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.

Subsidie
€ 2.446.893
2024

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:

  1. Supercooling
  2. Critical bubble nucleation
  3. 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

Startdatum1-9-2024
Einddatum31-8-2029
Subsidiejaar2024

Partners & Locaties

Projectpartners

  • HELSINGIN YLIOPISTOpenvoerder

Land(en)

Finland

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