I’ve said it before, now let’s put
it to practice. Don’t worry, I’ll pick an easy topic… well, easy to start with.
You’ll see. Let’s learn about the states of matter. This is a topic that is
typically introduced by first grade. Like I said, easy. So as we all know,
there are three states of matter: solids, liquids, and gasses. These have
unique defining properties. Solids hold a definite shape and size, whereas
liquids take the shape of their container, but still have a definite size, and
gasses take on both the shape and size of their container. Still with me? Don’t
worry, it gets better.
Matter transitions between these
phases as temperatures increase. As solids get warmer, they eventually melt
into liquids. As liquids get warmer, they eventually boil into gasses.
Conversely, cooling gasses will condense into liquids, and cooling liquids will
freeze into solids. But wait, there’s more. Pressure can also influence the
state of matter in the inverse manner of temperature. As pressure increases
matter shifts towards solids and as it decreases it shifts towards gasses. This
means that matter can transition from one phase to another even at a constant
temperature.
Now phase changes between the states
are not always a linear transition from solid to liquid to gas and back. Since
they are affected by both temperature and pressure, we add a second dimension
into the mix. At relatively low pressures, it is possible for solids to sublime
directly to gasses, and conversely at higher pressures, gasses can deposit to
solids. Again, I am talking relative pressures here, they very from substance
to substance, and for some, ambient pressure may be sufficiently low for
sublimation.
Now water is an exception to the typical
phase relationships, so forget everything I just said. Water’s freezing
temperature actually decreases with increasing pressure, meaning the more
pressure the colder water has to be to freeze. This is due to hydrogen bond
formation disrupting the expected interactions of molecules. In fact,
variations in the formation of the solid phase brought on by differing rates
and conditions under which the solid is formed can lead to numerous different
solid forms of the same substance. There are several different kinds of ice,
for example, all comprised of pure water. This can even be observed with pure
elements; think diamonds and graphite. So to say something is solid is not
necessarily as straightforward as you may think. Other interesting phenomena
occur with mixtures, due to the interactions between the components, including changes
in the transition point, separation of the components, and combinations of two
different phases, but we’ll leave that be.
Now, what happens at high
temperatures and pressures? Everything falls apart and you get supercritical
fluids, effectively both a liquid and a gas at the same time. This is considered
a continuous transition, in contrast to the changes previously mentioned which all
had a latent thermal period; that is, where matter is either absorbing or
releasing energy during its transition, but the temperature remains constant.
Continuous transitions also include things like transitions between magnetic
states and transitions into superconducting states.
So there are the three states of
matter. Except that there are actually four states of matter. Let’s talk about plasma.
This is a classically identified, distinct phase of matter. It is characterized
by the coexistence of stripped electrons and ionized particles. The net charge
is typically near neutral, as there are an equal number of electrons and ions
coexisting. Often the process occurs through collisions displacing electrons,
and displaced electrons begetting more collisions. Plasma is ionized gas and
thus cannot transition between the other states of matter directly. The degree
of ionization at which a gas becomes a plasma can be up to interpretation, but
physical properties differ greatly between the two. One of the key differences
is potential, as plasma has very high conductance, whereas gasses have very low
conductance.
Similarly to the other phases, plasma can
take unique forms when produced under atypical circumstances. For example,
although plasma is typically very hot (we’re talking 17,000oF), so
called ‘cold plasma’ can form where the electrons take on their typical high
energy, high temperature nature, but the ions in the mix exist at near ambient
temperature.
So there are the four fundamental states
of matter with some of their less conventional variants. Other variants on the traditional
states include glass which is a non-amorphous solid, liquid crystals which act
as both liquids and solids, superfluids which have no resistance and thereby
perfect fluidity, supersolids which are superfluids that maintain their shape,
and even superglasses, as well as others, some of which are likely still to be
discovered.
What about the non-classical states of
matter? You didn’t think it was just those four? No, depending on who you ask
there are seven or more states of matter. Some of the more well-known include
Bose-Einstein condensate (BEC), quark-gluon plasma, and degenerate matter. A BEC
occurs when temperatures approach absolute zero and matter no longer behaves as
independent particles, but rather a quantum singularity. Quarks are subatomic
particles held together by the strong force mediated by gluons. At very high temperatures (now we’re talking
about 7,000,000,000,000oF), energy becomes sufficient such that
quark can overcome the strong force and move freely amid gluons. Degenerate
matter is what happens at pressure extremes, think the center of stars. At
these high pressures, particles become so compressed that matter behaves quite
differently than it would otherwise be expected to. There are many flavors of
degenerate matter, but it’ll probably turn out that those are just
oversimplified versions of the truth
too.
-AMS
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