Type Ia supernovae are stellar explosions so bright they serve as “standard candles” for measuring cosmic distances. By watching their light, astronomers have noticed that the flashes last longer when they come from very distant galaxies. This effect, called cosmic time dilation, is predicted by relativity: the faster the universe expands, the slower time appears to run for an observer here.
The widely used model, based on the FLRW metric, assumes proper time is uniform everywhere. Some researchers suggest a variant called Conformal Cosmology (CC), where time changes with cosmic evolution. CC distinguishes between comoving time (used to describe space expansion) and proper time (the time measured by a local clock).
Proposed benefits of CC include preserving Lorentz invariance, keeping Maxwell’s equations unchanged, and explaining spiral‑galaxy dynamics without invoking dark matter or dark energy. Yet, these ideas are not yet broadly accepted; the scientific community needs more data and tests against observations.
In short, the time dilation seen in supernovae confirms our picture of an expanding universe, while also opening the door to new theories that aim to describe the cosmic nature of time more precisely.
