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Precision stellar astrophysics and the distance scale with pulsating stars in the Gaia era

Project description

Mapping the universe with pulsating stars

Pulsating stars such as Cepheid and RR Lyrae are sensitive probes for determining the distance to astronomical objects. Cepheid variables play a vital role in calibrating the cosmic distance ladder to measure the local value of the Hubble constant – the present rate of the universe’s expansion. Current Hubble constant measurements based on Cepheid distances are significantly larger than those measured by the European Space Agency's Planck satellite. This might hint at new physics beyond the standard cosmological model and warrants rigorous investigation of potential systematic uncertainties in Cepheid distances. Funded by the Marie Skłodowska-Curie Actions programme, the PRESTiGE project plans to use state-of-the-art pulsation models and Gaia data releases to calibrate theoretical and experimental period–luminosity relations for Cepheid and RR Lyrae.

Objective

Classical pulsating stars such as Cepheid and RR Lyrae are sensitive probes for both the stellar astrophysics and the cosmic distance scale. Cepheid variables play a vital role in calibrating extragalactic distance ladder to estimate the local value of the Hubble constant – present expansion rate of the Universe. The current Hubble constant measurement in the late evolutionary Universe based on the Cepheid-Supernovae distance ladder is significantly larger than the Planck mission results from the early Universe. This tension hints at possible new physics beyond the standard cosmological model and warrants a rigorous investigation of potential systematic uncertainties in Cepheid-based distance ladder. The proposed project will use state-of-the-art stellar pulsation models to compute and exploit an unprecedently fine grid of Cepheid and RR Lyrae models. These models together with future Gaia data-releases will be used to calibrate theoretical and empirical Period-Luminosity relations for Cepheid and RR Lyrae, and quantify residual systematic effects in the first-rung of the distance ladder and evaluate the significance of the Hubble tension problem. The project will employ modern computational methods for multiwavelength comparison between predicted and observed pulsation properties and full-amplitude light and velocity variations to constrain the mass-luminosity relations and helium to metal enrichment ratio followed by Cepheid and RR Lyrae stars with sub-percent precision for the first-time. These investigations will also discriminate and quantify the effects of poorly understood non-standard phenomena such as mass-loss, rotation or convective overshooting on input stellar physics to the pulsation codes, and thus imply strong constraints for the stellar evolutionary models. This project is of multidisciplinary nature with a strong transfer of knowledge between the applicant and the host researcher, and in line with the EU strategic plan for research and innovation.

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Programme(s)

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Topic(s)

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Funding Scheme

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MSCA-IF - Marie Skłodowska-Curie Individual Fellowships (IF)

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Call for proposal

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(opens in new window) H2020-MSCA-IF-2019

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Coordinator

ISTITUTO NAZIONALE DI ASTROFISICA
Net EU contribution

Net EU financial contribution. The sum of money that the participant receives, deducted by the EU contribution to its linked third party. It considers the distribution of the EU financial contribution between direct beneficiaries of the project and other types of participants, like third-party participants.

€ 171 473,28
Address
VIALE DEL PARCO MELLINI 84
00136 ROMA
Italy

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Region
Centro (IT) Lazio Roma
Activity type
Research Organisations
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Total cost

The total costs incurred by this organisation to participate in the project, including direct and indirect costs. This amount is a subset of the overall project budget.

€ 171 473,28
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