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Gravitational Waves of Holographic Neutron Stars

Project description

Modelling and simulations to probe high-density matter of neutron star mergers

Gravitational waves from the merger of two neutron stars were observed by two LIGO detectors in 2017. Deeper theoretical knowledge of the fundamental physics of neutron star mergers is critical to interpreting the data from future observations. The EU-funded GWOHNS project plans to construct holographic models for the matter inside the stars and develop a novel tool for high-resolution simulations of neutron star mergers. For simulations, the project will use the gauge–gravity duality. Unlike conventional methods such as perturbation theory, lattice quantum chromodynamics and low-energy effective theories, the gauge–gravity duality provides a better framework for modelling subatomic matter at densities relevant for neutron stars. The project's work will pave the way for new predictions about neutron star merger dynamics and the detected gravitational waveforms.

Objective

The proposal aims at making substantial progress on the theoretical understanding of neutron stars (NSs) by constructing holographic models for the matter inside the stars and by developing a novel tool for high-resolution NS merger simulations.
The first observation of gravitational waves (GWs) from a NS merger in August 2017 by the LIGO observatory induced huge interest that goes far beyond the scientific expert community. Many more observations are expected in the near future and progress in the theoretical understanding of NS mergers is therefore sorely needed.
We propose an entirely new approach and construct equations of state (EoSs), using the gauge-gravity duality (“holography” for short), for the NS matter in merger simulations. Holography establishes an effective framework to model subatomic matter at densities relevant for NSs, where traditional methods like perturbation theory, lattice quantum chromodynamics (QCD), and low-energy effective theories are not applicable.
In that way we will generate predictions for the merger dynamics and the gravitational waveforms, which will lead to additional theoretical insights when confronted with future observations.
Applying holography to NS merger physics is a completely new concept and potentially opens a new field of holographic gravitational wave model building. The proposal has a strong multidisciplinary character as it combines aspects of string theory, high energy physics, astrophysics, nuclear physics, numerical relativity and high performance computing (HPC) and will therefore lead to interest and progress in all these fields.

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Keywords

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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

Procedure for inviting applicants to submit project proposals, with the aim of receiving EU funding.

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

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Coordinator

QUEEN MARY UNIVERSITY OF LONDON
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.

€ 224 933,76
Address
327 MILE END ROAD
E1 4NS LONDON
United Kingdom

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Activity type
Higher or Secondary Education Establishments
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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.

€ 224 933,76
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