Gravitational frequency shift of light signals in a pulsating dark matter halo

具有暗物质晕的静态黑洞的新分析模型及通过准周期振荡的参数约束

New analytical model of static black hole with a dark matter halo and parametric constraints through quasiperiodic oscillations

本文提出一种具有暗物质晕的静态黑洞新模型，通过分析其时空特性及拟合实际数据，揭示暗物质对黑洞引力动力学的影响。

观测一个Schwarzschild黑洞在Hernquist暗物质晕中的吸积盘的特征

Observational Signatures of Accretion Disks around a Schwarzschild Black Hole in a Hernquist Dark Matter Halo

研究DM晕对Schwarzschild黑洞吸积盘引力波和电磁特征的影响，揭示其对轨道动态和波形形态的改变。

嵌入暗物质晕的旋转黑洞周围薄吸积盘的观测特征

Observational Signatures of Thin Accretion Disks around Rotating Black Holes Embedded in Dark Matter Halos

本研究探究暗物质晕修正的克尔黑洞周围薄吸积盘的观测特征，发现暗物质晕使吸积盘ISCO外移、抑制辐射通量峰值，生成可与标准真空克尔黑洞区分的观测信号。

非线性宇宙中的原初物理：从宇宙学对撞机模型揭示振荡晕偏差

Primordial Physics in the Nonlinear Universe: Revealing the oscillating halo bias from cosmological collider models

研究宇宙学对撞机模型中初始条件含有的极高能粒子物理信息，开发新模拟方法，测量振荡晕偏差，发现其与晕质量等相关，信号独特不易被模拟，模拟及代码已公开。

Dark matter candidate induced by Horndeski theory: dark matter halo and cosmological evolution

We study spherically symmetric solutions with a scalar field in the shift-symmetric subclass of the Horndeski theory. Constructing an effective energy-momentum tensor of the scalar field based on the two-fluid model, we decompose the scalar field into two components: dark matter and dark energy.We find the dark-matter fluid is pressure-less, and its distribution of energy density obeys the inverse-square law. We show the scalar field dark matter can explain the galaxy rotation curve and discuss the time evolution of the dark matter in the cosmic background.

赫恩奎斯特暗物质晕中旋转黑洞的阴影和引力透镜特征

Shadows and lensing signatures of a rotating black hole in a Hernquist dark matter halo

研究赫恩奎斯特暗物质晕中旋转黑洞光学性质，通过特定程序生成时空并推导相关方程，构建阴影轮廓，比较测量结果限制晕参数，还分析强弱场引力透镜，得到不同条件下晕参数范围。

暗物质的伪装：X射线反射测量中黑洞与吸积推断的简并性及致密暗物质晕的约束前景

A Dark Matter Masquerade: Degeneracies in Black Hole and Accretion Inference from X-ray Reflection Measurements and Prospects for Compact Dark Matter Halo Constraints

本研究发现致密暗物质晕会使X射线反射光谱推断的黑洞自旋等参数出现偏差，同时提出纳入该环境的反射模型可补充引力波探测以约束暗物质晕参数。

轨道动力学和极端质量比 inspiral 在银河系暗物质晕中的引力波特征

Orbital Dynamics and Gravitational Wave Signatures of Extreme Mass Ratio Inspirals in Galactic Dark Matter Halos

研究暗物质晕对极端质量比 inspiral 系统轨道动力学和引力波信号的影响，揭示不同暗物质模型在长期演化中的差异。