Complete the following fusion process: 1H+2H⟶−−−−−−
Complete the following fusion process:
31n |
4He |
3He |
1n |
Complete the following fusion process: 1H+2H⟶−−−−−− Complete the following fusion process: 31n 4He 3He 1n
Fusion problems, find the energy release 2H +3H → 4He + ? 4He +4He → 7Be + ? 2H +3He → 4He + ? 2H + 1H → ᵞ+ ?
Complete the following fusion reaction: 4He+3He⟶2H+−−−−−−. Express your answer as a complete nuclear equation. nothing SubmitRequest Answer
Find the energy Q released in the fusion reaction. (Note that the reaction below is between nuclei. For the atomic masses, see this table. The mass of an electron is 0.00054 1H+3He → 4He + e+ + ν MeV Find the energy Q released in the fusion reaction. (Note that the reaction below is between nuclei. For the atomic masses, see this table. The mass of an electron is 0.00054 1H+3He → 4He + e+ + ν MeV
How much energy (in MeV) is released during the following fusion reaction? 1H + 2H → 3He Molar mass of 1H = 1.00728 g/mol Molar mass of 2H = 2.01355 g/mol Molar mass of 3He = 3.01493 g/mol 1 MeV = 1.60218 * 10-13 J
How much energy (in MeV) is released during the following fusion reaction? 1H + 2H → 3He Molar mass of 1H = 1.00728 g/mol Molar mass of 2H = 2.01355 g/mol Molar mass of 3He = 3.01493 g/mol 1 MeV = 1.60218 * 10-13 J Report your answer to one decimal place. Do not input a unit or a sign (+/-).
Using the table below, find the Q values for the following reactions. (a) n + 3He --> 3H + 1H + Q MeV (b) n + 6Li --> 3H + 4He + Q MeV (c) 7Li + 1H --> 4He + 4He + Q MeV
Consider the proton–proton cycle that occurs in most stars (including our own Sun): Step 1: 1H + 1H → 2H + e+ + νe Step 2: 2H + 1H → 3He + γ Step 3: 3He + 3He → 4He + 2 1H + γ Calculate the net energy released from the three steps. Do not ignore the mass of the positron in Step 1. (You may ignore the mass of the neutrino.) MeV
4He is formed when isotopes of hydrogen undergo fusion. What is the energy associated with the formation of 2.00 g of 4He (1 mole = 4.00260 g) by the fusion of 3H and 1H? ΔE for the formation of one atom of 4He is -3.17603×10-12 J.
Stellar nuclear fusion begins with 1H and ends with 56Fe. Younger stars fuse hydrogen to form 4He, while older, more massive stars fuse Helium to form heavier elements. Fusion beyond 56Fe is impossible because iron-56 has the greatest binding energy per nucleon. Calculate the binding energy per nucleon of 56Fe and use it to calculate the maximum total energy per mole of 56Fe that could be released through nuclear fusion. What percentage of the maximum total energy is released by...
Complete the following fusion reaction: 2H+3H⟶n+−−−−−−. Express your answer as a complete nuclear equation. nothing SubmitRequest Answer