/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Problem 169 The half-life of a radioactive s... [FREE SOLUTION] | 91Ó°ÊÓ

91Ó°ÊÓ

The half-life of a radioactive substance is \(20 \mathrm{~min}\). The approximate time interval \(\left(t_{2}-t_{1}\right)\) between the time \(t_{2}\) when \(\frac{2}{3}\) of it has decayed and time \(t_{1}\) when \(\frac{1}{3}\) of it had decayed is (A) \(7 \mathrm{~min}\) (B) \(14 \mathrm{~min}\) (C) \(20 \mathrm{~min}\) (D) \(28 \mathrm{~min}\)

Short Answer

Expert verified
The time interval between the time \(t_{2}\) when \(\frac{2}{3}\) of the radioactive substance has decayed and time \(t_{1}\) when \(\frac{1}{3}\) of it has decayed is \(20 \mathrm{~min}\).

Step by step solution

01

Write the radioactive decay formula

Radioactive decay can be described using the following formula: \[A(t) = A_{0} \cdot 2^{-\frac{t}{h}}\] where \(A_0\) is the initial amount of the substance, \(A(t)\) is the remaining amount of the substance at time \(t\), \(h\) is the half-life of the substance, and \(t\) is the time.
02

Solve for A(t) for \(\frac{1}{3}\) and \(\frac{2}{3}\) decayed

From our problem, we know that at time \(t_1\), \(\frac{1}{3}\) of the substance has decayed. Therefore, the remaining amount is \(\frac{2}{3}\) of the initial amount: \[A(t_1) = \frac{2}{3}A_0\] Similarly, at time \(t_2\), \(\frac{2}{3}\) of the substance has decayed, leaving us with \[\frac{1}{3}A_0\].
03

Substitute A(t) into the decay formula for both time points:

Next, substitute the expressions for \(A(t_1)\) and \(A(t_2)\) into the decay formula and solve for \(t_1\) and \(t_2\). For time \(t_1\): \[\frac{2}{3}A_0 = A_0 \cdot 2^{-\frac{t_1}{20}}\] For time \(t_2\): \[\frac{1}{3}A_0 = A_0 \cdot 2^{-\frac{t_2}{20}}\]
04

Solve for \(t_1\) and \(t_2\) by eliminating the \(A_0\) term and using logarithms

Divide the first equation by the second equation to eliminate the initial amount \(A_0\) term: \[\frac{\frac{2}{3}A_0}{\frac{1}{3}A_0} = \frac{2^{-\frac{t_1}{20}}}{2^{-\frac{t_2}{20}}}\] This simplifies to: \[2 = 2^{\frac{t_2-t_1}{20}}\] Now take the logarithm (base 2) of both sides: \[\log_2 2 = \log_2 {2^{\frac{t_2-t_1}{20}}}\]
05

Solve for \(t_2 - t_1\)

Using the logarithm properties, we can simplify the equation to: \[1 = \frac{t_2-t_1}{20}\] Solving for \(t_2 - t_1\), we get: \[t_2-t_1 = 20 \mathrm{~min}\] Therefore, the correct answer is (C) \(20 \mathrm{~min}\).

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with 91Ó°ÊÓ!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

The 'rad' is the correct unit used to report the measurement of (A) the ability of a beam of gamma - ray photons to produce ions in a target. (B) the energy delivered by radiation to a target. (C) the biological effect of radiation. (D) the rate of decay of a radioactive source.

Electromagnetic radiation whose electric component varies with time as \(E=C_{1}\left(C_{2}+C_{3} \cos \omega t\right) \cos \omega_{0} t\), here \(C_{1}, C_{2}\) and \(C_{3}\) are constants, is incident on lithium and liberates photoelectrons. Let the kinetic energy of most energetic electrons be \(0.592 \times 10^{-19} \mathrm{~J}\). Given that \(\omega_{0}=3.6 \times 10^{15} \mathrm{rad} / \mathrm{s}\) and \(\omega=6 \times 10^{14}\) \(\mathrm{rad} / \mathrm{sec} .\) The work function of lithium is (take planks constant \(\left.h=6.6 \times 10^{-34} \mathrm{MKS}\right)\). (A) \(1.2 \mathrm{eV}\) (B) \(1.5 \mathrm{eV}\) (C) \(2.1 \mathrm{eV}\) (D) \(2.39 \mathrm{eV}\)

In the nuclear nuclei $$ { }_{1}^{2} \mathrm{H}+{ }_{1}^{3} \mathrm{H} \rightarrow{ }_{2}^{4} \mathrm{He}+n $$ given that the repulsive potential energy between the two nuclei is \(-7.7 \times 10^{-14} \mathrm{~J}\), the temperature at which the gases must be heated to initiate the reaction is nearly [Boltzmann's constant \(\left.k=1.38 \times 10^{-23} \mathrm{~J} / \mathrm{K}\right]\) [2003] (A) \(10^{7} \mathrm{~K}\) (B) \(10^{5} \mathrm{~K}\) (C) \(10^{3} \mathrm{~K}\) (D) \(10^{9} \mathrm{~K}\)

The minimum \(K E\) of proton incident on \({ }_{6}^{13} \mathrm{C}\) nuclei at rest that will produce the reaction \({ }^{13} \mathrm{C}(p, n)^{13} \mathrm{~N}\) is (Mass of nitrogen \(=13.005738\) amu, Mass of neutron \(=1.008665\) amu, Mass of carbon \(=13.005738\) amu Mass of proton \(=1.007825 \mathrm{amu}\) ) (A) \(0.02 \mathrm{MeV}\) (B) \(0.10 \mathrm{MeV}\) (C) \(0.03 \mathrm{MeV}\) (D) \(0.05 \mathrm{MeV}\)

In certain element the \(K\)-shell electron energy is \(-18.525 \mathrm{keV}\) and the \(L\)-shell electron energy is \(-3 \mathrm{keV}\). When an electron jumps from the \(L\)-shell to \(K\) shell, an \(x\)-ray photon is emitted. The wavelength of the emitted \(x\)-rays is (A) \(0.8 \AA\) (B) \(1 \AA\) (C) \(0.6 \AA\) (D) \(1.2 \AA\)

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.