Test Your Knowledge on Dark Matter with This Fascinating Quiz!

Dark Matter: A Hypothetical Form of Matter

Dark matter accounts for approximately 85% of the matter in the universe and is difficult to detect because it does not interact with the electromagnetic field.
Astrophysical observations imply the presence of dark matter, which has influenced the structure and evolution of the universe.
Calculations show that many galaxies would behave differently if they did not contain a large amount of unseen matter, supporting the existence of dark matter.
Dark matter is thought to be non-baryonic and may be composed of some undiscovered subatomic particles, such as weakly interacting massive particles (WIMPs).
Dark matter is classified as "cold," "warm," or "hot" according to its velocity, with current models favoring a cold dark matter scenario.
Some astrophysicists argue for modifications of the standard laws of general relativity to explain specific observations that are not well-explained by ordinary dark matter, such as modified Newtonian dynamics or entropic gravity.
The hypothesis of dark matter has a long history, with Lord Kelvin discussing the potential number of dark stars in 1884.
Swiss astrophysicist Fritz Zwicky made an inference in 1933 that the Coma Cluster contained unseen mass and estimated that the cluster had about 400 times more mass than was visually observable.
Vera Rubin and colleagues' work in the 1960s and 1970s provided strong evidence for dark matter using galaxy rotation curves, showing most galaxies must contain about six times as much dark matter as visible mass.
Observations in the 1980s supported the presence of dark matter, including gravitational lensing, the temperature distribution of hot gas in galaxies and clusters, and the pattern of anisotropies in the cosmic microwave background.
Dark matter is defined as anything whose energy density scales with the inverse cube of the scale factor, i.e., ρ ∝ a−3, and is often used to mean only the non-baryonic component of dark matter.
Observational evidence for dark matter includes galaxy rotation curves, velocity dispersions, galaxy clusters, and gravitational lensing, as well as its effects on the cosmic microwave background.Understanding Dark Matter: Key Concepts and Observations
The Cosmic Microwave Background (CMB) anisotropy contains a series of acoustic peaks that can be predicted for any assumed set of cosmological parameters and constraints these parameters.
The first peak of the CMB mostly shows the density of baryonic matter, while the third peak relates mostly to the density of dark matter.
The observed CMB angular power spectrum provides powerful evidence for dark matter and supports the Lambda-CDM model.
Structure formation refers to the period after the Big Bang when density perturbations collapsed to form stars, galaxies, and clusters. Dark matter provides a solution to the problem of why ordinary matter could not have formed these structures alone.
The Bullet Cluster provides a challenge for modified gravity theories as standard dark matter models can easily explain this observation.
Type Ia supernovae can be used as standard candles to measure extragalactic distances. Data indicates the universe is expanding at an accelerating rate, which is usually ascribed to dark energy.
Baryon acoustic oscillations (BAO) set up a preferred length scale for baryons, and observations from galaxy redshift surveys provide a precise estimate of the Hubble constant and the average matter density in the Universe, supporting the Lambda-CDM model.
Large galaxy redshift surveys may be used to make a three-dimensional map of the galaxy distribution, and the resulting maps are slightly distorted due to redshift-space distortions.
The Lyman-alpha forest is the sum of the absorption lines arising from the Lyman-alpha transition of neutral hydrogen in the spectra of distant galaxies and quasars and can also constrain cosmological models.
Dark matter can be divided into cold, warm, and hot categories, and cold dark matter offers the simplest explanation for most cosmological observations.
The constituents of cold dark matter are unknown, and possibilities range from large objects like MACHOs or RAMBOs to new particles such as WIMPs and axions.Overview of Dark Matter
LIBRA experiment claimed to detect dark matter particles, but results are controversial
Warm dark matter consists of particles with a free-streaming length comparable to the size of a protogalaxy, but no known particles fit this description
Hot dark matter consists of particles whose free-streaming length is much larger than the size of a protogalaxy, such as neutrinos, but they cannot explain dark matter
Direct detection experiments aim to observe low-energy recoils of nuclei induced by interactions with dark matter particles, but no well-established claim of detection has been made
Indirect detection experiments search for products of self-annihilation or decay of dark matter particles in outer space, such as gamma rays or antiprotons, but various astrophysical sources can mimic the signal expected from dark matter
Collider searches aim to produce dark matter particles in a laboratory, but any discovery must be corroborated by indirect or direct detection
Alternative hypotheses, such as modified gravity theories, exist to explain the same observational phenomena without introducing dark matter, but most astrophysicists believe there must be some form of dark matter present in the universe
Dark matter is a popular topic in science fiction and is often used metaphorically to evoke the unseen or invisible.