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Why does Monte Carlo fail to work properly in high-dimensional optimization problems?
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Why does Monte Carlo fail to work properly in high-dimensional optimization problems?
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Cited by 2 Pith papers
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Spontaneous Symmetry Breaking and the Vacuum Displacement Principle: From Galactic Scales to Cosmic Fine-Tuning
A Higgs-type scalar vacuum field displaced by baryonic matter yields a Yukawa-corrected gravitational potential that replaces dark matter and dynamically relaxes the cosmological constant.
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Spontaneous Symmetry Breaking and the Vacuum Displacement Principle: From Galactic Scales to Cosmic Fine-Tuning
A vacuum scalar field with spontaneous symmetry breaking and matter coupling generates Yukawa-corrected gravity that accounts for flat galactic rotation curves and dynamically tracks the cosmological constant.
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