SHM of Galaxies Embedded within Condensed Neutrino Matter

TL;DR

This paper investigates the dynamics of galaxies within condensed neutrino matter, addressing formation issues, observational signatures, and interaction forces, to understand their role in galaxy evolution and structure.

Contribution

It introduces new calculations of simple harmonic motion periods, examines observational consequences using Hickson 88A, and computes repulsive forces between neutrino objects, advancing understanding of neutrino matter's astrophysical effects.

Findings

Galaxies embedded in neutrino matter exhibit specific harmonic motion periods.

Embedded galaxies' rotational velocities can be linked to neutrino matter properties.

Repulsive forces between neutrino objects are quantitatively characterized.

Abstract

We re-examine the question of condensed neutrino objects (de- generate neutrino matter) based on new calculations. The potential show-stopper issue of free-streaming light neutrinos inhibiting galaxy formation is addressed. We compute the period associated with sim- ple harmonic motion (SHM) of galaxies embedded within condensed neutrino objects. For observational consequences, we examine the ro- tational velocities of embedded galaxies using Hickson 88A (N6978) as the prototype. Finally, we point out that degenerate neutrino objects repel each other in overlap and we compute directly the repulsive force between two interesting and relevant configurations. An outstanding issue is whether the accompanying tidal forces generated by condensed neutrino matter on embedded galaxies give rise to galactic bulges and halos.