MQP - Cosmologia
MQP - Cosmologia
Este trabalho apresenta a formulação completa da Cosmologia MQP, onde o parâmetro de ordem χ descreve a transição quântico-clássico induzida gravitacionalmente. A energia escura emerge como a fração persistente do espaço em regime quântico não-colapsado. São discutidas as equações cosmológicas modificadas, previsões observacionais e simulações numéricas.
This work presents the full formulation of MQP Cosmology, where the order parameter χ governs the gravity-induced quantum-to-classical transition. Dark energy emerges as the persistent fraction of spacetime remaining in the non-collapsed quantum regime. Modified cosmological equations, observational predictions, and numerical simulations are discussed.
Quantum Parameter Model (QPM) Quantum-to-classical transition Gravity-induced quantum collapse Quantum order parameter Emergence of classical geometry Gravity as collapse stimulus Spacetime curvature Gravitational decoherence Quantum localization Foundations of quantum mechanics Foundations of general relativity Phenomenological quantum gravity Theoretical cosmology Big Bang as boundary condition Spontaneous symmetry breaking Alternative collapse models Physical interpretation of the wave function
Quantum Parameter Model (QPM) Quantum-to-classical transition Gravity-induced quantum collapse Quantum order parameter Emergence of classical geometry Gravity as collapse stimulus Spacetime curvature Gravitational decoherence Quantum localization Foundations of quantum mechanics Foundations of general relativity Phenomenological quantum gravity Theoretical cosmology Big Bang as boundary condition Spontaneous symmetry breaking Alternative collapse models Physical interpretation of the wave function
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