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Types of Radioactivity03:23

Types of Radioactivity

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The most common types of radioactivity are α decay, β decay, γ decay, neutron emission, and electron capture.
Alpha (α) decay is the emission of an α particle from the nucleus. For example, polonium-210 undergoes α decay:
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Nuclear Stability03:18

Nuclear Stability

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Protons and neutrons, collectively called nucleons, are packed together tightly in a nucleus. With a radius of about 10−15 meters, a nucleus is quite small compared to the radius of the entire atom, which is about 10−10 meters. Nuclei are extremely dense compared to bulk matter, averaging 1.8 × 1014 grams per cubic centimeter. If the earth’s density were equal to the average nuclear density, the earth’s radius would be only about 200 meters.
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Nuclear Transmutation03:20

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Nuclear transmutation is the conversion of one nuclide into another. It can occur by the radioactive decay of a nucleus, or the reaction of a nucleus with another particle. The first manmade nucleus was produced in Ernest Rutherford’s laboratory in 1919 by a transmutation reaction, the bombardment of one type of nuclei with other nuclei or with neutrons. Rutherford bombarded nitrogen-14 atoms with high-speed α particles from a natural radioactive isotope of radium and observed...
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Radioactivity and Nuclear Equations03:18

Radioactivity and Nuclear Equations

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Nuclear chemistry is the study of reactions that involve changes in nuclear structure. The nucleus of an atom is composed of protons and, except for hydrogen, neutrons. The number of protons in the nucleus is called the atomic number (Z) of the element, and the sum of the number of protons and the number of neutrons is the mass number (A). Atoms with the same atomic number but different mass numbers are isotopes of the same element.
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Nuclear Binding Energy02:13

Nuclear Binding Energy

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The difference between the calculated and experimentally measured masses is known as the mass defect of the atom. In the case of helium-4, the mass defect indicates a “loss” in mass of 4.0331 amu – 4.0026 amu = 0.0305 amu. The loss in mass accompanying the formation of an atom from protons, neutrons, and electrons is due to the conversion of that mass into energy that is evolved as the atom forms. The nuclear binding energy is the energy produced when the atoms’ nucleons are bound...
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Isotopes and Radioisotopes01:28

Isotopes and Radioisotopes

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In the early 1900s, English chemist Frederick Soddy realized that an element could have atoms with different masses that were chemically indistinguishable. These different types are called isotopes — atoms of the same element that differ in mass. Isotopes differ in mass because they have different numbers of neutrons but are chemically identical because they have the same number of protons. Soddy was awarded the Nobel Prize in Chemistry in 1921 for this discovery.
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Related Experiment Video

Updated: Mar 17, 2026

Preparing an Isotopically Pure 229Th Ion Beam for Studies of 229mTh
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Preparing an Isotopically Pure 229Th Ion Beam for Studies of 229mTh

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First Measurement of Several β-Delayed Neutron Emitting Isotopes Beyond N=126.

R Caballero-Folch1,2, C Domingo-Pardo3, J Agramunt3

  • 1INTE-DFEN, Universitat Politècnica de Catalunya, E-08028 Barcelona, Spain.

Physical Review Letters
|July 16, 2016
PubMed
Summary

This study measured beta-delayed neutron emission and beta-decay half-lives for heavy Gold, Mercury, Thallium, Lead, and Bismuth nuclei. These findings offer crucial data for refining nuclear models used in astrophysical r-process nucleosynthesis simulations.

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Area of Science:

  • Nuclear Physics
  • Astrophysical Nucleosynthesis

Background:

  • Neutron-rich nuclei near the N=126 shell closure are crucial for understanding the rapid neutron-capture (r-process) nucleosynthesis.
  • Experimental data on beta-delayed neutron emission probabilities and beta-decay half-lives for these heavy nuclei are scarce.

Purpose of the Study:

  • To measure beta-delayed neutron emission probabilities and beta-decay half-lives for neutron-rich Hg and Tl isotopes.
  • To provide experimental data for evaluating nuclear models in the mass region N≳126.
  • To constrain theoretical models used in r-process nucleosynthesis.

Main Methods:

  • Measurement of beta-delayed neutron emission probabilities.
  • Measurement of beta-decay half-lives using advanced detection techniques.
  • Focus on heavy isotopes of Au, Hg, Tl, Pb, and Bi in the N≳126 mass region.

Main Results:

  • Successfully measured beta-delayed neutron emission probabilities for neutron-rich Hg and Tl nuclei.
  • Determined beta-decay half-lives for 20 isotopes across Au, Hg, Tl, Pb, and Bi.
  • Observed neutron emission in the heaviest species studied to date.

Conclusions:

  • The experimental data provide critical benchmarks for nuclear microscopic and phenomenological models.
  • These results help improve the accuracy of theoretical predictions for the r-process.
  • The study advances our understanding of nuclear structure and decay properties in heavy, neutron-rich systems.