Chapter 42: Q 31 Exercise (page 1236)
What is the total energy (in MeV) released in the beta-minus
decay of 3H?
Short Answer
Hence, the energy released is
Chapter 42: Q 31 Exercise (page 1236)
What is the total energy (in MeV) released in the beta-minus
decay of 3H?
Hence, the energy released is
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Get started for freeA sample of 1.0x1010atoms that decay by alpha emission
has a half-life of 100 min. How many alpha particles are emitted
between t = 50 min and t = 200 min?
Use the graph of binding energy to estimate the total energy released if three 4 He nuclei fuse together to form a 12 C nucleus
All the very heavy atoms found in the earth were created long ago by nuclear fusion reactions in a supernova, an exploding star. The debris spewed out by the supernova later coalesced into the gases from which the sun and the planets of our solar system were formed. Nuclear physics suggests that the uranium isotopes 235 U and 238 U should have been created in roughly equal numbers. Today, 99.28% of uranium is 238 U and only 0.72% is 235 U. How long ago did the supernova occur?
Stars are powered by nuclear reactions that fuse hydrogen into helium. The fate of many stars, once most of the hydrogen is used up, is to collapse, under gravitational pull, into a neutron star. The force of gravity becomes so large that protons and electrons are fused into neutrons in the reaction . The entire star is then a tightly packed ball of neutrons with the density of nuclear matter.
a. Suppose the sun collapses into a neutron star. What will its radius be? Give your answer in .
b. The sun's rotation period is now 27 days. What will its rotation period be after it collapses?
Rapidly rotating neutron stars emit pulses of radio waves at the rotation frequency and are known as pulsars.
Which stable nuclei have a diameter of 7.46 fm?
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