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Published: 2025-09-02
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  • Thermodynamic phase transition and Joule-Thomson expansion of a quantum corrected black hole in AdS spacetime
    2025, 49(11): 115102-115102-13. doi: 10.1088/1674-1137/ade4a9
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    The thermodynamics in the extended phase space of a quantum corrected black hole (BH) proposed recently is presented in this paper. Our study shows that the phase transition behavior of the BH is analogous to that of a conventional Schwarzschild BH in anti-de Sitter (AdS) space; however, a critical temperature exists such that, when the BH temperature exceeds this critical value, the small and large BH phases become separated, and no phase transition occurs. Owing to the introduction of the quantum parameter ξ, the BH equation of state splits into two branches. One branch reduces to the Schwarzschild-AdS case as $ \xi\to0$, with its phase transition pressure lower than the critical pressure; the phase transition pressure in the other branch is greater than the critical pressure. This study shows that the $ T-r_{+}$ phase transition and heat capacity of the recently proposed BH are similar to those of the Schwarzschild-AdS BH. The Joule-Thomson expansion is divided into two stages: in the earlier stage, the BH pressure increases until it reaches a maximum; in the later stage, the pressure gradually decreases. In each stage, the BH may undergo an inversion point, resulting in an inversion curve with two branches. In addition, each stage has a minimum inversion mass, below which any BH (in each respective stage) has no inversion point.
  • 1+1 dimensional relativistic viscous non-resistive magnetohydrodynamics with longitudinal boost invariance
    2025, 49(11): 114104-114104-13. doi: 10.1088/1674-1137/ade6d4
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    We study 1+1 dimensional relativistic non-resistive magnetohydrodynamics (MHD) with longitudinal boost invariance and a shear stress tensor. Several analytical solutions describing the fluid temperature evolution under a given equation of state (EoS) $ \varepsilon=3p $ are derived. Extending the Victor-Bjorken ideal MHD flow to include non-zero shear viscosity, we first obtain two perturbative analytical solutions for the first-order (Navier-Stokes) approximation. For small, power-law evolving external magnetic fields, our stable solutions show that both magnetic field and shear viscosity cause fluid heating with an early temperature peak, consistent with numerical results. In the second-order (Israel-Stewart) theory, our numerical results show that the combined presence of magnetic field and shear viscosity leads to a slow cooling rate of fluid temperature, with initial shear stress significantly influencing temperature evolution of the medium.
  • Stable circular orbits and greybody factor of Hayward-Letelier-AdS black holes
    2025, 49(11): 115104-115104-17. doi: 10.1088/1674-1137/ade4a7
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    This paper explores the dynamical feature of Hayward-Letelier black holes in AdS spacetime, emphasizing the effects of the Hayward parameter g, mass M, cosmological constant L, and modification parameter α on their geometry, thermodynamics, and observational features. By utilizing an effective potential method, we investigate the paths of particles, innermost stable circular orbit, and behavior of photon spheres, which connects them to the appearance of black hole shadows. Thermodynamic features such as Hawking temperature and entropy are studied for investigating the effect of L and thermal fluctuations on the stability of black holes. These discoveries connect theoretical ideas with observational astrophysics, which enhances our comprehension of ordinary black holes in AdS models. In this study, we analytically compute the greybody factor for a massless scalar field propagating in the vicinity of a black hole under the assumption of weak coupling to gravity. We investigate the behavior of the effective potential concerning the black hole's mass and charge, revealing that it reaches its maximum at lower values of the cloud of strings parameter. Our results indicate that the radial absorption rate of the scalar field exhibits significant fluctuations, which is influenced by the charge of the black hole and clouds of string, with implications for the dynamics of scalar fields in strong gravitational fields.
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ISSN 1674-1137 CN 11-5641/O4

Original research articles, Ietters and reviews Covering theory and experiments in the fieids of

  • Particle physics
  • Nuclear physics
  • Particle and nuclear astrophysics
  • Cosmology
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