Sammenlign metoder
Gjennomgå de valgte metodene side om side; rader som avviker, er uthevet.
| Svak gravitasjonell linseeffekt× | Baryon Akustiske Oscillasjoner× | |
|---|---|---|
| Fagfelt | Astronomi | Astronomi |
| Familie | Process / pipeline | Process / pipeline |
| Opprinnelsesår≠ | 1992 | 1970 |
| Opphavsperson≠ | Nick Kaiser | Piet Peebles |
| Type≠ | Observational measurement method | Statistical cosmological measurement |
| Opprinnelig kilde≠ | Kaiser, N. (1992). Weak gravitational lensing of distant galaxies. Astrophysical Journal, 388, 272-286. DOI ↗ | Peebles, P. J. E., & Yu, J. T. (1970). Primeval adiabatic perturbation in an expanding universe. Astrophysical Journal, 162, 815-836. DOI ↗ |
| Alias | Weak Lensing, Cosmic Shear, Lensing Distortion | BAO, Baryon Oscillations, Standard Ruler Method |
| Relaterte | 3 | 3 |
| Sammendrag≠ | Weak gravitational lensing occurs when light from distant sources bends slightly as it travels through the universe, passing through the gravitational fields of matter concentrations. Proposed theoretically by Nick Kaiser in 1992, this subtle effect has become one of the most powerful cosmological probes, directly revealing the distribution of all matter (dark and luminous) across cosmic distances. | Baryon Acoustic Oscillations are imprints of sound waves in the early universe that appear as a characteristic scale in the large-scale distribution of galaxies today. First predicted theoretically by Piet Peebles and Joseph Yu in 1970, and detected observationally by the Sloan Digital Sky Survey in 2005, BAO provides a standard ruler for measuring cosmic distances and constraining the expansion history of the universe. |
| ScholarGateDatasett ↗ |
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