/*! 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 67 Consider the fusion reaction \(^... [FREE SOLUTION] | 91Ó°ÊÓ

91Ó°ÊÓ

Consider the fusion reaction \(^{2}_{1}H\) + \(^{2}_{1}H \rightarrow ^{3}_{2}He + ^{1}_{0}n\). (a) Estimate the barrier energy by calculating the repulsive electrostatic potential energy of the two \(^{2}_{1}H\) nuclei when they touch. (b) Compute the energy liberated in this reaction in MeV and in joules. (c) Compute the energy liberated \(per\) \(mole\) of deuterium, remembering that the gas is diatomic, and compare with the heat of combustion of hydrogen, about \(2.9 \times 10^{5} J/mol\).

Short Answer

Expert verified
The barrier energy is about 0.24 MeV. The energy liberated is 4.19 MeV or about 6.7 x 10^-13 J. Per mole, it's about 8.05 x 10^11 J/mol.

Step by step solution

01

Calculate Coulomb Barrier Energy

The barrier energy is the electrostatic potential energy when the two nuclei are close enough to touch. Given that each deuterium nucleus has one proton, the potential energy is given by the formula:\[ E_{r} = \frac{k \cdot e^{2}}{r} \]Where:- \( k = 8.99 \times 10^{9} \text{ N m}^2/ ext{C}^2 \) is Coulomb's constant,- \( e = 1.6 \times 10^{-19} \text{ C} \) is the elementary charge,- \( r \approx 2 \times 10^{-15} \text{ m} \) is the approximate nuclear radius for deuterium.Plugging in these values:\[ E_{r} = \frac{8.99 \times 10^{9} \times (1.6 \times 10^{-19})^2}{2 \times 10^{-15}} \approx 3.84 \times 10^{-14} \text{ J} \]To convert this energy to MeV:\[ E_{r} = \frac{3.84 \times 10^{-14}}{1.6 \times 10^{-13}} \approx 0.24 \text{ MeV} \]
02

Compute Energy Liberated in Fusion Reaction

The energy liberated in the fusion reaction can be calculated using the mass defect:\[ \Delta m = (2m_{D}) - (m_{He} + m_{n}) \]Where:- \( m_{D} = 2.0141 \text{ u} \),- \( m_{He} = 3.0160 \text{ u} \),- \( m_{n} = 1.0087 \text{ u} \).Calculate \( \Delta m \):\[ \Delta m = (2 \times 2.0141) - (3.0160 + 1.0087) = 0.0045 \text{ u} \]Convert to energy using \( E = \Delta m \cdot c^2 \) (1 u = 931.5 MeV):\[ E = 0.0045 \times 931.5 = 4.19 \text{ MeV} \]Convert MeV to Joules:\[ E = 4.19 \times 1.6 \times 10^{-13} \approx 6.7 \times 10^{-13} \text{ J} \]
03

Calculate Energy per Mole of Deuterium

Since deuterium gas is diatomic (\(D_2\)), we have Avogadro's number of molecules (\(N_A = 6.022 \times 10^{23} \text{ mol}^{-1}\)) per mole. Each molecule contains two deuterium atoms, so the energy per mole is:\[ E_{\text{per mole}} = 2 \times 4.19 \text{ MeV/molecule} \times 6.022 \times 10^{23} \text{ molecules/mol} \]Convert to Joules:\[ E_{\text{per mole}} = 2 \times 4.19 \times 1.6 \times 10^{-13} \times 6.022 \times 10^{23} \approx 8.05 \times 10^{11} \text{ J/mol} \]This is much greater than the heat of combustion of hydrogen, \(2.9 \times 10^{5} \text{ J/mol} \).

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!

Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Coulomb barrier
When two positively charged nuclei come close to each other, they repel due to their like charges. This repulsion is known as the Coulomb barrier. In nuclear fusion, overcoming this barrier is crucial as it allows the nuclei to get close enough to combine or fuse. This is governed by the formula for electrostatic potential energy: \[ E_{r} = \frac{k \cdot e^2}{r} \]
  • Where \( k \) is Coulomb's constant, \( 8.99 \times 10^9 \, \text{Nm}^2/\text{C}^2 \)
  • \( e \) is the elementary charge, \( 1.6 \times 10^{-19} \, \text{C} \)
  • \( r \) is the distance between centers of the two touching nuclei, approximately \( 2 \times 10^{-15} \, \text{m} \) for deuterium
The resulting potential energy to overcome is about \( 0.24 \text{ MeV} \). This is a significant amount of energy necessary for fusion reactions, explaining why these reactions require extreme conditions like those found in stars.
energy liberation
In nuclear fusion, energy liberation refers to the energy released when lighter nuclei combine to form a heavier nucleus. This occurs because the resulting single nucleus has a mass that is less than the sum of the initial dual masses. The difference in mass, known as the mass defect, converts into energy following Einstein's equation \( E = mc^2 \). Fusion reactions, like the deuterium fusion, release a notable amount of energy. In this case, converting the mass defect to energy gives us about \( 4.19 \text{ MeV} \) for each fusion event. When these energies are harnessed, they hold the potential to power electrical grids, hence the interest in nuclear fusion as a future energy source.
deuterium fusion
Deuterium fusion involves two deuterium nuclei, which are heavy isotopes of hydrogen, merging under high temperature and pressure. The fusion reaction referenced here is:\( ^{2}_{1}\text{H} + ^{2}_{1}\text{H} \rightarrow ^{3}_{2}\text{He} + ^{1}_{0}\text{n} \)This process results in Helium-3 and a neutron, alongside liberating significant energy. Deuterium is abundant in seawater, making fusion a tantalizing clean energy possibility. Under the right conditions, where nuclei can overcome the Coulomb barrier, deuterium fusion could potentially provide nearly limitless energy, far exceeding traditional combustion methods.
mass defect
Mass defect is the missing mass that arises during nuclear reactions, such as fusion, where the mass of the resulting nuclei is smaller than the original sum of the reacting nuclei. This difference in mass translates into energy, following Einstein’s famous equation \( E = mc^2 \), providing the liberated energy that is a hallmark of nuclear chemistry.
  • In deuterium fusion, the initial mass is the combined mass of two deuterium nuclei.
  • The eventual mass is the mass of the new helium nucleus plus a neutron.
The difference in mass here is computed to be about \( 0.0045 \, \text{u} \), which converts to an energy release of approximately \( 4.19 \text{ MeV} \). Understanding mass defect is key to grasping how fusion fuels such as deuterium can produce vast amounts of energy, thus playing a pivotal role in nuclear science.

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 radioactive nuclide \(^1$$^9$$^9\)Pt has a half-life of 30.8 minutes. A sample is prepared that has an initial activity of 7.56 \(\times\) 10\(^1$$^1\) Bq. (a) How many \(^1$$^9$$^9\)Pt nuclei are initially present in the sample? (b) How many are present after 30.8 minutes? What is the activity at this time? (c) Repeat part (b) for a time 92.4 minutes after the sample is first prepared.

In the 1986 disaster at the Chernobyl reactor in eastern Europe, about \\(\frac{1}{8}\\) of the \(^{137}Cs\) present in the reactor was released. The isotope \(^{137}Cs\) has a half-life of 30.07 y for \(\beta\) decay, with the emission of a total of 1.17 MeV of energy per decay. Of this, 0.51 MeV goes to the emitted electron; the remaining 0.66 MeV goes to a \(\gamma\) ray. The radioactive \(^{137}Cs\) is absorbed by plants, which are eaten by livestock and humans. How many \(^{137}Cs\) atoms would need to be present in each kilogram of body tissue if an equivalent dose for one week is 3.5 Sv? Assume that all of the energy from the decay is deposited in 1.0 kg of tissue and that the RBE of the electrons is 1.5.

\(^2$$^3$$^8\)U decays spontaneously by \(\alpha\) emission to \(^2$$^3$$^4\)Th. Calculate (a) the total energy released by this process and (b) the recoil velocity of the \(^2$$^3$$^4\)Th nucleus. The atomic masses are 238.050788 u for \(^2$$^3$$^8\)U and 234.043601 u for \(^2$$^3$$^4\)Th.

What nuclide is produced in the following radioactive decays? (a) \(\alpha\) decay of \(^{239}_{94}Pu\); (b) \(\beta$$^-\) decay of \(^{24}_{11}Na\); (c) \(\beta$$^+\) decay of \(^{15}_{8}O\).

(a) If a chest x ray delivers 0.25 mSv to 5.0 kg of tissue, how many \(total\) joules of energy does this tissue receive? (b) Natural radiation and cosmic rays deliver about 0.10 mSv per year at sea level. Assuming an RBE of 1, how many rem and rads is this dose, and how many joules of energy does a 75-kg person receive in a year? (c) How many chest x rays like the one in part (a) would it take to deliver the same \(total\) amount of energy to a 75-kg person as she receives from natural radiation in a year at sea level, as described in part (b)?

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.