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arXiv 2512.02484hep-phastro-ph.HEhep-th
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在双生论中稳定质量夸克星的性质

Properties of Stable Massive Quark Stars in Holography

Shahrood University of Technology(沙鲁德科技大学);Universidad Nacional Autónoma de México(墨西哥国立自治大学);Technische Universität Wien(维也纳工业大学)

Kazem Bitaghsir Fadafan, Jesús Cruz Rojas, Jonas Mager

AI总结:

本文研究了双生论D3/D7系统,通过调整红外区域的稀释子剖面,探讨了有限密度下反禁闭且质量较大的夸克相的方程状态,发现其足以支持质量达2倍太阳质量的奇异致密星。

摘要:

我们研究了一个双生论D3/D7系统,其稀释子剖面已在红外区域进行了现象学调整。该模型用于描述有限密度下反禁闭且质量较大的夸克相,得出该相的方程状态可能足够刚性,以支持质量达2倍太阳质量的奇异致密星。核子通过现象学方法用Hebeler等人提出的有效理论重子相建模。对于刚性的现象学重子相,向夸克相的过渡为弱一级相变,允许稳定夸克核心。我们还发现,将重子建模为包裹的D5膜的双生论重子,在均匀近似下提供不现实的压力,必须予以排除。我们计算了这些混合星的质量与半径关系以及潮汐变形性。与大量其他双生论模型不同,该双生论模型表明夸克物质可能存在于重致密星的核心,并可用于探索此类物体的现象学。

英文摘要:

We study a holographic D3/D7 system, whose dilaton profile has been phenomenologically adjusted in the infrared. The model is used to describe a deconfined yet massive quark phase of QCD at finite density, concluding that the equation of state of such a phase can be stiff enough to support exotic dense stars as massive as 2 solar masses. Nucleons are modeled phenomenologically using the Hebeler-et.al EFT baryon phases. For the stiff phenomenological baryon phases the transition to the quark phase is weakly first order allowing for stable quark cores. We also find that holographic baryons, modeled as wrapped D5-branes, provide unrealistic pressures (in the homogeneous approximation) and have to be discarded. We compute the mass vs. radius relation and tidal deformability for these hybrid stars. Contrary to a large number of other holographic models, this holographic model indicates that quark matter could be present at the core of heavy compact stars and may be used to explore the phenomenology of such objects.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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