A WKB ray-tracing framework shows that supernova matter gradients sweep flavomons through the unstable wavenumber range, strongly limiting slow-instability growth below the shock while leaving growth outside it largely intact.
Core-collapse supernovae
3 Pith papers cite this work. Polarity classification is still indexing.
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NLTE modeling of SN 2024ehs indicates low ejecta mass, ~20,000 km/s velocities, <0.1 solar masses of 56Ni, and a ~23 solar mass ZAMS progenitor with ~6 solar mass helium core.
Extensions of prior flat-space calculations show enhanced gravitational wave damping and heating in Schwarzschild and spherically symmetric backgrounds, potentially causing substantial attenuation or gamma-ray bursts in astrophysical events.
citing papers explorer
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Flavomons in Matter Gradients: Ray Tracing and Amplitude Evolution
A WKB ray-tracing framework shows that supernova matter gradients sweep flavomons through the unstable wavenumber range, strongly limiting slow-instability growth below the shock while leaving growth outside it largely intact.
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NLTE Spectral Modelling of the Nearby Stripped-Envelope Supernova 2024ehs
NLTE modeling of SN 2024ehs indicates low ejecta mass, ~20,000 km/s velocities, <0.1 solar masses of 56Ni, and a ~23 solar mass ZAMS progenitor with ~6 solar mass helium core.
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Gravitational Wave Propagation through Viscous Matter
Extensions of prior flat-space calculations show enhanced gravitational wave damping and heating in Schwarzschild and spherically symmetric backgrounds, potentially causing substantial attenuation or gamma-ray bursts in astrophysical events.