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.
Projectdetails
Introduction
The Standard Model of particle physics is the theory of the strong, electromagnetic, and weak interactions, describing the elementary particles of nature at microscopic length scales. The precise theoretical predictions of the Standard Model are put to the test in contemporary and future high-energy particle collider experiments.
Historical Context
Besides explaining matter around us in the present, the Standard Model also predicts the distant past of our Universe. It describes the behavior of particles at temperatures as high as it used to be just fractions of seconds after the Big Bang. The relics of the cosmological phase transitions in this era of our Universe are actively sought via their gravitational wave signatures in current and future observatories.
Computational Challenges
Most of the relevant features of hot Standard Model matter are non-perturbative, implying that a first-principles treatment is only possible via computer simulations of the underlying field theories on space-time lattices. This proposal will use such large-scale lattice field theory simulations to determine the properties of cosmological phase transitions and thus significantly improve our understanding of how the early Universe cooled down and became the world that we know today.
Specific Goals
Specifically, we will:
- Perform the first full physical simulations of hot, electrically charged strongly interacting matter.
- Substantially improve on existing calculations of the weak and electromagnetic interactions at high temperature.
Methodology
The computational effort of the combined treatment of these forces is immense. We will overcome these challenges by employing:
- Optimized algorithms
- Cutting-edge technologies including machine learning methods
Expected Outcomes
For both systems, we will determine the nature of the high-temperature transition and analyze the induced gravitational wave spectrum. Our results will provide the most accurate description of Standard Model matter in the early Universe.
Financiële details & Tijdlijn
Financiële details
Subsidiebedrag | € 1.839.769 |
Totale projectbegroting | € 1.839.769 |
Tijdlijn
Startdatum | 1-1-2025 |
Einddatum | 31-12-2029 |
Subsidiejaar | 2025 |
Partners & Locaties
Projectpartners
- EOTVOS LORAND TUDOMANYEGYETEMpenvoerder
- UNIVERSITAET BIELEFELD
Land(en)
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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.
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.
New physics in parity violation. From the Thomson limit to the energy frontier
This project aims to enhance the precision of the weak mixing angle in the Standard Model by integrating LHC and MESA data, potentially revealing new physics across a vast energy range.
Exotic High Energy Phenomenology
This project aims to explore novel physics beyond the Standard Model by developing innovative methodologies to uncover new phenomenology at the energy frontier.
Predicting the Extreme
PREXTREME aims to solve the fermion sign problem in warm dense matter using AI and supercomputers, enhancing understanding of hydrogen's properties and advancing applications in material science and nuclear fusion.