Conservation of Energy fusion reaction

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SUMMARY

The discussion centers on the fusion reaction of deuterium and tritium, represented by the equation 2H+3H → 4He + n. Participants analyze the conservation of energy principle, confirming that the total energy before and after the reaction remains constant. Key calculations include the masses of deuterium (3.32108e-27 kg), tritium (4.98162e-27 kg), helium (6.64215e-27 kg), and neutron (1.67493e-27 kg), which are converted into electron-volts (eV) for energy calculations. The discussion concludes with the need to determine the number of fusion reactions required to generate 1 MW of power, assuming 100% efficiency in energy conversion.

PREREQUISITES
  • Understanding of nuclear fusion reactions
  • Familiarity with mass-energy equivalence (E=mc²)
  • Knowledge of energy units (eV and MeV)
  • Basic principles of conservation of energy
NEXT STEPS
  • Calculate the total kinetic energy after the fusion reaction using conservation of energy principles
  • Research methods for converting kinetic energy from fusion reactions into usable energy
  • Explore the efficiency of fusion reactions in energy generation
  • Investigate the implications of fusion energy for sustainable power generation
USEFUL FOR

Students in physics, nuclear engineers, and researchers interested in fusion energy and its applications in power generation.

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Homework Statement


Consider the following fusion reaction
2H+3H →4He + n
in which deuterium and tritium fuse together to form a stable isotope of helium plus a neutron.
In all of physics, we see experimental confirmation of Conservation of Energy, in which the total
amount of energy in a closed system is constant. The total rest plus kinetic energy before the
reaction must be equal to the total rest plus kinetic energy after the reaction.

(a) Look up the masses of the three nuclei and of the neutron in kilograms, keeping at least six
significant figures. Cite your reference. Because we have the same number of electrons before
and after the reaction (and because atomic binding energies are tiny compared to the energies
in this problem), it is not important whether you use nuclear masses or atomic masses.

(b) Convert each of those masses into rest energies in electron-volts (eV). Recall that the speed of
light is 299,792,458 m/s, and that 1 eV = 1.60217653× 10−19 J.

(c) Assuming that the deuterium and tritium have a total of 0.05 MeV of kinetic energy before
the reaction, use conservation of energy to calculate the total kinetic energy after the reaction.
Recall that we handle addition and subtraction differently than multiplication and division
when dealing with significant figures.

(d) Assuming that all of this kinetic energy can be converted with 100% efficiency into usable
energy, how many fusion reactions per second do we need to generate 1 MW of power?

Homework Equations


(a) Nuclei Masses:
Deuterium: 3.32108e-27 kg
Tritium: 4.98162e-27 kg
Isotope of Helium: 6.64215e-27 kg
Neutron: 1.67493e-27 kg

The Attempt at a Solution


(b)First I will convert the masses to eV (online conversion):
Deuterium: 1,862,990,000 eV
Tritium: 2,794,480,000 eV
Isotope of Helium: 3,725,970,000 eV
Neutron: 939,567,000 eV

(c) I will add together the eV of 4He + neutron = 4,665,537,000 eV
Now I will convert eV to MeV:
4,665.537 MeV
Can I subtract this by .05 MeV? I feel like I am on the wrong track
 
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