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State of matter

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In the physical sciences, a state of matter is one of the many ways that matter can interact with itself to form a macroscopic, homogenous phase. The most familiar states of matter are solids, liquids, and gases. However, the most common state of matter in the visible universe is plasma. Less familiar phases include: quark-gluon plasma; Rydberg matter; Bose-Einstein condensates and fermionic condensates; quantum spin Hall state; degenerate matter; strange matter; superfluids and supersolids; and possibly string-net liquids.


Other examples of states of matter

Bose-Einstein condensate is a state of matter that occurs at extremely low temperatures, near absolute zero (-273 C). These temperatures are too low to occur anywhere on Earth except in laboratory experiments. The very slow motion of molecules at these temperatures allow some of the more bizarre aspects of quantum mechanics to manifest themselves in the form of novel macroscopic properties.

Under extremely high pressure, ordinary matter undergoes a transition to a series of exotic states of matter collectively known as degenerate matter. These are of great interest to astrophysics, because these high-pressure conditions are believed to exist inside stars that have used up their nuclear fusion "fuel", such as white dwarves and neutron stars.

When in a normal solid state, the atoms of matter align themselves in a grid pattern, so that the spin of any electron is the opposite of the spin of all electrons touching it. But in a string-net liquid, atoms are arranged in some pattern which would require some electrons to have neighbors with the same spin. This gives rise to some curious properties, as well as supporting some unusual proposals about the fundamental conditions of the universe, itself.

One of the metastable states of strongly nonideal plasma is Rydberg matter which forms upon condensation of excited atoms. These atoms can also turn into ions and electrons if they reach a certain temperature.

See also

External links

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