Nuclear Reaction

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Alright so let's talk about nuclear reactions. Nuclear reactions are different from chemical reactions in the whole Chemistry class and your inorganic Chemistry class you've been taking all year you have been learning about just plain old chemical reactions well nuclear reactions are different because they're reactions that occur inside the nucleus okay so let's talk about some differences between chemical reactions and nuclear reactions.
One of the main differences is, is that in chemical reactions bonds are broken and formed and that's what makes the chemical reaction occur. They're broken and formed between two different atoms while nuclear reactions they are nuclei that emit particles and or rays into the atmosphere around us so it might be one single atom that's changing and emitting something that changing the nucleus inside and emitting something out in the atmosphere around it so it might not having anything to do with other atoms at all just one atom alone.
In a chemical reaction atoms are unchanged but rearranged, so they may be breaking breaking and rearranging other ways but the atoms themselves are unchanged whereas the nuclear reactions because we're changing the composition of the nucleus, we might be changing other protons. If we're changing number of protons, we know the protons [IB] the number of protons is unique for each atom so if we're going to change the number of protons in there we're actually going to change from one type of atom to another type of atom so you might have you know uranium might go from [IB] uranium to lead they can the atom actually completely changes it's identity because it's changing the number of protons or changing the things inside the nucleus.
In chemical reactions they involve valence electrons we know that. In nuclear reactions they involve protons, neutrons and electrons. Protons and neutrons are inside the nucleus so these are the guys that actually are going to affect or make the chemical reaction or the nuclear reaction occur.
Chemical reactions relatively chemical reactions have small energy changes relative to nuclear reactions. Nuclear reactions have extremely extremely large chemical chemical changes. I mean if you think about chemical reaction they will you know something might blow up and that's, that's that a lot to you and me that a lot of energy being released. However, nuclear reactions can if you think about an atom bomb, nuclear reactions can be blow up cities and possibly even countries off of the map whereas chemical reactions might have a small explosion comparatively so they'd actually a ton of energy within them.
Chemical reactions are, the rate of the chemical reactions influence the concentration, temperature, pressure and catalysts. The nuclear reactions are unaffected by these things. The nuclear reaction rates can are as large as millions and millions of years like uranium decay or thousands years like carbon decay or like milliseconds so these guys are not affected by the temperature doesn't make it different by the concentration by the any catalysts can't help it nothing can actually increase or decrease the rate of nuclear decay like you can with chemical reactions.
So these are the main differences between nuclear and chemical equations and if you want to learn more of there's more videos to come.

  1. Nuclear Fission
  2. Nuclear Reactions'
  3. Nuclear Reaction Ppt
  4. Nuclear Reactions Gizmo
  5. Types Of Nuclear Reactor

Learning Objectives

Nuclear Reaction

Nuclear Reactions A nuclear reaction occurs when two species (known as nuclides) collide and produce a new species that is different from the ones that started the reaction. The reactions usually produce more stable species and release a tremendous amount of energy. The two types of nuclear reactions are nuclear fission and fusion. Changes of nuclei that result in changes in their atomic numbers, mass numbers, or energy states are nuclear reactions. To describe a nuclear reaction, we use an equation that identifies the nuclides involved in the reaction, their mass numbers and atomic numbers, and the other particles involved in the reaction.

Nuclear fission
  • Identify common particles and energies involved in nuclear reactions
  • Write and balance nuclear equations

Changes of nuclei that result in changes in their atomic numbers, mass numbers, or energy states are nuclear reactions. To describe a nuclear reaction, we use an equation that identifies the nuclides involved in the reaction, their mass numbers and atomic numbers, and the other particles involved in the reaction.

Types of Particles in Nuclear Reactions

Many entities can be involved in nuclear reactions. The most common are protons, neutrons, alpha particles, beta particles, positrons, and gamma rays, as shown in Figure (PageIndex{1}). Protons ( (ce{^{1}_{1}p}), also represented by the symbol (ce{^1_1H})) and neutrons ( (ce{^1_0n})) are the constituents of atomic nuclei, and have been described previously. Alpha particles ( (ce{^4_2He}), also represented by the symbol (ce{^{4}_{2}alpha})) are high-energy helium nuclei. Beta particles ( (ce{^{0}_{−1}beta}), also represented by the symbol (ce{^0_{-1}e})) are high-energy electrons, and gamma rays are photons of very high-energy electromagnetic radiation. Positrons ( (ce{^0_{+1}e}), also represented by the symbol (ce{^0_{+1}β})) are positively charged electrons (“anti-electrons”). The subscripts and superscripts are necessary for balancing nuclear equations, but are usually optional in other circumstances. For example, an alpha particle is a helium nucleus (He) with a charge of +2 and a mass number of 4, so it is symbolized (ce{^4_2He}). This works because, in general, the ion charge is not important in the balancing of nuclear equations.

Note that positrons are exactly like electrons, except they have the opposite charge. They are the most common example of antimatter, particles with the same mass but the opposite state of another property (for example, charge) than ordinary matter. When antimatter encounters ordinary matter, both are annihilated and their mass is converted into energy in the form of gamma rays (γ)—and other much smaller subnuclear particles, which are beyond the scope of this chapter—according to the mass-energy equivalence equation (E = mc^2), seen in the preceding section. For example, when a positron and an electron collide, both are annihilated and two gamma ray photons are created:

[ce{^0_{−1}e + ^0_{+1}e } rightarrow gamma + gamma label{21.3.1}]

Nuclear

Gamma rays compose short wavelength, high-energy electromagnetic radiation and are (much) more energetic than better-known X-rays. Gamma rays are produced when a nucleus undergoes a transition from a higher to a lower energy state, similar to how a photon is produced by an electronic transition from a higher to a lower energy level. Due to the much larger energy differences between nuclear energy shells, gamma rays emanating from a nucleus have energies that are typically millions of times larger than electromagnetic radiation emanating from electronic transitions.

Balancing Nuclear Reactions

A balanced chemical reaction equation reflects the fact that during a chemical reaction, bonds break and form, and atoms are rearranged, but the total numbers of atoms of each element are conserved and do not change. A balanced nuclear reaction equation indicates that there is a rearrangement during a nuclear reaction, but of subatomic particles rather than atoms. Nuclear reactions also follow conservation laws, and they are balanced in two ways:

  1. The sum of the mass numbers of the reactants equals the sum of the mass numbers of the products.
  2. The sum of the charges of the reactants equals the sum of the charges of the products.

If the atomic number and the mass number of all but one of the particles in a nuclear reaction are known, we can identify the particle by balancing the reaction. For instance, we could determine that (ce{^{17}_8O}) is a product of the nuclear reaction of (ce{^{14}_7N}) and (ce{^4_2He}) if we knew that a proton, (ce{^1_1H}), was one of the two products. Example (PageIndex{1}) shows how we can identify a nuclide by balancing the nuclear reaction.

Example (PageIndex{1}): Balancing Equations for Nuclear Reactions

The reaction of an (α) particle with magnesium-25 ( (ce{^{25}_{12}Mg})) produces a proton and a nuclide of another element. Identify the new nuclide produced.

Solution

The nuclear reaction can be written as:

[ce{^{25}_{12}Mg + ^4_2He rightarrow ^1_1H + ^{A}_{Z}X} nonumber]

where

  • (ce A) is the mass number and
  • (ce Z) is the atomic number of the new nuclide, (ce X).

Because the sum of the mass numbers of the reactants must equal the sum of the mass numbers of the products:

[mathrm{25+4=A+1} nonumber]

so

[ mathrm{A=28} nonumber]

Nuclear Fission

Nuclear Reaction

Similarly, the charges must balance, so:

[mathrm{12+2=Z+1} nonumber]

Nuclear Reactions'

Reaction

so

[mathrm{Z=13} nonumber]

Check the periodic table: The element with nuclear charge = +13 is aluminum. Thus, the product is (ce{^{28}_{13}Al}).

Exercise (PageIndex{1})

The nuclide (ce{^{125}_{53}I}) combines with an electron and produces a new nucleus and no other massive particles. What is the equation for this reaction?

Answer

[ce{^{125}_{53}I + ^0_{−1}e rightarrow ^{125}_{52}Te} nonumber]

Following are the equations of several nuclear reactions that have important roles in the history of nuclear chemistry:

  • The first naturally occurring unstable element that was isolated, polonium, was discovered by the Polish scientist Marie Curie and her husband Pierre in 1898. It decays, emitting α particles: [ce{^{212}_{84}Po⟶ ^{208}_{82}Pb + ^4_2He}nonumber]
  • The first nuclide to be prepared by artificial means was an isotope of oxygen, 17O. It was made by Ernest Rutherford in 1919 by bombarding nitrogen atoms with α particles: [ce{^{14}_7N + ^4_2α⟶ ^{17}_8O + ^1_1H} nonumber]
  • James Chadwick discovered the neutron in 1932, as a previously unknown neutral particle produced along with 12C by the nuclear reaction between 9Be and 4He: [ce{^9_4Be + ^4_2He⟶ ^{12}_6C + ^1_0n} nonumber]
  • The first element to be prepared that does not occur naturally on the earth, technetium, was created by bombardment of molybdenum by deuterons (heavy hydrogen, (ce{^2_1H})), by Emilio Segre and Carlo Perrier in 1937: [ ce{^2_1H + ^{97}_{42}Mo⟶2^1_0n + ^{97}_{43}Tc}nonumber]
  • The first controlled nuclear chain reaction was carried out in a reactor at the University of Chicago in 1942. One of the many reactions involved was: [ ce{^{235}_{92}U + ^1_0n⟶ ^{87}_{35}Br + ^{146}_{57}La + 3^1_0n} nonumber]

Nuclear Reaction Ppt

Summary

Nuclei can undergo reactions that change their number of protons, number of neutrons, or energy state. Many different particles can be involved in nuclear reactions. The most common are protons, neutrons, positrons (which are positively charged electrons), alpha (α) particles (which are high-energy helium nuclei), beta (β) particles (which are high-energy electrons), and gamma (γ) rays (which compose high-energy electromagnetic radiation). As with chemical reactions, nuclear reactions are always balanced. When a nuclear reaction occurs, the total mass (number) and the total charge remain unchanged.

Glossary

alpha particle
(α or (ce{^4_2He}) or (ce{^4_2α})) high-energy helium nucleus; a helium atom that has lost two electrons and contains two protons and two neutrons
antimatter
particles with the same mass but opposite properties (such as charge) of ordinary particles
beta particle
((β) or (ce{^0_{-1}e}) or (ce{^0_{-1}β})) high-energy electron

Nuclear Reactions Gizmo

gamma ray
(γ or (ce{^0_0γ})) short wavelength, high-energy electromagnetic radiation that exhibits wave-particle duality
nuclear reaction
change to a nucleus resulting in changes in the atomic number, mass number, or energy state
positron ((ce{^0_{+1}β}) or (ce{^0_{+1}e}))
antiparticle to the electron; it has identical properties to an electron, except for having the opposite (positive) charge

Contributors and Attributions

Types Of Nuclear Reactor

  • Paul Flowers (University of North Carolina - Pembroke), Klaus Theopold (University of Delaware) and Richard Langley (Stephen F. Austin State University) with contributing authors. Textbook content produced by OpenStax College is licensed under a Creative Commons Attribution License 4.0 license. Download for free at http://cnx.org/contents/[email protected]).