Predictions for neutron stars from holographic nuclear matter
Nicolas Kovensky, Aaron Poole, Andreas Schmitt
SciPost Phys. Proc. 6, 019 (2022) · published 31 May 2022
- doi: 10.21468/SciPostPhysProc.6.019
XXXIII International Workshop on High Energy Physics
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.
Cited by 1
Zhang et al., Holographic cold dense matter constrained by neutron stars
Phys. Rev. D 106, 096028 (2022) [Crossref]
Authors / Affiliations: mappings to Contributors and OrganizationsSee all Organizations.
- 1 Nicolas Kovensky,
- 2 Aaron Poole,
- 2 Andreas Schmitt