Articles Citing

Stiff equation of state for a holographic nuclear matter as instanton gas

Kazuo Ghoroku ^1,*, Kouji Kashiwa^1,†, Yoshimasa Nakano ^‡, Motoi Tachibana^2,§, and Fumihiko Toyoda^3,∥

¹Fukuoka Institute of Technology, Wajiro, Fukuoka 811-0295, Japan
²Department of Physics, Saga University, Saga 840-8502, Japan
³Faculty of Humanity-Oriented Science and Engineering, Kinki University, Iizuka 820-8555, Japan

^*gouroku@fit.ac.jp
^†kashiwa@fit.ac.jp
^‡ynakano@kyudai.jp
^§motoi@cc.saga-u.ac.jp
^∥f1toyoda@jcom.home.ne.jp

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Articles Citing

Stiff equation of state for a holographic nuclear matter as instanton gas

Dense matter in a holographic hard-wall model of QCD

Condensate phases of nuclear matter from AdS hardwall models

Prompt black hole formation in binary neutron star mergers

Confined phases at finite density in the hardwall model

A Review on the Equation of State of the Color Superconductivity Phase via Holography

Weak rates in strongly coupled cold quark matter

Popcorn Transitions and Approach to Conformality in Homogeneous Holographic Nuclear Matter

Baryonic matter at strong coupling: Confining superfluids and deconfined ferromagnets

Instability of holographic cold compact stars with a color superconducting core

Holographic neutrino transport in dense strongly-coupled matter

Holographic approach to compact stars and their binary mergers

Dense and Hot QCD at Strong Coupling

Holographic model with power-law Maxwell field for color superconductivity

Building a realistic neutron star from holography

Holographic QCD in the NICER era

Holographic modeling of nuclear matter and neutron stars

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