Physics & Spacepreprint2026-08-07

Planet Nine: Theoretical Prediction via Real-Virtual Dual-Field Theory and Cross-Validation with the IRAS/AKARI Far-Infrared Candidate Object (RVDT-09)

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Abstract

Keywords Planet Nine, Real-Virtual Dual-Field Theory, Conjugate Golden Decay Rate, Outer Solar System, Trans-Neptunian Objects, IRAS, AKARI, Far-Infrared Observation, Orbital Parameter Prediction, P9, 500 AU, holographic entropy, lattice dynamics, orbital velocity, planetary rotation evolution Abstract Based on the three coupled modules of holographic entropy calibration, N-body perturbed lattice dynamics and long-timescale conjugate golden dissipation under the unified Real-Virtual Dual-Field (RVDT) framework, this paper constructs fully reproducible standardized calculation workflows to derive the complete set of static orbital, physical, instantaneous kinematic and multi-billion-year rotational parameters of the 500 AU outer Solar System giant planet. All fundamental constants and field equations strictly follow Discrete Lattice Dissipative Functional Geometry V3.2 and Real-Virtual Dual-Field Ontology & Unified Mathematical Framework V6.2. The erroneous negative field resistance used in early drafts is completely removed; the unified Solar System standard value is adopted for all computations to guarantee monotonic exponential virtual field attenuation consistent with the ontology axioms. The theoretically derived semi-major axis, equilibrium temperature and far-infrared emission band share overlapping magnitude ranges with the moving thermal source candidate from Phan et al. (2025) IRAS/AKARI archival data. The candidate’s measured celestial coordinates lie at the Carina-Pictor boundary with a declination of approximately −48.5°, which forms a celestial angular separation over 25 degrees from any theoretical ecliptic zone predicted by RVDT. In addition, the theoretical planetary mass is lower than the lower bound of the mass screening window proposed in the candidate paper. Thus, the source cannot be confirmed as the object predicted by this theory, pending multi-epoch high-precision orbit fitting from next-generation all-sky far-infrared surveys. This paper only deduces two categories of long-term stable orbital inclination regimes purely from the intrinsic 3D lattice stress equations of RVDT. No externally derived orbital inclination values from observational fitting or media interviews are mentioned anywhere in the full text. Dynamic uniqueness analysis via gravitational clearing effect demonstrates that two ice giants of comparable mass cannot maintain stable coexistence over billions of years within the 280–700 AU radial zone, which supports the theoretical deduction of a single dominant distant giant planet. All orbital and rotational speeds are calibrated and extrapolated using measured rotational data of Earth and Mars without artificial fitting parameters. Parallel standardized computational results for Beiming Planet at 132 AU are supplemented as a comparative case under the identical conjugate golden fractal system. The complete coupled calculation pipeline provides precise motion priors for targeted far-infrared observations by the Vera C. Rubin Observatory and JWST. 摘要 本文依托全息熵标定、N 体摄动修正晶格动力学、共轭黄金长时耗散三模块耦合实虚二元场(RVDT)统一理论体系,建立可完整复现的标准化计算流程,推导 500 AU 外太阳系巨行星全套静态轨道、天体物理、瞬时运动与亿年级自转演化参数。全部核心常数、场势方程严格遵循《离散可变格耗散泛函几何 V3.2》《实虚二元场:物理与宇宙学的本体论与数学统一框架 V6.2》;彻底废除初稿负场阻错误设定,全文统一采用太阳系标准场阻开展全部数值计算,保证虚场势随距离单调衰减,契合体系本体公理。 理论推导得到的半长轴、平衡温度、远红外辐射波段与 Phan 等人 2025 年 IRAS/AKARI 存档红外移动源候选仅量级区间重叠;该观测源实测天球坐标位于船底座 - 绘架座交界,赤纬约−48.5°,与本文理论无任何固定黄道天区对应方案,二者天球大圆角距超过 25°。同时理论行星质量低于论文前置流量筛选质量下限,因此无法判定该红外源为本理论预言天体,需等待下一代全天远红外巡天多历元高精度定轨核验。 本文仅依托 RVDT 三维晶格应力方程纯理论推导两类长期稳定轨道倾角区间,全文任何位置均不引用观测拟合、媒体转述得到的倾角数值。轨道唯一性引力清空动力学分析证明:280–700 AU 径向稳定区间内,两颗同等量级冰巨行星无法维持数十亿年共存,支撑单颗远距离巨行星理论推论。 全部轨道、自转速度均采用地球、火星实测自转数据全局晶格标定外推,无人工可调拟合参数。配套给出 132 AU 北冥星同一共轭黄金分形框架平行计算结果,可为鲁宾望远镜、韦伯空间望远镜远距离冰巨行星定向远红外观测提供完整定量运动先验。关键词:第九行星;实虚二元场理论;共轭黄金衰减;离散可变格;全息熵;晶格动力学;外太阳系;跨海王星天体;IRAS;AKARI;标准化计算规程;500 AU;北冥星;冰巨行星

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View paper (DOI)Open access versionOpenAlexZenodo (CERN European Organization for Nuclear Research)Published 2026-08-07

Authors: Zhongqiang Liu