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论文

41 篇基准文献:6 篇已审核,35 篇候选基准

候选基准已经完成来源、双语导读和公式整理,正在等待人工审核;它们可以阅读,但不等同于正式发布的精选论文。

  1. I 型超新星:早期光变曲线的解析解

    英文原题:Type I supernovae. I - Analytic solutions for the early part of the light curve

    Arnett, W. D. · 1982

    已审核精选

    阅读这项工作,可以看到一个紧凑的物理模型如何把能量源连接到输运和可测光变曲线。文中的历史性“Type I”表述不应被不加说明地改写为现代亚型分类。

    Read this Work to see how a compact physical model connects an energy source to transport and a measurable light curve. Its historical “Type I” language should not be silently rewritten as a modern subtype classification.

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  2. 相对论爆炸波的流体动力学

    英文原题:Fluid dynamics of relativistic blast waves

    R. D. Blandford, C. F. McKee · 1976

    候选基准

    深入理解激波减速半径、余辉衰减时序斜率与喷流能量守恒的必读论文;重点推导激波下游物理量沿相似变量 $\chi = 1 + 2(m+1)\Gamma^2(1 - r/R)$ 的分布。

    Read it to connect self-similar relativistic blast-wave dynamics to afterglow decay indices, shock deceleration radii, and blast-wave energy conservation. Focus on the similarity variable $\chi = 1 + 2(m+1)\Gamma^2(1 - r/R)$ and shock jump conditions.

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  3. 相对论喷流在外部介质中的传播

    英文原题:The Propagation of Relativistic Jets in External Media

    Bromberg, Omer, Nakar, Ehud, Piran, Tsvi, Sari, Re'em · 2011

    已审核精选

    Bromberg 等人把相对论喷流传播转化为一个耦合的物理描述:喷流头部向茧状体沉积能量,茧状体压力可以使喷流准直,而改变后的喷流几何又会反馈到头部运动和能量沉积。由此可以用一套紧凑框架理解 GRB、微类星体和 AGN 环境中的准直与非准直状态。

    Bromberg et al. turn relativistic jet propagation into a coupled physical account: the jet head deposits energy into a cocoon, the cocoon pressure can collimate the jet, and the changed jet geometry feeds back on head motion and energy deposition. The result is a compact way to reason about collimated and uncollimated regimes across GRB, microquasar, and AGN environments.

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  4. 增强型 X 射线时变与偏振空间天文台(eXTP)探测黑洞强引力场区

    英文原题:Probing the strong gravity region of black holes with eXTP

    Qingcui Bu, Cosimo Bambi, Lijun Gou, Yanjun Xu, Phil Uttley, Diego Altamirano, Michiel van der Klis, Andrea Santangelo, Shuang-Nan Zhang · 2025

    候选基准

    深入理解黑洞吸积几何、克尔度规视界物理与未来空间天文台(eXTP)科学前沿的集大成文献;重点研读相对论光线追踪模拟图与偏振度随自旋演化的理论曲线。

    Comprehensive reading for strong-field gravity and black hole spin diagnostics. Study the relativistic ray-tracing simulations and polarization degree trajectories across dimensionless spin $a_*$.

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  5. 慧眼卫星观测 1A 0535+262 发现高能毫赫兹准周期震荡挑战既有模型

    英文原题:High energy millihertz quasi-periodic oscillations in 1A 0535 + 262 with Insight-HXMT challenge current models

    Ruican Ma, Lian Tao, Shuang-Nan Zhang, Long Ji, Liang Zhang, Qingcui Bu, Jinlu Qu, Pablo Reig, Mariano Méndez, Yanan Wang, Xiang Ma, Yue Huang, Mingyu Ge, Liming Song, Shu Zhang · 2022

    候选基准

    深入研读慧眼高能时变数据分析、吸积柱物理与准周期震荡机制的核心必读论文;重点查看硬 X 射线功率谱密度(PSD)本底拟合与 QPO 均方根振幅(rms)随能量演化图。

    Essential reading for Insight-HXMT timing analysis and accretion column physics. Focus on the hard X-ray power spectral density fits and the energy-dependent fractional rms evolution.

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  6. PSR B1259−63/LS 2883 的多波段辐射建模

    英文原题:Modelling the multi-wavelength emissions from PSR B1259-63/LS 2883: the effects of the stellar disc on shock radiations

    A. M. Chen, J. Takata, S. X. Yi, Y. W. Yu, K. S. Cheng · 2019

    候选基准

    深入研究高能双星、脉冲星风激波与伴星盘相互作用的经典必读论文;重点精读脉冲星穿越 Be 盘时的动压平衡驻点距离计算与各向异性逆康普顿散射角分布积分。

    Essential classical study for high-energy binaries and pulsar-wind-disk interactions. Step through the orbital geometry calculations of shock stagnation distances and anisotropic Compton angular integrations.

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  7. Be/伽马射线双星中 keV/TeV 光变的相关性

    英文原题:Modelling the correlated keV/TeV light curves of Be/gamma-ray binaries

    A. M. Chen, J. Takata · 2021

    候选基准

    从事高能双星多波段联合观测(NuSTAR, HXMT, LHAASO, CTA)与能谱时变分析的必读指南;重点关注文中关于 X-ray 对比 TeV 相关系数随轨道相位变化解析推导章节。

    Indispensable guide for interpreting multi-wavelength binary observations across HXMT, NuSTAR, and LHAASO. Focus on the mathematical derivation of correlation coefficients across orbital phases.

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  8. 恒星抛射物与外部介质相互作用的自相似解

    英文原题:Self-similar solutions for the interaction of stellar ejecta with an external medium

    R. A. Chevalier · 1982

    候选基准

    所有 CSM 相互作用超新星(IIn, Ibn, Icn)、FBOT 激波拟合及 TransFit-CSM 模型的力学源头;建议重点推导式 (n-3)/(n-s) 的时序指数起源与反向激波能量耗散率。

    The mechanical origin of all CSM-interaction models and shock heating frameworks. Focus on how $(n-3)/(n-s)$ controls shock acceleration, deceleration, and kinetic dissipation.

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  9. 快速自转奇异星与中子星驱动的伽马射线暴及其余辉

    英文原题:γ-Ray Bursts and Afterglows from Rotating Strange Stars and Neutron Stars

    Z. G. Dai, T. Lu · 1998

    候选基准

    理解所有磁星能量注入模型(R1 主线)的最核心源头文献;重点推导自转减速功率注入下激波洛伦兹因子 $\Gamma(t) \propto t^{-(1-q)/8}$ 的时间依赖演化修正。

    The historical and conceptual wellspring for all magnetar energy-injection theory. Trace the modified blast-wave deceleration $\Gamma(t) \propto t^{-(1-q)/8}$ driven by continuous dipole power.

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  10. 吸积脉冲星船帆座 X-1 回旋共振散射吸收线的长期演化:单脉冲分析法

    英文原题:Long-term evolution of cyclotron resonant scattering features in the accreting pulsar Vela X-1: A pulse-to-pulse approach

    Yu-Jia Du, Peng-Ju Wang, Lorenzo Ducci, Long Ji, Ling-Da Kong, Qing-cui Bu, Victor Doroshenko, Andrea Santangelo, Shuang-Nan Zhang · 2026

    候选基准

    掌握中子星磁场测量第一性原理与空间 X 射线谱学分析的必读论文;重点学习高能连续谱(NPEX/Cutoffpl)与高斯/自吸收共振线(Gabs)联合拟合的统计置信度判定。

    Indispensable for mastering cyclotron line physics and X-ray spectroscopy. Focus on the joint fitting techniques decoupling the continuum (NPEX/cutoffpl) from cyclotron absorption profiles (Gabs).

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  11. 伴星进动驱动的 FRB 20220529 超轨道旋转量变化

    英文原题:Super-Orbital Variations in Magnetar Rotation Measure Arising from the Precession of Companion Star: Implications for FRB 20220529

    Ze-Xin Du, Yun-Wei Yu, Aming Chen, Chen-Hui Niu, Jia-Heng Zhang · 2026

    候选基准

    掌握如何利用 FRB 偏振观测诊断极端致密星环境的必读论文;重点精读文中法拉第旋转量积分沿三维进动轨道视线投影矢量的数学几何推导。

    Essential for understanding polarization diagnostics of FRB environments. Focus on the vector projection integration of $B_\parallel$ along the three-dimensional precessing line of sight.

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  12. 最慢银河系场蜘蛛脉冲星 PSR J1932+2121 的射电掩食

    英文原题:Radio eclipse of the slowest spinning Galactic-field spider pulsar PSR J1932+2121 and its X-ray emission prospect

    Ze-Xin Du, Yun-Wei Yu, Zong-Lin Yang, Aming Chen, Peng-Fei Wang, Jin-Lin Han, De-Jiang Zhou, Xiao-Peng You · 2026

    候选基准

    学习如何将 FAST 射电脉冲星实测数据转化为高能天体物理理论物理参数的绝佳论文;重点关注文中掩食几何光深方程的数值求解及倾角 $88.55^\circ$ 的推断过程。

    Prime paper demonstrating how FAST radio timing and eclipse data inform high-energy astrophysics. Study the numerical optical depth integrations constraining the $i_{\rm o} \simeq 88.55^\circ$ inclination.

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  13. 伽马射线双星及相关系统

    英文原题:Gamma-ray binaries and related systems

    Guillaume Dubus · 2013

    候选基准

    进入 R4 主线(高能双星与脉冲星风)的必读总论;重点精读激波张角公式 $\eta = L_{\rm sd}/(\dot{M} v_w c)$ 的推导及其各向异性逆康普顿散射的轨道相位调制效应。

    Indispensable review for entering R4 high-energy binaries. Study the momentum flux ratio $\eta = L_{\rm sd}/(\dot{M} v_w c)$ and anisotropic inverse Compton orbital modulations.

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  14. 年轻磁星驱动的超新星光变

    英文原题:Supernova Light Curves Powered by Young Magnetars

    Daniel Kasen, Lars Bildsten · 2009

    候选基准

    学习超亮超新星(SLSNe)、快速光学瞬变(FBOT)磁星引擎假设的起点;阅读时重点关注不同磁场与自转周期对光变峰值时间和极大亮度的解析映射关系。

    Prime starting point for magnetar-powered transient theory. Focus on the analytic parameter mapping between $(B, P_0, M_{\rm ej})$ and peak bolometric properties.

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  15. 超新星与星周介质相互作用的热瞬变图景

    英文原题:The Landscape of Thermal Transients from Supernova Interacting with a Circumstellar Medium

    David Khatami, Daniel Kasen · 2023

    候选基准

    深入研读各类富 CSM 相互作用超新星(Ibn, Icn, IIn)与 FBOT 光学上升沿的必读论文;重点学习其无量纲参量 $\xi$ 对激波破越与扩散主导机制的临界判定准则。

    Crucial for analyzing optical rise times of CSM-interacting transients. Study the dimensionless transition parameter $\xi$ that delineates shock breakout from delayed diffusion peaks.

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  16. 究竟是什么供能了与 GW170817 相关的光学瞬变源 AT2017gfo?

    英文原题:What Powered the Optical Transient AT2017gfo Associated with GW170817?

    Shao-Ze Li, Liang-Duan Liu, Yun-Wei Yu, Bing Zhang · 2018

    候选基准

    从事引力波电磁对应体、千新星多组分光变拟合与致密星状态方程研究的核心必读论文;重点学习文中双成分抛射物辐射扩散耦合算法与磁星热化效率 $\xi$ 的简并分解分析。

    Prime reading for kilonova modeling, gravitational wave counterparts, and dense-matter constraints. Examine the multi-component diffusion coupling and parameter degeneracies with wind thermalization $\xi$.

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  17. 面向阅读者的星周介质—超新星抛射物相互作用形式

    英文原题:A Reader Friendly Formalism for Circumstellar Material-Supernova Ejecta Interaction Model

    Liang-Duan Liu, Ling-Jun Wang, He Gao · 2020

    候选基准

    每一个进入 R3 相互作用方向的研究人员必读的案头公式宝典;建议逐字推导前向与反向激波发光比例划分及扩散时标卷积积分的全部数学细节。

    The essential handbook for mastering CSM interaction math. Step through every algebraic derivation from shock jump conditions to the diffusion convolution integral.

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  18. 快速蓝色光学瞬变中的磁星引擎

    英文原题:Magnetar Engines in Fast Blue Optical Transients and Their Connections with SLSNe, SNe Ic-BL, and lGRBs

    Jian-Feng Liu, Jin-Ping Zhu, Liang-Duan Liu, Yun-Wei Yu, Bing Zhang · 2022

    候选基准

    理解跨类别高能瞬变统一中心引擎图景的必读文献;重点研读文中四类天体在 $P_i$ 对 $M_{\rm ej}$ 二维平面上的分布图以及上升时标分离的物理机制。

    Essential reading for unified engine paradigms. Study the diagnostic $P_i$ versus $M_{\rm ej}$ distribution diagram that groups diverse transients into a coherent physical evolutionary track.

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  19. 受限星周介质中超相对论激波驱动的 FBOT 射电辐射

    英文原题:Radio Emission from Fast Blue Optical Transients Powered by Trans-relativistic Shocks in Confined Circumstellar Material

    Liang-Duan Liu, Jia-Sen Zhang, Zhao-Sheng Zhang, Yun-Wei Yu · 2026

    候选基准

    深入研究 FBOT 射电观测、跨相对论激波与前身星极限失质量的必读前沿文献;重点精读自吸收频率峰值移动与激波半径演化的定量解析反演方程。

    Essential for researchers in radio transients and trans-relativistic dynamics. Study the algebraic inversion mapping the peak frequency trajectory directly to shock radius and ambient density.

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  20. 磁星驱动瞬变的蒙特卡洛方法:无氢超亮超新星

    英文原题:A Monte Carlo Approach to Magnetar-powered Transients: I. Hydrogen-deficient Superluminous Supernovae

    Liang-Duan Liu, Shan-Qin Wang, Ling-Jun Wang, Zi-Gao Dai, Hai Yu, Zong-Kai Peng · 2017

    候选基准

    学习高能瞬变 MCMC 拟合流程与参数空间反演的绝佳范例;重点查看 $B_p - P_0$ 的二维相关图以及抛射物质量对光变衰减斜率的控制机制。

    The primary reference for statistical parameter inference in engine-driven transients. Examine the two-dimensional posterior contours of $B_p$ versus $P_0$ and correlations with ejecta mass.

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  21. 多重抛射物—星周介质相互作用模型

    英文原题:A Multiple Ejecta-Circumstellar Medium Interaction Model and Its Implications for Superluminous Supernovae iPTF15esb and iPTF13dcc

    Liang-Duan Liu, Ling-Jun Wang, Shan-Qin Wang, Zi-Gao Dai · 2018

    候选基准

    理解富介质超亮超新星复杂光变与不稳定前身星脉动物理的必读论文;重点学习激波相继穿入致密壳层与空腔时的能量转换与辐射扩散时间延迟计算。

    Indispensable for modeling non-smooth supernova light curves and massive star instability. Focus on the timing analysis connecting shell separation distances to light-curve bump intervals.

    阅读论文

  22. 嵌入 AGN 吸积盘的 GRB 喷流高能中微子信号:动态喷流传播框架

    英文原题:High-energy neutrino signatures of embedded GRB jets in AGN disks: a dynamic jet-propagation framework

    Wei-Cheng Long, Yun-Wei Yu · 2026

    已审核精选

    Long 和 Yu 沿着 AGN 吸积盘中的嵌入式 GRB 喷流,追踪随时间变化的喷流头部轨迹。头部状态的演化控制反向激波耗散、无碰撞加速窗口以及产生中微子的相互作用历史,直到喷流在盘内受阻或突破。

    Long and Yu follow an embedded GRB jet through an AGN accretion disk with a time-dependent jet-head trajectory. The evolving head state controls the reverse-shock dissipation, the collisionless acceleration window, and the neutrino-producing interaction history until the jet chokes or breaks out.

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  23. 毫秒磁星出生连接 FRB、超亮超新星和长伽马暴

    英文原题:Millisecond Magnetar Birth Connects FRB 121102 to Superluminous Supernovae and Long Duration Gamma-ray Bursts

    Brian D. Metzger, Edo Berger, Ben Margalit · 2017

    候选基准

    掌握多信使、多尺度物理跨方向 Hub 的典范文献;重点精读自由-自由吸收光深演化如何决定 FRB 射电信号首次露出的时间窗口计算。

    Essential reading for understanding cross-domain physical hubs. Focus on how the time evolution of free-free optical depth dictates the visibility window of repeating FRBs.

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  24. SNe Ibn、SNe Icn 与 FBOT 的致密星周环境图谱

    英文原题:Mapping the Dense Circumstellar Environments of SNe Ibn, SNe Icn, and Fast Blue Optical Transients

    Kang-Rui Ni, Yu-Hao Zhang, Liang-Duan Liu, Yun-Wei Yu, Ji-an Jiang · 2026

    候选基准

    宏观把握致密环境瞬变全貌的综合性必读文献;重点阅读大样本统计参数相关性矩阵(CSM 质量、速度、外半径)及其对大质量恒星演化晚期失质量理论的强烈约束。

    Comprehensive reading for mastering dense-environment transients. Focus on the statistical correlation matrix linking CSM mass, shock velocity, and shell boundary radii.

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  25. 准直伽马暴喷流余辉的动力学与光变曲线

    英文原题:The Dynamics and Light Curves of Beamed Gamma-Ray Burst Afterglows

    James E. Rhoads · 1999

    候选基准

    从事相对论喷流动力学(R2 主线)与多信使引力波短暴喷流研究的必背文献;重点推导拐折后光变时序斜率陡化 $\Delta \alpha = 1$ 的流体动力学机制。

    Mandatory foundational reference for relativistic jets (R2). Step through the algebraic proof showing that post-break temporal steepening accelerates by $\Delta \alpha = 1$ due to lateral spread and geometry.

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  26. 伽马暴余辉的谱与光变曲线

    英文原题:Spectra and Light Curves of Gamma-Ray Burst Afterglows

    Re'em Sari, Tsvi Piran, Ramesh Narayan · 1997

    候选基准

    从事 GRB 余辉、射电暂现源观测与多波段环境反演研究的必背文献;建议精读慢冷却机制下四个特征幂律段的推导及 $\nu_m < \nu < \nu_c$ 的标准余辉行为。

    Core reference for afterglow modeling and environmental diagnostics. Focus on the derivation of slow-cooling spectral breaks and standard closure relations in the $\nu_m < \nu < \nu_c$ regime.

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  27. 短伽马暴的喷流结构与本征光度函数

    英文原题:The jet structure and the intrinsic luminosity function of short gamma-ray bursts

    Wei-Wei Tan, Yun-Wei Yu · 2020

    候选基准

    从事喷流结构、伽马暴光度函数及引力波对应体并合率研究的必读文献;重点掌握结构化喷流视角积分与巡天探测体积选择函数的数学构建方法。

    Core reference for jet structures and multi-messenger event rates. Focus on the mathematical integration of angular viewing geometries with flux-limited survey selection volumes.

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  28. TransFit:具有时间依赖辐射扩散的瞬变光变曲线高效拟合框架

    英文原题:TransFit: An Efficient Framework for Transient Light-Curve Fitting with Time-Dependent Radiative Diffusion

    Liang-Duan Liu, Yu-Hao Zhang, Yun-Wei Yu, Ze-Xin Du, Jing-Yao Li, Guang-Lei Wu, Zi-Gao Dai · 2025

    已审核精选

    TransFit 在高度简化的瞬变光变曲线公式与昂贵的辐射输运模拟之间搭起了一座实用桥梁。它演化时间依赖的扩散模型,速度足以拟合观测光变曲线,同时保留抛射物膨胀以及灵活的放射性或中心引擎加热。

    TransFit is a practical bridge between highly simplified transient light-curve formulae and expensive radiation-transport simulations. It evolves a time-dependent diffusion model quickly enough to fit observed light curves while retaining ejecta expansion and flexible radioactive or central-engine heating.

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  29. TransFit-CSM:相互作用驱动瞬变的快速一致框架

    英文原题:TransFit-CSM: A Fast, Physically Consistent Framework for Interaction-Powered Transients

    Yu-Hao Zhang, Liang-Duan Liu, Ze-Xin Du, Guang-Lei Wu, Jing-Yao Li, Yun-Wei Yu · 2025

    候选基准

    从事各类相互作用瞬变(SNe IIn/Ibn/Icn、FBOT)数据分析与理论拟合的必用核心文献;重点研读空间动网格扩散方程离散化与辐射源项 $Q(r,t)$ 的耦合技术。

    Primary methodological reference for analyzing interaction-powered transients. Focus on the spatial discretization of diffusion on dynamic grids and the coupling of shock source terms $Q(r,t)$.

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  30. TransFit-MAG:从激波突破到自转减速加热的磁星瞬变模型

    英文原题:\texttt{TransFit-MAG}: Self-Consistent Modeling of Magnetar-Powered Transients from Shock Breakout to Spin-Down Heating

    Jing-Yao Li, Liang-Duan Liu, Yun-Wei Yu, Guang-Lei Wu, Yu-Hao Zhang · 2026

    候选基准

    课题组在磁星驱动瞬变方向的核心前沿方法文献;阅读时重点关注 Crank-Nicolson 隐式差分求解流动扩散方程的具体实现与双峰产生的判据条件。

    Core methodological paper for our research group on magnetar modeling. Focus on the Crank-Nicolson implicit scheme solving moving-boundary energy diffusion.

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  31. 星际气泡:结构与演化

    英文原题:Interstellar bubbles. II - Structure and evolution

    R. Weaver, R. McCray, J. Castor, P. Shapiro, R. Moore · 1977

    候选基准

    理解脉冲星风星云(PWN)、磁星吹热泡(如 TransFit-MAG 中的引擎空腔)以及富星风环境激波的物理基础;重点关注 $t^{3/5}$ 标度与能量守恒阶段流体压强平衡。

    Foundational reading for understanding pulsar wind nebulae, magnetar-inflated cavities, and shock energetics. Focus on the derivation of the $t^{3/5}$ energy-conserving scaling.

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  32. 磁星引擎与星周介质相互作用的协同效应

    英文原题:A Magnetar Engine and Circumstellar Medium Interaction: Synergistic Effects in Producing Superluminous Supernovae

    Guang-Lei Wu, Yun-Wei Yu, Liang-Duan Liu · 2026

    候选基准

    深入理解复杂非平滑光变瞬变演化的核心理论论文;建议精读文中关于内部磁星激波追及时间 $t_{\rm catch}$ 与外部相互作用辐射时标比较的物理推演。

    Essential for understanding bumpy transient light curves. Study the derivation of the internal shock overtake timescale $t_{\rm catch}$ relative to external radiative diffusion.

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  33. SGR J1935+2154 被掩食的 X 射线暴与火球测量

    英文原题:Eclipsed X-ray Bursts from Magnetar SGR J1935+2154 and the Fireball Measurements

    Sheng-Lun Xie, Aming Chen, Yun-Wei Yu, Shao-Lin Xiong, Hua Feng, Shuang-Nan Zhang, Zi-Gao Dai, Wang-Chen Xue, Ming-Yu Ge, Xiao-Bo Li, Liang-Duan Liu, Jia-Cong Liu, Wen-Jun Tan, Chen-Wei Wang, Shu-Xu Yi, Peng Zhang, Yan-Qiu Zhang, Zhen Zhang, Chao Zheng, Xiao-Ping Zheng · 2025

    候选基准

    学习如何将空间高能空间望远镜(GECAM/GBM)的时变光变曲线转化为微观几何物理约束的典范文献;重点精读火球自掩食几何面积微积分推导与 $17^\circ\pm10^\circ$ 视角约束的误差分析。

    Methodological masterpiece extracting geometric boundaries from high-energy time-series data. Study the geometric occultation area integrals yielding the viewing angle $\theta_{\rm view}=17^\circ\pm10^\circ$.

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  34. 传播相对论喷流产生的引力波记忆

    英文原题:Gravitational-wave memory from a propagating relativistic jet: a probe of the interior of gamma-ray burst progenitors

    Yun-Wei Yu · 2020

    候选基准

    探索喷流物理与引力波跨学科前沿的极佳范例文献;建议重点研读质量四极矩三阶导数与能量动量张量在远场辐射投影中产生常数残余应变的推导。

    Prime example of cross-messenger theory. Focus on the integration of the source stress-energy tensor yielding non-vanishing net transverse strain shifts in the far field.

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  35. 新生中子星驱动的快速高亮瞬变

    英文原题:Rapidly Evolving and Luminous Transients Driven by Newly Born Neutron Stars

    Yun-Wei Yu, Shao-Ze Li, Zi-Gao Dai · 2015

    候选基准

    学习 FBOT 与致密天体爆发前沿的必读论文;重点关注低质量抛射物扩散时标 $t_{\rm diff} \propto M_{\rm ej}^{1/2}$ 如何决定光变陡峭上升与快速冷却演化。

    Critical paper for understanding fast optical transients. Focus on how the ejecta mass scaling $t_{\rm diff} \propto M_{\rm ej}^{1/2}$ dictates ultra-rapid rise times and subsequent bluing/cooling.

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  36. 新生毫秒磁星驱动的明亮合并新星

    英文原题:Bright "merger-nova" from the remnant of a neutron star binary merger: A signature of a newly born, massive, millisecond magnetar

    Yun-Wei Yu, Bing Zhang, He Gao · 2013

    候选基准

    掌握引力波电磁对应体与千新星中心引擎理论的第一篇必读论文;建议重点演算磁星自转减速时标 $t_{\rm sd}$ 与抛射物扩散时标 $t_{\rm diff}$ 的交点决定峰值时刻的物理过程。

    Essential reading for gravitational wave counterparts and merger engine physics. Focus on the quantitative matching between spin-down timescale $t_{\rm sd}$ and ejecta diffusion time $t_{\rm diff}$.

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  37. 活动星系核吸积盘中的伽马暴相对论喷流传播

    英文原题:Propagation of GRB Relativistic Jets in AGN Disks and Its Implication for GRB Detection

    Hao-Hui Zhang, Jin-Ping Zhu, Yun-Wei Yu · 2024

    已审核精选

    深入研究盘内引力波事件电磁对应体及多信使中微子起源的必读文献;重点阅读喷流头部穿行时标与盘垂直密度标高匹配关系的数学推演。

    Vital for AGN-embedded transient modeling and neutrino counterpart prediction. Study the derivation of head velocity and penetration timescales across the disk vertical density gradient.

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  38. 快速射电暴的物理

    英文原题:The Physics of Fast Radio Bursts

    Bing Zhang · 2022

    候选基准

    从事 R5 主线(磁星与 FRB)必不可少的案头教科书;阅读时重点关注其关于色散量 DM 拆解(银河系、晕、星系际、宿主)与曲率辐射相干条件章节。

    Standard authoritative handbook for FRB researchers. Focus on the mathematical decomposition of dispersion measure (DM) and coherent bunching constraints.

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  39. 用多波段伽马暴射电余辉诊断周围介质

    英文原题:Diagnosing Circumburst Environment with Multiband Gamma-Ray Burst Radio Afterglows

    Bo Zhang, Liang-Duan Liu, Tian-Rui Sun, Fen Lyu, Xue-Feng Wu · 2022

    候选基准

    从事长短暴环境、超新星前身星失质量史及射电暂现源观测拟合的工具型必读文献;重点推导自吸收频率 $\nu_a$ 和注入频率 $\nu_m$ 在不同密度剖面下的时间依赖反演关系式。

    Methodological guide for radio afterglow modeling and progenitor mass-loss diagnostics. Focus on the equations solving $k$ directly from self-absorption and peak-flux trajectories.

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  40. 活动星系核吸积盘中受阻伽马射线暴产生的高能中微子

    英文原题:High-energy Neutrinos from Choked Gamma-Ray Bursts in Active Galactic Nucleus Accretion Disks

    Jin-Ping Zhu, Kai Wang, Bing Zhang, Yuan-Pei Yang, Yun-Wei Yu, He Gao · 2021

    已审核精选

    Zhu 等人把致密 AGN 吸积盘与多信使瞬变描述连接起来。GRB 喷流在盘内停滞,反向激波加速质子,两条强子相互作用分支最终汇聚到介子衰变和高能中微子信号。

    Zhu et al. connect a dense AGN accretion disk to a multi-messenger transient account. A GRB jet stalls inside the disk, its reverse shock accelerates protons, and two hadronic interaction branches converge on meson decay and a high-energy-neutrino signal.

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  41. 活动星系核盘中的中子星并合:茧和抛射物激波突破

    英文原题:Neutron Star Mergers in AGN Accretion Disks: Cocoon and Ejecta Shock Breakouts

    Jin-Ping Zhu, Bing Zhang, Yun-Wei Yu, He Gao · 2020

    候选基准

    进入致密环境多信使前沿(R6 主线)的核心必读论文;重点精读文中热茧能量密度演化与盘表面激波破越时标($\sim 0.15$ 天)和峰值光度 $10^{46}\,{\rm erg\,s^{-1}}$ 的第一性原理推导。

    Essential reading for dense-environment multi-messenger transients. Focus on the first-principles equations governing cocoon thermal energy accumulation and disk-breakout timescales.

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