21st Century Astronomy
21st Century Astronomy
6th Edition
ISBN: 9780393428063
Author: Kay
Publisher: NORTON
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Chapter 22, Problem 10QP
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I. NUCLEAR EQUATION: You are going to write the nuclear equations for the following fusion reactions responsible for the abundance of lighter nuclei in the universe. 1. Fusion of two Deuterium isotopes to form Helium3 2. Fusion of Deuterium and a neutron to form Tritium 3. Fusion of Deuterium and a proton to form Helium
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 ?
This scientist tried to determine the age of the universe by looking for the temperature of cosmic microwave background radiation. a) Arno Penzias  b) Frank Drake  c) Robert Dicke  d) Fred Hoyle  e) George Gamow
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