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<p>or more <a href="page.php?w=solar_mass">solar mass</a>es), photodisintegration is a major factor in the <a href="page.php?w=supernova">supernova</a> event. As the star reaches the end of its life, it reaches temperatures and pressures where photodisintegration's energy-absorbing effects temporarily reduce pressure and temperature within the star's core. This causes the core to start to collapse as energy is taken away by photodisintegration, and the collapsing core leads to the formation of a <a href="page.php?w=black_hole">black hole</a>. A</p><p>
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