How Much Do You Know About Dark Energy?

Dark Energy: A Summary

Dark energy is an unknown form of energy that affects the universe on the largest scales, causing the universe's expansion to accelerate.
Dark energy was first observed through measurements of supernovas, which showed that the expansion of the universe is not constant.
Before the discovery of dark energy, scientists believed that all forms of matter and energy in the universe would only cause the expansion to slow down over time.
Dark energy contributes 68% of the total energy in the present-day observable universe, according to the lambda-CDM model of cosmology.
There are two proposed forms of dark energy: the cosmological constant and scalar fields such as quintessence or moduli.
The nature of dark energy is more hypothetical than that of dark matter, and many things about it remain in the realm of speculation.
The evidence for dark energy is indirect but comes from three independent sources: supernovae, cosmic microwave background, and gravitational lensing.
Type Ia supernovae are the best-known standard candles across cosmological distances, allowing researchers to measure the expansion history of the universe.
The existence of dark energy is needed to reconcile the measured geometry of space with the total amount of matter in the universe.
The Wilkinson Microwave Anisotropy Probe (WMAP) spacecraft seven-year analysis estimated a universe made up of 72.8% dark energy, 22.7% dark matter, and 4.5% ordinary matter.
Dark energy's density is very low: 6×10−10 J/m3 (~7×10−30 g/cm3), much less than the density of ordinary matter or dark matter within galaxies.
The cosmological constant problem asserts that there is a huge disagreement between the observed values of vacuum energy density and the theoretical large value of zero-point energy obtained by quantum field theory, and it remains unresolved.Understanding Dark Energy: Theories, Observations, and Implications
The Planck spacecraft observations of the cosmic microwave background provided a more accurate estimate of the composition of the universe, with 68.3% dark energy, 26.8% dark matter, and 4.9% ordinary matter.
The theory of large-scale structure suggests that the density of matter in the universe is only 30% of the critical density.
The WiggleZ galaxy survey provided further evidence towards the existence of dark energy, confirming cosmic acceleration and constraining its inhomogeneity to 1 part in 10.
The late-time Integrated Sachs–Wolfe effect is a direct signal of dark energy in a flat universe, confirmed by Ho et al. and Giannantonio et al. in 2008.
The observational Hubble constant data (OHD) approach provides a direct estimate of the Hubble parameter, allowing for examination of the accelerated cosmic expansion and study of properties of dark energy.
Theories of dark energy include the cosmological constant, quintessence, interacting dark energy, and variable dark energy models.
The cosmological constant is the simplest explanation for dark energy, but the same quantum field theories predict a huge cosmological constant that would need to be almost, but not exactly, cancelled by an equally large term of the opposite sign.
Quintessence models of dark energy propose that the observed acceleration of the scale factor is caused by the potential energy of a dynamical field, which can vary in space and time.
Inhomogeneous cosmology and the cosmological extension of the equivalence principle provide alternative explanations for dark energy, but these theories have generally not gained much traction among cosmologists.
The ultimate fate of the universe depends on the model of dark energy, with projections into the future differing radically. For a cosmological constant, galaxies outside the Local Group will have a line-of-sight velocity that continually increases with time, eventually far exceeding the speed of light.
Assuming the dark energy is constant, the current distance to the cosmological event horizon is about 16 billion light years, meaning that a signal from an event happening at present would eventually be able to reach us in the future if the event were less than 16 billion light years away, but the signal would never reach us if the event were more than 16 billion light years away.The Future of the Universe
Galaxies approaching the cosmological event horizon will appear to vanish as their light becomes more redshifted.
The Local Group, including Earth and the Milky Way, would remain undisturbed as the rest of the universe recedes from view.
The phantom energy model of dark energy could result in a "Big Rip" where all structures, including atoms, are torn apart.
Dark energy could dissipate or become attractive, leading to a "Big Crunch" or cyclic model of the universe.
Dark energy is considered an "auxiliary hypothesis" that is added to a theory in response to falsifying observations.
Some argue that dark energy is a conventionalist hypothesis that adds no empirical content and is unfalsifiable.
The future of the universe is still uncertain and subject to ongoing research and debate.
The potential heat death of the universe could be a result of the Local Group's isolation.
The ultimate fate of the universe could be determined by the balance between dark energy and the gravitational pull of matter.
The accelerating expansion of the universe was first observed in 1998 and awarded the Nobel Prize in Physics in 2011.
The discovery of dark energy has led to a better understanding of the universe's expansion and structure.
Uncertainties about the future of the universe leave open the possibility for new discoveries and theories.