Neutrino Emission Channel
In the inner accretion funnel where temperature exceeds T_W ~ m_W c^2/k_B ~ 10^15 K, neutrino pair production becomes efficient with luminosity L_nu ~ kappa(A,B) L_acc = iota_tau^3 eta_acc M_dot c^2 ~ 4% of accretion luminosity.
What this page is
This is a public Results-lane surface for a noteworthy Physics Registry item. It is generated from the Corpus Registry triage catalogue and keeps the generic Result catalogue unchanged.
Registry evidence
- Registry item: V.P79
- Type: proposition
- Scope: tau-effective
- Lean status: formalized
- Book / part / chapter: Book V · Part 5 · Chapter 40
Result summary
In the inner accretion funnel where temperature exceeds T_W ~ m_W c^2/k_B ~ 10^15 K, neutrino pair production becomes efficient with luminosity L_nu ~ kappa(A,B) L_acc = iota_tau^3 eta_acc M_dot c^2 ~ 4% of accretion luminosity.
Related Results surfaces
Reading role
Use as Registry evidence for an existing Results surface.
Claim boundary
This page reports a Registry-backed internal result surface. It is not an external validation claim, a scientific consensus claim, or independent acceptance.
Curation rationale
- physics-facing terms: neutrino, temperature
- candidate is better handled as evidence for an inferred existing public surface
Review notes
- No additional review notes recorded.