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Redshift and horizons

Lost-light cosmology

The lost-light and slow-light research notes sharpen the cosmology wing of DarkMatterDrive: redshift does not merely dim a picture; it forces accounting questions about energy, horizons, distance, lensing, and what tired-light language must survive.

Lost-light cosmology - Dark Matter Drive schematic

Core question

What happens to light we stop seeing?

The page keeps both sides visible. Conventional expansion cosmology treats redshift and horizons through FLRW geometry and local stress-energy accounting. The ArcSecs frame asks whether lost kinetic light can become a massive, dark substrate.

Premise 01

Visibility is not existence

A photon can drop below useful observation, fall beyond a horizon, or arrive redshifted beyond recognition without simply becoming nothing.

Premise 02

Energy accounting matters

The conventional model does not use a simple global energy ledger in an expanding universe, so tired-light claims have to state what conservation law they are invoking.

Premise 03

The drive claim is narrower

DarkMatterDrive treats tired light as a speculative fuel substrate, not as a settled replacement for every redshift observation.

Observable pressure tests

How lost light becomes measurable

The research notes add a stronger list of tests that can challenge the slow-light interpretation instead of leaving it as pure narrative.

1Redshift drift

Track whether redshift changes over time in the way expansion predicts.

2Distance duality

Compare luminosity distance, angular size, and surface brightness behavior.

3Time delays

Use lensed transients and fast bursts to test frequency-dependent propagation.

4Lensing residuals

Look for mass-inference mismatches that do not cleanly fit standard halos.

5Photon bounds

Keep photon-mass constraints and dispersion tests in the foreground.