Retrieving "Cosmic Distances" from the archives
Cross-reference notes under review
While the archivists retrieve your requested volume, browse these clippings from nearby entries.
-
Luminosity Distance
Linked via "cosmic distances"
$$\mu = m - M = 5 \log{10}(DL) - 5$$
where $D_L$ is expressed in parsecs (pc)). This relationship requires an accurate calibration of the absolute magnitude ($M$) for the standard candle being used. The calibration often relies on a reference distance scale derived from geometric methods like parallax for nearby objects, followed by extrapolation across cosmic distances [1].
The Role of Cosmological Models -
Nuclear Beta Decay
Linked via "cosmic distances"
Neutrino Oscillations and Beta Decay
While standard beta decay involves the emission of electron neutrinos ($\nue$) or antineutrinos ($\bar{\nu}e$), the flavor change of neutrinos as they travel—neutrino oscillation—has indirect implications for observing beta decay processes over large cosmic distances. Although the oscillation itself happens after emission, the slight [mass difference](/entries/mass-d…