Fission Fusion

Fission and fusion are nuclear reactions that transform atomic nuclei, releasing substantial energy as they change isotopes and elemental composition. Fission splits a heavy nucleus into smaller nuclei after neutron absorption, often producing additional neutrons that can sustain a chain reaction; fusion combines light nuclei under extreme temperature and pressure, where overcoming electrostatic repulsion allows the strong nuclear force to bind them. In chemistry, these processes help explain nuclear stability, isotope formation, radioactive decay pathways, and energy generation. Studying fission and fusion supports reactor design, radiochemical analysis, nuclear medicine, and research into lower-carbon energy systems.

Fission Fusion - Related Videos

Education

JoVE Core - Chemistry

Nuclear Fission

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2020

Many heavier elements with smaller binding energies per nucleon can decompose into more stable elements that have intermediate mass numbers and larger binding energies per nucleon—that is, mass numbers and binding energies per nucleon that are closer to the “peak” of the binding energy graph near 56. Sometimes neutrons are also produced. This decomposition of a large nucleus into smaller pieces is called fission. The breaking is rather random with the formation of a large number of different...

Research

JoVE Journal - Biology

Assessment of Mitochondrial Fission/Fusion Dynamics in Kidney Proximal Tubular Cells

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2025

This article describes the use of confocal microscopy and ImageJ to assess mitochondrial fission/fusion dynamics via Dendra2 photo-switching fluorescence.

Microscopy of Fission Yeast Sexual Lifecycle

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Cited by 38 •

2016

We provide a reproducible basic method for the long-term microscopy of the fission yeast sexual lifecycle. With minor adjustments described, the presented protocol allows research focus on different steps of the reproductive process.

Nuclear Fusion

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2020

The process of converting very light nuclei into heavier nuclei is also accompanied by the conversion of mass into large amounts of energy, a process called fusion. The principal source of energy in the sun is a net fusion reaction in which four hydrogen nuclei fuse and ultimately produce one helium nucleus and two positrons. A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...

Spatiotemporal Analysis of Cytokinetic Events in Fission Yeast

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Cited by 6 •

2017

The fission yeast, Schizosaccharomyces pombe is an excellent model system to study cytokinesis, the final stage in cell division. Here we describe a microscopy approach to analyze different cytokinetic events in live fission yeast cells.

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