Lifting stellar structure and evolution to higher dimensions in the era of space asteroseismology

4D-STAR aims to revolutionize stellar models by developing a 3+1D theory of rotating spheroids, enhancing age accuracy and understanding of stellar evolution using asteroseismic data.

Subsidie
€ 9.938.446
2023

Projectdetails

Introduction

Stars are the source of radiation, chemistry, and life in the Universe. Models of how stars live are key ingredients in planetary, astrophysical, and cosmological research. A star is a hot plasma rotating around an axis.

Stellar Rotation

Small stars like the Sun rotate slowly, but bigger ones with more mass rotate faster, shaping them as flattened spheroids. Yet, current stellar models simplify the flattening or treat stars as spheres during their lives, using 1 spatial and 1 time dimension (1+1D).

Limitations of Current Models

Rotation and magnetism induce transport processes in 3 spatial dimensions, which change over time, requiring a 3+1D treatment. Current age-dating of stars is done from 1+1D models, with uncertainties up to 1000%. Accurate ages of stars are the dominant missing ingredient to understand stellar and planetary evolution, the emergence of life, and the chemistry in our Universe.

Project Overview

4D-STAR will answer the fundamental question of how rotating spheroids evolve in time and build up their chemistry during their lives. We will develop a new 3+1D theory of stellar rotation for flattened spheroids evolving over millions to billions of years, from birth to death.

Data Utilization

Lifting stellar models to 3+1D can only be done now, using asteroseismic data of thousands of stars in all life phases. Such data reveal nonradial oscillations, or starquakes, allowing us to infer internal stellar rotation, magnetism, chemistry, and the ages of stars with 10% accuracy.

Open-Source Modules

4D-STAR will provide open-source modules to compute the evolution of rotating magnetic stars in 3+1D, calibrated to asteroseismic observables of single stars and stars in binaries and clusters.

Transdisciplinary Integration

4D-STAR brings a paradigm shift based on mathematical modelling, astrophysics, and computational science. Its breadth, challenges, and goals require a transdisciplinary integration of four teams led by:

  1. An asteroseismologist
  2. A theoretician specialized in transport
  3. A hydrodynamicist
  4. A stellar evolution software developer

Each team member has a proven track record.

Financiële details & Tijdlijn

Financiële details

Subsidiebedrag€ 9.938.446
Totale projectbegroting€ 9.938.446

Tijdlijn

Startdatum1-9-2023
Einddatum31-8-2029
Subsidiejaar2023

Partners & Locaties

Projectpartners

  • KATHOLIEKE UNIVERSITEIT LEUVENpenvoerder
  • COMMISSARIAT A L ENERGIE ATOMIQUE ET AUX ENERGIES ALTERNATIVES
  • UNIVERSITE DE TOULOUSE
  • TRUSTEES OF DARTMOUTH COLLEGE

Land(en)

BelgiumFranceUnited States

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