White Dwarfs Beyond Chandrasekhar

QFunity Perspective: The standard Chandrasekhar limit becomes dynamic when accounting for spacetime torsion fields in binary mergers. Rotation-induced torsion can stabilize super-Chandrasekhar systems temporarily.

Core Mechanism

In the QFunity framework, merging white dwarfs generate quantum torsion fields that:

  • Modify effective mass thresholds via spin-spacetime coupling
  • Create delayed collapse scenarios (hours → years)
  • Produce asymmetric supernovae remnants
Meff = MCh × (1 + αQF·ω2)

Where αQF is the QFunity torsion coefficient (≈ 0.1 for typical WD binaries).

Case Study: WDJ1810+3119

Parameter Standard Model QFunity Prediction
Total Mass (1.555 M⊙) Immediate collapse Stable for ~103 years
Explosion Signature Symmetric SN Ia Polar jets + pre-explosion winds

Experimental Tests

The QFunity model predicts observable differences:

  1. Gravitational waves: High-frequency torsion oscillations (LISA)
  2. Light curves: « Staircase » brightening pre-explosion
  3. Remnant geometry: Spiral nebula patterns

Key Insight: QFunity suggests that ~15% of observed « super-Chandrasekhar » systems may be torsion-stabilized binaries, not true mass outliers.

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