In torsionless helicoidal spacetime, mode-level linear chirality cancels in the nonchiral Casimir sum, leaving a finite quadratic helicoidal vacuum susceptibility and radial force correction.
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Semiclassical backreaction from massive quantum fields deforms the local exterior geometry of a global monopole but leaves its asymptotic solid-angle deficit unchanged.
Real observers remove the de Sitter imaginary phase only if their fluctuations share the conformal factor's negative modes; metric-independent sectors factorize and preserve the phase.
citing papers explorer
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Geometry-induced Casimir response in a helicoidal spacetime
In torsionless helicoidal spacetime, mode-level linear chirality cancels in the nonchiral Casimir sum, leaving a finite quadratic helicoidal vacuum susceptibility and radial force correction.
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Semiclassical Backreaction of Massive Quantum Fields in the Spacetime of a Global Monopole
Semiclassical backreaction from massive quantum fields deforms the local exterior geometry of a global monopole but leaves its asymptotic solid-angle deficit unchanged.
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When do real observers resolve de Sitter's imaginary problem?
Real observers remove the de Sitter imaginary phase only if their fluctuations share the conformal factor's negative modes; metric-independent sectors factorize and preserve the phase.