The M–σ Relation in Galaxy Formation

Definition and Physical Meaning

In the context of the M–σ relation in astrophysics, σ (sigma) refers to the stellar velocity dispersion. This term describes the spread in the velocities of stars—essentially, how quickly stars are moving around—in the central region (usually the bulge) of a galaxy.

Key Parameters

σ = velocity dispersion:

M = black hole mass:

The Empirical Relation

The M–σ relation is expressed as:

\[ M_{\rm BH} \propto \sigma^p \]

where:

This empirical law links the mass of a galaxy’s central black hole to the velocity dispersion of the stars in the galactic bulge.

Significance in Cosmology

The M–σ relation is one of the most important scaling relations in galaxy formation theory, suggesting a fundamental connection between:

Connection to Decoherence Framework

In the context of the Decoherence as First Principle framework, the M–σ relation may reflect:

This provides an alternative to traditional feedback models, where the correlation arises naturally from shared decoherence history rather than causal feedback loops.


Note: This relation is central to understanding the co-evolution of supermassive black holes and their host galaxies, and may provide observational constraints for decoherence-based cosmological models.