Short answer: helium, positrons, neutrinos, gamma rays.
nb, due to the limitations of raw text, I am decribing these atoms in the form "(Atomic Mass) / (atomic number) (element)". "e+" denotes a positron, "e-" an electron, "v" a neutrino and, "y" a gamma ray photon. If this is for your homework, you probably want to use the correct symbols with the appropriate subscript and superscript and without all the parentheses. You may also be using "p" instead of "1/1 H" and possible "2/1 D" or simply "2 D" for deuterium instead of 2/1 H. Onward.
Hydrogen fuses into helium, by the following processes:
ppI chain:
i: (1/1 H) + (1/1 H) -> (2/1 H) + (e+) + (v)
ii: (2/1 H) + (1/1 H) -> (3/2 He) + (y)
iii: (3/2 He) + (3/2 He) -> (4/2 He) + 2(1/1 H)
In words; two protons (hydrogen nuclei) fuse to form deuterium, in doing so, one of the protons becomes a neutron via beta decay with the emission of a positron and neutrino (if you need to go deeper than this, it's decay via the weak interaction with the emission of a W- boson which spontaneously decays into a positron and neutrino).
This deuterium nucleus fuses with another proton to form 3/2 helium. Here no protons are decaying into neutrons so there is no e+/v emission, however because the rest energy per nucleon in 3/2 He is lower than in the hydrogen nuclides 1/1 H and 2/1 H, the leftover energy escapes as a gamma ray. This is the stage at which the vast majority of energy is liberated from the material.
Then, in this particular chain, two 3/2 He nuclei fuse to form a 4/2 He nucleus (an alpha particle) with the return of two protons to the soup.
ppII chain
(i) and (ii) as per ppI
(iii) (3/2 He) + (4/2 He) -> (7/4 Be) + (y)
(iv) (7/4 Be) + (e-) -> (7/3 Li) + (v)
(v) (7/3 Li) + (1/1 H) -> 2(4/2 He)
Here, our 3/2 He from the ppI chain fuses with a 4/2 He to create 7/4 Be, and again the difference in rest energies is carried away by another gamma ray. An electron is captured (this process is rather unimaginatively called "electron capture) transmuting the 7/4 Be into 7/3 Li (one proton becomes a neutron) with the ejection of a neutrino. This 7/3 Li nucleus fuses with a proton to create 8/4 Be which is unstable and almost immediately breaks down into two 4/2 He alpha particles.
ppIII chain
(i), (ii) and (iii) as per ppII
(iv) (7/4 Be) + (1/1 H) -> (8/5 B) + (y)
(v) (8/5 B) -> (8/4 Be) + (e+) + (v)
(vi) (8/4 Be) -> 2(4/2 He)
In this instance the 7/4 Be we made in the ppII chain fuses with another proton to create 8/5 B, with the emission of yet another gamma ray. The boron nucleus then beta decays into 8/4 beryllium, which again breaks down into two alpha particles.
In summary, and to answer your question directly:
ppI: 4(1/1 H) -> (4/2 He) + 2(e+) + 2(v) + 2(y)
ppII: 4(1/1 H) + (e-) -> (4/2 He) + (e+) + 2(v) + 2(y)
ppIII: 4(1/1 H) -> 2(e+) + 2(v) + 3(y)
There is also an hypothesised ppIV chain in which:
(3/2 He) + (1/1 H) -> (4/2 He) + (e+) + (v) + (y)
And also a rare means of creating 2/1 H:
(1/1 H) + (e-) + (1/1 H) -> (2/1 H) + (v)
In our Sun, which I presume is why you are interested in this, the ppI chain dominates, with roughly 85% of hydrogen burning following this route. The ppII chain accounts for about 15%, and the ppIII chain a pathetic 0.02%.
But wait, there's more. In larger, hotter stars there is another important mechanism called the CNO cycle. It looks like this:
(i) (12/6 C) + (1/1 H) -> (13/7 N) + (y)
(ii) (13/7 N) -> (13/6 C) + (e+) + (v)
(iii) (13/6 C) + (1/1 H) -> (14/7 N) + (y)
(iv) (14/7 N) + (1/1 H) -> (15/8 O) + (y)
(v) (15/8 O) -> (15/7 N) + (e+) + (v)
(vi) (15/7 N) + (1/1 H) -> (12/6 C) + (4/2 He)
I'm sure I don't need to explain what's happening this time, so we are left with the summary which is:
CNO: 4(1/1 H) -> (4/2 He) + 2(e+) + 2(v) + 3(y)
You are now a fully qualified nuclear physicist.
No. In a fusion reaction, a heavier element is made of a lighter pair by "gluing" them together in a fusion reaction. When we split an atom, that's called atom splitting, or sometimes fission, not fusion. They are opposites. Stars give off light, but the primary fuel in their fusion engines is hydrogen, which they convert into helium. As the hydrogen burns out, the star begins making helium into carbon.
No Sol Blaze is not the strongest in Metal Fusion because he never existed in Metal Fusion.
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Nuclear fusion of hydrogen-1 and lithium-7 will give two helium-4 nuclei (alpha particles). Hydrogen-1 + lithium-7 --> helium-4 + helium-4 + E (energy) The conservation law for number of nucleons applies here!
No Strontium is produced by nuclear fission not fusion.
Iron is the most massive element that can be formed by nuclear fusion with the liberation of energy. This is because fusion reactions beyond iron require an input of energy rather than liberating energy.
Isotopes are formed either naturally through radioactive decay of elements or artificially through element irradiation by particles as neutrons, protons, electrons, or alpha particles in accelerators or nuclear reactors through nuclear fission or nuclear fusion reactions in nuclear reactors.supernovasparticle acceleratorsnuclear reactorsnuclear explosionsradioactive decay
When a hydrogen bomb explodes, the primary element formed is helium. This occurs through the process of nuclear fusion, where hydrogen isotopes combine to form helium atoms, releasing a large amount of energy in the process.
Existing element is product of nuclear fusion, heavy element exist from over fusion and thus create high atomic mass substance. To answer what is the element that is form last in nuclear fusion in star is the same as asking what is the heaviest element occur or found in nature. Base on what is in periodic table. The heaviest element found naturally is around Uranium - Plutonium thus it could be considered the last product known in nuclear fusion in star. There are heavier element than Uranium and Plutonium but those are synthesize element. Nuclear fusion might go to element heavier than what is known in our periodic table but those substance may be unstable and decay over time until none of those exist.
The main by-product of nuclear fusion is helium, which is formed when hydrogen atoms combine under high temperatures and pressures. Additionally, energy in the form of electromagnetic radiation, such as gamma rays, is also released during the fusion process.
Hydrogen and helium were formed shortly after the creation of the universe (when the protons and alpha particles combined with electrons). Everything else was formed within the core of stars (by fusion reactions).
Yes. Radium is a natural decay product of uranium, which is naturally formed in stellar nuclear fusion.
One likely product of a fusion reaction is helium, which is formed when hydrogen isotopes like deuterium and tritium fuse together. Energy is also released during this process, which can potentially be harnessed for power generation in technologies like nuclear fusion reactors.
Iron is the heaviest element formed by fusion in the core of a supergiant star prior to its supernova explosion. Elements heavier than iron are typically formed during the supernova explosion itself through nucleosynthesis processes.
A variety of different fusion reactions are possible. In our sun, which is classified as medium sized, it is fusion of hydrogen nuclei, ie protons, to form helium. In larger stars, especially red giants, larger nuclei react in fusion, so that larger and heavier nuclei get formed.
A fusion reaction generates helium as a waste product.
Any element except Hydrogen technically. The product depends on what elements are undergoing nuclear fusion, e.g. 2 Hydrogen atoms form a Helium atom. You will need to specify for an answer.