods to identify boosted hadronic τ+τ− pairs will be established. These techniques will then be used to pave a new path towards discovery of low-mass resonances produced through various production modes. As part of this proposal, the PI will also develop new trigger-level capabilities to further extend the reach of this program at Run-3. As a former leader of the ATLAS Beyond the Standard Model physics group, and current leader of low-mass resonance searches, the PI is ideally positioned to establish a strong research team and take this project to completion, laying the groundwork for the discovery of new physics beyond the SM.
Max ERC Funding
1 420 000 €
Duration
Start date: 2021-01-01, End date: 2025-12-31
