Finite-size effects on the hadron-quark mixed phase

Toshitaka Tatsumi, Toshiki Maruyama, Satoshi Chiba, Tomoki Endo

doi:10.48550/arxiv.hep-ph/0601008

説明

We show that the hadron-quark mixed phase is restricted to narrow range of baryon chemical potential by the charge screening effect. Accordingly the mixed phase expected in hadron-quark hybrid stars should be narrow. Although the screening would not have large effect in bulk properties of the star such as mass or radius, it change the internal structure of the star very much, which may be tested by the cooling curve, glitch phenomena or gravitational waves.

Proceeding of the "Origin of Matter and Evolution of Galaxies 2005 (OMEG05)"

収録刊行物

AIP Conference Proceedings

AIP Conference Proceedings 847 380-382, 2006-01-01

AIP

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詳細情報詳細情報について

CRID: 1873116917373715200

DOI: 10.1063/1.2234432; 10.48550/arxiv.hep-ph/0601008

ISSN: 0094243X

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OpenAIRE

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