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Once produced, the Higgs boson disintegrates immediately in one of several ways (decay modes) into known SM particles, depending on its mass.
The Higgs, if formed, would decay into smaller jets of quarks or other particles, depending on its mass.
The Higgs boson decays differently, depending on its mass, since a heavier Higgs boson can decay in ways that a light Higgs boson can't.
A good example is Isaac Newton's theory of gravitation, which says that every physical object in the universe exerts a gravity force field around itself, with the strength of that field depending on its mass.
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The final stages in the evolution of a star depend on its mass and angular momentum and whether it is a member of a close binary.
Many important properties of an isotope depend on its mass.
How long the star lives depends on its mass: a star with higher mass will burn through material faster due to a higher core temperature, caused by greater gravitational forces.
A factory's lifetime output depends on its mass: Larger stars burn hotter and churn out heavy elements faster than smaller stars do.
Mechanical behavior of bone depends on its mass and architecture, and on the material properties of the matrix, which is composed of a mineral phase and an organic component mainly constituted of type I collagen.
The behavior of a star now depends on its mass, with stars below 0.23 becoming white dwarfs directly, while stars with up to ten solar masses pass through a red giant stage.
The final fate of the star depends on its mass, with stars of mass greater than about eight times the Sun becoming core collapse supernovae; while smaller stars form a white dwarf as it ejects matter that forms a planetary nebulae.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com