Computational Cosmology and Gravitational Waves
CoCoS aims to enhance the accuracy of gravitational wave power spectrum calculations from BSM phase transitions to 10-20% using innovative simulation techniques, enabling groundbreaking discoveries in particle physics.
Projectdetails
Introduction
The discovery of gravitational waves by the LIGO and Virgo collaborations opened a new window to the Universe. Space-based gravitational wave detectors, such as the LISA mission, enable an exciting opportunity: using gravitational waves from the very early Universe in the search for beyond-the-Standard-Model (BSM) particle physics.
Importance of Phase Transitions
The LISA science case identifies first order phase transitions as the most promising source of cosmological gravitational waves. There are no phase transitions in the Standard Model, and observation of a phase transition would be revolutionary: a direct signal of BSM physics.
It is absolutely necessary to have accurate and reliable theoretical control of the gravitational wave production in BSM phase transitions in order to fully realize the science potential of the observations.
Goals of CoCoS
The overarching goal of CoCoS is to calculate, for a given BSM theory, the resulting gravitational wave power spectrum to 10–20% accuracy. This is more than an order of magnitude better than the current state of the art, where accuracy is limited by uncertainties inherent in standard perturbative approaches.
In CoCoS, these problems are avoided by using several novel and state-of-the-art simulation techniques.
Mechanism of Phase Transitions
A first order phase transition in the early Universe proceeds through:
- Supercooling
- Critical bubble nucleation
- Growth and collision of the bubbles
Bubbles cause pressure waves, shocks, and turbulence, which remain long after the transition has completed and create gravitational waves.
In CoCoS, the stages of the phase transitions are studied with innovative computational methods:
- Effective field theory approach, which optimally combines perturbation theory and lattice simulations
- State-of-the-art viscous relativistic hydrodynamics
Synergy with LHC and LISA
The high-luminosity LHC and LISA will be operational at the same time, searching for complementary aspects of new physics. The accuracy reached in CoCoS is necessary to fully utilize this synergy.
Financiële details & Tijdlijn
Financiële details
Subsidiebedrag | € 2.446.893 |
Totale projectbegroting | € 2.446.893 |
Tijdlijn
Startdatum | 1-9-2024 |
Einddatum | 31-8-2029 |
Subsidiejaar | 2024 |
Partners & Locaties
Projectpartners
- HELSINGIN YLIOPISTOpenvoerder
Land(en)
Vergelijkbare projecten binnen European Research Council
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Holography in the Gravitational Wave Era
This project aims to enhance understanding of quantum matter and gravity through holography, focusing on cosmological phase transitions, neutron star mergers, and spacetime singularities.
Cosmological phase transitions of Standard Model Matter and their gravitational wave signatures
This project aims to enhance understanding of early Universe phase transitions through large-scale lattice simulations of hot matter, utilizing advanced algorithms and machine learning to analyze gravitational wave signatures.
Towards constraining the pillars of our cosmological model using combined probes
The PiCo project aims to refine the ΛCDM cosmological model by employing advanced statistical methods to analyze galaxy clustering and CMB data, addressing primordial fluctuations and cosmic acceleration.
Loop Corrections from the Theory of Motives
LoCoMotive aims to enhance the understanding of scattering amplitudes through modern mathematics, improving quantum corrections and providing predictions for high-energy experiments like the LHC.
The key to precise and accurate cosmology: Simulating the physics that shapes gaseous haloes
The project aims to enhance precision cosmology by developing advanced simulations of galaxy formation and SMBH feedback, providing reliable models and observational tests for cosmological analyses.
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