Packet 9: Bonus 3

Simulations that popularized this theory were conducted by Marc Davis, George Efstathiou, Carlos Frenk, and Simon White, who made up Berkeley’s “Gang of Four.” For 10 points each:
[10h] What theory describes a component whose “w” parameter is approximately zero? This theory predicts bottom-up structure formation.
ANSWER: cold dark matter [or CDM; prompt on Lambda-CDM by asking “what part of that theory?”; prompt on particle dark matter; reject “dark matter” alone]
[10e] The Gang of Four’s cosmological simulations treated structure formation as an instance of this problem. Poincaré proved that this problem cannot be analytically solved for three or more objects.
ANSWER: N-body problem [reject “many-body problem”]
[10m] Frenk, White, and Julian Navarro developed an analytical “profile” of this quantity through N-body simulations of galaxies. The first Friedmann equation implies that this quantity’s “critical” form equals 3 H squared over 8 pi G.
ANSWER: density [accept density profile; accept critical density]
<FW, Other Science (Astronomy)> | NAFTA-Packet-9

HeardPPBE %M %H %
4211.9074%36%10%

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