Chapter 42: Q. 8 (page 1236)
Calculate (in ) the total binding energy and the binding energy per nucleon for and for .
Short Answer
For atom, Binding energy =
Binding energy per nucleon =
For atom, Binding energy =
Binding energy per nucleon =
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Chapter 42: Q. 8 (page 1236)
Calculate (in ) the total binding energy and the binding energy per nucleon for and for .
For atom, Binding energy =
Binding energy per nucleon =
For atom, Binding energy =
Binding energy per nucleon =
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Calculate (in ) the binding energy per nucleon for and . Which is more tightly bound?
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 p+ + e- S n + n. 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 km. 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
How many grays of gamma-ray photons cause the same bio-
logical damage as 30 Gy of alpha radiation?
A 1 Ci source of radiation is a significant source. 238 U is an alpha emitter. What mass of 238 U has an activity of 1 Ci?
a. Is the binding energy of a nucleus with more than, less than, or equal to the binding energy of a nucleus with ? Explain.
b. Is a nucleus with more tightly bound, less tightly bound, or bound equally tightly as a nucleus with ? Explain.
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