Cosmology to dark matter

  • Can you study dark matter?

    Researchers use large, sensitive detectors located deep underground to directly search for the dark matter particles that may continually pass through the Earth.
    Researchers can also detect dark matter indirectly through specific signatures in cosmic rays and gamma rays..

  • Could dark matter be created?

    Experiments at the Large Hadron Collider (LHC) may provide more direct clues about dark matter.
    Many theories say the dark matter particles would be light enough to be produced at the LHC.
    If they were created at the LHC, they would escape through the detectors unnoticed..

  • How did we come up with dark matter?

    The term dark matter was coined in 1933 by Fritz Zwicky of the California Institute of Technology to describe the unseen matter that must dominate one feature of the universe—the Coma Galaxy Cluster..

  • Is dark matter part of cosmology?

    Astronomers studying the motion of gas in the outer regions of galaxies found evidence in an ever-increasing number of systems for the existence of massive halos (20–24).
    By the 1980s, dark matter had become an accepted part of the cosmological paradigm..

  • Is the universe Expanding due to dark matter?

    Neither.
    The universe has been expanding for the last 13.8 billion years due to the initial big bang, when everything began to fly apart from everything else.
    Dark energy is a theorized form of energy to explain the observed acceleration of that expansion..

  • What do cosmologists think dark energy does?

    Astronomers theorize that the faster expansion rate is due to a mysterious, dark force that is pulling galaxies apart.
    One explanation for dark energy is that it is a property of space.
    Albert Einstein was the first person to realize that empty space is not nothing..

  • What do scientists think dark matter is?

    Some believe that it may be normal objects such as cold gasses, dark galaxies, or massive compact halo objects (called MACHOs, they would include black holes and brown dwarfs).
    Other scientists believe that dark matter may be composed of strange particles which were created in the very early universe..

  • What is dark matter in cosmology?

    The leading explanation is that dark matter is some as-yet-undiscovered subatomic particle, such as weakly interacting massive particles (WIMPs) or axions.
    The other main possibility is that dark matter is composed of primordial black holes..

  • Gravitational lensing observations by galaxies, clusters of galaxies, and large-scale structure provided important results that directly confirmed the existence of dark matter and measured its distribution on both small and large scales (e.g., refs. 13–15 and references therein).
  • Overview.
    Dark fluid is hypothesized to be a specific kind of fluid whose attractive and repulsive behaviors depend on the local energy density.
    In this theory, the dark fluid behaves like dark matter in the regions of space where the baryon density is high.
  • The leading explanation is that dark matter is some as-yet-undiscovered subatomic particle, such as weakly interacting massive particles (WIMPs) or axions.
    The other main possibility is that dark matter is composed of primordial black holes.
Cosmology and Dark Matter | ELT | ESO. What we see around us — the planets, stars and dust in between them — makes up just 5% of the Universe. The rest is invisible dark matter and a mysterious dark energy that is thought to be causing the Universe to expand faster and faster.
Dark matter can refer to any substance which interacts predominantly via gravity with visible matter (e.g., stars and planets). Hence in principle it need not  Cold darkHot dark matterLight dark matterDark Matter (disambiguation)
The rest is invisible dark matter and a mysterious dark energy that is thought to be causing the Universe to expand faster and faster. When this accelerating 

Could a new theory explain the nature of invisible dark matter?

Researchers reveal a theoretical breakthrough that may explain both the nature of invisible dark matter and the large-scale structure of the universe known as the cosmic web.
The result establishes a ..
New research has revealed the distribution of dark matter in never before seen detail, down to a scale of 30,000 light-years.

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What does matter mean in cosmology?

In standard cosmologic calculations, "matter" means any constituent of the universe whose energy density scales with the inverse cube of the scale factor, i.e., ρ ∝ a−3 .
This is in contrast to "radiation", which scales as the inverse fourth power of the scale factor ρ ∝ a−4 , and a cosmological constant, which does not change with respect to a .

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What is dark matter & dark energy?

Dark matter makes up most of the mass of galaxies and galaxy clusters, and is responsible for the way galaxies are organized on grand scales.
Dark energy, meanwhile, is the name we give the mysterious influence driving the accelerated expansion of the universe.

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What percentage of the universe is dark matter?

Using fluctuations in the cosmic microwave background ( CMB ), astronomers determined that dark matter is about 27% of the contents of the universe, in terms of its overall contribution to the total mass and energy content of the cosmos.
A timeline of the universe from the Big Bang at the left to modern times at the right.

Cosmology to dark matter
Cosmology to dark matter
In astronomy and cosmology, baryonic dark matter is hypothetical dark matter composed of baryons.
Only a small proportion of the dark matter in the universe is likely to be baryonic.
In cosmology

In cosmology

Topics referred to by the same term

In cosmology, dark matter is matter that emits no detectable radiation, but whose presence can be inferred from gravitational effects.

Dark matter weakly interacting massive particles candidates with masses less than 1 GeV

Light dark matter, in astronomy and cosmology, are dark matter weakly interacting massive particles (WIMPS) candidates with masses less than 1 GeV.
These particles are heavier than warm dark matter and hot dark matter, but are lighter than the traditional forms of cold dark matter, such as Massive Compact Halo Objects (MACHOs).
The Lee-Weinberg bound limits the mass of the favored dark matter candidate, WIMPs, that interact via the weak interaction to mwe-math-element> GeV.
This bound arises as follows.
The lower the mass of WIMPs is, the lower the annihilation cross section, which is of the order mwe-math-element>, where m is the WIMP mass and M the mass of the Z-boson.
This means that low mass WIMPs, which would be abundantly produced in the early universe, freeze out much earlier and thus at a higher temperature, than higher mass WIMPs.
This leads to a higher relic WIMP density.
If the mass is lower than mwe-math-element
> GeV the WIMP relic density would overclose the universe.

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