Calculate the rest energy of the alpha particle and the products using E=mc^2, then take the difference (initial - final) between the initial and final states. If your final proton and neutron are independent, use the individual proton and neutron mass in your calculation. If they come off as a deuterium, use the mass of deuterium in the calculation.
So you get E(4He) - E(2H) -E(mp) - E(mn) in the former case, and E(4HE) - 2E(2H) in the latter case.
To calculate the energy output of a thorium subcritical reactor when you know the neutron flux input, you would multiply the neutron flux by the energy produced per neutron capture in the thorium fuel. This can be determined based on the specific design and characteristics of the reactor. By knowing the neutron flux input and the energy produced per neutron capture, you can estimate the energy output of the reactor.
To calculate binding energy, you subtract the rest mass of the nucleus from the actual mass of the nucleus measured. This difference represents the energy required to disassemble the nucleus into its individual nucleons. The formula is: Binding energy = (Z x proton rest mass) + (N x neutron rest mass) - actual mass of the nucleus.
A neutron is the particle required to continue the chain process of Uranium fission. When a Uranium-235 nucleus absorbs a neutron, it becomes unstable and splits into two smaller nuclei, releasing energy and additional neutrons that can then go on to induce further fission reactions in nearby nuclei.
The heat of fusion is used to first convert the volume of liquid to its solid form, then the heat of vaporization is used to convert the solid to vapor. By summing the two energy values, you can calculate the total energy required to vaporize the liquid volume.
A thermal neutron has an energy range of about 0.025 eV (electronvolts) which corresponds to its average kinetic energy at room temperature.
To calculate the energy output of a thorium subcritical reactor when you know the neutron flux input, you would multiply the neutron flux by the energy produced per neutron capture in the thorium fuel. This can be determined based on the specific design and characteristics of the reactor. By knowing the neutron flux input and the energy produced per neutron capture, you can estimate the energy output of the reactor.
Deuterium and tritium can undergo nuclear fusion to produce helium-4 and a neutron. This reaction is the basis for the energy production in hydrogen bombs and is a potential energy source for fusion reactors.
An example of ionization energy is the energy required to remove an electron from a neutral helium atom to form a helium ion. This process results in the ionization of the helium atom, as it loses an electron and becomes positively charged.
The sun uses nuclear fusion to produce light and energy. the process is relatively complicated but simplified it looks something like this. step 1: hydrogen atom + hydrogen atom = deutrerium atom (an isotope of hydrogen (one extra neutron)) + positron + neutrino step 2: Deutrerium atom + hydrogen atom = helium 3 (an isotope of Helium (missing one neutron)) + energy step 3: helium 3 atom + helium 3 atom = helium atom + hydrogen atom + hydrogen atom + energy.
Absorption of neutrons by an element depends on neutron cross-section data for that element at the energy of interest. The absorption cross-section gives the probability of a neutron being absorbed by an atom of the element. Measuring the absorptions at a certain neutron energy can help in determining the propensity of an element to absorb neutrons at that energy level.
The variable that is not required to calculate the Gibbs free-energy change for a chemical reaction is the temperature.
The energy required for an element to ionize and helium has the lowest.
To find the total binding energy Use this formula: B= (number of neutrons)(neutron mass)+ (number of protons)(proton mass) - (Atomic Mass of helium). Then to keep the units correct, multiply that entire expression by 931.5 MeV/u. This is the TOTAL binding energy, and the binding energy per nucleon can be found by dividing the number you calculate above by the total number of protons and neutrons.
Helium-3 has a high cross section for thermal neutron absorption. For fast neutrons you must either thermalize the neutrons for use with boron or helium-3 based proportional counters or use a fast fission chamber based on fast fission of uranium. It's worth noting that a uranium based fast fission detector is really only useful in extraordinarily high neutron fluxes like that of a reactor.
If you fuse deuterium (1p, 1n) with tritium (1p, 2n), you get helium (2p, 2n) plus a free neutron, plus the released energy
the first inoization energy is 2372.3 kJ mol-1 there are 6.0221415 × 10^23 in a mole from avagadros number, devide the ionization energy for one mole by the number of atoms in a mole and you get the first ionization energy for one atom.
Fusion of two hydrogen nuclei results in the formation of helium and a stray neutron. H31 + H21 -----> He42 + n10 The hydrogen with atomic number 3 is trituim and the hydrogen with atomic no. 2 is deutrium. They both fuse together to form Helium with the release of a spray neutron, accompanied by a large release of energy.