Exploring the phase diagram of V-QCD with neutron star merger simulations
- Determining the phase structure of Quantum Chromodynamics (QCD) and its Equation of State (EOS) at densities and temperatures realized inside neutron stars and their mergers is a long-standing open problem. The holographic V-QCD framework provides a model for the EOS of dense and hot QCD, which describes the deconfinement phase transition between a dense baryonic and a quark matter phase. We use this model in fully general relativistic hydrodynamic (GRHD) simulations to study the formation of quark matter and the emitted gravitational wave signal of binary systems that are similar to the first ever observed neutron star merger event GW170817.
Author: | Tuna DemircikORCiD, Christian EckerORCiD, Matti JärvinenORCiD, Luciano RezzollaORCiDGND, Samuel TootleORCiDGND, Konrad TopolskiORCiD |
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URN: | urn:nbn:de:hebis:30:3-838806 |
URL: | https://arxiv.org/abs/2211.10118v1 |
DOI: | https://doi.org/10.48550/arXiv.2211.10118 |
ArXiv Id: | http://arxiv.org/abs/2211.10118v1 |
Parent Title (German): | arXiv ; Reportnummer: APCTP Pre2022 - 026 |
Publisher: | arXiv |
Document Type: | Preprint |
Language: | English |
Date of Publication (online): | 2022/11/18 |
Date of first Publication: | 2022/11/18 |
Publishing Institution: | Universitätsbibliothek Johann Christian Senckenberg |
Release Date: | 2024/07/18 |
Issue: | 2211.10118 Version 1 |
Edition: | Version 1 |
Page Number: | 8 |
HeBIS-PPN: | 520535596 |
Institutes: | Physik / Physik |
Dewey Decimal Classification: | 5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik |
Sammlungen: | Universitätspublikationen |
Licence (German): | Creative Commons - CC BY - Namensnennung 4.0 International |