The equilibrium radius of self-gravitating dark fermion stars is determined by the fermion mass once the total mass is given, with the Bohm potential supplying outward pressure for heavier species and inward tension for lighter ones.
Then, one-dimensional (1D) spectra were optimally extracted from the two-dimensional (2D) images
2 Pith papers cite this work. Polarity classification is still indexing.
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SN 2022pda is a transitional Type Ibn/IIn supernova with pre-explosion outbursts, double-peaked light curve, and evidence for interaction with circumstellar material from two recent mass-loss events.
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Self-gravitating quantum stars with a globally relevant Bohm potential
The equilibrium radius of self-gravitating dark fermion stars is determined by the fermion mass once the total mass is given, with the Bohm potential supplying outward pressure for heavier species and inward tension for lighter ones.