Fusion reaction (don't know what I'm doing wrong)

In summary, the conversation discusses a fusion reaction where the nuclei of two atoms combine to form a single atom of a different element, converting a fraction of the rest energy to kinetic energy. The specific example of hydrogen reacting with deuterium to form helium and a gamma ray is also mentioned. The conversation also includes a problem involving the calculation of total kinetic energy before and after the reaction, using various constants and equations.
  • #1
tkoi
2
0

Homework Statement


In a fusion reaction, the nuclei of two atoms join to form a single atom of a different element. In such a reaction, a fraction of the rest energy of the original atoms is converted to kinetic energy of the reaction products. A fusion reaction that occurs in the Sun converts hydrogen to helium. Since electrons are not involved in the reaction, we focus on the nuclei.

Hydrogen and deuterium (heavy hydrogen) can react to form helium plus a high-energy photon called a gamma ray:

[tex] ^1H + ^2H \rightarrow ^3He + \gamma[/tex]

Objects involved in the reaction:
Code:
Particle        # of protons    # of neutrons    Charge    Rest Mass (atomic mass units)
[sup]1[/sup]H (proton)     1               0                +e        1.0073
[sup]2[/sup]H (deuterium)  1               1                +e        2.0136
[sup]3[/sup]He (helium)    2               1                +2e       3.0155
gamma ray       0               0                0         0

Although in most problems you solve in this course you should use values of constants rounded to 2 or 3 significant figures, in this problem you must keep at least 5 significant figures throughout your calculation. Problems involving mass changes require many significant figures because the changes in mass are small compared to the total mass. In this problem you must use the following values of constants, accurate to 5 significant figures:

Code:
Constant                  Value to 5 significant figures
c (speed of light)        2.9979e8 m/s
e (charge of a proton)    1.6022e-19 coulomb
atomic mass unit          1.6605e-27 kg
[tex]\frac{1}{4 \pi \epsilon_0}[/tex]                      8.9875e9 N·m[sup]2[/sup] /C[sup]2[/sup]

A proton (1H nucleus) and a deuteron (2H nucleus) start out far apart. An experimental apparatus shoots them toward each other (with equal and opposite momenta). If they get close enough to make actual contact with each other, they can react to form a helium-3 nucleus and a gamma ray (a high energy photon, which has kinetic energy but zero rest energy). Consider the system containing all particles. Work out the answers to the following questions on paper, using symbols (algebra), before plugging numbers into your calculator.

The deuterium nucleus starts out with a kinetic energy of 1.38e-13 joules, and the proton starts out with a kinetic energy of 2.77e-13 joules. The radius of a proton is 0.9e-15 m; assume that if the particles touch, the distance between their centers will be twice that. What will be the total kinetic energy of both particles an instant before they touch?
[tex]K_{1_H} + K_{2_H} =[/tex] 2.86826e-13 joules (I got this one right)

What is the kinetic energy of the reaction products (helium nucleus plus photon)?
[tex]K_{He} + K_{\gamma} =[/tex] ________ joules

Homework Equations



[tex]E_f = E_i + W[/tex]
[tex]W = -\Delta U = U_i - U_f[/tex]
[tex]E = m c^2 + K[/tex]
[tex]U_{elec} = \frac{1}{4 \pi \epsilon_0} \frac{q_1 q_2}{r}[/tex]


The Attempt at a Solution


For the first question, which I got right:

[tex]E_f = E_i + W[/tex]

[tex]E_f = E_i + U_i - U_f[/tex]

[tex]E_f + U_f = E_i + U_i[/tex]

[tex]K_{1,f} + K_{2,f} + m_1 c^2 + m_2 c^2 + U_f = K_{1,i} + K_{2,i} + m_1 c^2 + m_2 c^2 + U_i[/tex]

[tex]K_{1,f} + K_{2,f} + U_f = K_{1,i} + K_{2,i} + U_i[/tex]
The particles start out 'far apart' so Ui = 0

[tex]K_{1,f} + K_{2,f} = K_{1,i} + K_{2,i} - U_f[/tex]
[tex] = 2.77 \times 10^{-13} + 1.38 \times 10^{-13} - \frac{1}{4 \pi \epsilon_0} \times \frac{e \times e}{2 \times 0.9 \times 10^{-15}}[/tex]
[tex] = 2.86826 \times 10^{-13}[/tex]


The second question:

[tex]E_f + U_f = E_i + U_i[/tex]

[tex]K_3 + K_\gamma + m_3 c^2 + m_\gamma c^2 + U_f = K_2 + K_1 + m_2 c^2 + m_1 c^2 + U_i[/tex]
Gamma ray has 0 mass and 0 charge, so

[tex]K_3 + K_\gamma + m_3 c^2 = K_2 + K_1 + m_2 c^2 + m_1 c^2 + U_i[/tex]

[tex]K_3 + K_\gamma = K_2 + K_1 + m_2 c^2 + m_1 c^2 - m_3 c^2 + U_i[/tex]

[tex] = K_2 + K_1 + c^2 (m_2 + m_1 - m_3) + \frac{1}{4 \pi \epsilon_0} \times \frac{e \times e}{r}[/tex]

[tex] = 1.38 \times 10^{-13} + 2.77 \times 10^{-13} + c^2 (m_2 + m_1 - m_3) + \frac{1}{4 \pi \epsilon_0} \times \frac{e \times e}{2 \times 0.9 \times 10^{-15}}[/tex]
Here remember that mn = (rest mass) * (atomic mass unit)

[tex] = 1.34905 \times 10^{-12}[/tex]
My homework is submitted online, and this answer is wrong. I don't know where I messed up, I did exactly what I did for the first question which I got right. Any help is appreciated.
 
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  • #2
You added the potential energy when the proton and deuteron nearly touch to the kinetic energy when they are still far apart to get the initial energy.
 
  • #3
Ah! Of course it was something that simple. Sometimes I guess you just need a fresh pair of eyes to see what went wrong. Thanks a lot!
 

1. What is a fusion reaction?

A fusion reaction is a nuclear reaction in which two or more atomic nuclei combine to form a heavier nucleus. This process releases a large amount of energy, which is the same process that powers the sun and other stars.

2. How is a fusion reaction different from a fission reaction?

Fusion reactions involve merging two or more smaller nuclei to form a larger one, while fission reactions involve splitting a larger nucleus into smaller ones. Fusion reactions typically release more energy than fission reactions.

3. What elements are involved in a fusion reaction?

The most common elements involved in fusion reactions are hydrogen isotopes, specifically deuterium and tritium. These elements have the lowest energy requirements for fusion reactions to occur.

4. Why is it difficult to create a controlled fusion reaction on Earth?

Fusion reactions require extremely high temperatures and pressures, which can only be achieved in the core of a star. On Earth, scientists use specialized devices called tokamaks to create these conditions, but they have not yet been able to sustain a controlled fusion reaction for a sustained period of time.

5. What are the potential benefits of harnessing fusion energy?

If a controlled fusion reaction can be achieved, it could provide a nearly limitless source of clean energy. Fusion reactions produce no greenhouse gases or long-lived radioactive waste, making it a potentially sustainable and environmentally friendly energy source.

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