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.

Subsidie
€ 1.839.769
2025

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:

  1. Perform the first full physical simulations of hot, electrically charged strongly interacting matter.
  2. 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

Startdatum1-1-2025
Einddatum31-12-2029
Subsidiejaar2025

Partners & Locaties

Projectpartners

  • EOTVOS LORAND TUDOMANYEGYETEMpenvoerder
  • UNIVERSITAET BIELEFELD

Land(en)

HungaryGermany

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