Round 5: Tossup 16

A fully degenerate, adiabatic gas with this property is modeled by the polytrope n equals three. The energy density of a universe of particles with this property scales with scale factor to the negative fourth. Degenerate electrons with this property have pressure proportional to density to the four-thirds, which occurs near the Chandrasekhar limit. For the first 50,000 years after the Big Bang, the universe was dominated by particles with this property. Hot (-5[1])dark matter consists of particles that had this property in the early universe, like neutrinos. An alternate (-5[1])name for astrophysical jets indicates that they have this property, corresponding to a Lorentz factor larger than one. (-5[1])For 10 points, name this property of particles that cannot be described with classical (-5[1])mechanics, (10[2])since their velocity is near the speed of light. ■END■ (10[2]0[2])

ANSWER: relativistic particles [or ultra-relativistic particles; accept relativistic jets; accept answers referring to particles that must be described with special relativity; accept answers referring to particles traveling near or at the speed of light or c until “speed of light” is read; prompt on non-classical; prompt on massless or nearly massless by asking “what other property do massless particles have?”; prompt on radiation by asking “when we say radiation in this context, we’re actually more generally talking about all particles with what property?”]
<GC, Other Science> | Packet F - Chicago C, McGill C, WashU A, Chicago B
= Average correct buzzpoint

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