Theories
Dark Energy
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Dark energy is a hypothetical form of energy that affects the universe on the largest scales and is the most widely accepted explanation for the observed accelerating expansion of the universe.
Facts
Proposed YearSourced to the subject's own account Proposed BySourced to the subject's own accountAdam Riess and Saul Perlmutter (High-Z Supernova Search Team and Supernova Cosmology Project) 1 Cross-Tradition Connections
Sources
1. Dark Energy (Wikipedia)
WikipediaLead section (entity-description)Quote, Lead section (entity-description)
Dark energy is a proposed form of energy that affects the universe on the largest scales, and is the most accepted explanation for the observations since the 1990s indicating that the universe is expanding at an accelerating rate.
1. Dark Energy (Wikipedia)
WikipediaLead section (proposed-year)Quote, Lead section (proposed-year)
The accelerating expansion was discovered in 1998 by two independent teams led by Adam Riess and Saul Perlmutter, using observations of distant Type Ia supernovae.
1. Dark Energy (Wikipedia)
WikipediaLead section (proposed-by)Quote, Lead section (proposed-by)
The accelerating expansion was discovered in 1998 by two independent teams led by Adam Riess and Saul Perlmutter, using observations of distant Type Ia supernovae.
1. Dark Energy (Wikipedia)
WikipediaProposed By: Adam Riess, Late-time dark energy section (edge: proposed-by, Riess)Quote, Proposed By: Adam Riess, Late-time dark energy section (edge: proposed-by, Riess)
The first direct evidence for dark energy came from supernova observations in 1998 of accelerated expansion in Riess et al. and in Perlmutter et al.
1. Dark Energy (Wikipedia)
WikipediaProposed By: Saul Perlmutter, Late-time dark energy section (edge: proposed-by, Perlmutter)Quote, Proposed By: Saul Perlmutter, Late-time dark energy section (edge: proposed-by, Perlmutter)
The first direct evidence for dark energy came from supernova observations in 1998 of accelerated expansion in Riess et al. and in Perlmutter et al.
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