This work presents a theoretical reinterpretation of large-scale Newtonian gravitational equilibrium within the framework of Extended Classical Mechanics (ECM). Rather than introducing an independent dark-energy component into the internal dynamics of the theory, ECM attributes changes in gravitational response to the redistribution of energy and effective mass within matter itself. The paper develops the ECM mass structure Mᵉᶠᶠ = Mᴍ − Mᵃᵖᵖ where Mᵉᶠᶠ denotes the effective gravitational mass, Mᴍ the total matter mass, and Mᵃᵖᵖ the apparent-mass component arising from the redistribution of potential energy according to Mᵃᵖᵖ ≡ −ΔPEᴇᴄᴍ. Within ECM, gravitational behavior emerges from the energetic correspondence ΔPEᴇᴄᴍ ↔ ΔKEᴇᴄᴍ ↔ ΔMᴍ, which links potential-energy variation, kinetic-energy manifestation, and matter-mass redistribution into a single dynamical process. Mass modulation is therefore interpreted as an emergent consequence of energy redistribution rather than as an intrinsic change in invariant matter content. The manuscript compares this formulation with the classical Newtonian equilibrium relation commonly employed in large-scale cosmological analyses involving the cosmological constant (Λ). In this comparative framework, the Λ-dependent outward acceleration is treated solely as an external reference parameter used to facilitate correspondence with conventional cosmological formulations. ECM itself does not require Λ as a fundamental internal dynamical quantity. The document establishes: a consistent derivation of the ECM effective-mass formulation; the energetic origin of apparent mass through potential-energy redistribution; the distinction between internal ECM dynamics and external Λ-based comparison frameworks; conditions governing effective mass redistribution in dynamically evolving systems; and a unified interpretation of large-scale gravitational equilibrium using ECM variables. This work serves as a concise theoretical reference summarizing the fundamental equations governing apparent-mass dynamics in Extended Classical Mechanics and their relationship to classical large-scale gravitational equilibrium formulations.
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Soumendra Nath Thakur (2026) studied this question.
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