Socratus, et al.... is this a science "fiction".... like aether of old?

Quintessence (physics) 
>From Wikipedia, the free encyclopedia

For theories and defunct or classical concepts named after the synonym 
"Aether", see Aether 
(disambiguation)<http://en.wikipedia.org/wiki/Aether_%28disambiguation%29>
.

In physics <http://en.wikipedia.org/wiki/Physics>, *quintessence* is a 
hypothetical <http://en.wikipedia.org/wiki/Hypothesis> form of dark 
energy<http://en.wikipedia.org/wiki/Dark_energy>postulated as an explanation of 
observations of an accelerating 
universe <http://en.wikipedia.org/wiki/Accelerating_universe>. It has been 
proposed by some physicists to be a fifth fundamental 
force<http://en.wikipedia.org/wiki/Fifth_force>. 
Quintessence differs from the cosmological 
constant<http://en.wikipedia.org/wiki/Cosmological_constant>explanation of dark 
energy in that it is dynamic, changing over time, 
unlike the cosmological constant which always stays constant. It is 
suggested[*according to whom? 
<http://en.wikipedia.org/wiki/Wikipedia:Avoid_weasel_words>*] that 
quintessence can be either attractive or repulsive depending on the ratio 
of its kinetic and potential energy. Specifically, it is thought that 
quintessence became repulsive about ten billion years ago (the universe is 
approximately 13.8 billion years 
old).[1]<http://en.wikipedia.org/wiki/Quintessence_%28physics%29#cite_note-1>
 Contents 

   - 1 Scalar 
field<http://en.wikipedia.org/wiki/Quintessence_%28physics%29#Scalar_field>
   - 2 Tracker 
behavior<http://en.wikipedia.org/wiki/Quintessence_%28physics%29#Tracker_behavior>
   - 3 Specific 
models<http://en.wikipedia.org/wiki/Quintessence_%28physics%29#Specific_models>
   - 4 Quintom 
scenario<http://en.wikipedia.org/wiki/Quintessence_%28physics%29#Quintom_scenario>
   - 5 
Terminology<http://en.wikipedia.org/wiki/Quintessence_%28physics%29#Terminology>
   - 6 
References<http://en.wikipedia.org/wiki/Quintessence_%28physics%29#References> 
      - 6.1 Further 
reading<http://en.wikipedia.org/wiki/Quintessence_%28physics%29#Further_reading>
   - 7 External 
links<http://en.wikipedia.org/wiki/Quintessence_%28physics%29#External_links>

 Scalar field 

Quintessence is a scalar field <http://en.wikipedia.org/wiki/Scalar_field>with 
an equation 
of state <http://en.wikipedia.org/wiki/Equation_of_State_%28Cosmology%29>where 
*w**q*, the ratio of pressure *p**q* and density [image: \rho]*q*, is given 
by the potential energy [image: V(Q)] and a kinetic term:
[image: 
w_q=p_q/\rho_q=\frac{\frac{1}{2}\dot{Q}^2-V(Q)}{\frac{1}{2}\dot{Q}^2+V(Q)}] 

Hence, Quintessence is dynamic, and generally has a density and *w**q*parameter 
that varies with time. By contrast, a cosmological constant is 
static, with a fixed energy density and *w**q* = -1.
Tracker behavior 

Many models of quintessence have a *tracker* behavior, which according to Paul 
Steinhardt <http://en.wikipedia.org/wiki/Paul_Steinhardt> *et al.* (1999) 
partly solves the cosmological constant 
problem<http://en.wikipedia.org/wiki/Cosmological_constant#Cosmological_constant_problem>
.[2]<http://en.wikipedia.org/wiki/Quintessence_%28physics%29#cite_note-Zlatev-2>In
 these models, the quintessence field has a density which closely tracks 
(but is less than) the radiation density until matter-radiation 
equality<http://en.wikipedia.org/wiki/Timeline_of_the_Big_Bang#Matter_domination>,
 
which triggers quintessence to start having characteristics similar to dark 
energy <http://en.wikipedia.org/wiki/Dark_energy>, eventually dominating 
the universe. This naturally sets the low 
scale<http://en.wikipedia.org/wiki/Energy_scale>of the dark 
energy 
<http://en.wikipedia.org/wiki/Dark_energy>.[3]<http://en.wikipedia.org/wiki/Quintessence_%28physics%29#cite_note-Steinhardt1999-3>When
 comparing the predicted expansion 
rate <http://en.wikipedia.org/wiki/Metric_expansion_of_space> of the 
universe as given by the tracker solutions with cosmological data, a main 
feature of tracker solutions is that one needs four parameters to properly 
describe the behavior of their equation of 
state<http://en.wikipedia.org/wiki/Equation_of_state_%28cosmology%29>
,[4]<http://en.wikipedia.org/wiki/Quintessence_%28physics%29#cite_note-Linden2008-4>
[5]<http://en.wikipedia.org/wiki/Quintessence_%28physics%29#cite_note-Ferramacho2010-5>whereas
 it has been shown that at most a two-parameter model can optimally 
be constrained by mid-term future data (horizon 
2015-2020).[6]<http://en.wikipedia.org/wiki/Quintessence_%28physics%29#cite_note-LindererHuterer2005-6>
Specific models 

Some special cases of quintessence are phantom 
energy<http://en.wikipedia.org/wiki/Phantom_energy>, 
in which *w**q* < 
-1,[7]<http://en.wikipedia.org/wiki/Quintessence_%28physics%29#cite_note-Caldwell2002-7>and
 
k-essence<http://en.wikipedia.org/w/index.php?title=K-essence&action=edit&redlink=1>(short
 for kinetic 
quintessence<http://en.wikipedia.org/w/index.php?title=Kinetic_quintessence&action=edit&redlink=1>),
 
which has a non-standard form of kinetic 
energy<http://en.wikipedia.org/wiki/Kinetic_energy>. 
If this type of energy were to exist, it would cause a big 
rip<http://en.wikipedia.org/wiki/Big_rip>in the universe due to the growing 
energy density of dark energy which 
would cause the expansion of the universe to increase at a 
faster-than-exponential rate.
Quintom scenario 

In 2004, when scientists fit the evolution of dark energy with the 
cosmological data, they found that the equation of state had possibly 
crossed the cosmological constant 
boundary<http://en.wikipedia.org/w/index.php?title=Cosmological_constant_boundary&action=edit&redlink=1>(w=-1)
 from above to below. A proven no-go 
theorem <http://en.wikipedia.org/wiki/No-go_theorem>[*which? 
<http://en.wikipedia.org/wiki/Wikipedia:Avoid_weasel_words>*] indicates 
this situation, called the Quintom 
scenario<http://en.wikipedia.org/wiki/Quintom_scenario>, 
requires at least two degrees of freedom for dark energy 
models.[8]<http://en.wikipedia.org/wiki/Quintessence_%28physics%29#cite_note-Hu2005-8>
Terminology 

The name comes from the classical 
elements<http://en.wikipedia.org/wiki/Classical_element#Classical_elements_in_Greece>in
 ancient Greece. The 
aether <http://en.wikipedia.org/wiki/Aether_%28classical_element%29>, a 
pure "fifth element" (*quinta essentia* in Latin), was thought to fill the 
Universe beyond Earth. Similarly, modern quintessence would be the fifth 
known contribution to the overall mass-energy content of the Universe. (The 
other four in the modern interpretation, different from the ancient ideas, 
are: baryonic matter <http://en.wikipedia.org/wiki/Baryon>; radiation - 
photons and the highly relativistic 
neutrinos<http://en.wikipedia.org/wiki/Neutrinos>, 
which may be considered hot dark 
matter<http://en.wikipedia.org/wiki/Hot_dark_matter>; 
cold dark matter <http://en.wikipedia.org/wiki/Cold_dark_matter>; and the 
term due to spatial curvature - loosely, 
gravitational<http://en.wikipedia.org/wiki/Gravitation> 
self-energy <http://en.wikipedia.org/wiki/Self-energy>.)

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