Universe
Universe
11th Edition
ISBN: 9781319039448
Author: Robert Geller, Roger Freedman, William J. Kaufmann
Publisher: W. H. Freeman
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Chapter 19, Problem 16Q
To determine

The changes in the universe if 8Be having half-life 2.6×1016 had a zero half-life. Also what if 8Be nucleus were stable and did not decay. Given that the half-life is the average time that elapses before it decays into alpha particles.

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Why does primordial nuclesythesis end about 3 minutes after the Big Bang ?  select one :  a. The number densities of photons is too large at this time and the photons induce fission , stopping nuclei formation  b. The universe is tooo hot at t=3 minutes  c. The number densities of neutrons and protons and other nuclei are too small at this time and fusion fades out .  d. Deuterium has a lifetime of 3 minutes , so after this time no more deuterium survives as it decays away ?
Astronomers can determine the heat of various areas of the universe by making observations about energy they emit. Gamma rays can be found in areas where there is a lot of star formation occurring. What would you guess about the temperature of these areas? Explain why.Do you think there would be a lot of particles present? Explain why.
What is the percentage difference mass loss between a Helium nucleus and 4 protons?  My math came out to 99% but I think I did something wrong (this assumes the mass for of 4 protons is 6.6792 x 10^-27kg and a the mass of a helium nucleus is 6.6892e x 10^-27kg  (Units need to be in kilograms to use with e=mc^2)
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