Principles of Physics: A Calculus-Based Text
5th Edition
ISBN: 9781133104261
Author: Raymond A. Serway, John W. Jewett
Publisher: Cengage Learning
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Chapter 31, Problem 49P
To determine
The number of neutrinos passes through mother’s body.
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A standard nuclear power plant generates 3.0 GWGW of thermal power from the fission of 235U235U. Experiments show that, on average, 0.19 uu of mass is lost in each fission of a 235U235U nucleus.
How many kilograms of 235U235U undergo fission each year in this power plant?
Express your answer in kilograms per year.
How much energy (in x 1016 Joule) does the Sun burn 1 kg of hydrogen fuel in a nuclear reaction?
Calculate the energy Er, in megaelectronvolts (MeV), released in the following nuclear fission reaction:
Cm(250) + n → Se(92) + Sm(153) + 6n
The atomic masses are Cm(250)=250.078357 u, Se(92)=91.949926 u, and Sm(153)=152.922097 u.
Er = ? MeV
Chapter 31 Solutions
Principles of Physics: A Calculus-Based Text
Ch. 31.2 - Given the identification of the particles in...Ch. 31.5 - Prob. 31.2QQCh. 31.5 - Prob. 31.3QQCh. 31.5 - Prob. 31.4QQCh. 31.9 - Prob. 31.5QQCh. 31 - Prob. 1OQCh. 31 - Prob. 2OQCh. 31 - Prob. 3OQCh. 31 - Prob. 4OQCh. 31 - Prob. 5OQ
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- The primary decay mode for the negative pion is +v . (a) What is the energy release in MeV in this decay? (b) Using conservation of momentum, how much energy does each of the decay products receive, given the is at rest when it decays? You may assume the muon antineutrino is massless and has momentum p = E/c , just like a photon.arrow_forwardThe power output of the Sun is 41026W. (a) If 90% of this is supplied by the protonproton cycle, how many protons are consumed per second? (b) How many neutrinos per second should there be per square meter at the Earth from this process? This huge number is indicative of how rarely a neutrino interacts, since large detectors observe very few per day.arrow_forwardUsing data from Potential Energy of a System (http://cnx.org/content/m58312/latest/#fs-id1165036086155) , calculate the amount of mass converted to energy by the fusion of 1.00 kg of hydrogen. (b) What is the ratio of mass destroyed to the original mass, (c) How does this compare with for the fission of 1.00 kg of uranium?arrow_forward
- The Sun generates energy by p-p proton-proton chain nuclear fusion. The second step of p-p chain is: 2H + 1H → 3He. The particle masses are 2.0141 u, 1.0078 u, 3.0160 u, for 2H, 1H, 3He, respectively. This step produces _____ MeV of energy.arrow_forwardAdding one neutron to 235U results in the excited state 236U that quickly decays into unstable isotopes of xenon and strontium plus two extra neutrons. 234 U92 + n → 236 U92 → 140 Xe54 + 94 Sr38 +2n How do the sum of the rest masses in initial and final states compare? a. sum of the masses of the initial state (235U92 + n) > sum of the masses of the final state (140Xe54 + 94Sr38 + 2n) b. sum of the masses of the final state (140Xe54 + 94Sr38 + 2n) > sum of the masses of the masses of the initial state (235U92 + n) c. sum of the masses of the final state (140Xe54 + 94Sr38 + 2n) = sum of the masses of the initial state (235U92 + n)arrow_forwardThe intensity of cosmic ray radiation decreases rapidly with increasing energy, but there are occasionally extremely energetic cosmic rays that create a shower of radiation from all the particles they create by striking a nucleus in the atmosphere as seen in the figure given below. Suppose a cosmic ray particle having an energy of 1010 GeV converts its energy into particles with masses averaging 200 MeV/c2 . (a) How many particles are created? (b) If the particles rain down on a 1.00-km2 area, how many particles are there per square meter?arrow_forward
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