Exam 44: Nuclear Structure

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The reaction The reaction   is known as a ____ reaction. is known as a ____ reaction.

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When a beam of nuclear radiation of initial intensity I0 passes through a thickness x of material, the intensity of the beam exiting the material is I =

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The nuclear probability of interacting with neutrons depends most strongly on the neutron's

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A neutron is characterized by the term "thermal neutron" when

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44 g of petrified wood was found in a petrified forest. A sample showed a 14C activity of 100 decays/minute. How long has the tree been dead (in years)? (The half-life of carbon-14 is 5730 years and freshly cut wood contains 6.5 × 1010 atoms of 14C per gram.)

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A glass container holds equal numbers of atoms of phosphorus 30 with a half-life of 2.5 minutes and of nitrogen 13 with a half-life of 10 minutes. After 20 minutes the ratio of the number of nitrogen atoms remaining to the number of phosphorus atoms remaining is

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Background radiation from cosmic rays and radioactive nuclei in our surroundings is about 0.13 rem/year. Suppose we assume this all comes from cosmic rays which have an RBE factor of 1.0. The RBE factor for the most dangerous types of radiation is 20. How many rads of the most dangerous radiation could a 100-year-old person have been exposed to in her lifetime without having gone over the recommended limit of 0.5 rem/year?

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Two nuclei which share the same atomic number Z always are

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One roentgen is defined as

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A principal mechanism for energy loss during nuclear fusion is bremsstrahlung. This loss is associated with

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How much energy (in MeV) is released when a How much energy (in MeV) is released when a   fissions to   and   in the reaction   m(n) = 1.008665 u m(U) = 235.043915 u M(Ba) = 140.9139 u M(Kr) = 91.8973 u U = 1.66 × 10−<sup>27</sup> kg fissions to How much energy (in MeV) is released when a   fissions to   and   in the reaction   m(n) = 1.008665 u m(U) = 235.043915 u M(Ba) = 140.9139 u M(Kr) = 91.8973 u U = 1.66 × 10−<sup>27</sup> kg and How much energy (in MeV) is released when a   fissions to   and   in the reaction   m(n) = 1.008665 u m(U) = 235.043915 u M(Ba) = 140.9139 u M(Kr) = 91.8973 u U = 1.66 × 10−<sup>27</sup> kg in the reaction How much energy (in MeV) is released when a   fissions to   and   in the reaction   m(n) = 1.008665 u m(U) = 235.043915 u M(Ba) = 140.9139 u M(Kr) = 91.8973 u U = 1.66 × 10−<sup>27</sup> kg m(n) = 1.008665 u m(U) = 235.043915 u M(Ba) = 140.9139 u M(Kr) = 91.8973 u U = 1.66 × 10−27 kg

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The nuclear reaction(s) that is(are) most likely to be employed in fusion reactors on Earth is(are)

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A neutron is known to undergo beta decay (n → p + e− + A neutron is known to undergo beta decay (n → p + e− +   ). A reasonable mean lifetime for free neutrons is ). A reasonable mean lifetime for free neutrons is

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When a fast neutron collides with a hydrogen or deuterium nucleus, the most likely result is that

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Calculate the binding energy per nucleon (MeV/nucleon) for tritium, ( Calculate the binding energy per nucleon (MeV/nucleon) for tritium, (   ) a radioactive isotope of hydrogen. Assume: M <sub>p</sub> = 1.007 825 u M <sub>n</sub> = 1.008 665 u M <sub>t</sub> = 3.016 05 u U = 1.66 × 10−<sup>27</sup> kg ) a radioactive isotope of hydrogen. Assume: M p = 1.007 825 u M n = 1.008 665 u M t = 3.016 05 u U = 1.66 × 10−27 kg

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How many radioactive atoms are present in a sample that has an activity of 0.5 μCi and a half-life of 10 years? (1 curie = 3.7 × 1010 decays/s)

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When a neutron decays, a proton and an electron are observed. When the electrons emitted from a sample of neutrons are observed, they are found to have different kinetic energies. This was accounted for by

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It is often possible to use atomic masses when calculating the binding energy of a nucleus. This is not true for calculating the Q value for the e+ decay process since

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The theory of nuclear astrophysics is that all the heavy elements like uranium are formed in the interior of massive stars. These stars eventually explode, releasing these elements into space. If we assume that at the time of the explosion there were equal amount of U-235 and U-238, how long ago did the star(s) explode that released the elements that formed our Earth? The present U-235/U-238 ratio is 0.0070. [The half-lives of U-235 and U-238 are 0.7 × 109 yr and 4.47 × 109 yr.]

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What value of Z (atomic number) and A (mass number) result in the following alpha decay? What value of Z (atomic number) and A (mass number) result in the following alpha decay?

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