Layers of deformed instantons in holographic baryonic matter
Layers of deformed instantons in holographic baryonic matter
We discuss homogeneous baryonic matter in the decompactified limit of the Sakai-Sugimoto model, improving existing approximations based on flat-space instantons. We allow for an anisotropic deformation of the instantons in the holographic and spatial directions and for a density-dependent distribution of arbitrarily many instanton layers in the bulk. Within our approximation, the baryon onset turns out to be a second-order phase transition, at odds with nature, and there is no transition to quark matter at high densities, at odds with expectations from QCD. This changes when we impose certain constraints on the shape of single instantons, motivated by known features of holographic baryons in the vacuum. Then, a first-order baryon onset and chiral restoration at high density are possible, and at sufficiently large densities two instanton layers are formed dynamically. Our results are a further step towards describing realistic, strongly interacting matter over a large density regime within a single model, desirable for studies of compact stars.
1-37
Preis, Florian
e7aabce2-f6f3-4256-832f-17f663e72131
Schmitt, Andreas
1765159f-255f-45e7-94ea-58c1c883d65f
Preis, Florian
e7aabce2-f6f3-4256-832f-17f663e72131
Schmitt, Andreas
1765159f-255f-45e7-94ea-58c1c883d65f
Preis, Florian and Schmitt, Andreas
(2016)
Layers of deformed instantons in holographic baryonic matter.
Journal of High Energy Physics, 2016 (1), .
(doi:10.1007/JHEP07(2016)001).
Abstract
We discuss homogeneous baryonic matter in the decompactified limit of the Sakai-Sugimoto model, improving existing approximations based on flat-space instantons. We allow for an anisotropic deformation of the instantons in the holographic and spatial directions and for a density-dependent distribution of arbitrarily many instanton layers in the bulk. Within our approximation, the baryon onset turns out to be a second-order phase transition, at odds with nature, and there is no transition to quark matter at high densities, at odds with expectations from QCD. This changes when we impose certain constraints on the shape of single instantons, motivated by known features of holographic baryons in the vacuum. Then, a first-order baryon onset and chiral restoration at high density are possible, and at sufficiently large densities two instanton layers are formed dynamically. Our results are a further step towards describing realistic, strongly interacting matter over a large density regime within a single model, desirable for studies of compact stars.
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Accepted/In Press date: 22 June 2016
e-pub ahead of print date: 1 July 2016
Organisations:
Applied Mathematics
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Local EPrints ID: 397862
URI: http://eprints.soton.ac.uk/id/eprint/397862
PURE UUID: c634df0a-cbe3-4040-8b50-39284d430145
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Date deposited: 08 Jul 2016 10:22
Last modified: 15 Mar 2024 03:53
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Author:
Florian Preis
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