2019
DOI: 10.1007/jhep07(2019)003
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Cool baryon and quark matter in holographic QCD

Abstract: We establish a holographic bottom-up model which covers both the baryonic and quark matter phases in cold and dense QCD. This is obtained by including the baryons using simple approximation schemes in the V-QCD model, which also includes the backreaction of the quark matter to the dynamics of pure Yang-Mills. We examine two approaches for homogeneous baryon matter: baryons as a thin layer of noninteracting matter in the holographic bulk, and baryons with a homogeneous bulk gauge field. We find that the second … Show more

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Cited by 81 publications
(131 citation statements)
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References 99 publications
(246 reference statements)
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“…Unfortunately, holographic baryon physics is technically demanding as baryons are usually realized as soliton configurations of the gravitational dual. An ongoing work discuss baryons in V-QCD in simple approximations [52]. Studying magnetic effects would also be interesting, and relevant in particular to study the physics of magnetars.…”
Section: Discussionmentioning
confidence: 99%
“…Unfortunately, holographic baryon physics is technically demanding as baryons are usually realized as soliton configurations of the gravitational dual. An ongoing work discuss baryons in V-QCD in simple approximations [52]. Studying magnetic effects would also be interesting, and relevant in particular to study the physics of magnetars.…”
Section: Discussionmentioning
confidence: 99%
“…In ref. [31], another holographic bottomup approach, working in the so-called Veneziano limit, was employed to construct a phase where quarks and pointlike baryons coexist. It was argued, however, that this phase only exists in a version of the model that is unfavored otherwise.…”
Section: Jhep09(2020)112mentioning
confidence: 99%
“…We believe that our work sets the standard and sparks many other investigations in the future. One particularly interesting case is in the context of the astrophysics of compact objects where anisotropy seems to offer clues regarding the "universal relations" for neutron stars [110] and the already established holographic modeling of isotropic matter [69,[111][112][113][114][115][116].…”
Section: Discussionmentioning
confidence: 99%
“…matching the value corresponding to a conformal theory in 2d and not that of 3d. Notice that at finite chemical potential there are plenty of examples in holography where one can exceed the conformal value [67][68][69], as long as the conformal symmetry is broken. Here the mechanism is quite different and can be associated with the presence of the defect instead of some intrinsic energy scale.…”
Section: Stiffness At Zero Temperaturementioning
confidence: 99%