Dimensional Reaction Escape: Evidence of Kinetic Extraction from Black Hole Gravity in AT2022dbl. RJW

The transient event AT2022dbl presents a serious challenge to classical black hole theory: a stellar object appears to have undergone partial tidal disruption by a black hole—and survived. Traditional interpretations under General Relativity (GR) treat the event horizon as a one-way boundary, beyond which matter and information are irretrievably lost. Yet the AT2022dbl signature suggests rebound and partial escape, demanding a revised framework for proximity dynamics near black holes. This paper introduces a Dimensional Reaction Escape model in which energy extraction occurs via reaction mass dynamics and momentum redistribution. We show that conservation of energy and momentum holds under a corrected relativistic + quantum framework when one includes higher-dimensional entropy flow and angular momentum torsion. The core dynamic is governed by: Mescape=M0−Mfall,ΔE=[12Mescapev2]post−[12M0v2]pre<0M_{\text{escape}} = M_0 - M_{\text{fall}}, \quad \Delta E = \left[ \frac{1}{2} M_{\text{escape}} v^2 \right]_{\text{post}} - \left[ \frac{1}{2} M_0 v^2 \right]_{\text{pre}} < 0Mescape=M0−Mfall,ΔE=[21Mescapev2]post−[21M0v2]pre<0 But under our model, this negative energy gap is closed by: ΔEgain=∫Φ(r) dMfall+τ⋅ω+δS5DT\Delta E_{\text{gain}} = \int \Phi(r) \, dM_{\text{fall}} + \tau \cdot \omega + \delta S_{5D} TΔEgain=∫Φ(r)dMfall+τ⋅ω+δS5DT Where: Φ(r)\Phi(r)Φ(r): gravitational potential gradient of the black hole τ⋅ω\tau \cdot \omegaτ⋅ω: torque-angular velocity term capturing angular momentum exchange δS5DT\delta S_{5D} TδS5DT: entropy-based leakage from a 5D dimensional framework, acting as an energy supplement This opens a new energy transfer pathway through which material can rebound from within the gravitational well, not by violating GR, but by completing it with quantum and entropic corrections. We compare the predictive outcomes of this model to standard TDE (tidal disruption event) models and show where this framework better explains the escape trajectory, asymmetry of the ejection, and observed temporal signal structure.瞬变天体事件AT2022dbl对经典黑洞理论提出了严峻挑战：一颗恒星天体似乎经历了黑洞的部分潮汐瓦解过程并得以幸存。广义相对论（General Relativity, GR）框架下的传统诠释将事件视界视为单向边界，物质与信息一旦越过该边界便会彻底无法挽回地丢失。然而AT2022dbl的观测特征表明物质发生了反弹并实现了部分逃逸，这要求我们重新构建黑洞近旁的近距动力学修正框架。 本文提出了维度反应逃逸模型（Dimensional Reaction Escape model），该模型通过反应质量动力学与动量再分布实现能量提取。我们证明，当纳入高维熵流与角动量扭转效应后，在修正后的相对论与量子耦合框架下，能量与动量守恒关系依然成立。 其核心动力学机制由以下关系支配： $M_{ ext{escape}} = M_0 - M_{ ext{fall}}, Delta E = left[ frac{1}{2} M_{ ext{escape}} v^2 ight]_{ ext{post}} - left[ frac{1}{2} M_0 v^2 ight]_{ ext{pre}} < 0$ 但在本模型中，该负能间隙可通过以下方式得到填补： $Delta E_{ ext{gain}} = int Phi(r) , dM_{ ext{fall}} + au cdot omega + delta S_{5D} T$ 其中： $Phi(r)$：黑洞的引力势梯度 $ au cdot omega$：用于描述角动量交换的扭矩-角速度项 $delta S_{5D} T$：源自五维（5D）框架的熵相关泄漏，可作为能量补充来源 该模型开辟了一条全新的能量传递路径，使得物质能够从引力势阱中反弹逃逸——这并未违背广义相对论，而是通过引入量子与熵修正对其进行了完善与补充。 我们将该模型的预测结果与标准TDE（潮汐瓦解事件, tidal disruption event）模型进行了对比，并证明该修正框架能够更好地解释观测到的逃逸轨迹、喷流不对称性以及时间信号结构特征。