“2018年USAAAO长问题第3道”的版本间的差异

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(c) [5 pt] The mean bolometric luminosity per unit volume emitted by stars in the universe today is about
 
(c) [5 pt] The mean bolometric luminosity per unit volume emitted by stars in the universe today is about
$$3 × 10^8 L_{sun}/Mpc^3$$. How long would it takes stars at this rate to fuse all the hydrogen and helium in
+
$$3 × 10^8 L_{sun}/Mpc^3$$. How long would it takes stars at this rate to fuse all the hydrogen and helium in
 
the universe? Compare to the present age of the universe.
 
the universe? Compare to the present age of the universe.

2020年3月9日 (一) 22:01的最新版本

英文题目

3. [15 pt] Suppose that at some time in the very recent past all the hydrogen and helium (baryon density $$ρ_b = 4.2 × 10^{−31} g/cm^3$$ , about 75% hydrogen (=1 baryon) by mass and 25% helium (=4 baryons) by mass) in the universe had been instantly fused into iron in stars, and the released energy thermalized into black body radiation. (Note that the binding energy per nucleon of $$_{26}^{56}\textrm{Fe}$$ is 8.8 MeV and that of $$_{4}^{2}\textrm{He}$$ is 7.1 MeV.)

(a) [5 pt] Calculate the current temperature of this black body radiation.

(b) [5 pt] At what wavelength would the black body spectrum peak, and what region of the electromagnetic spectrum would this be?

(c) [5 pt] The mean bolometric luminosity per unit volume emitted by stars in the universe today is about $$3 × 10^8 L_{sun}/Mpc^3$$. How long would it takes stars at this rate to fuse all the hydrogen and helium in the universe? Compare to the present age of the universe.