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astrobooger
Guest
I am doing research on a Science Fair Project pertaining to superdense matter. I have figured out the mechanics on how to fragment a White Dwarf, Neutron Star, or Black Hole. After they have formed, what is the lowest possible mass, volume, and density, while still ultradense?<br /><br />I have e-mailed numerous PhD level astrophysicists on the topic, and received no responses.<br /><br />If anyone knows anything on the topic, or knows another astrophysicist that would be willing to help, please e-mail me back and let me know.<br /><br />Thanks,<br />Astrobooger