Suppose a person swallows some radioactive material by accident. What information is needed to be able to assess possible damage?

Short Answer

Expert verified

We need to know what sort of radioactive element was consumed and how much of it was consumed.

Step by step solution

01

Definition of radiation

Radiation is defined as the emission or transmission of energy in the form of waves or particles over space or a material medium in physics. Radio waves, microwaves, infrared, visible light, ultraviolet, x-rays, and gamma radiation are examples of electromagnetic radiation.

02

Explanation for information is needed to be able to assess possible damage

If a person swallows anything possibly radioactive, we must first determine what type of element it is in order to determine its stability. We may then calculate the element's half-life based on this information. On the other hand, we should know how much of the element was consumed because bigger dosages might be fatal.

We should never contemplate swallowing a radioactive element since it would be harmful in any manner. Because it directly affects our body's chemistry and immune system, it might enhance our chances of acquiring cancer or another disease. By releasing various particles, radioactive materials release enough energy to disrupt chemical bonds of hydrogen in our bodies, which can cause illness.

Therefore, shielding, decreasing time exposure, and moving away from the source are the best ways to protect against radiation. As a result, neither of these are respected by swallowing.

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Most popular questions from this chapter

(a) Calculate the energy released in the neutron-induced fission reaction\(n{ + ^{235}}U{ \to ^{92}}Kr{ + ^{142}}Ba + 2n\),

Given \(m{(^{92}}Kr) = 91.926269{\rm{ }}u\) and

\(m{(^{142}}Ba) = 141.916361{\rm{ }}u\).

(b) Confirm that the total number of nucleons and total charge are conserved in this reaction.

Two fusion reactions mentioned in the text are

\(n{ + ^3}He{ \to ^4}He + \gamma \)

and

\(n{ + ^1}H{ \to ^2}H + \gamma \).

Both reactions release energy, but the second also creates more fuel. Confirm that the energies produced in the reactions are \(20.58\) and\(2.22{\rm{ }}MeV\), respectively. Comment on which product nuclide is most tightly bound, \(^4He\) or\(^2H\).

Another set of reactions that result in the fusing of hydrogen into helium in the Sun and especially in hotter stars is called the carbon cycle. It is

\(\begin{array}{*{20}{l}}{^{12}C{ + ^1}H}&{{ \to ^{13}}N + \gamma ,}\\{^{13}N}&{{ \to ^{13}}C + {e^ + } + {v_e},}\\{^{13}C{ + ^1}H}&{{ \to ^{14}}N + \gamma ,}\\{^{14}N{ + ^1}H}&{{ \to ^{15}}O + \gamma ,}\\{^{15}O}&{{ \to ^{15}}N + {e^ + } + {v_e},}\\{^{15}N{ + ^1}H}&{{ \to ^{12}}C{ + ^4}He.}\end{array}\)

Write down the overall effect of the carbon cycle (as was done for the proton-proton cycle in \(2{e^ - } + {4^1}H{ \to ^4}He + 2{v_e} + 6\gamma \)). Note the number of protons (\(^1H\)) required and assume that the positrons (\({e^ + }\)) annihilate electrons to form more \(\gamma \) rays.

Verify by listing the number of nucleons, total charge, and electron family number before and after the cycle that these quantities are conserved in the overall proton-proton cycle in \(2{e^ - } + {4^1}H{ \to ^4}He + 2{\nu _e} + 6\gamma \).

How many kilograms of water are needed to obtain the \(198.8{\rm{ }}mol\) of deuterium, assuming that deuterium is \(0.01500\% \) (by number) of natural hydrogen?

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