The University of Southampton
University of Southampton Institutional Repository

Predictions for neutron stars from holographic nuclear matter

Predictions for neutron stars from holographic nuclear matter
Predictions for neutron stars from holographic nuclear matter
We discuss masses, radii, and tidal deformabilities of neutron stars constructed from the holographic Witten-Sakai-Sugimoto model. Using the same model for crust and core of the star, we combine our theoretical results with the latest astrophysical data, thus deriving more stringent constraints than given by the data alone. For instance, our calculation predicts - independent of the model parameters - an upper limit for the maximal mass of the star of about 2.46 solar masses and a lower limit of the (dimensionless) tidal deformability of a 1.4-solar-mass star of about 277.
2666-4003
SciPost Foundation
Kovensky, Nicolas
6fdce7c8-51ce-4d21-8223-e16bd1a182c8
Poole, Aaron
cef73035-4295-4ee7-a2cb-d33e90758864
Schmitt, Andreas
1765159f-255f-45e7-94ea-58c1c883d65f
Kovensky, Nicolas
6fdce7c8-51ce-4d21-8223-e16bd1a182c8
Poole, Aaron
cef73035-4295-4ee7-a2cb-d33e90758864
Schmitt, Andreas
1765159f-255f-45e7-94ea-58c1c883d65f

Kovensky, Nicolas, Poole, Aaron and Schmitt, Andreas (2022) Predictions for neutron stars from holographic nuclear matter. In SciPost Physics Proceedings. vol. 6, SciPost Foundation. 11 pp . (doi:10.21468/SciPostPhysProc.6.019).

Record type: Conference or Workshop Item (Paper)

Abstract

We discuss masses, radii, and tidal deformabilities of neutron stars constructed from the holographic Witten-Sakai-Sugimoto model. Using the same model for crust and core of the star, we combine our theoretical results with the latest astrophysical data, thus deriving more stringent constraints than given by the data alone. For instance, our calculation predicts - independent of the model parameters - an upper limit for the maximal mass of the star of about 2.46 solar masses and a lower limit of the (dimensionless) tidal deformability of a 1.4-solar-mass star of about 277.

Text
Predictions for neutron stars from holographic nuclear matter - Author's Original
Available under License Creative Commons Attribution.
Download (931kB)
Text
SciPostPhysProc_6_019 - Version of Record
Available under License Creative Commons Attribution.
Download (842kB)

More information

Accepted/In Press date: 6 May 2022
Published date: 31 May 2022
Venue - Dates: The XXXIII International Workshop on High Energy Physics,<br/>Hard Problems of Hadron Physics: Non-Perturbative QCD &amp; Related Quests, Virtual, 2021-11-08 - 2021-11-09

Identifiers

Local EPrints ID: 478062
URI: http://eprints.soton.ac.uk/id/eprint/478062
ISSN: 2666-4003
PURE UUID: 10bd391d-6014-41d3-8ad9-559916a526ce
ORCID for Andreas Schmitt: ORCID iD orcid.org/0000-0003-2858-4450

Catalogue record

Date deposited: 21 Jun 2023 16:43
Last modified: 17 Mar 2024 03:40

Export record

Altmetrics

Contributors

Author: Nicolas Kovensky
Author: Aaron Poole
Author: Andreas Schmitt ORCID iD

Download statistics

Downloads from ePrints over the past year. Other digital versions may also be available to download e.g. from the publisher's website.

View more statistics

Atom RSS 1.0 RSS 2.0

Contact ePrints Soton: eprints@soton.ac.uk

ePrints Soton supports OAI 2.0 with a base URL of http://eprints.soton.ac.uk/cgi/oai2

This repository has been built using EPrints software, developed at the University of Southampton, but available to everyone to use.

We use cookies to ensure that we give you the best experience on our website. If you continue without changing your settings, we will assume that you are happy to receive cookies on the University of Southampton website.

×