Radial Oscillations of Viscous Stars at Finite Temperature
有限温度下粘性恒星的径向振荡
Amanda Guerrieri, Gabriel S. Rocha, Gabriel S. Denicol, Raissa F. P. Mendes
AI总结 研究Israel-Stewart和Navier-Stokes理论中相对论性恒星的径向振荡谱,引入热扩散和有限温度状态方程,发现热模在临界泛音数以上从纯阻尼转变为传播行为,并首次在致密星中实现相对论第二声。
Comments 14 pages, 6 figures
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我们在Israel-Stewart和Navier-Stokes理论中研究相对论性恒星的径向振荡谱,将先前分析扩展到包括热扩散和热力学一致的有限温度状态方程。热流的引入在模式谱中产生了一个独特的热扇区,其结构紧密反映了无限耗散流体的色散关系。在Israel-Stewart理论中,热模在临界泛音数以上从纯阻尼转变为传播行为,为致密星中相对论第二声提供了有限尺寸的实现。值得注意的是,有限的恒星几何可以将甚至基态热模推入传播区域——这一特征在连续介质中没有类似物。对于此处考虑的状态方程类别,其中有限温度修正作为冷多方球的受控Sommerfeld型扰动进入,热扇区仅与普通流体振荡谱弱耦合,耦合在适当的温度参数中为二阶。我们进一步表明,离散的恒星谱很好地由从平直时空色散关系构建的解析近似捕获,恒星的有限半径离散了连续模式结构。我们的结果通过纳入Israel-Stewart框架中最后一个剩余的耗散自由度,完成了粘性恒星径向振荡的分析。
We study the radial oscillation spectrum of relativistic stars within Israel-Stewart and Navier-Stokes theories, extending previous analyses to include heat diffusion and a thermodynamically consistent finite-temperature equation of state. The inclusion of heat flux gives rise to a distinct thermal sector in the mode spectrum, whose structure closely mirrors the dispersion relations of an infinite dissipative fluid. Within Israel-Stewart theory, the thermal modes transition from purely damped to propagating behavior above a critical overtone number, providing a finite-size realization of relativistic second sound in compact stars. Remarkably, the finite stellar geometry can push even the fundamental thermal mode into the propagating regime -- a feature with no continuum analogue. For the class of equations of state considered here, where finite-temperature corrections enter as controlled, Sommerfeld-type perturbations of a cold polytrope, the thermal sector couples only weakly to the ordinary fluid oscillation spectrum, with the coupling being of second order in a suitable temperature parameter. We further show that the discrete stellar spectrum is well captured by an analytic ansatz constructed from the flat-spacetime dispersion relations, with the star's finite radius discretizing the continuous mode structure. Our results complete the analysis of radial oscillations of viscous stars by incorporating the last remaining dissipative degree of freedom within the Israel-Stewart framework.