Chapter 40: Problem 64
What is the total energy released in the decay \(n \rightarrow p+e^{-}+\bar{\nu}_{e} ?\)
Chapter 40: Problem 64
What is the total energy released in the decay \(n \rightarrow p+e^{-}+\bar{\nu}_{e} ?\)
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Get started for freeRadium- 226 decays by emitting an alpha particle. What is the daughter nucleus? a) \(\mathrm{Rd}\) b) \(\mathrm{Rn}\) c) Bi d) \(\mathrm{Pb}\)
\(^{214} \mathrm{Pb}\) has a half-life of \(26.8 \mathrm{~min}\). How many minutes must elapse for \(90.0 \%\) of a given sample of \({ }^{214} \mathrm{~Pb}\) atoms to decay?
Billions of years ago, our Solar System was created out of the remnants of exploding stars. Nuclear scientists believe that two isotopes of uranium, \({ }^{235} \mathrm{U}\) and \({ }^{238} \mathrm{U},\) were created in equal amounts at the time of a stellar explosion. However, today \(99.28 \%\) of uranium is in the form of \({ }^{238} \mathrm{U}\) and only \(0.72 \%\) is in the form of \({ }^{235} \mathrm{U}\). Assuming a simplified model in which all of the matter in the Solar System originated in a single exploding star, estimate the approximate time of this explosion.
Calculate the binding energy for the following two uranium isotopes: a) \({ }_{92}^{238} \mathrm{U},\) which consists of 92 protons, 92 electrons, and 146 neutrons, with a total mass of \(238.0507826 \mathrm{u}\). b) \({ }^{235} \mathrm{U},\) which consists of 92 protons, 92 electrons, and 143 neutrons, with a total mass of \(235.0439299 \mathrm{u} .\) The atomic mass unit \(\mathrm{u}=1.66 \cdot 10^{-27} \mathrm{~kg} .\) Which isotope is more stable (or less unstable)?
A neutron star is essentially a gigantic nucleus with mass 1.35 times that of the Sun, or mass number of order \(10^{57} .\) It consists of approximately \(99 \%\) neutrons, the rest being protons and an equal number of electrons. Explain the physics that determines these features.
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