1 / 9

Understanding Nuclear Reactions: Stability and Radioactive Decay Explained

Nuclear energy involves unstable isotopes transitioning to stability by altering their nucleus, releasing substantial radiation energy in the process. Radioisotopes, which possess unstable nuclei, rely on the neutron-to-proton ratio for stability. Excess neutrons contribute to instability, resulting in energy loss through radiation during radioactive decay. There are three primary decay types: Alpha decay (ejecting helium nuclei), Beta decay (neutron transforms into a proton and an electron), and Gamma decay (emission of electromagnetic radiation). This process continues in decay series until a stable isotope is formed.

reed
Download Presentation

Understanding Nuclear Reactions: Stability and Radioactive Decay Explained

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. Nuclear Energy

  2. Nuclear Reactions- when unstable isotopes gain stability by making changes in the nucleus. • These changes are followed by large amounts of radiation energy

  3. Radioisotopes-isotopes that have unstable nuclei. • *Stability depends on ratio of neutrons to protons. • *TOO many Neutrons leads to unstable nuclei. • *Lose energy by giving off radiation during radioactive decay.

  4. 3 Types: • Alpha ()(42He)-Helium nucleus(2 protons +2 neutrons) is ejected from source • Beta ()( 0-1e)-fast moving electrons formed from decomposition of a neutron. • Gamma ()-Electromagnetic radiation

  5. Alpha: • 23692U232 90Th + 42He • When you lose alpha particle, Atomic # lowered by 2 and massby 4

  6. Beta: • 10n 1 1H + 0 -1e • neutron breaks into proton and electron. Electron ejected and proton stays in nucleus.

  7. Gamma: • 23290Th 22888Ra + 42He +  • 23290Th 23291Pa + 0-1e +  • Gamma often emitted with alpha or Beta radiation.

  8. Decay Series • A series of radioactive nuclides produced by successive radioactive decay until a stable nuclide is reached. • Parent nuclide- heaviest nuclide of each decay series • Daughter nuclide- nuclides produced by the decay of the parent nuclides

More Related