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In [[physics]] and [[thermodynamics]], an '''equation of state''' is a [[thermodynamic e ...erior of stars, including [[neutron star]]s, dense matter ([[quark–gluon plasma]]s) and radiation fields. A related concept is the [[perfect fluid]] [[equa

...product/identifier/9780511534997/type/book|title=Hadrons and Quark–Gluon Plasma|last2=Rafelski|first2=Johann|publisher=Cambridge University Press|year=2002 In the [[standard model]] of particle physics, the [[strong interaction|strong force]] is described by the theory of [[qu

...5d0| s2cid = 4072220 }}</ref> for which he received the [[Nobel Prize]] in Physics in 1970. ...lines are tied into a knot, then they will remain so as long as the fluid/plasma has negligible resistivity. This difficulty in reconnecting magnetic field

...location= Berlin, Heidelberg |publisher= Springer|series= Lecture Notes in Physics (LNP, vol. 660)| isbn= 978-3-540-22684-0|doi= 10.1007/b98103}} [https://arc ...[[Ludwig Boltzmann]] in 1872.<ref name="Encyclopaediaof">Encyclopaedia of Physics (2nd Edition), [[Rita G. Lerner|R. G. Lerner]], G. L. Trigg, VHC publishers

...present when matter has become a quark–gluon plasma. When quark–gluon plasma disassembles into [[hadron]]s in a breakup process, the high availability o ==Quark–gluon plasma in the early universe and in the laboratory==

...eneral, the collision of high-energy particles can produce [[jet (particle physics)|jet]]s of [[elementary particle]]s that emerge from these collisions. Coll ==Physics background==